Comets, Meteors & Celestial Wonders : A Cosmic Special

Comets, Meteors & Celestial Wonders : A Cosmic Special

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Comets, Meteors, and Celestial Wonders In this engaging episode of Space Nuts, hosts Andrew Dunkley and Professor Jonti Horner dive deep into the fascinating world of comets and meteors. With Professor Fred Watson away, Jonti brings his expertise to explore these celestial phenomena, their historical significance, and the science behind them.
Episode Highlights:
Understanding Comets and Meteors: Andrew and Jonti kick off the episode by discussing the importance of comets and meteors in both ancient cultures and modern astronomy. They delve into how these celestial objects have been perceived throughout history and their impact on human events.
Recent Discoveries and Predictions: The hosts share insights on recent comet discoveries, including the intriguing Comet Chichin Chan, and discuss what we can expect from this comet in the near future. They also touch on the challenges of predicting comet brightness and visibility.
Meteor Showers Explained: Jonti explains how meteor showers occur, the significance of radiant points, and what conditions are best for viewing these spectacular events. They discuss the most notable meteor showers and when listeners can catch them in action.
The Impact of Media on Public Perception: The conversation takes a turn as Andrew and Jonti address the role of media in shaping public understanding of astronomical events, particularly the sensationalism surrounding potential alien encounters and the importance of relying on scientific facts.

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Stay curious, keep looking up, and join us next time for more stellar insights and cosmic wonders. Until then, clear skies and happy stargazing.

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00:00:00 --> 00:00:01 Andrew Dunkley: Hello again. Thank you for joining us on

00:00:01 --> 00:00:04 another episode of Space Nuts. My name is

00:00:04 --> 00:00:06 Andrew Dunkley, your host. It's great to have

00:00:06 --> 00:00:09 your company. As I mentioned last episode,

00:00:09 --> 00:00:12 Fred is away for a few weeks or

00:00:12 --> 00:00:15 a couple of years. Now it's a few weeks. And,

00:00:15 --> 00:00:17 uh, in his stead, we'll be joined by

00:00:17 --> 00:00:20 Professor Jonti Horner, who you know and love

00:00:20 --> 00:00:22 because he's been with us before and uh, he's

00:00:22 --> 00:00:25 a part of the team. So, uh, we will be

00:00:25 --> 00:00:28 doing over the next, uh, several episodes,

00:00:28 --> 00:00:31 um, taking a different approach. Uh, we're

00:00:31 --> 00:00:34 going to, to uh, focus on specific topics

00:00:34 --> 00:00:37 within each of the episodes. Uh,

00:00:37 --> 00:00:40 we could call them specials if you like. And

00:00:40 --> 00:00:42 today our focus will be on

00:00:42 --> 00:00:45 comets and meteors. Stick around.

00:00:45 --> 00:00:47 We're doing all of that on this episode of

00:00:47 --> 00:00:50 space nuts. 15 seconds. Guidance

00:00:50 --> 00:00:53 is internal. 10, 9,

00:00:53 --> 00:00:55 ignition sequence start.

00:00:55 --> 00:00:57 Jonti Horner: Space nuts. 5, 4, 3, 2.

00:00:57 --> 00:01:00 Andrew Dunkley: 1, 2, 3, 4, 5, 5, 4, 3,

00:01:00 --> 00:01:01 2, 1.

00:01:01 --> 00:01:02 Jonti Horner: Space nuts.

00:01:02 --> 00:01:05 Andrew Dunkley: Astronauts. Feels good and

00:01:05 --> 00:01:07 it's great to have him back. Professor Jonti

00:01:07 --> 00:01:10 Horner, professor of Astrophysics at the

00:01:10 --> 00:01:13 University of Southern Queensland. Jonti,

00:01:13 --> 00:01:13 hello.

00:01:13 --> 00:01:15 Jonti Horner: Ah, uh, hey, how are you going? Good.

00:01:15 --> 00:01:16 Andrew Dunkley: Great to see you again.

00:01:17 --> 00:01:19 Jonti Horner: Well, it's good to be back. It's something

00:01:19 --> 00:01:20 nice to keep me entertained while I'm having

00:01:20 --> 00:01:22 a little bit of a restful couple of weeks.

00:01:22 --> 00:01:24 I'm, you know, I've got a bit of leave, so

00:01:24 --> 00:01:27 I'm recovering from a minor surgery and

00:01:27 --> 00:01:29 therefore I can give my entire forecast to.

00:01:29 --> 00:01:31 Talking about fun things rather than doing

00:01:31 --> 00:01:34 admin effectively means I get to see a little

00:01:34 --> 00:01:35 bit of the life Fred gets to live.

00:01:35 --> 00:01:38 Andrew Dunkley: Yeah, maybe. Yes. Although he doesn't seem to

00:01:38 --> 00:01:41 slow down much. Um, in fact, I think

00:01:41 --> 00:01:43 the worst thing you can do when you retire is

00:01:43 --> 00:01:46 slow down because the brain matter decides to

00:01:46 --> 00:01:48 give up the ghost and that's when it's all

00:01:48 --> 00:01:51 over. Red Rover. But, uh, no, he, he's going,

00:01:51 --> 00:01:52 going great guns.

00:01:52 --> 00:01:55 And um, you didn't mention that you're having

00:01:55 --> 00:01:58 a little bit of a recuperation. Are

00:01:58 --> 00:02:00 you in a position to talk about that or

00:02:01 --> 00:02:02 too embarrassing?

00:02:03 --> 00:02:04 Jonti Horner: Well, it's one of those things that when I,

00:02:04 --> 00:02:06 when I first had this pointed out, I a bit

00:02:06 --> 00:02:08 embarrassed about it, but I don't think as

00:02:08 --> 00:02:10 bloats we ever talk about health that much

00:02:10 --> 00:02:13 until it's worth muscling past a little bit

00:02:13 --> 00:02:16 of embarrassment. So I'm in my late 40s and

00:02:16 --> 00:02:18 I went to the doctor about a year ago

00:02:18 --> 00:02:20 because, had a little bit of bleeding when I

00:02:20 --> 00:02:21 was sitting down and stuff like this and

00:02:21 --> 00:02:24 nothing dramatic. Um, But I found out two

00:02:24 --> 00:02:26 things. Firstly, in Australia, and I don't

00:02:26 --> 00:02:27 know about the rest of the world, you should

00:02:27 --> 00:02:29 look this up. But when you're in your 40s,

00:02:30 --> 00:02:32 the Medicare system here affords the

00:02:32 --> 00:02:34 opportunity for you to get health checks.

00:02:34 --> 00:02:36 Yep. Which is brilliant. So you basically get

00:02:36 --> 00:02:38 what in the UK they'd call an MOT for a car.

00:02:39 --> 00:02:41 You get everything run over and you get your

00:02:41 --> 00:02:43 blood pressure done and your heart rate done

00:02:43 --> 00:02:44 and everything else. And then you go back

00:02:44 --> 00:02:46 every three months and do it again and again

00:02:46 --> 00:02:48 and again, and it's basically you're at an

00:02:48 --> 00:02:50 edge where things start to break. Let's get

00:02:50 --> 00:02:52 on top of it early so that you can enjoy the

00:02:52 --> 00:02:55 rest of your life in peace, effectively. I

00:02:55 --> 00:02:56 think it's a really good idea and I suspect

00:02:56 --> 00:02:58 from a government point of view, makes a lot

00:02:58 --> 00:03:00 of sense, because if you find things easy

00:03:00 --> 00:03:02 earlier, they're easier and quicker and

00:03:02 --> 00:03:05 cheaper to solve. Um, what it turned out from

00:03:05 --> 00:03:07 that was I spent about two months going back

00:03:07 --> 00:03:09 and forth with a doctor who thought I had one

00:03:09 --> 00:03:11 thing wrong, which is not what it was. And

00:03:11 --> 00:03:13 then I got. Got sent to this specialist who

00:03:13 --> 00:03:15 said, you've got something called a fistula

00:03:15 --> 00:03:18 down near your backside, which, not life

00:03:18 --> 00:03:19 threatening, not the end of the world, not

00:03:19 --> 00:03:22 doomed, but it's uncomfortable. Um, and, you

00:03:22 --> 00:03:24 know, it's been slightly embarrassing in that

00:03:24 --> 00:03:27 I've had to learn more about sanitary pads

00:03:27 --> 00:03:29 and, you know, um, you would have expected,

00:03:29 --> 00:03:32 you know, which the women in the audience are

00:03:32 --> 00:03:33 going, about bloody time a man learned about

00:03:33 --> 00:03:36 this. Um, but it's a weird

00:03:36 --> 00:03:38 one because it's not life threatening. It's

00:03:38 --> 00:03:40 nothing of a problem, something 10 or 20% of

00:03:40 --> 00:03:42 guys apparently get them, but they contain

00:03:42 --> 00:03:45 multiple surgeries to fix. And when I went in

00:03:45 --> 00:03:48 for the first surgery in January, there was

00:03:48 --> 00:03:50 another guy there who was on surgery number

00:03:50 --> 00:03:50 seven.

00:03:50 --> 00:03:51 Andrew Dunkley: Wow.

00:03:51 --> 00:03:54 Jonti Horner: Which he had deep and joyous, um, kind of day

00:03:54 --> 00:03:55 surgery. But you get a full general and you

00:03:55 --> 00:03:57 go under and Dr. Does snippy, snippy things

00:03:57 --> 00:03:59 and you get a couple of weeks off work, which

00:03:59 --> 00:04:01 is where I am now. So I've just had surgery

00:04:01 --> 00:04:04 number two and the doctor is hopeful,

00:04:04 --> 00:04:05 confident, whatever, that surgery number

00:04:05 --> 00:04:08 three will be the final fix. And it's one of

00:04:08 --> 00:04:09 these weird things because people say, what's

00:04:09 --> 00:04:11 wrong with you? And if it's a sore arm, you

00:04:11 --> 00:04:13 just say, I've hurt my arm, or you've broken

00:04:13 --> 00:04:15 your arm or something. Or in Australia, a

00:04:15 --> 00:04:17 really common one, a melanoma. People have

00:04:17 --> 00:04:19 been in the sun too much going into hospital.

00:04:19 --> 00:04:20 What do you get, I've, ah, got a melanoma

00:04:20 --> 00:04:22 taken off. But as soon as it's anywhere

00:04:22 --> 00:04:24 between about your belly button and your

00:04:24 --> 00:04:25 knee, people are bashful about talking about

00:04:25 --> 00:04:28 it. And I first few months I was mortified

00:04:28 --> 00:04:30 and like, wouldn't talk about it. And

00:04:30 --> 00:04:32 realization is that if you don't talk about

00:04:32 --> 00:04:35 it, people don't get checked. And we as

00:04:35 --> 00:04:37 men are terrible for that. And so, yeah,

00:04:37 --> 00:04:39 worth talking about. I'm a bit embarrassed

00:04:39 --> 00:04:41 about it, but I shouldn't be. And it's good,

00:04:41 --> 00:04:42 it's going to tune up. And it means that in

00:04:42 --> 00:04:45 40 years time I'll still be up and kicking

00:04:45 --> 00:04:47 and having a lot of fun rather than in

00:04:47 --> 00:04:48 discomfort and grumbling about a problem I

00:04:48 --> 00:04:49 could have got fixed.

00:04:49 --> 00:04:52 Andrew Dunkley: Yeah, yeah. And, um, I think you're

00:04:52 --> 00:04:55 right. I think men do tend to keep things to

00:04:55 --> 00:04:58 themselves. Uh, a lot of them go into denial

00:04:58 --> 00:05:00 or they just think, well, no, that won't

00:05:00 --> 00:05:03 happen to me, so no problem. But,

00:05:04 --> 00:05:06 uh, when I was diagnosed with prostate

00:05:06 --> 00:05:09 cancer, it was like a bolt from the blue. And

00:05:09 --> 00:05:12 I didn't, I never expected

00:05:12 --> 00:05:14 to get it because there was next to no

00:05:14 --> 00:05:17 history of it in my family. So, um, that was

00:05:17 --> 00:05:20 a bit of a shock. And this is. How long is

00:05:20 --> 00:05:23 it now? Three years. Three years. And I'm

00:05:23 --> 00:05:26 still working my way through it. So,

00:05:27 --> 00:05:30 um, but the latest scans are all good.

00:05:30 --> 00:05:32 So fingers crossed that we've, you know,

00:05:33 --> 00:05:36 reached a good position. But, um, it's

00:05:36 --> 00:05:37 just an ongoing thing in your life. You just

00:05:37 --> 00:05:40 got to get used to it. But you. My

00:05:40 --> 00:05:42 advice to men is go and get checked. If

00:05:42 --> 00:05:45 you're over 50, go and get a

00:05:45 --> 00:05:48 prostate exam, go and get your PSA tests

00:05:48 --> 00:05:51 done. Because if you don't and

00:05:51 --> 00:05:53 then they find it, it might be too far along.

00:05:54 --> 00:05:57 Um, and then the treatment becomes more

00:05:57 --> 00:06:00 dramatic. So anyway, um, it's a good

00:06:00 --> 00:06:01 thing to bring up.

00:06:01 --> 00:06:03 Jonti Horner: It is. And it goes for the mental health

00:06:03 --> 00:06:05 stuff as well. I have a former partner of

00:06:05 --> 00:06:07 mine, kind of 20 years ago, who was very

00:06:07 --> 00:06:10 severely bipolar, had a lot of challenges

00:06:10 --> 00:06:12 and she was continually frustrated by

00:06:12 --> 00:06:14 people's responses to that in public, in that

00:06:14 --> 00:06:17 it's a hidden illness there. She's getting

00:06:17 --> 00:06:19 treatment. But what she always said is, it's

00:06:19 --> 00:06:21 really frustrating. If I, if I had a broken

00:06:21 --> 00:06:23 leg or I had an injury to my arm and people

00:06:23 --> 00:06:26 could see it, they'd be supportive. But with

00:06:26 --> 00:06:27 mental health, she got a hell of a lot of,

00:06:27 --> 00:06:29 I'll just get over it, uh, or toughen up or.

00:06:29 --> 00:06:30 Andrew Dunkley: Yep. Yeah.

00:06:30 --> 00:06:33 Jonti Horner: And, yeah, and, you know, she was female,

00:06:33 --> 00:06:35 so she's more likely to go to the doctor and

00:06:35 --> 00:06:38 talk about it. Statistically, men with mental

00:06:38 --> 00:06:40 health challenges tend to avoid that even

00:06:40 --> 00:06:42 more than they'll go to the doctor with

00:06:42 --> 00:06:44 physical health challenges. And it's

00:06:44 --> 00:06:46 something I'd like to change. I come from a

00:06:46 --> 00:06:48 working class background in Yorkshire where

00:06:48 --> 00:06:49 men m. Don't talk about anything. You know,

00:06:49 --> 00:06:52 you're meant to be stoic and the only, the

00:06:52 --> 00:06:53 only expression of emotion you're allowed is

00:06:53 --> 00:06:56 rage or a single manly tear. You know, it's,

00:06:56 --> 00:06:58 it's really creative the way we're

00:06:58 --> 00:07:00 conditioned. And even though I'm, you know, I

00:07:00 --> 00:07:02 went to uni, I've had a life, I've grown up.

00:07:02 --> 00:07:03 All this stuff still there at the back of

00:07:03 --> 00:07:05 your head and you've got to fight against it

00:07:05 --> 00:07:07 because the instinct is, ah, there's nothing

00:07:07 --> 00:07:09 wrong. I won't bother, you know. Yeah.

00:07:09 --> 00:07:11 Andrew Dunkley: And, um, yeah, you see it way too often.

00:07:12 --> 00:07:14 Um, I know it's a departure from what this

00:07:14 --> 00:07:16 podcast is all about, but I,

00:07:17 --> 00:07:19 when given the opportunity, will

00:07:20 --> 00:07:23 openly, um, say to men, um, you know,

00:07:23 --> 00:07:26 don't, don't hesitate to go to the

00:07:26 --> 00:07:29 doctor. Not, not when you think something's

00:07:29 --> 00:07:32 wrong. Just preemptively go and get. Once a

00:07:32 --> 00:07:33 year, go and get checked and make sure

00:07:33 --> 00:07:35 everything's where it's supposed to be or

00:07:36 --> 00:07:38 whatever. Um, we do it, do it for

00:07:38 --> 00:07:40 Jonti Horner: our cars, we do it for our pets.

00:07:40 --> 00:07:40 Andrew Dunkley: Yeah.

00:07:40 --> 00:07:42 Jonti Horner: Do it for yourself as well.

00:07:42 --> 00:07:43 Andrew Dunkley: Yeah, exactly.

00:07:43 --> 00:07:44 Jonti Horner: And yeah, I think it's probably a record for

00:07:44 --> 00:07:46 the quickest we've ever got off topic. And

00:07:46 --> 00:07:48 possibly we shouldn't have a trigger warning

00:07:48 --> 00:07:49 at the front of it and all the rest of it,

00:07:49 --> 00:07:51 but no good way to start even though it is

00:07:51 --> 00:07:52 off topic.

00:07:52 --> 00:07:54 Andrew Dunkley: It's okay, we'll get on to topic right now

00:07:54 --> 00:07:57 because, uh, uh, as I mentioned, these,

00:07:57 --> 00:08:00 these, uh, next, uh, several, uh,

00:08:00 --> 00:08:02 episodes are going to be dedicated to

00:08:02 --> 00:08:04 singular topics each. And today

00:08:05 --> 00:08:07 it's, uh, well, related topics. Comets and

00:08:07 --> 00:08:10 meteors. Uh, this is a, this is pet

00:08:11 --> 00:08:12 topic of yours, I imagine.

00:08:13 --> 00:08:15 Jonti Horner: It is. I, I've always been a bit more into

00:08:15 --> 00:08:17 the nearby stuff than the more distant stuff.

00:08:17 --> 00:08:19 So it always tickles me a little bit that

00:08:19 --> 00:08:21 when questions come in when I'm on the show,

00:08:21 --> 00:08:23 we get all the Big bang and cosmology ones.

00:08:23 --> 00:08:25 And I'm sure if you've got uh, someone like

00:08:25 --> 00:08:26 the wonderful Tamara Davis on to talk

00:08:26 --> 00:08:28 cosmology, she get all the planets questions.

00:08:28 --> 00:08:31 It's always the way it goes. Yeah, but comets

00:08:31 --> 00:08:33 and meteors are a big part of what hooked me

00:08:33 --> 00:08:35 into astronomy as A kid. And, um, my thinking

00:08:35 --> 00:08:38 behind this is that we're recording in

00:08:38 --> 00:08:41 advance. You know, um, obviously Fred

00:08:41 --> 00:08:43 is away, but you've got recordings with Fred

00:08:43 --> 00:08:45 already. And so the news that we would

00:08:45 --> 00:08:47 normally talk about hasn't happened yet. So

00:08:48 --> 00:08:50 I, I have many talents, but seeing into the

00:08:50 --> 00:08:52 future isn't one of them to that degree. And

00:08:52 --> 00:08:54 so I thought it better to have a discussion

00:08:54 --> 00:08:56 about the general stuff in a bit more depth

00:08:57 --> 00:08:59 than go into particular news topics. And

00:08:59 --> 00:09:01 it's. It could almost be a bit of an

00:09:01 --> 00:09:03 explainer, a bit of the background, and

00:09:03 --> 00:09:05 hopefully at least gives my insight into why

00:09:05 --> 00:09:07 a given topic's interesting, but also what

00:09:07 --> 00:09:09 people can look out for in the future and how

00:09:09 --> 00:09:12 they can get more into and more out

00:09:12 --> 00:09:15 of that particular topic, if that makes

00:09:15 --> 00:09:17 sense. Yeah, Um, a little bit different, I

00:09:17 --> 00:09:19 understand. For some listeners it might be a

00:09:19 --> 00:09:22 bit of an abrupt departure and a change. So

00:09:22 --> 00:09:23 it'll be interesting to see what feedback you

00:09:23 --> 00:09:26 get. But hopefully people like it as a little

00:09:26 --> 00:09:28 bit of a change in a breath of fresh air. And

00:09:28 --> 00:09:29 if they don't, well, there's only a couple of

00:09:29 --> 00:09:31 episodes and Fred's back anyway, so you'll

00:09:31 --> 00:09:33 have to deal with it and we'll see.

00:09:33 --> 00:09:34 Andrew Dunkley: I'm sure it'll be fine.

00:09:34 --> 00:09:37 Uh, comets and meteors are a very popular,

00:09:37 --> 00:09:40 uh, topic. So, um, uh, where do we

00:09:40 --> 00:09:41 start? Maybe, maybe look at a bit of the

00:09:41 --> 00:09:42 history of this.

00:09:43 --> 00:09:45 Jonti Horner: Yeah, I think that is always a good place.

00:09:46 --> 00:09:48 It sets the context of where we are now. And,

00:09:48 --> 00:09:51 um, for both comets and meteors, there's a

00:09:51 --> 00:09:53 kind of global connection societally that

00:09:53 --> 00:09:56 really predates by a long, long way

00:09:56 --> 00:09:59 our scientific knowledge. Essentially the

00:09:59 --> 00:10:01 modern scientific viewpoint and the

00:10:01 --> 00:10:03 scientific method. All cultures across the

00:10:03 --> 00:10:05 world, from our wonderful, uh, traditional

00:10:05 --> 00:10:07 owners here in Australia to the peoples of

00:10:07 --> 00:10:09 every continent and every land, um, both

00:10:09 --> 00:10:12 current and past, historically had a

00:10:12 --> 00:10:14 really firm connection to the night sky. They

00:10:14 --> 00:10:15 knew the night sky better than most people

00:10:15 --> 00:10:17 these days do because it wasn't light

00:10:17 --> 00:10:19 pollution, there weren't TVs and Xboxes.

00:10:20 --> 00:10:22 So the sky was something people much more

00:10:22 --> 00:10:25 exposed to. A lot of cultures have

00:10:25 --> 00:10:27 this kind of idea of as above, so below, as

00:10:27 --> 00:10:30 below, so above. So they were very firmly of

00:10:30 --> 00:10:32 the idea that major events on the Earth were

00:10:32 --> 00:10:35 reflected in the sky. And, uh, major events

00:10:35 --> 00:10:37 in the sky would have their counterparts on

00:10:37 --> 00:10:40 the Earth. And that's where astrology

00:10:40 --> 00:10:42 was born. And for a long time, astrology and

00:10:42 --> 00:10:44 astronomy were one and the same. You know,

00:10:44 --> 00:10:47 people doing astronomy studies were doing it

00:10:47 --> 00:10:48 because they wanted to understand the events

00:10:48 --> 00:10:51 that would influence what's on the Earth. And

00:10:51 --> 00:10:53 there are good examples of this in terms of

00:10:53 --> 00:10:55 the nominally fixed stars, uh, things like

00:10:55 --> 00:10:58 the ancient Egyptians using the rising of

00:10:58 --> 00:11:01 Sirius in the dawn sky after it disappeared

00:11:01 --> 00:11:03 in the evenings as a predictor of the

00:11:03 --> 00:11:04 flooding of the Nile, for example, the use of

00:11:04 --> 00:11:07 the night sky as a calendar, lots of stuff

00:11:07 --> 00:11:10 like that. But because people are so aware of

00:11:10 --> 00:11:12 the night sky, anything that was ephemeral,

00:11:13 --> 00:11:15 anything that was transitory, that appeared

00:11:15 --> 00:11:17 and then disappeared, that was unexpected,

00:11:17 --> 00:11:19 was often seen as kind of a portent or an

00:11:19 --> 00:11:22 omen, something that was an

00:11:22 --> 00:11:24 indication either of major change and

00:11:24 --> 00:11:26 upheaval currently happening or one soon to

00:11:26 --> 00:11:28 come. And really bright comets and, um,

00:11:28 --> 00:11:31 spectacular meteor showers kind of often fill

00:11:31 --> 00:11:33 this role. And you can go back through

00:11:33 --> 00:11:36 ancient history where we have the records and

00:11:36 --> 00:11:38 see good examples of this. I've got, in one

00:11:38 --> 00:11:41 of my talks, talks about a

00:11:41 --> 00:11:43 guy called, uh, Mithridates,

00:11:44 --> 00:11:46 um, Jupiter 6, I think his name was. He was

00:11:46 --> 00:11:48 one of the great enemies of the Roman Empire.

00:11:48 --> 00:11:51 And there are quotes ascribed to him saying

00:11:51 --> 00:11:54 things like, um, even the heavens predicted

00:11:54 --> 00:11:56 the greatness of this man. For in the year in

00:11:56 --> 00:11:57 which he was born and the year in which he

00:11:57 --> 00:12:00 came to reign, a comet shone through Both

00:12:00 --> 00:12:02 periods for 70 days as

00:12:02 --> 00:12:04 bright as the sun. Um, each rising and

00:12:04 --> 00:12:07 setting took four hours each. And that's kind

00:12:07 --> 00:12:09 of hyperbolic, but it gives this idea that

00:12:09 --> 00:12:12 people saw something in the sky that was

00:12:12 --> 00:12:15 unusual and tied it to events on Earth.

00:12:15 --> 00:12:17 Another good example would be the alleged

00:12:17 --> 00:12:20 comet called Caesar's Comet in 44 BC

00:12:20 --> 00:12:23 43-43, which

00:12:23 --> 00:12:26 is recorded in Roman writings from

00:12:26 --> 00:12:28 a century or two later, talking

00:12:29 --> 00:12:31 about after the death of Caesar, a comet

00:12:31 --> 00:12:34 blazed in the sky for seven days that was

00:12:34 --> 00:12:36 spectacularly bright, then disappeared and

00:12:36 --> 00:12:38 was never seen again. Now, that comet is a

00:12:38 --> 00:12:40 really good example of the challenge people

00:12:40 --> 00:12:42 have with historical records,

00:12:43 --> 00:12:45 because on the one hand you've got these

00:12:45 --> 00:12:48 clear reports from the Roman Empire, none of

00:12:48 --> 00:12:50 them at the time, though, all of them a bit

00:12:50 --> 00:12:52 later on. But that comet is not recorded from

00:12:52 --> 00:12:54 anywhere else on the planet. And there were

00:12:54 --> 00:12:56 cultures around the globe leaving records

00:12:56 --> 00:12:58 like ancient China and ancient Korea, who

00:12:58 --> 00:13:01 would have seen it. So was that comet real,

00:13:02 --> 00:13:04 or was it a case of after the event, people

00:13:04 --> 00:13:07 inventing a night sky phenomena to tie

00:13:07 --> 00:13:09 with the soul of the emperor rising to

00:13:09 --> 00:13:11 heaven? It's one of the challenges people in

00:13:11 --> 00:13:13 the kind of cultural astronomy space face, I

00:13:13 --> 00:13:16 think, in terms of disentangling the

00:13:16 --> 00:13:18 narrative from the events that prompted it,

00:13:18 --> 00:13:21 if that kind of makes sense. Yeah, but what's

00:13:21 --> 00:13:23 certainly true is, uh, for as long as we've

00:13:23 --> 00:13:25 looked at the sky, really bright comets and,

00:13:25 --> 00:13:28 um, unusually powerful meteor showers

00:13:28 --> 00:13:30 were things that people took note of. And

00:13:30 --> 00:13:32 recently there was a lot of media, media

00:13:32 --> 00:13:35 coverage of the April Lyrid meteor shower,

00:13:35 --> 00:13:37 which is not one of the strongest of the

00:13:37 --> 00:13:40 year, but one of the reasonable, moderate

00:13:40 --> 00:13:41 ones. It's kind of one that if you're a

00:13:41 --> 00:13:43 meteor enthusiast, you'll go out and watch,

00:13:43 --> 00:13:45 but isn't worth going out if you're not that

00:13:45 --> 00:13:46 interested because there's too few.

00:13:48 --> 00:13:49 I had to grumble about some of the coverage

00:13:49 --> 00:13:51 here in Australia because it's not a great

00:13:51 --> 00:13:53 shower for us. But that meteor shower

00:13:53 --> 00:13:56 was recognized by the traditional owners in

00:13:56 --> 00:13:57 Australia. And there are stories from

00:13:57 --> 00:14:00 Victoria, from, I think, the Burong people,

00:14:00 --> 00:14:01 although I stand to be corrected on that,

00:14:02 --> 00:14:04 that associate this meteor shower with the

00:14:04 --> 00:14:05 Mallee Fowl, one of the big ground nesting

00:14:05 --> 00:14:08 birds in Australia, which nests around that

00:14:08 --> 00:14:10 time of year. The meteors seen shrieking from

00:14:10 --> 00:14:12 low in the northern sky were viewed as being

00:14:12 --> 00:14:15 the dust being kicked up by the nesting bird

00:14:15 --> 00:14:17 celestially. So they recorded this meteor

00:14:17 --> 00:14:19 shower, even though it isn't a particularly

00:14:19 --> 00:14:21 strong one. But our oldest

00:14:22 --> 00:14:24 written record of any meteor shower is the

00:14:24 --> 00:14:26 April Lyrids, and it's dated back to

00:14:26 --> 00:14:28 something like 687 BCE, when

00:14:28 --> 00:14:30 stars fell like rain, when there was a major

00:14:30 --> 00:14:33 storm from the Lyrids, and it was significant

00:14:33 --> 00:14:36 enough for people to record. So comets

00:14:36 --> 00:14:39 and meteors, way before the modern

00:14:39 --> 00:14:41 scientific understanding of them really had

00:14:41 --> 00:14:44 this important cultural role,

00:14:44 --> 00:14:46 um, even in the Battle of Hastings. If you

00:14:46 --> 00:14:48 ever go to see the Bayer Tapestry, this

00:14:48 --> 00:14:50 wonderful woven record of the Battle of

00:14:50 --> 00:14:52 Hastings and the invasion of William the

00:14:52 --> 00:14:55 Conqueror, Comet Hallie features prominently

00:14:55 --> 00:14:57 on that, because in 1066,

00:14:58 --> 00:15:00 you had the second best apparition of Comet

00:15:00 --> 00:15:02 Hallie in the last 2 years. Arguably, it

00:15:02 --> 00:15:04 was very spectacular in the sky at the time

00:15:04 --> 00:15:06 the conquest was going on. And, um, that was

00:15:06 --> 00:15:09 considered important enough to be recorded in

00:15:09 --> 00:15:12 the tapestry that was woven at the time. You

00:15:12 --> 00:15:14 know, it's amazing that you've got this panel

00:15:14 --> 00:15:16 where there's all the peasants pointing up at

00:15:16 --> 00:15:18 this thing in the sky and somebody whispering

00:15:18 --> 00:15:20 in King Harold's ear about the comet that's

00:15:20 --> 00:15:23 visible. So, yeah, don't know whether the

00:15:23 --> 00:15:25 invading forces took it as a good sign or a

00:15:25 --> 00:15:26 bad sign, but they thought it was important

00:15:27 --> 00:15:29 enough to include. So that in

00:15:29 --> 00:15:31 itself is fairly breathtaking. And so when we

00:15:31 --> 00:15:33 see these objects, it's a lovely connection

00:15:33 --> 00:15:36 to thousands of years of our heritage of

00:15:36 --> 00:15:39 people looking at the night sky in wonder I

00:15:39 --> 00:15:42 think the first step we had really,

00:15:43 --> 00:15:46 in moving from cultural

00:15:46 --> 00:15:48 cometary astronomy to modern scientific

00:15:48 --> 00:15:51 astronomy, in a way, came with the Great

00:15:51 --> 00:15:54 Comet of 1577, which was

00:15:54 --> 00:15:56 another of the really amazing, spectacular,

00:15:56 --> 00:15:59 bright comets that was widely

00:15:59 --> 00:16:02 observed, hence why it's a great comet.

00:16:02 --> 00:16:04 But it was observed by the great astronomer

00:16:04 --> 00:16:07 Tycho Brahe. And, um, I'm sure Brahe is

00:16:07 --> 00:16:09 featured on the podcast many times before,

00:16:09 --> 00:16:11 but the quirky individual he was, it's well

00:16:11 --> 00:16:14 worth looking up. His Wikipedia record is

00:16:14 --> 00:16:17 this wealthy nobleman with a silver

00:16:17 --> 00:16:19 replacement nose after he lost half his nose

00:16:19 --> 00:16:22 in a duel. He's that guy. Yes,

00:16:22 --> 00:16:24 yes. Um, he had a pet moose that died when it

00:16:24 --> 00:16:26 fell down the steps because it got drunk at a

00:16:26 --> 00:16:29 banquet. He really odd, odd

00:16:29 --> 00:16:32 man. Um, but probably viewed as being

00:16:32 --> 00:16:35 the last great pre telescope astronaut,

00:16:35 --> 00:16:36 astronomical observer, if that makes sense.

00:16:36 --> 00:16:39 Naked eye observer. Now, at this time,

00:16:39 --> 00:16:41 comets were kind of thought to be probably

00:16:41 --> 00:16:44 atmospheric phenomenon. They were nearby,

00:16:44 --> 00:16:47 high in the atmosphere, and so

00:16:47 --> 00:16:49 that was what was going on. People had that

00:16:49 --> 00:16:52 kind of idea. He realized that if that were

00:16:52 --> 00:16:55 true, these things would display a noticeable

00:16:55 --> 00:16:57 parallax if people observe them from

00:16:57 --> 00:16:59 different locations. Uh-huh. So in other

00:16:59 --> 00:17:01 words, people looking from different

00:17:01 --> 00:17:03 locations would see the comet in a different

00:17:04 --> 00:17:06 place in the sky because it was in the

00:17:06 --> 00:17:08 foreground. It's the same technique we use to

00:17:08 --> 00:17:10 measure the distance to the nearest stars. If

00:17:10 --> 00:17:12 you put your finger in front of your face and

00:17:12 --> 00:17:13 look at it through one eye and then look

00:17:13 --> 00:17:15 through the other, you'll see your finger

00:17:15 --> 00:17:18 blinking side to side. And the further away

00:17:18 --> 00:17:20 your finger is, the less it moves. We use

00:17:20 --> 00:17:22 that to measure the distance to stars by

00:17:22 --> 00:17:24 observing from one side of the Earth's orbit,

00:17:24 --> 00:17:26 then the other. But what Brahe did was

00:17:26 --> 00:17:28 collect observations from around Europe of

00:17:28 --> 00:17:31 where the comet was in the sky. With those

00:17:31 --> 00:17:33 observations, he would have been able to

00:17:33 --> 00:17:36 detect a parallax for the comet if it were

00:17:36 --> 00:17:39 closer than the orbit of the Moon. So if it

00:17:39 --> 00:17:40 was atmospheric, absolutely, definitely would

00:17:40 --> 00:17:43 do. But no measurable parallax was found

00:17:44 --> 00:17:45 which showed the comet had to be at least a

00:17:45 --> 00:17:47 couple of million kilometers away. And in

00:17:47 --> 00:17:49 fact, it was probably several tens of

00:17:49 --> 00:17:52 millions of kilometers distant. He got this

00:17:52 --> 00:17:54 beautiful figure, and I've. I use this in my

00:17:54 --> 00:17:57 talks occasionally. That is his drawing of

00:17:57 --> 00:17:59 the motion of the comet. And it's fascinating

00:17:59 --> 00:18:01 from a cultural point of view because it's

00:18:01 --> 00:18:03 clearly at the time when you still have the

00:18:03 --> 00:18:05 geocentric model, the Earth was the center of

00:18:05 --> 00:18:06 the universe. So you've got the Earth in the

00:18:06 --> 00:18:09 middle, the sun going around the Earth but

00:18:09 --> 00:18:11 then Mercury, Venus and the moon going around

00:18:11 --> 00:18:13 the sun. This kind of weird hybrid thing.

00:18:13 --> 00:18:15 Yeah, but you've got the path of the comet

00:18:15 --> 00:18:17 moving through there that he's determined.

00:18:17 --> 00:18:19 And what's really interesting to me, what's

00:18:19 --> 00:18:22 really fascinating is he's got the tails

00:18:22 --> 00:18:24 pointing away from the sun all the time. So

00:18:24 --> 00:18:26 he's got the phenomenology of where the comet

00:18:26 --> 00:18:28 is in the solar system. Modular.

00:18:30 --> 00:18:32 The sun's going around the Earth and the

00:18:32 --> 00:18:34 tails pointing the right way as it moves.

00:18:34 --> 00:18:36 Tails of comets always pointing away from the

00:18:36 --> 00:18:39 sun. And to me that kind of marks the

00:18:39 --> 00:18:42 dawn of the modern scientific view

00:18:42 --> 00:18:45 of comets from the cultural. We don't

00:18:45 --> 00:18:48 know what they are, but they are important.

00:18:50 --> 00:18:52 That's a real kind of boundary point for me.

00:18:52 --> 00:18:53 Andrew Dunkley: Yeah, yeah, fascinating.

00:18:53 --> 00:18:55 I was actually going to ask you about the uh,

00:18:55 --> 00:18:57 you know, the point in time where we went

00:18:57 --> 00:18:59 from the mythology m to the

00:19:00 --> 00:19:03 understanding that this, this was something

00:19:03 --> 00:19:05 else. And yeah, you covered that beautifully.

00:19:05 --> 00:19:08 Gonna just take a breath on space nuts. Uh,

00:19:08 --> 00:19:10 you're with Andrew Dunkley and Professor

00:19:10 --> 00:19:11 Jonti Horner.

00:19:14 --> 00:19:17 Jonti Horner: 0G and I feel fine. Space nuts.

00:19:17 --> 00:19:18 Andrew Dunkley: I did say a breath. That was quick.

00:19:18 --> 00:19:21 Um, let's continue talking about, uh, comets

00:19:21 --> 00:19:24 and meteors. There have been a lot of them in

00:19:24 --> 00:19:26 the news of late. Um, Comet

00:19:26 --> 00:19:29 Pan Stars is, um, you know, it was very,

00:19:29 --> 00:19:32 very popular, uh, late

00:19:32 --> 00:19:35 April. Uh, and uh,

00:19:35 --> 00:19:38 we've seen in recent times, um, a

00:19:38 --> 00:19:40 new kind of comet. And those are the ones

00:19:40 --> 00:19:43 that are coming from other systems, uh,

00:19:43 --> 00:19:45 not the ones that are

00:19:45 --> 00:19:48 continually rotating through our own solar

00:19:48 --> 00:19:51 system. We've had these exo comets that have

00:19:52 --> 00:19:54 been quite intriguing and um,

00:19:54 --> 00:19:56 opening up all sorts of new ideas and

00:19:56 --> 00:19:59 questions about, uh, comets and other

00:19:59 --> 00:20:02 parts of the universe and what we could learn

00:20:02 --> 00:20:05 from them. Um, and

00:20:05 --> 00:20:07 new comets are being discovered all the time.

00:20:08 --> 00:20:09 That doesn't mean they haven't been here

00:20:09 --> 00:20:12 before, but it does mean that they've got

00:20:12 --> 00:20:15 very longitudinal travel times.

00:20:15 --> 00:20:18 So, um, you know, some we won't ever see

00:20:18 --> 00:20:20 because we'll have been and gone before they

00:20:20 --> 00:20:22 get here and others we'll

00:20:23 --> 00:20:25 maybe see several times during our lifetimes.

00:20:26 --> 00:20:29 Jonti Horner: Absolutely. Now historically, people broke

00:20:29 --> 00:20:31 the comets we found down into two categories.

00:20:31 --> 00:20:34 We had short period comets, which are

00:20:34 --> 00:20:36 comets. The definition when I was a kid was

00:20:36 --> 00:20:38 comets whose orbital periods were less than

00:20:38 --> 00:20:41 200 years shorter than that and you were a

00:20:41 --> 00:20:42 short period comet, longer than that and you

00:20:42 --> 00:20:44 were a long period comet. Now there are

00:20:44 --> 00:20:46 subtleties within that, within the short

00:20:46 --> 00:20:48 period comets. We have comets like Comet

00:20:48 --> 00:20:49 Hallie, which are called the Hallie type

00:20:49 --> 00:20:52 comets which come round with a period

00:20:52 --> 00:20:54 comparable to a human lifetime or a bit

00:20:54 --> 00:20:56 longer. The two brightest and most famous of

00:20:56 --> 00:20:57 those are Comet Hallie and Comet Swift

00:20:57 --> 00:20:59 Tuttle. You then have the Jupiter family

00:20:59 --> 00:21:01 comets, which are comets whose orbits, uh,

00:21:01 --> 00:21:04 are just a few years and are typically under

00:21:04 --> 00:21:06 Jupiter's control. And when I was a kid,

00:21:06 --> 00:21:08 anything longer than 200 years was considered

00:21:08 --> 00:21:11 long period. Now that kind of got smashed

00:21:11 --> 00:21:13 into the ground a bit in the early 2000s when

00:21:13 --> 00:21:16 Comet IKEA Jang was sighted, because Comet

00:21:16 --> 00:21:19 Ikea Zhang was very well observed,

00:21:19 --> 00:21:20 its orbit was well calculated and it was

00:21:20 --> 00:21:23 found to have a period of 366 years, I think

00:21:23 --> 00:21:26 it is. And that allowed people to identify

00:21:26 --> 00:21:28 the previous observations of that comet from

00:21:28 --> 00:21:30 the last time it was around. So that's

00:21:30 --> 00:21:33 currently the record holder where we're

00:21:33 --> 00:21:36 absolutely certain that it's been seen on

00:21:36 --> 00:21:38 multiple occasions and it has a

00:21:38 --> 00:21:41 periodic comet designation now. Now a

00:21:41 --> 00:21:43 subtlety to that is we do have the Kreutz sun

00:21:43 --> 00:21:45 grazing comets. I can talk more about them a

00:21:45 --> 00:21:47 little later where we have a strong

00:21:47 --> 00:21:50 identification between an observation of

00:21:50 --> 00:21:52 the comet, say with comedy kaya Seki in

00:21:52 --> 00:21:55 1965 and um, a previous

00:21:55 --> 00:21:58 apparition in the 1100s, which is about

00:21:58 --> 00:22:00 an 800 year return. Yeah, that's a bit

00:22:00 --> 00:22:03 woolier because the comets we observe now are

00:22:03 --> 00:22:06 fragments of one comet back then, and

00:22:06 --> 00:22:08 so therefore several comets tied to that

00:22:08 --> 00:22:09 initial apparition. So there's all that

00:22:09 --> 00:22:12 complexity there. We then have the long

00:22:12 --> 00:22:14 period comets, which, like I say were

00:22:14 --> 00:22:17 200 years or more. It still kind

00:22:17 --> 00:22:19 of is. But with those objects that are both

00:22:19 --> 00:22:22 long period and short period thanksgiang,

00:22:22 --> 00:22:23 you've got these objects whose orbital

00:22:23 --> 00:22:26 periods are so long that they are markedly

00:22:26 --> 00:22:28 longer than a human lifetime, even if they're

00:22:28 --> 00:22:30 comets that have been through before. So a

00:22:30 --> 00:22:32 good example of a really bright comet that is

00:22:32 --> 00:22:35 considered long period but has been through

00:22:35 --> 00:22:38 many times before is Comet Hale Bopp. Yes,

00:22:38 --> 00:22:41 was spectacular in 96, 97. It was visible

00:22:41 --> 00:22:43 with a naked eye for 18 months, shattering

00:22:43 --> 00:22:45 all the records. It will be back in about the

00:22:45 --> 00:22:47 year 4400. It was the last round when the

00:22:47 --> 00:22:50 Egyptians were building pyramids. And that is

00:22:50 --> 00:22:53 perversely a long period comet with a

00:22:53 --> 00:22:55 relatively short period orbit for a long

00:22:55 --> 00:22:58 period of comet. And so scientifically we'd

00:22:58 --> 00:23:01 call that dynamically old or not a

00:23:01 --> 00:23:02 new comet because it's been around a number

00:23:02 --> 00:23:05 of times at the very long period

00:23:05 --> 00:23:07 end of the long period comets, you get things

00:23:07 --> 00:23:09 that are coming in from halfway to the

00:23:09 --> 00:23:12 nearest star from a region we describe as the

00:23:12 --> 00:23:14 Oort Cloud or the Opic Oort cloud. And

00:23:14 --> 00:23:17 those things on their way in have

00:23:17 --> 00:23:20 calculated orbital periods of hundreds of

00:23:20 --> 00:23:23 thousands or even millions of years. And many

00:23:23 --> 00:23:25 of those actually only come through once. And

00:23:25 --> 00:23:27 then they get nudged and ejected from the

00:23:27 --> 00:23:29 solar system, never to return, going out to

00:23:29 --> 00:23:32 wander among the stars. And it's objects like

00:23:32 --> 00:23:34 that that will become the interstellar comets

00:23:34 --> 00:23:37 for other stars, in the same way that

00:23:37 --> 00:23:38 this third group of comets that you alluded

00:23:38 --> 00:23:41 to that we found recently are interstellar

00:23:41 --> 00:23:43 comets in our system. So these are the

00:23:43 --> 00:23:45 objects coming through so quickly that they

00:23:45 --> 00:23:47 are not gravitationally bound to the sun,

00:23:47 --> 00:23:49 but also so quickly that there is no

00:23:49 --> 00:23:52 possibility that they ever were. They've been

00:23:52 --> 00:23:54 flung in so quickly that they must come from

00:23:55 --> 00:23:58 another place. The most recent one was Three

00:23:58 --> 00:24:00 Eye Atlas, which got talked about a huge

00:24:00 --> 00:24:03 amount. Yes. Was definitely not an alien

00:24:03 --> 00:24:05 spaceship. And to avoid getting too

00:24:05 --> 00:24:07 political, just a very brief comment on that

00:24:07 --> 00:24:09 because it needs to be stated and restated,

00:24:09 --> 00:24:12 which is, uh, the arguments of that being an

00:24:12 --> 00:24:14 alien spaceship were the work of one person.

00:24:15 --> 00:24:17 One person who is not a solar system

00:24:17 --> 00:24:19 astronomer historically, but has reached that

00:24:19 --> 00:24:22 age and level of senility that they believe

00:24:22 --> 00:24:24 they can be an expert in things that they are

00:24:24 --> 00:24:27 not and has a certain financial interest in

00:24:27 --> 00:24:29 keeping people interested in aliens because

00:24:29 --> 00:24:31 they buy his book.

00:24:31 --> 00:24:31 Andrew Dunkley: Click.

00:24:32 --> 00:24:35 Jonti Horner: The community of astronomers has been very

00:24:35 --> 00:24:37 upset and very Shrek about that because it

00:24:37 --> 00:24:39 diverts attention from what is a really

00:24:39 --> 00:24:41 fascinating object on the fact that it's

00:24:41 --> 00:24:44 really fascinating, but also breeds a certain

00:24:44 --> 00:24:45 amount of fear. And I genuinely had people

00:24:45 --> 00:24:48 reaching out to me when he was pushing

00:24:48 --> 00:24:50 this narrative of it being aliens that were

00:24:50 --> 00:24:51 going to invade because they were frightened,

00:24:51 --> 00:24:54 heightened, they were genuinely worried

00:24:54 --> 00:24:55 because a Harvard astronomer was saying

00:24:55 --> 00:24:58 aliens were going to come and beat us all up.

00:24:58 --> 00:24:59 Andrew Dunkley: Yeah.

00:24:59 --> 00:25:01 Jonti Horner: And it's problematic because it hides the

00:25:01 --> 00:25:03 science, but it's also more widely

00:25:03 --> 00:25:06 problematic at a time when we have lowering

00:25:06 --> 00:25:09 levels of engagement with science and very

00:25:09 --> 00:25:11 much lowering levels of trust in science and

00:25:11 --> 00:25:14 scientists. It's very bad to have someone

00:25:14 --> 00:25:17 acting disingenuously, telling lies

00:25:17 --> 00:25:19 on muddying the water. Um, and then

00:25:19 --> 00:25:21 arguing that everybody else is wrong and mean

00:25:21 --> 00:25:23 to me and I'm the only one telling the truth.

00:25:23 --> 00:25:26 And it's part of that whole fake news thing

00:25:26 --> 00:25:29 that I think is dangerous and damaging.

00:25:29 --> 00:25:32 You know, we need people to have trust and

00:25:32 --> 00:25:33 faith in science because it's so integral to

00:25:33 --> 00:25:36 our lives. And it's good to question. But

00:25:36 --> 00:25:38 it's bad when people say things that they

00:25:38 --> 00:25:40 fundamentally know are not true just to get

00:25:40 --> 00:25:42 hits or clicks or money. Yeah.

00:25:43 --> 00:25:46 Andrew Dunkley: And it's important to debunk that

00:25:46 --> 00:25:49 kind of, uh, approach because

00:25:49 --> 00:25:51 I've had people come up to me very recently

00:25:51 --> 00:25:54 who know I do this podcast, uh,

00:25:54 --> 00:25:56 who've said to me, oh, what do you think of

00:25:56 --> 00:25:58 that alien spaceship? And I go, it's,

00:25:59 --> 00:26:01 it's, that's what I think

00:26:01 --> 00:26:04 because it's, it's somebody trying to get

00:26:04 --> 00:26:05 media attention. It's got nothing. It's a

00:26:05 --> 00:26:08 rock. It's actually, it's, it's a, it's an

00:26:08 --> 00:26:10 ice conglomerate. It's, it's not a, it's not

00:26:10 --> 00:26:13 a spaceship at all. It's not behaving like a

00:26:13 --> 00:26:15 spaceship would. It's behaving like something

00:26:15 --> 00:26:17 passing through our solar system.

00:26:18 --> 00:26:21 Um, and people, people. The thing is,

00:26:21 --> 00:26:22 Jonti, people are buying

00:26:22 --> 00:26:25 Jonti Horner: this rubbish, but there's an old saying

00:26:25 --> 00:26:28 that you know, like, and run around the

00:26:28 --> 00:26:30 world before the truth has got its boots on,

00:26:30 --> 00:26:32 especially when it's an attractive light.

00:26:32 --> 00:26:35 It's, I mean, again, digging into my

00:26:35 --> 00:26:36 memories of Terry Pratchett stuff which

00:26:36 --> 00:26:39 happens a lot. It's the old quote when

00:26:39 --> 00:26:41 they're talking about newspapers and nobody

00:26:41 --> 00:26:43 really ever wants to hear a story about dog

00:26:43 --> 00:26:44 bites mum because it happens all the time.

00:26:44 --> 00:26:46 But if you've got a story that says Mum bites

00:26:46 --> 00:26:48 dog, everybody's fascinated.

00:26:48 --> 00:26:48 Andrew Dunkley: Yeah.

00:26:48 --> 00:26:51 Jonti Horner: And this story has all the elements. It's so

00:26:51 --> 00:26:53 salacious that it gets coverage and people

00:26:53 --> 00:26:56 who don't normally read or digest science

00:26:56 --> 00:26:58 are not interested, will see this and hook

00:26:58 --> 00:27:00 into it. And when the byline is Harvard

00:27:00 --> 00:27:03 astronomer, that gives it a huge amount of

00:27:03 --> 00:27:03 credence.

00:27:03 --> 00:27:04 Andrew Dunkley: It does.

00:27:04 --> 00:27:06 Jonti Horner: Uh, and nobody hears the rebuttals. It's

00:27:07 --> 00:27:09 a bit like, you know, when there are claims

00:27:09 --> 00:27:10 of life on a planet around another star.

00:27:10 --> 00:27:13 Nobody remembers the, the follow

00:27:13 --> 00:27:15 ups that say actually it wasn't. They just

00:27:15 --> 00:27:17 remember, oh, we found aliens and we haven't.

00:27:18 --> 00:27:20 I mean, I think that story that,

00:27:20 --> 00:27:23 Andrew Dunkley: uh, the most recent story

00:27:23 --> 00:27:26 that I recall where that, that claim was made

00:27:26 --> 00:27:29 was um, the one about the

00:27:29 --> 00:27:31 something they. What was it they found in

00:27:31 --> 00:27:33 the, in the atmosphere of Venus. It was

00:27:34 --> 00:27:34 phosphine.

00:27:34 --> 00:27:37 Jonti Horner: Yes. I can go on a little bit of a side rant

00:27:37 --> 00:27:39 about that. My heart broke. Um, the

00:27:39 --> 00:27:42 lead author on that study was Jane Greaves in

00:27:42 --> 00:27:44 the uk, who's someone I knew very well when I

00:27:44 --> 00:27:46 was in the uk and she's a fabulous science

00:27:46 --> 00:27:49 and just all around wonderful individual. And

00:27:49 --> 00:27:51 the story was led by a UK team

00:27:52 --> 00:27:54 who, if you actually read the paper, don't

00:27:54 --> 00:27:57 say anything that is, this is life. What they

00:27:57 --> 00:28:00 say is we found a very weak signal of

00:28:00 --> 00:28:02 this gas in Venus's atmosphere. It's right

00:28:02 --> 00:28:04 down in the noise. So there is a chance it's

00:28:04 --> 00:28:07 a false positive anyway, so there needs to be

00:28:07 --> 00:28:09 a bit of extra work done. It's a little bit

00:28:09 --> 00:28:12 interesting because on the Earth, the only

00:28:12 --> 00:28:15 processes that produce this peculiar gas

00:28:15 --> 00:28:18 are, uh, technology and industry or life.

00:28:19 --> 00:28:20 Yeah. We don't know of any other way that

00:28:20 --> 00:28:22 it's made, but that doesn't mean that there

00:28:22 --> 00:28:23 aren't other ways that it's made.

00:28:23 --> 00:28:25 Andrew Dunkley: Isn't that a tasty morsel for the popular

00:28:25 --> 00:28:26 press?

00:28:26 --> 00:28:26 Jonti Horner: Absolutely.

00:28:26 --> 00:28:28 But what happened then was that there is an

00:28:29 --> 00:28:32 American outreach journal,

00:28:32 --> 00:28:34 um, science communication journal, that broke

00:28:34 --> 00:28:37 embargo on this story, didn't talk to Jane

00:28:37 --> 00:28:39 and her colleagues, but instead ran a story

00:28:39 --> 00:28:41 saying British scientists found life on

00:28:41 --> 00:28:43 Venus. Which is not what they'd said at all.

00:28:43 --> 00:28:45 No, that's what started the absolute bum

00:28:45 --> 00:28:48 fight. And the vitriol on the hair and the

00:28:48 --> 00:28:50 death threats, believe it or not, that Jane

00:28:50 --> 00:28:53 Grieves got because of this were

00:28:53 --> 00:28:55 astonishing. It was absolutely terrible. And

00:28:55 --> 00:28:58 instead of being able to managed to deploy

00:28:58 --> 00:29:00 this wonderful story about this fascinating

00:29:00 --> 00:29:02 new result they got, they spent all their

00:29:02 --> 00:29:05 time in damage control because this

00:29:06 --> 00:29:08 publication chose to break the embargo

00:29:08 --> 00:29:11 early and run a story that was not factually

00:29:11 --> 00:29:13 true, but again would get them clicks. Yep.

00:29:13 --> 00:29:16 Andrew Dunkley: Yeah. And that's unfortunately, the modern

00:29:16 --> 00:29:19 media and, um, the Internet's to

00:29:19 --> 00:29:21 blame. Well, it's not the Internet that's to

00:29:21 --> 00:29:23 blame. It's the people who use it that are to

00:29:23 --> 00:29:26 blame. And it's one of the, um,

00:29:26 --> 00:29:27 one of the things you've really got to be

00:29:27 --> 00:29:30 careful of when you are, uh, following

00:29:30 --> 00:29:33 a story, whether it's an exocomet that's not

00:29:33 --> 00:29:36 a spaceship or, uh, life that's

00:29:36 --> 00:29:38 not in Venus's atmosphere,

00:29:38 --> 00:29:41 um, and even to a lesser

00:29:41 --> 00:29:43 degree, and you and I mentioned this before

00:29:43 --> 00:29:45 we started, the way the media gets its

00:29:45 --> 00:29:48 information confused, such as

00:29:48 --> 00:29:51 reporting, uh, on, um, upcoming spectacular

00:29:51 --> 00:29:54 meteor showers that, uh, everyone

00:29:54 --> 00:29:56 gets excited about and then they realize

00:29:56 --> 00:29:57 they're on the wrong side of the planet.

00:29:57 --> 00:30:00 Jonti Horner: Absolutely. And this is a caution I give to

00:30:00 --> 00:30:02 everybody, both for comets and for meteors

00:30:02 --> 00:30:03 actually, but particularly for those of us in

00:30:03 --> 00:30:06 the Southern hemisphere, um, meteor showers

00:30:07 --> 00:30:10 and comets are things that are best seen

00:30:10 --> 00:30:12 from some latitudes and not from others. And

00:30:12 --> 00:30:13 for each comet or for each meteor shower

00:30:13 --> 00:30:16 that's different. Now, I'll talk later on

00:30:16 --> 00:30:18 about a newly discovered comet that might be

00:30:18 --> 00:30:20 very spectacular in late 2028.

00:30:21 --> 00:30:22 That comet is primarily going to be a

00:30:22 --> 00:30:25 Southern hemisphere object. So it will

00:30:25 --> 00:30:26 probably be better for us in Australia and

00:30:26 --> 00:30:28 New Zealand than it will be for people in the

00:30:28 --> 00:30:30 UK or the us Just as an example,

00:30:31 --> 00:30:33 when events are happening that are, uh,

00:30:33 --> 00:30:35 primarily good for the Northern Hemisphere.

00:30:35 --> 00:30:36 The Northern Hemisphere has more people and

00:30:36 --> 00:30:39 more media. And what I've seen happen more

00:30:39 --> 00:30:41 and more is that, uh, the media in Australia,

00:30:42 --> 00:30:44 and I know the Australian stuff because

00:30:44 --> 00:30:46 that's local to us. It's probably just the

00:30:46 --> 00:30:48 same in New Zealand, South Africa, South

00:30:48 --> 00:30:50 America, all these other places. But the

00:30:50 --> 00:30:52 media there will pick up these stories and

00:30:52 --> 00:30:54 just run them without running

00:30:54 --> 00:30:57 the sanity filter. So the April

00:30:57 --> 00:30:59 Lyrids are a really good example of this. But

00:30:59 --> 00:31:01 a better one is probably the Perseid meteor

00:31:01 --> 00:31:03 shower in August. Now, it's a little bit of

00:31:03 --> 00:31:06 background here. When we've got a meteor

00:31:06 --> 00:31:08 shower, we're getting bits of dust and debris

00:31:08 --> 00:31:11 hitting the Earth's atmosphere and ablating

00:31:11 --> 00:31:13 at an altitude of about 80 km. Now,

00:31:14 --> 00:31:16 ablation is a slightly weird thing. People

00:31:16 --> 00:31:18 often describe this as burning up, but it's

00:31:18 --> 00:31:20 not burning up in the sense of a flame being

00:31:20 --> 00:31:22 lit and a fire burning. It's rather that

00:31:22 --> 00:31:24 these things push into the atmosphere at

00:31:24 --> 00:31:26 really high speed, pile the air up in front

00:31:26 --> 00:31:28 of them, getting the air superheated,

00:31:28 --> 00:31:30 creating a load of plasma. And the heat from

00:31:30 --> 00:31:33 that makes and vaporizes the bit of debris.

00:31:33 --> 00:31:35 So it's not burning up in the traditional

00:31:35 --> 00:31:37 sense. And anytime you see a meteor, you see

00:31:37 --> 00:31:39 a shooting star, that's what you're seeing.

00:31:39 --> 00:31:40 And, uh, the bigger the bit of dust, the

00:31:40 --> 00:31:43 brighter it will be. The faster it's moving

00:31:43 --> 00:31:45 at a given size, the more energy it's got. So

00:31:45 --> 00:31:47 again, the brighter it'll be. Yeah. And you

00:31:47 --> 00:31:50 see shooting stars on any night of the year,

00:31:50 --> 00:31:53 typically, uh, three or four an hour in the

00:31:53 --> 00:31:55 evenings, five or six an hour in the

00:31:55 --> 00:31:57 mornings, potentially. And that difference is

00:31:57 --> 00:31:58 just because in the mornings you're facing

00:31:58 --> 00:32:00 the direction the Earth's moving. So you're

00:32:00 --> 00:32:02 getting collisions that are head on. So the

00:32:02 --> 00:32:05 average collision speed is higher. So a grain

00:32:05 --> 00:32:07 of dust that's the same size will be a bit

00:32:07 --> 00:32:09 brighter. Therefore, the things that in the

00:32:09 --> 00:32:11 evening that will be too faint to see become

00:32:11 --> 00:32:13 visible. So you get a slight increase in the

00:32:13 --> 00:32:15 rate towards morning. Then in the evening,

00:32:16 --> 00:32:17 um, it's also you're probably getting a

00:32:17 --> 00:32:19 slightly increased amount of stuff entering

00:32:19 --> 00:32:20 the atmosphere because you always see more

00:32:20 --> 00:32:22 flies hit your windscreen than your air

00:32:22 --> 00:32:24 windscreen. Same kind of idea. Yeah.

00:32:25 --> 00:32:27 When we get a meteor shower, what's happening

00:32:27 --> 00:32:30 is we're passing through the area of

00:32:30 --> 00:32:32 space where the Earth passes near the orbit

00:32:32 --> 00:32:34 of either a comet or an asteroid. And

00:32:34 --> 00:32:36 typically it's a comet. Now, every time a

00:32:36 --> 00:32:39 comet goes around the sun, that dirty

00:32:39 --> 00:32:42 snowball or snowy dirt ball gets hot. The

00:32:42 --> 00:32:44 volatile material on the surface is too hot

00:32:44 --> 00:32:47 to stay solid, so becomes a gas in a

00:32:47 --> 00:32:50 process called sublimation. And you get jets

00:32:50 --> 00:32:52 erupting from the comet, shrouding in gas,

00:32:53 --> 00:32:55 which is then blown away from the sun to give

00:32:55 --> 00:32:57 you the tails. Those jets erupting into

00:32:57 --> 00:32:59 space carry with them dust.

00:33:00 --> 00:33:03 Now, biggest bits of dust are pushed away so

00:33:03 --> 00:33:04 gently, they'll fall back to the comet and

00:33:04 --> 00:33:06 clog it up. And some comets eventually turn

00:33:06 --> 00:33:08 off because of. This also is the reason most

00:33:08 --> 00:33:11 comets are only active from a few locations

00:33:11 --> 00:33:13 on the surface, not uniformly, because most

00:33:13 --> 00:33:15 of the surface is clogged up and you've just

00:33:15 --> 00:33:17 got a few active areas where volatile

00:33:17 --> 00:33:20 material is exposed. Yeah, but that dust

00:33:20 --> 00:33:22 that's ejected from the comet is ejected with

00:33:22 --> 00:33:24 speeds measured in meters per second or

00:33:24 --> 00:33:27 centimetres per second from an object that's

00:33:27 --> 00:33:28 traveling at a speed measured in tens of

00:33:28 --> 00:33:31 kilometers a second. So what that means is

00:33:31 --> 00:33:34 that, uh, that dust is moving away from

00:33:34 --> 00:33:36 the comet at a speed almost identical to the

00:33:36 --> 00:33:39 speed the comet's traveling itself. I guess

00:33:39 --> 00:33:41 it's like if you. You're driving along the

00:33:41 --> 00:33:43 road and you drop a tennis ball out of the

00:33:43 --> 00:33:45 window until the wind resistance pushes it

00:33:45 --> 00:33:47 back. If there wasn't a wind resistance

00:33:47 --> 00:33:50 there, it would move along with the car, just

00:33:50 --> 00:33:51 drifting away very slightly based on the

00:33:51 --> 00:33:53 speed you pushed it out of the window. Same

00:33:53 --> 00:33:54 idea. Yeah.

00:33:54 --> 00:33:57 Andrew Dunkley: I actually saw a really great experiment once

00:33:57 --> 00:33:59 where they were.

00:34:01 --> 00:34:03 How did they do it? They had a guy on the

00:34:03 --> 00:34:06 back of a truck, and they

00:34:06 --> 00:34:08 were driving at, like, uh, 100

00:34:08 --> 00:34:11 kilometers an hour, and they shot him

00:34:11 --> 00:34:14 off the truck in the opposite direction at

00:34:14 --> 00:34:17 the same speed, and he just stopped where he

00:34:17 --> 00:34:17 landed.

00:34:17 --> 00:34:19 Jonti Horner: Well, it's brilliant. I think mythbusters did

00:34:19 --> 00:34:22 something similar, and it's amazing. Our

00:34:22 --> 00:34:24 common sense is physics, really

00:34:25 --> 00:34:27 simple physics is great, but our common sense

00:34:27 --> 00:34:30 breaks down in some situations because our

00:34:30 --> 00:34:32 common sense is a naturally inherited thing

00:34:32 --> 00:34:34 about the world at the speeds we experience

00:34:34 --> 00:34:37 it. And so we tend to think if you're running

00:34:37 --> 00:34:39 forwards at 10km an hour and you throw

00:34:39 --> 00:34:41 something forwards, it will travel a bit

00:34:41 --> 00:34:43 faster. That breaks down when you get to

00:34:43 --> 00:34:45 relativity. There's all these weird things

00:34:45 --> 00:34:47 around it where our common sense gets it

00:34:47 --> 00:34:50 wrong for comets and for the dust. And it

00:34:50 --> 00:34:51 took me a long while to get my head around

00:34:51 --> 00:34:54 this because it's a bit counterintuitive if

00:34:54 --> 00:34:56 you eject Dust from a comet. You can eject

00:34:56 --> 00:34:58 the dust forward or backwards. So you can

00:34:58 --> 00:35:00 imagine this jet from the comet working a bit

00:35:00 --> 00:35:03 like a geyser, turning off when it gets dark

00:35:03 --> 00:35:05 and it gets cold, and then turning off again

00:35:05 --> 00:35:07 in the morning when it gets hot again. That

00:35:07 --> 00:35:09 can throw dust forwards, sidewards, and, um,

00:35:09 --> 00:35:12 backwards, or any combination of the above.

00:35:12 --> 00:35:14 So that means this comet is throwing out dust

00:35:14 --> 00:35:17 at a speed of meters per second, a bit like a

00:35:17 --> 00:35:19 sprinkler into space. The

00:35:19 --> 00:35:22 dust has a forward component to its speed.

00:35:22 --> 00:35:24 So it could be going sideways but a little

00:35:24 --> 00:35:25 forward, or it could be going head on in

00:35:25 --> 00:35:28 front of the comet that is now traveling

00:35:28 --> 00:35:30 around the sun faster than the comet is,

00:35:30 --> 00:35:32 which means it will move onto, um, an orbit

00:35:32 --> 00:35:35 with a longer period than the comet. So the

00:35:35 --> 00:35:36 next time the comet comes round, that grain

00:35:36 --> 00:35:39 of dust will arrive after the comet. So dust

00:35:39 --> 00:35:42 thrown forward ends up behind. And similarly,

00:35:42 --> 00:35:44 dust thrown backwards is moving slower than

00:35:44 --> 00:35:45 the comet, which puts it on a slightly

00:35:45 --> 00:35:48 shorter period orbit, and therefore it will

00:35:48 --> 00:35:50 arrive ahead of the comet next time. And that

00:35:50 --> 00:35:52 little bit of sidewards motion also means it

00:35:52 --> 00:35:54 will spread out a little bit in space. What

00:35:54 --> 00:35:57 this means over, uh, time periods is that,

00:35:57 --> 00:35:58 uh, comets, every time they come round,

00:35:59 --> 00:36:01 essentially shed what becomes like a javelin

00:36:01 --> 00:36:04 shape, a spear of dust into space with a

00:36:04 --> 00:36:07 comet at the center, like a

00:36:07 --> 00:36:09 spike. And that spike gradually diffuses over

00:36:09 --> 00:36:11 time, spreads out further and further ahead

00:36:11 --> 00:36:13 and behind the comet. And so over a long time

00:36:13 --> 00:36:16 scale, you eventually end up with the comet's

00:36:16 --> 00:36:18 orbit shrouded in dust. And the dust can be

00:36:18 --> 00:36:20 quite spread out over millions of kilometers.

00:36:21 --> 00:36:23 Yeah, these orbits are oriented randomly in

00:36:23 --> 00:36:26 space. So many of them don't intersect the

00:36:26 --> 00:36:28 Earth. Even if the comet gets closer to the

00:36:28 --> 00:36:31 sun than we are at its closest, passes above

00:36:31 --> 00:36:33 or below the Earth's orbit, nothing happens.

00:36:33 --> 00:36:36 But for a subset of them, the comet

00:36:37 --> 00:36:39 will, in its orbit, have the potential to get

00:36:39 --> 00:36:41 very close to the Earth. So its orbit and the

00:36:41 --> 00:36:43 Earth get very close together. And in those

00:36:43 --> 00:36:46 cases, every time we go around the sun, if

00:36:46 --> 00:36:47 that comet's been laying dust down for a

00:36:47 --> 00:36:50 while, we'll run into the dust every time we

00:36:50 --> 00:36:52 go around. And that dust will hit the Earth's

00:36:52 --> 00:36:54 M atmosphere, which means we're going through

00:36:54 --> 00:36:56 a dirtier bit of the solar system and we get

00:36:56 --> 00:36:58 more meteors. That's when we get a meteor

00:36:58 --> 00:37:00 shower. But the other telltale thing for the

00:37:00 --> 00:37:03 meteor shower is all the dust grains that hit

00:37:03 --> 00:37:05 the Earth in a meteor shower are moving

00:37:05 --> 00:37:07 essentially parallel to each other.

00:37:07 --> 00:37:08 They're all following the same Orbit around

00:37:08 --> 00:37:09 the sun, hitting the Earth, the Earth from

00:37:09 --> 00:37:11 the same direction at the same speed.

00:37:13 --> 00:37:15 So all this dust is coming towards you from a

00:37:15 --> 00:37:17 single point in space. So from your point of

00:37:17 --> 00:37:19 view, looking at the sky, when you see those

00:37:19 --> 00:37:22 meteors, part of a meteor shower, they appear

00:37:22 --> 00:37:25 to appear anywhere in the sky. But if

00:37:25 --> 00:37:26 you trace them back, they'll all point to a

00:37:26 --> 00:37:28 single point in the sky, that something we

00:37:28 --> 00:37:31 call the radiant. And that's effectively the

00:37:31 --> 00:37:33 point in space they're traveling towards us

00:37:33 --> 00:37:35 from. And um, they diverge because they

00:37:35 --> 00:37:37 perspective, they're coming closer to you. So

00:37:37 --> 00:37:40 every meteor shower has a radiant in the sky.

00:37:40 --> 00:37:42 The April Lyrids have their radiant in

00:37:43 --> 00:37:45 Lyra, although for a fair part of their time

00:37:45 --> 00:37:47 it's actually in Hercules, it m drifts a bit.

00:37:47 --> 00:37:49 The Perseids have their radiant in Perseus,

00:37:50 --> 00:37:52 the Geminids in Gemini and so on.

00:37:53 --> 00:37:56 So that's all well and good. If the

00:37:56 --> 00:37:59 radiant is below the horizon, that means the

00:37:59 --> 00:38:00 meteors are hitting the other side of the

00:38:00 --> 00:38:02 Earth and you can't see them because the

00:38:02 --> 00:38:04 Earth's in the way. So first point with a

00:38:04 --> 00:38:07 meteor shower is unlike some of the media

00:38:07 --> 00:38:09 reports, you can't see meteors for that

00:38:09 --> 00:38:12 meteor shower at any time of night. You can

00:38:12 --> 00:38:13 only see them when the radiance above the

00:38:13 --> 00:38:15 horizon point, number one

00:38:16 --> 00:38:18 point. The second is the higher in the sky

00:38:18 --> 00:38:21 that radiant is, the more head on into the

00:38:21 --> 00:38:23 stream you're going. So the more meteors

00:38:23 --> 00:38:26 you'll see. Now the analogy I'd ah, use here

00:38:26 --> 00:38:28 is if you imagine getting your hose pipe and

00:38:28 --> 00:38:30 having it on that shower mode, you know,

00:38:30 --> 00:38:32 where water's coming out from many holes all

00:38:32 --> 00:38:35 at once. If you hold that hose pipe

00:38:35 --> 00:38:37 vertically and turn the tap on, all the water

00:38:37 --> 00:38:38 from that hose pipe will hit a relatively

00:38:38 --> 00:38:41 small area of the ground. If you turn that

00:38:41 --> 00:38:44 hose pipe to 45 degrees, that water will

00:38:44 --> 00:38:46 spread out over a larger surface area.

00:38:47 --> 00:38:47 Andrew Dunkley: Yep.

00:38:47 --> 00:38:49 Jonti Horner: Now if you imagine the meteors, the dust in a

00:38:49 --> 00:38:51 meteor shower coming in towards the Earth,

00:38:52 --> 00:38:54 the more directly overhead

00:38:54 --> 00:38:57 your point that they're coming from is the

00:38:57 --> 00:38:59 more meteors you'll get in a certain volume

00:38:59 --> 00:39:01 of the atmosphere and the lower to the

00:39:01 --> 00:39:03 horizon that point is, the more you'll spread

00:39:03 --> 00:39:05 those same number of grains of dust out.

00:39:06 --> 00:39:09 So the higher in the sky the radiant is, the

00:39:09 --> 00:39:10 more dust is hitting the part of the

00:39:10 --> 00:39:13 atmosphere you can see from your location. So

00:39:13 --> 00:39:15 the more meteors you get, and what this means

00:39:15 --> 00:39:17 is that the lower in the sky the rating is a

00:39:17 --> 00:39:20 few meteors you see. And so you see the most

00:39:20 --> 00:39:22 Meteors. For a given meteor shower, when the

00:39:22 --> 00:39:24 radiant is near what we call culmination,

00:39:24 --> 00:39:26 where it's nearly highest in the sky. For the

00:39:26 --> 00:39:28 southern hemisphere, when it's nearly due

00:39:28 --> 00:39:31 north, for the northern hemisphere rain, the

00:39:31 --> 00:39:33 radiant's nearly due south. So

00:39:33 --> 00:39:36 all well and good, but what that means is

00:39:36 --> 00:39:38 that ah, from different locations on the

00:39:38 --> 00:39:40 earth, a given meteor shower will give you a

00:39:40 --> 00:39:42 different strength of display. The April

00:39:42 --> 00:39:45 Lyrids, their radiant is

00:39:46 --> 00:39:48 34 degrees north of the equator. So that

00:39:48 --> 00:39:50 means if you lived 34 degrees north of the

00:39:50 --> 00:39:53 equator at about 2am in the morning, the

00:39:53 --> 00:39:55 radiant will be overhead and you're in the

00:39:55 --> 00:39:56 best place on the planet to see the meteors.

00:39:57 --> 00:40:00 If you had perfect vision, perfectly dark

00:40:00 --> 00:40:03 sky, you'd see a number of meteors, 15

00:40:03 --> 00:40:05 to 20 per hour for the April Lyrids and

00:40:05 --> 00:40:07 that's called the zenithal hourly rate.

00:40:07 --> 00:40:09 That's the number of meters you'd see in

00:40:09 --> 00:40:11 perfect conditions with perfect eyesight,

00:40:11 --> 00:40:13 with no light pollution if the radiant was

00:40:13 --> 00:40:16 overhead. The lower the radiant is in the

00:40:16 --> 00:40:18 sky, the more that number shrinks. So the

00:40:18 --> 00:40:21 ZHR is the theoretical maximum number

00:40:21 --> 00:40:23 you'd see. So good

00:40:23 --> 00:40:25 meteor shower, not a great one from the

00:40:25 --> 00:40:27 northern hemisphere, but for us in Brisbane,

00:40:27 --> 00:40:29 let's say 26 degrees south.

00:40:30 --> 00:40:32 The radiant of the April Lyrids at its

00:40:32 --> 00:40:34 highest in the sky is only 30 degrees above

00:40:34 --> 00:40:37 the horizon. That means that the

00:40:37 --> 00:40:40 volume of space where the dust is arriving is

00:40:40 --> 00:40:42 doubled. So you'd only see half the number of

00:40:42 --> 00:40:45 meteors. So instead of 20 per

00:40:45 --> 00:40:46 hour, you're down to 10 an hour

00:40:47 --> 00:40:50 immediately before anything else kicks in.

00:40:50 --> 00:40:52 And the further south you go, the lower the

00:40:52 --> 00:40:55 rates are. But the problem is the journalists

00:40:55 --> 00:40:56 covering this will pick up on a Northern

00:40:56 --> 00:40:58 hemisphere article and just repeat it.

00:40:58 --> 00:41:00 There's this meteor shower happening. You can

00:41:00 --> 00:41:02 see them all night, every night. Well that's

00:41:02 --> 00:41:04 not right. If the radiance below the horizon,

00:41:04 --> 00:41:06 you can't see them and you'll see 100 per

00:41:06 --> 00:41:08 hour and M that's because they've seen the

00:41:08 --> 00:41:10 zenithal hourly rate, quoted as 100 per hour.

00:41:10 --> 00:41:12 And they just use it as a number.

00:41:12 --> 00:41:13 Andrew Dunkley: Yeah.

00:41:13 --> 00:41:15 Jonti Horner: Unless you are incredibly, incredibly

00:41:15 --> 00:41:18 fortunate, you will never see the same number

00:41:18 --> 00:41:20 of meteors as the ZHR predicts

00:41:21 --> 00:41:23 because the radiant might be directly

00:41:23 --> 00:41:25 overhead. So the rate gets lower. Your eyes

00:41:25 --> 00:41:27 are not perfect unless you're one of the very

00:41:27 --> 00:41:30 rare observers. The rates will get lower,

00:41:30 --> 00:41:32 there might be light pollution. The phantom

00:41:33 --> 00:41:35 meteors are not seen, the rates get lower.

00:41:35 --> 00:41:37 The moon might be in the sky. The phantom

00:41:37 --> 00:41:39 meters are not seen. The rates are lower. So

00:41:40 --> 00:41:42 you will never see a number of meteors in the

00:41:42 --> 00:41:45 sky equal to the ZHR unless the meteor

00:41:45 --> 00:41:48 shower is more active than predicted in which

00:41:48 --> 00:41:49 case the ZHR will be higher and you'd see

00:41:49 --> 00:41:52 more. Where this really comes in is for

00:41:52 --> 00:41:54 meteor showers like the Perseids. The

00:41:54 --> 00:41:56 Perseids are one of the big three. There are

00:41:56 --> 00:41:59 AH3 awesome meteor showers a year that are by

00:41:59 --> 00:42:01 far the best in a given year.

00:42:01 --> 00:42:03 They're the highest rates, the most dust

00:42:04 --> 00:42:06 coming in. Other high speed, the Quadrantids

00:42:06 --> 00:42:09 in early January are very, very short

00:42:09 --> 00:42:11 lived. They're a wage shower. You've got a

00:42:11 --> 00:42:13 very low rate of meteors for most of the time

00:42:13 --> 00:42:14 they're active and then a very narrow spike

00:42:14 --> 00:42:17 that can be very big. But if you manage

00:42:17 --> 00:42:19 to see that spike there's a lot of meteors.

00:42:19 --> 00:42:21 They're only really visible from the northern

00:42:21 --> 00:42:24 hemisphere. The Perseids in August are

00:42:24 --> 00:42:26 probably uh, the most storied meteor shower

00:42:27 --> 00:42:30 with long history of observations

00:42:31 --> 00:42:32 linked to comet Swift Tuttle which goes

00:42:32 --> 00:42:34 around every 120. 130 years

00:42:35 --> 00:42:37 incidentally will be incredibly spectacular

00:42:37 --> 00:42:39 in the year 2126 if people hang around to see

00:42:39 --> 00:42:40 it.

00:42:40 --> 00:42:42 Andrew Dunkley: Yeah, okay, I'll write that in my diary.

00:42:43 --> 00:42:45 Jonti Horner: Um, Perseids are brilliant but their radiant

00:42:45 --> 00:42:48 is at about 55 degrees north in the sky.

00:42:49 --> 00:42:51 Fabulous from northern Europe, fabulous from

00:42:51 --> 00:42:53 North America, places north of the equator to

00:42:53 --> 00:42:55 get a really good show. But we get articles

00:42:55 --> 00:42:58 every year on commercial media here in

00:42:58 --> 00:43:00 Australia saying the persons are happening go

00:43:00 --> 00:43:02 up tonight and you'll see 100 meters an hour.

00:43:02 --> 00:43:04 And for most of Australia the radiant never

00:43:04 --> 00:43:07 even rises, never, you know, south of about

00:43:07 --> 00:43:10 35 degrees south the radiant will never rise.

00:43:10 --> 00:43:12 I think that's about the latitude of Sydney.

00:43:13 --> 00:43:15 North of that it will rise but it'll be very

00:43:15 --> 00:43:16 low to the horizon. So you'll see a much

00:43:16 --> 00:43:19 lower rate unless you're in the top, top end.

00:43:19 --> 00:43:20 If you're in the top end of Australia it's a

00:43:20 --> 00:43:23 bit different. And so when you see

00:43:23 --> 00:43:26 articles like this you need to engage

00:43:26 --> 00:43:28 your science brain and say the journalist

00:43:28 --> 00:43:30 wrong. Yeah, where's my location?

00:43:30 --> 00:43:33 What's the radiance? Declination which

00:43:33 --> 00:43:36 is latitude in the sky effectively figure out

00:43:36 --> 00:43:38 how high in the sky it'll get and that will

00:43:38 --> 00:43:39 give you a feel for what you might actually

00:43:39 --> 00:43:42 see. Now if you want to um, look

00:43:42 --> 00:43:44 at the meteor shower calendar and figure out

00:43:44 --> 00:43:46 when there are good ones happening, the

00:43:46 --> 00:43:48 International Meteor Organization is my go to

00:43:48 --> 00:43:51 on this. They're a fabulous organization that

00:43:51 --> 00:43:53 put together every year a calendar and that

00:43:53 --> 00:43:55 calendar lists all the meteor showers from

00:43:55 --> 00:43:57 the incredibly minor ones that give one

00:43:57 --> 00:43:59 meteor every two hours, you know, to the

00:43:59 --> 00:44:02 major ones. And every year it writes about

00:44:02 --> 00:44:05 the conditions in terms of moonlight as well.

00:44:05 --> 00:44:08 Because if the moon is bright, you will see

00:44:08 --> 00:44:11 far fewer meteors. And coming up in a couple

00:44:11 --> 00:44:13 of weeks from when we're having this

00:44:13 --> 00:44:15 discussion, but in the past, as we actually

00:44:15 --> 00:44:17 go live to air, you've got the peak of the

00:44:17 --> 00:44:19 Ytraquarids. Now the Yter Aquarids are one of

00:44:19 --> 00:44:21 the few showers that's better for Southern

00:44:21 --> 00:44:22 hemisphere than Northern Hemisphere

00:44:22 --> 00:44:24 hemisphere. Fragments of Comet Hallie, and

00:44:24 --> 00:44:26 they're at their peak around the 3rd to the

00:44:26 --> 00:44:29 7th may have quite a broad peak, but

00:44:29 --> 00:44:32 this year the moon is a waning

00:44:32 --> 00:44:34 gibbous. So at the time of night when you

00:44:34 --> 00:44:36 could see these meteors, the sky will be

00:44:36 --> 00:44:38 really bright and so far fewer will be

00:44:38 --> 00:44:41 visible than normal. And you can get that

00:44:41 --> 00:44:42 from these calendars. But the highlight of

00:44:42 --> 00:44:44 every year for meteor showers is the Geminids

00:44:45 --> 00:44:48 in December. And they are pretty much global

00:44:48 --> 00:44:50 as a phenomenon and they're brilliant

00:44:50 --> 00:44:52 everywhere. Obviously better for the Northern

00:44:52 --> 00:44:53 hemisphere than the south. That's like a

00:44:53 --> 00:44:55 recurring theme, but

00:44:56 --> 00:44:59 they are great every year. And this year,

00:44:59 --> 00:45:01 Moon will be effectively new. So if you want

00:45:01 --> 00:45:03 to go see the Geminids peaking on the 14th or

00:45:03 --> 00:45:06 15th of December, they're the highlight this

00:45:06 --> 00:45:07 year and pretty much every year.

00:45:08 --> 00:45:10 Andrew Dunkley: Okay, uh, we're going to take another breath

00:45:10 --> 00:45:12 and then we'll come back and wrap it all up

00:45:12 --> 00:45:14 in this episode of Space Nuts with Andrew

00:45:14 --> 00:45:15 Dunkley and Jonti Horner.

00:45:20 --> 00:45:21 Jonti Horner: Tranquility Base here.

00:45:21 --> 00:45:23 Andrew Dunkley: The eagle has landed.

00:45:23 --> 00:45:23 Jonti Horner: Space gnats.

00:45:24 --> 00:45:27 Andrew Dunkley: One of my big frustrations, uh,

00:45:27 --> 00:45:29 when I want to observe comets is I live on a

00:45:29 --> 00:45:32 very flat area of the planet. Uh,

00:45:32 --> 00:45:35 we don't have mountains nearby, we barely

00:45:35 --> 00:45:38 have hills. And a lot of the comets

00:45:38 --> 00:45:41 are visible, uh, in the low

00:45:41 --> 00:45:44 horizon just after sunset or

00:45:45 --> 00:45:47 thereabouts. And they're short lived

00:45:48 --> 00:45:51 and they're below the horizon way too

00:45:51 --> 00:45:53 quick. Uh, which makes astrophotography a

00:45:53 --> 00:45:56 real pain in the butt for me. But it is

00:45:57 --> 00:45:59 just a quirk of where I live.

00:45:59 --> 00:46:01 Um, I believe

00:46:02 --> 00:46:05 that we do have some pretty spectacular ones

00:46:05 --> 00:46:08 coming up. The one that I've seen

00:46:08 --> 00:46:11 in my life that was the most spectacular for

00:46:11 --> 00:46:13 me was in 2007, January

00:46:13 --> 00:46:16 2007. Uh, the, it

00:46:16 --> 00:46:19 was Comet McNaught. It was amazing,

00:46:19 --> 00:46:22 like naked eye, comet wise. It

00:46:22 --> 00:46:25 was unmissable. Uh, it dominated

00:46:25 --> 00:46:28 the sky for quite some time. Uh, we don't see

00:46:28 --> 00:46:29 many like that though, do we?

00:46:30 --> 00:46:32 Jonti Horner: We don't now. Comet McNaught was probably the

00:46:32 --> 00:46:35 brightest comet since the 1960s and it was

00:46:35 --> 00:46:37 truly a great comet. Now when we talk

00:46:37 --> 00:46:40 about the brightest comets and the ones

00:46:40 --> 00:46:42 people want to see, great comet is the

00:46:42 --> 00:46:44 Appalachian people attached to comets. And

00:46:44 --> 00:46:46 it's got a woolly ish definition. It's

00:46:46 --> 00:46:48 basically the comet was bright enough and

00:46:48 --> 00:46:50 spectacular enough that even people who

00:46:50 --> 00:46:51 weren't that interested could just step

00:46:51 --> 00:46:53 outside and see it. Comet McNaughts

00:46:53 --> 00:46:56 definitely like that. Arguably Comet Chichin

00:46:56 --> 00:46:59 Chan Atlas in 2024 and Comet Atlas in

00:46:59 --> 00:47:02 early 2025 just made that threshold.

00:47:02 --> 00:47:04 So if you saw those comets, you'd probably

00:47:04 --> 00:47:07 say they are right at the lower end of what

00:47:07 --> 00:47:10 we consider a great comet. On average,

00:47:10 --> 00:47:12 if you go back through historical comic

00:47:12 --> 00:47:14 records, you'd probably get about 10 great

00:47:14 --> 00:47:17 comets per century with very wide

00:47:17 --> 00:47:20 variants. And that's not one every 10 years.

00:47:20 --> 00:47:22 They're like buses. You wait 30 years and two

00:47:22 --> 00:47:24 come along at once. And you saw that back in

00:47:24 --> 00:47:27 1996 with Comet Hale Bop and Comet Hyakitake,

00:47:27 --> 00:47:29 which were visible in the sky at the same

00:47:29 --> 00:47:32 time as great comets. It's really

00:47:32 --> 00:47:33 hard to predict when they're going to come

00:47:33 --> 00:47:35 in. But we've seen some really fascinating

00:47:35 --> 00:47:38 advances in the last few years on two fronts.

00:47:38 --> 00:47:41 Firstly, our ability to find things

00:47:41 --> 00:47:43 early has improved. We've got better

00:47:43 --> 00:47:46 telescopes, more automated surveys, and,

00:47:46 --> 00:47:48 um, comet maps earlier this year, which

00:47:48 --> 00:47:49 turned out to be a bit of a disappointment

00:47:49 --> 00:47:51 for many people, is a really good example of

00:47:51 --> 00:47:53 that. That's a member of the Kreutz

00:47:53 --> 00:47:56 sungrazing family. And the Kreuz sungrazers

00:47:56 --> 00:47:58 have numbered many of the brightest great

00:47:58 --> 00:48:00 comets of the last couple of thousand years.

00:48:01 --> 00:48:03 Comet maps was the earliest we've ever found

00:48:03 --> 00:48:06 a Kreutz sungrazer on the way in, earlier

00:48:06 --> 00:48:09 even than Comedike Oseci, which was probably

00:48:09 --> 00:48:11 the brightest comet in the 20th century back

00:48:11 --> 00:48:14 in the late 1960s. And so people's hopes were

00:48:14 --> 00:48:16 high. But in reality it was quite a small

00:48:16 --> 00:48:18 fragment of the Kreutz parents

00:48:19 --> 00:48:20 sungrazer. These Kreutz comets are all

00:48:20 --> 00:48:23 fragments of a bigger comet in the past, and

00:48:23 --> 00:48:25 it just fell apart on its way in. Nothing to

00:48:25 --> 00:48:28 see here. But our ability to find

00:48:28 --> 00:48:30 things earlier means that we get more

00:48:30 --> 00:48:32 warning when a bright comet's coming. Now

00:48:32 --> 00:48:35 that's not absolutely guaranteed. We had a

00:48:35 --> 00:48:37 comet and the name of it slipped my mind. Um,

00:48:37 --> 00:48:40 Comet 12, 18 months ago. Um, no,

00:48:40 --> 00:48:43 I think it was like last September

00:48:44 --> 00:48:46 that was discovered when it was almost naked

00:48:46 --> 00:48:49 eye visibility. It just about became naked

00:48:49 --> 00:48:51 eye visible wasn't great by any means. Swan.

00:48:51 --> 00:48:54 We got no warning. That's it, Comet Swan. And

00:48:54 --> 00:48:56 the reason that that was found so late was it

00:48:56 --> 00:48:58 came at us from behind the sun and suddenly

00:48:58 --> 00:49:01 popped into view. So that does still happen,

00:49:01 --> 00:49:04 but with facilities like Vera Rubin coming

00:49:04 --> 00:49:05 online, we're going to find comets earlier

00:49:05 --> 00:49:08 and earlier, which means we get more prior

00:49:08 --> 00:49:10 warning. But it also means that the

00:49:10 --> 00:49:12 uncertainty about how bright they're going to

00:49:12 --> 00:49:13 get is possibly even higher because we're

00:49:13 --> 00:49:16 almost finding them now before they've really

00:49:16 --> 00:49:18 started to become active. While they're far

00:49:18 --> 00:49:19 enough from the sun that we're almost seeing

00:49:19 --> 00:49:22 a bare nuclear nucleus, or we're seeing

00:49:22 --> 00:49:24 a much smaller comet that's had a little bit

00:49:24 --> 00:49:26 of an outburst at that distance and whether

00:49:26 --> 00:49:28 that far away, we effectively can't tell the

00:49:28 --> 00:49:30 difference. They're still like a single

00:49:30 --> 00:49:32 pixel. There's a really good example of this

00:49:32 --> 00:49:35 in the form of Comet Chu Chin Shan. Um,

00:49:35 --> 00:49:37 not come to Chin Chan ATLAS from a couple of

00:49:37 --> 00:49:38 years ago, but Comet Chu Chin Shan that has

00:49:38 --> 00:49:40 just been discovered in the last couple of

00:49:40 --> 00:49:42 months, Comet C 2026

00:49:42 --> 00:49:45 C1. As we record this, that

00:49:45 --> 00:49:48 comet is still more distant from the sun than

00:49:48 --> 00:49:50 the orbit of Saturn. It was found a couple of

00:49:50 --> 00:49:52 months ago. It will not be at its closest to

00:49:52 --> 00:49:55 some perihelion until November

00:49:55 --> 00:49:57 2028. So we've got two and a half years to

00:49:57 --> 00:50:00 wait. Now, what factors

00:50:00 --> 00:50:01 into a comet's brightness is very

00:50:01 --> 00:50:04 complicated. Um, but it can boil down to a

00:50:04 --> 00:50:06 few different things. Firstly, if everything

00:50:06 --> 00:50:09 else is equal. So imagine we only change one

00:50:09 --> 00:50:11 thing. Typically, the bigger the nucleus of

00:50:11 --> 00:50:14 the comet, the bigger its surface area is. So

00:50:14 --> 00:50:17 the more dust and gas it can produce. And we

00:50:17 --> 00:50:19 see the comet from the light that is

00:50:19 --> 00:50:21 reflected from the dust and gas. That's what

00:50:21 --> 00:50:23 makes the tails and the coma. The snowballs,

00:50:23 --> 00:50:24 ah, at the head were actually pretty small.

00:50:24 --> 00:50:27 Comet McNaught was only about 5km across

00:50:27 --> 00:50:30 for the nucleus, but it grew tails more than

00:50:30 --> 00:50:31 300 million kilometers long.

00:50:32 --> 00:50:33 Andrew Dunkley: Yeah, that's a little bit different.

00:50:33 --> 00:50:34 Incredible.

00:50:34 --> 00:50:36 Jonti Horner: So if you have two cometary nuclei that, uh,

00:50:36 --> 00:50:39 are in all senses identical other than their

00:50:39 --> 00:50:41 size, the bigger one will typically be more

00:50:41 --> 00:50:43 active and produce more gas and dust.

00:50:44 --> 00:50:47 However, some comets have a m larger fraction

00:50:47 --> 00:50:49 of their surface active than others. Some

00:50:49 --> 00:50:51 comets are almost dormant because they're

00:50:51 --> 00:50:53 clogged up and there's very little activity

00:50:53 --> 00:50:55 even from a larger nucleus. So already a bit

00:50:55 --> 00:50:58 complex. But first rule of thumb, um, the

00:50:58 --> 00:50:59 bigger the nucleus, the more likelihood there

00:50:59 --> 00:51:01 is that it will be able to produce a lot of

00:51:01 --> 00:51:03 gas and Dust and be more spectacular. With

00:51:03 --> 00:51:06 Comet Chu Chen Shan, that's interesting. We

00:51:06 --> 00:51:08 found it so far away, which suggests it is

00:51:08 --> 00:51:10 either a comet with quite a large nucleus,

00:51:10 --> 00:51:12 because it's probably not that active at that

00:51:12 --> 00:51:15 distance, but it may have just had a bit of

00:51:15 --> 00:51:17 an outburst of activity driven by something

00:51:17 --> 00:51:20 like carbon monoxide, which can turn from

00:51:20 --> 00:51:22 solid gas at a very low temperature. So it

00:51:22 --> 00:51:24 might be masquerading as a bigger comet than

00:51:24 --> 00:51:25 it is, and we don't know.

00:51:26 --> 00:51:27 Andrew Dunkley: Okay.

00:51:27 --> 00:51:29 Jonti Horner: The next thing that factors into how bright a

00:51:29 --> 00:51:30 comet gets is how close it gets to the Sun.

00:51:30 --> 00:51:33 So the closer it gets to the sun, the hotter

00:51:33 --> 00:51:35 its surface gets and the more strongly it

00:51:35 --> 00:51:38 will be active. So with Comet McNaught, you

00:51:38 --> 00:51:40 had a five kilometer nucleus, which is fairly

00:51:40 --> 00:51:42 respectable, but not as big as Hale Bopp,

00:51:42 --> 00:51:45 which was 50km. Hale Bok was ridiculous.

00:51:45 --> 00:51:48 But Comet McNaught got very close into the

00:51:48 --> 00:51:50 Sun. Um, so it got really incredibly

00:51:50 --> 00:51:52 intensely active, was throwing off huge

00:51:52 --> 00:51:55 amounts of gas and dust. So that contributed

00:51:55 --> 00:51:57 again to more stuff to reflect sunlight. And

00:51:57 --> 00:51:59 also being nearer to the sun, the intensity

00:51:59 --> 00:52:01 of light reflecting off its higher as well.

00:52:01 --> 00:52:03 So kind of get a double whammy there. The

00:52:03 --> 00:52:05 other factor is how close they get to the

00:52:05 --> 00:52:07 Earth. So if you have two comets that are the

00:52:07 --> 00:52:09 same size and the same distance from the sun,

00:52:10 --> 00:52:11 and, um, one is closer to the Earth than the

00:52:11 --> 00:52:13 other, the one closer to the Earth will be

00:52:13 --> 00:52:15 brighter, but will also potentially be more

00:52:15 --> 00:52:17 spread out and more diffuse in the sky. So

00:52:17 --> 00:52:19 that brightness might be spread over a

00:52:19 --> 00:52:21 different area. You've then got

00:52:21 --> 00:52:24 subtleties of how dusty or gassy they are.

00:52:24 --> 00:52:27 Some comets, like Comet Pan, stars seem

00:52:27 --> 00:52:29 to be more gassy. Some comets like Church and

00:52:29 --> 00:52:31 Chan Atlas was more dusty. And that can have

00:52:31 --> 00:52:33 an impact on how they brighten. Bringing all

00:52:33 --> 00:52:35 this back together, though, for Comet Chu

00:52:35 --> 00:52:38 Chin Chan, at its closest to the sun,

00:52:38 --> 00:52:40 it will be a little bit further from the sun

00:52:40 --> 00:52:41 than the Earth, uh, is. So it's not like

00:52:41 --> 00:52:43 Comet McNaught that's going to get really

00:52:43 --> 00:52:46 close in. But one AU from the Sun's fairly

00:52:46 --> 00:52:48 respectable. It can still maintain a fairly

00:52:48 --> 00:52:49 decent level of activity at that distance.

00:52:49 --> 00:52:51 Comet Hale Bopp didn't get much closer than

00:52:51 --> 00:52:54 that and was fantastic. So that's in its

00:52:54 --> 00:52:56 favorite. It's going to get close enough in

00:52:56 --> 00:52:57 that you could get a decent level of

00:52:58 --> 00:53:01 activity. Also, because

00:53:01 --> 00:53:03 it's only going to get that close to the sun,

00:53:03 --> 00:53:04 it'll take a bit longer to pass through the

00:53:04 --> 00:53:06 inner solar system. Comets that get really

00:53:06 --> 00:53:08 close to the sun get traveling incredibly

00:53:08 --> 00:53:10 quickly at that point. So they tend to whip

00:53:10 --> 00:53:11 in and whip out fairly quickly. Whereas with

00:53:11 --> 00:53:14 cometary chinchan, it's going to hang around

00:53:14 --> 00:53:16 for a fair while. It is

00:53:16 --> 00:53:19 potentially quite a large cometary nucleus,

00:53:19 --> 00:53:22 but we don't know yet. This is the caution I

00:53:22 --> 00:53:24 give. If it turns out that we've caught it

00:53:24 --> 00:53:25 during an outburst, it may be a bit of a

00:53:25 --> 00:53:27 disappointment. If we've actually seen it as

00:53:27 --> 00:53:30 a bare nucleus. That augurs very, very

00:53:31 --> 00:53:33 well. What this all suggests is that Comet

00:53:33 --> 00:53:35 Chichin Shan, um, has a potential to be

00:53:35 --> 00:53:37 bright in late 2028.

00:53:38 --> 00:53:40 Depending on which fit to its current

00:53:40 --> 00:53:43 brightness you use. It could become barely

00:53:43 --> 00:53:45 naked eye visible, which is still pretty

00:53:45 --> 00:53:47 good. You know, we see 20 or 30 comets a year

00:53:48 --> 00:53:50 and very, uh, only maybe one will get to

00:53:50 --> 00:53:52 naked eye visibility. Or it could get as

00:53:52 --> 00:53:54 bright as the brightest stars. And if it gets

00:53:54 --> 00:53:56 as bright as the brightest stars, then it

00:53:56 --> 00:53:58 gets into great comet type territory.

00:53:59 --> 00:54:01 That's a factor of 100 difference in

00:54:01 --> 00:54:03 brightness between those two extremes. And,

00:54:03 --> 00:54:05 um, it could get brighter than the brightest

00:54:05 --> 00:54:06 extreme there or fainter than the faintest

00:54:06 --> 00:54:09 extreme. We just don't know yet. But having

00:54:09 --> 00:54:11 found it so early augurs well. But typically,

00:54:12 --> 00:54:14 predicting the next great comet is a fool's

00:54:14 --> 00:54:17 bargain until it's discovered. What we can

00:54:17 --> 00:54:20 say is that there are a few periodic comets

00:54:20 --> 00:54:23 that will be great in the future. Comet

00:54:23 --> 00:54:25 Hallie will be a lot better in 2061 than it

00:54:25 --> 00:54:28 was in 1986. In 1986, we had the

00:54:28 --> 00:54:30 worst separation of Comet Hallie for 2

00:54:30 --> 00:54:30 years.

00:54:30 --> 00:54:31 Andrew Dunkley: Tell me about it.

00:54:31 --> 00:54:34 Jonti Horner: Yeah, a bit disappointing. 2071

00:54:34 --> 00:54:35 will be better.

00:54:35 --> 00:54:38 Andrew Dunkley: Oh, good. I don't know if I'll be around by

00:54:38 --> 00:54:40 then, but, um, probably not.

00:54:40 --> 00:54:43 Jonti Horner: I'll be 99, make everybody

00:54:43 --> 00:54:45 feel really cheerful. It's now closer to

00:54:45 --> 00:54:47 Comet Hallie's next apparition than the last

00:54:47 --> 00:54:49 one. It turned around, I think, last year. So

00:54:49 --> 00:54:51 it's on its way back. Yeah, Comet Hallie will

00:54:51 --> 00:54:54 be even better in 21:35, will

00:54:54 --> 00:54:55 be really good that year. And that will be

00:54:55 --> 00:54:57 the best apparition for a couple of hundred

00:54:57 --> 00:55:00 years. Comet Swift Tuttle will be incredible

00:55:00 --> 00:55:02 in 21:26. We know that because we know pretty

00:55:02 --> 00:55:03 much exactly when it'll come back. We know

00:55:03 --> 00:55:05 where it will be compared to the Earth and

00:55:05 --> 00:55:07 the Sun. There is a suggestion that in

00:55:07 --> 00:55:10 2097 we may have the comet of the century, or

00:55:10 --> 00:55:12 close to it. This is research that came out

00:55:12 --> 00:55:15 last year. One of the greatest comets of the

00:55:15 --> 00:55:18 last thousand years was Comet De chezo, uh,

00:55:18 --> 00:55:21 in 1744, also called Comet

00:55:21 --> 00:55:23 Clinkenberg comet that is famous for having

00:55:23 --> 00:55:26 had six tails, incredibly bright, almost

00:55:26 --> 00:55:28 visible in broad daylight. A couple of

00:55:28 --> 00:55:30 astronomers, I think the lead researcher on

00:55:30 --> 00:55:33 this was Mike Meyer, published a paper last

00:55:33 --> 00:55:35 year that went back through historical

00:55:35 --> 00:55:38 observations and found a number of previous

00:55:38 --> 00:55:40 comets over the last 2 years that were

00:55:40 --> 00:55:42 all incredibly bright, really spectacular,

00:55:43 --> 00:55:45 but seem to have been moving the same as that

00:55:45 --> 00:55:47 comet. Linked them together and it's a very

00:55:47 --> 00:55:50 compelling tale that if their research is

00:55:50 --> 00:55:52 correct, that comet actually has an orbital

00:55:52 --> 00:55:55 period of just a little bit less. Just around

00:55:55 --> 00:55:57 450 years, I think. 400 years?

00:55:57 --> 00:56:00 No, 350 years. Wouldn't it do the mental

00:56:00 --> 00:56:03 arithmetic? Yeah, about 350 years,

00:56:03 --> 00:56:05 which means it should return in 2097.

00:56:06 --> 00:56:09 And if it does, it will be awesome.

00:56:09 --> 00:56:11 Um, sadly I don't think you or I will be

00:56:11 --> 00:56:12 around for that.

00:56:12 --> 00:56:14 Andrew Dunkley: Probably not, probably not.

00:56:14 --> 00:56:16 Jonti Horner: But things like that we can predict. But most

00:56:16 --> 00:56:18 Fred will be. But um, absolutely, Fred is

00:56:18 --> 00:56:20 indestructible and I'll stand um, by that.

00:56:21 --> 00:56:23 But most of the big cometary nuclei coming

00:56:23 --> 00:56:26 through are on such long period orbits, with

00:56:26 --> 00:56:28 the exception of Hallie and Swift Tuttle,

00:56:28 --> 00:56:30 that their apparitions are so infrequent that

00:56:30 --> 00:56:32 we've not identified them as periodic

00:56:32 --> 00:56:34 visitors. And many of them have periods of

00:56:34 --> 00:56:37 thousands or tens of thousands of years. So

00:56:37 --> 00:56:39 we typically only find them on their way in a

00:56:39 --> 00:56:42 few weeks or a few months before

00:56:42 --> 00:56:44 apparition. In case of Comet Hale Bopp, it

00:56:44 --> 00:56:47 was two years, which was exceptional at the

00:56:47 --> 00:56:49 time. Case of Comet Chichin Shan, it's more

00:56:49 --> 00:56:51 than two and a half years away, but our

00:56:51 --> 00:56:54 technology has improved hugely. So I don't

00:56:54 --> 00:56:56 think it's fair necessarily to say that

00:56:56 --> 00:56:59 Church and Chan will be another hell bop. But

00:56:59 --> 00:57:01 if you look at the brighter end of the

00:57:01 --> 00:57:02 predictions, it could be naked eye visible

00:57:02 --> 00:57:04 for three, four, five months.

00:57:04 --> 00:57:04 Andrew Dunkley: Wow.

00:57:04 --> 00:57:06 Jonti Horner: Would be awesome. And it would potentially be

00:57:06 --> 00:57:08 circumpolar for us in the Southern Hemisphere

00:57:08 --> 00:57:10 because at its closest to the center of the

00:57:10 --> 00:57:12 Earth, it's going to be way south, not going

00:57:12 --> 00:57:15 to be good for the Northern Hemisphere. But

00:57:15 --> 00:57:16 we can't really predict that. It's the same

00:57:16 --> 00:57:18 with meteor showers. We can predict the

00:57:18 --> 00:57:20 annual ones roughly how good they're going to

00:57:20 --> 00:57:23 be. And if you go back to when I was a

00:57:23 --> 00:57:25 kid, we couldn't really predict meteor

00:57:25 --> 00:57:27 storms, meteor outbursts, and that's one of

00:57:27 --> 00:57:28 the things people really love to see. So

00:57:28 --> 00:57:30 Geminids are great Northern Hemisphere,

00:57:30 --> 00:57:33 you'll see maybe even 80 or 100 an hour at

00:57:33 --> 00:57:35 their peak in the early hours of the morning.

00:57:35 --> 00:57:37 I've seen 50 an hour from our latitude near

00:57:37 --> 00:57:38 Brisbane.

00:57:38 --> 00:57:40 They're really good. But what people really

00:57:40 --> 00:57:42 want to see are meteor storms and they're

00:57:42 --> 00:57:45 much rarer. There's a few amazing ones.

00:57:45 --> 00:57:47 Historically. There was one in

00:57:47 --> 00:57:50 1833 that was linked to the Leonid meteor

00:57:50 --> 00:57:53 shower that had a rate in excess

00:57:53 --> 00:57:56 of a hundred thousand an hour, was best seen

00:57:56 --> 00:57:59 from the contiguous US and

00:57:59 --> 00:58:01 um, it was bright enough. There were

00:58:01 --> 00:58:04 sufficient meteors in the sky that miners in

00:58:04 --> 00:58:07 the US were woken from their campsites

00:58:07 --> 00:58:09 by the light shining through their tents. And

00:58:09 --> 00:58:11 people were convinced that the end times had

00:58:11 --> 00:58:14 come. The Apocalypse was here because he were

00:58:14 --> 00:58:16 getting as many as 20 meteors per second.

00:58:17 --> 00:58:17 Andrew Dunkley: Incredible.

00:58:17 --> 00:58:20 Jonti Horner: Um, now that in the way that kind of Tycho's

00:58:20 --> 00:58:23 observations in 1577 were probably the birth

00:58:23 --> 00:58:25 of modern cometary astronomy.

00:58:25 --> 00:58:28 1833, I think was possibly the birth of

00:58:28 --> 00:58:30 modern meteor astronomy. Because there'd been

00:58:30 --> 00:58:33 a storm from the Leonidas in 1799. People

00:58:33 --> 00:58:35 predicted that there might be another one in

00:58:35 --> 00:58:37 1866 because maybe this was happening every

00:58:37 --> 00:58:40 33 years when the comet came back. And indeed

00:58:40 --> 00:58:42 that happened in 1866.

00:58:43 --> 00:58:45 And so that was a bit like the birth of

00:58:45 --> 00:58:48 modern meteor science. And after that people

00:58:48 --> 00:58:50 said, well, there'll be one in 1899 and there

00:58:50 --> 00:58:52 wasn't. So that then tripped people up.

00:58:52 --> 00:58:55 So thanks to that we've gradually developed

00:58:55 --> 00:58:57 a better understanding of the physics of how

00:58:57 --> 00:59:00 meteor showers work. And I'm aware time is

00:59:00 --> 00:59:02 running away from us, but for people

00:59:02 --> 00:59:05 interested in this, in the run up to, uh, the

00:59:05 --> 00:59:08 heavily activity in 1999 through to

00:59:08 --> 00:59:10 2002, there was some amazing research

00:59:11 --> 00:59:13 done by um, David Asher

00:59:13 --> 00:59:16 from Amar Observatory and I think fondly on

00:59:16 --> 00:59:18 David because he was a lovely mentor to me

00:59:18 --> 00:59:20 when I visited Armagh in 1999. Very

00:59:20 --> 00:59:22 quiet guy, but incredibly talented

00:59:22 --> 00:59:25 scientists. And he did this remarkable

00:59:25 --> 00:59:28 work making predictions of when we would

00:59:28 --> 00:59:31 and wouldn't get Leonid storms by

00:59:31 --> 00:59:33 modeling the ejection of dust from the

00:59:33 --> 00:59:35 cometary nucleus and evolving the dust

00:59:35 --> 00:59:38 forward in time and go back. Way earlier on I

00:59:38 --> 00:59:40 mentioned these javelin spikes.

00:59:41 --> 00:59:43 He effectively modelled those and figured out

00:59:43 --> 00:59:45 where the spikes will be in a slight nudge up

00:59:45 --> 00:59:47 or down means that, uh, the Earth will run

00:59:47 --> 00:59:48 through the spike or not. And the great

00:59:48 --> 00:59:51 Leonid storms are produced by dust left

00:59:51 --> 00:59:54 behind just one or two revolutions ago. So

00:59:54 --> 00:59:56 the activity between 1999 and

00:59:56 --> 00:59:59 2002 resulted from a few different

00:59:59 --> 01:00:02 streams. The older they are, the more diffuse

01:00:02 --> 01:00:04 they get. But now we have the ability for

01:00:04 --> 01:00:06 comets we know well and meteor showers we

01:00:06 --> 01:00:08 know well to figure out where those spikes

01:00:08 --> 01:00:10 are roughly going to be how long they are

01:00:10 --> 01:00:13 and, uh, make predictions going forward. Now,

01:00:13 --> 01:00:15 there aren't any great meteor storms

01:00:15 --> 01:00:17 predicted in the relatively near future. The

01:00:17 --> 01:00:19 Leonids are not likely to give major storms

01:00:19 --> 01:00:22 in 2033 or 2066, but will give

01:00:22 --> 01:00:25 increased activity. The reason for that is

01:00:25 --> 01:00:27 Jupiter and Saturn are pulling those javelins

01:00:27 --> 01:00:29 around and making them miss the Earth.

01:00:30 --> 01:00:32 The leanings will probably return in force

01:00:32 --> 01:00:35 in, I think, 2097 with the possibility of a

01:00:35 --> 01:00:38 storm of like 20 an hour. But

01:00:38 --> 01:00:40 we're getting to understand that. So with

01:00:40 --> 01:00:42 meteor showers, we can predict the annual

01:00:42 --> 01:00:45 showers. They're very reliable. They

01:00:45 --> 01:00:46 gradually get better and worse with time as

01:00:46 --> 01:00:49 the streams move around and we intersect more

01:00:49 --> 01:00:51 of the material or less. But they're pretty

01:00:51 --> 01:00:54 reliable. Outbursts are harder

01:00:54 --> 01:00:56 to predict, but we're getting better at doing

01:00:56 --> 01:00:59 it. But predicting an

01:00:59 --> 01:01:00 outburst from a shower we've never seen

01:01:00 --> 01:01:03 before or a shower that's incredibly rare,

01:01:03 --> 01:01:06 we typically can't do until it happens

01:01:06 --> 01:01:08 because we need to have a feel for what it's

01:01:08 --> 01:01:10 done in the past. So we occasionally will get

01:01:10 --> 01:01:12 an outburst of a meteor shower we've never

01:01:12 --> 01:01:15 seen before. And you can't predict that. And

01:01:15 --> 01:01:17 that's when it's really exciting because then

01:01:17 --> 01:01:19 you can start to learn about a new meteor

01:01:19 --> 01:01:21 shower being born. You can learn about the

01:01:21 --> 01:01:23 comet that birthed it. It put all that

01:01:23 --> 01:01:24 together. And, um, that's one of the things

01:01:24 --> 01:01:26 where I'll go out and I love my meteor

01:01:26 --> 01:01:28 showers. I'll sit out under the sky and watch

01:01:28 --> 01:01:30 them. But I would love to just be outside

01:01:30 --> 01:01:31 when there's an unexpected outburst, when we

01:01:31 --> 01:01:33 see something new like a meteor shower being

01:01:33 --> 01:01:35 born for the first time.

01:01:35 --> 01:01:38 Andrew Dunkley: And, and that's what we recommend to all our

01:01:38 --> 01:01:40 Spacenads listeners. Uh, get up at 2 o' clock

01:01:40 --> 01:01:43 every morning, every day and go

01:01:43 --> 01:01:45 out and just wait and, you know, one day

01:01:45 --> 01:01:48 you'll get lucky. Might take 20 years, but it

01:01:48 --> 01:01:48 doesn't

01:01:48 --> 01:01:51 Jonti Horner: have to be 2:00am I mean, there is a little

01:01:51 --> 01:01:53 bit of a preference for meteor showers to be

01:01:53 --> 01:01:56 more active in the morning hours, in the

01:01:56 --> 01:01:57 evening hours. But that's purely a geometry

01:01:57 --> 01:01:59 thing. It's linked a little bit to the

01:01:59 --> 01:02:01 direction of the Earth's motion and the

01:02:01 --> 01:02:02 direction things are crossing the Earth's

01:02:02 --> 01:02:04 orbit in that if you think about something

01:02:04 --> 01:02:07 crossing the Earth's orbit at right angles to

01:02:07 --> 01:02:09 the Earth because the Earth's Moving forward

01:02:09 --> 01:02:12 at 30km a second, the direction you would see

01:02:12 --> 01:02:14 that coming from is actually a bit ahead of

01:02:14 --> 01:02:15 you because you've got the addition of the,

01:02:15 --> 01:02:17 the speed the debris is going on the speed

01:02:17 --> 01:02:20 the Earth's moving. So meteor showers

01:02:21 --> 01:02:24 that are uh, visible with radiance that will

01:02:24 --> 01:02:26 be in the morning sky, you've got a little

01:02:26 --> 01:02:27 bit of an additive effect between the speed

01:02:27 --> 01:02:29 the debris is going and the speed the Earth's

01:02:29 --> 01:02:32 moving, which means the average impact speed

01:02:32 --> 01:02:33 of the debris is higher and you get more

01:02:33 --> 01:02:36 meteors. But also you get this effect of

01:02:36 --> 01:02:37 the Earth's motion being a bit like you're

01:02:37 --> 01:02:40 driving into a snowstorm. You know, if you're

01:02:40 --> 01:02:42 driving into a snowstorm where there's no

01:02:42 --> 01:02:43 wind and the snowflakes are falling down

01:02:43 --> 01:02:45 vertically, vertically, you will perceive

01:02:45 --> 01:02:47 them as coming from in front of your car, not

01:02:47 --> 01:02:49 overhead. And so there's a preference for

01:02:49 --> 01:02:51 meteor showers to be slightly more likely to

01:02:51 --> 01:02:53 have activity that peaks in the morning hours

01:02:53 --> 01:02:55 in the evening. But that's not a guarantee.

01:02:55 --> 01:02:58 There are some meteor showers that are at the

01:02:58 --> 01:02:59 highest where the radiant culminates in the

01:02:59 --> 01:03:02 evening sky. It just depends. Some

01:03:03 --> 01:03:05 like the Utrecht, are only visible for a

01:03:05 --> 01:03:06 couple of hours before dawn. Um, there's even

01:03:06 --> 01:03:08 a few meteor showers that are daylight

01:03:08 --> 01:03:10 showers where the radiance only really above

01:03:10 --> 01:03:12 the horizon during the hours of daylight. And

01:03:12 --> 01:03:14 we know about them primarily from radio

01:03:14 --> 01:03:17 observations. Radar, well not radar. People

01:03:17 --> 01:03:20 listening to radio reflecting off the ionized

01:03:20 --> 01:03:22 streaks that the meteors leave in the

01:03:22 --> 01:03:24 ionosphere. That allows you to see over the

01:03:24 --> 01:03:27 horizon to radio sessions that are

01:03:27 --> 01:03:28 broadcasting that you don't normally get. So

01:03:28 --> 01:03:31 you can hear meteor showers? Yeah, so we know

01:03:31 --> 01:03:33 there are daytime showers that uh, we cannot

01:03:33 --> 01:03:35 see at night. And some of them are possibly

01:03:35 --> 01:03:37 as active as the Geminids of the Perseids.

01:03:37 --> 01:03:40 If, you know, if we could turn the sun off, I

01:03:40 --> 01:03:41 mean that would be a bad thing. Please don't

01:03:41 --> 01:03:43 do it. If you're a super villain listening,

01:03:43 --> 01:03:46 do not take this as an idea, but if we

01:03:46 --> 01:03:47 could turn the sun off and see there are a

01:03:47 --> 01:03:49 couple of meteor showers in the daytime that

01:03:49 --> 01:03:51 could be pretty spectacular.

01:03:52 --> 01:03:54 Andrew Dunkley: It is all very fascinating and I suppose the

01:03:54 --> 01:03:57 best advice would be to go and look for the,

01:03:58 --> 01:04:01 the better sources of forecasting rather than

01:04:01 --> 01:04:02 trying to figure it out for yourself.

01:04:02 --> 01:04:04 And uh, and, and you've mentioned a couple of

01:04:04 --> 01:04:07 already comet, uh, maps and, and uh,

01:04:07 --> 01:04:09 what was the other one about meteors?

01:04:09 --> 01:04:11 Jonti Horner: For meteors, I really strongly recommend the

01:04:11 --> 01:04:13 International Meteor Organization. If you go

01:04:13 --> 01:04:16 to their website, hover over the resources

01:04:16 --> 01:04:18 link, click on it to get the drop down. Click

01:04:18 --> 01:04:20 on meteor shower calendar. They have on the

01:04:20 --> 01:04:23 right hand side the best showers of the year

01:04:23 --> 01:04:25 with information and what the moon will be

01:04:25 --> 01:04:27 like. But there's also on the left side a PDF

01:04:27 --> 01:04:29 that you can download that goes into much

01:04:29 --> 01:04:31 more minute detail and talks about even the

01:04:31 --> 01:04:33 more minor showers. Um, and that's a very

01:04:33 --> 01:04:36 good point of truth for meteor showers. Well,

01:04:36 --> 01:04:38 I kind of describe them being like three

01:04:38 --> 01:04:40 tiers of meteor showers, ignoring the

01:04:40 --> 01:04:42 outbursts. There are the big three, which are

01:04:42 --> 01:04:44 the Quadrantids, the Persons and the

01:04:44 --> 01:04:47 Geminids, which are uh, even if you're not

01:04:47 --> 01:04:49 that interested at all in space, and if you

01:04:49 --> 01:04:51 are, thanks for listening to the podcast

01:04:51 --> 01:04:53 anyway, but it's not really our target

01:04:53 --> 01:04:55 audience. But even people who are not that

01:04:55 --> 01:04:57 interested, that's a spectacle you can go out

01:04:57 --> 01:04:58 and see with them and share with them them.

01:04:59 --> 01:05:00 Just make sure that you figure out when the

01:05:00 --> 01:05:02 radiant rises from your location because you

01:05:02 --> 01:05:05 don't want to turn people off by looking at a

01:05:05 --> 01:05:07 time when you can't see meteors. So for the

01:05:07 --> 01:05:10 Geminids the best time is around 2am but

01:05:10 --> 01:05:12 depending on where you are in the world, from

01:05:12 --> 01:05:15 our latitude you're looking at, you can't see

01:05:15 --> 01:05:17 any before 9:30, 10:00 clock at night.

01:05:17 --> 01:05:18 Obviously if you're somewhere with daylight

01:05:18 --> 01:05:20 savings in the southern hemisphere, add an

01:05:20 --> 01:05:23 hour to that. So for you down in New South

01:05:23 --> 01:05:24 Wales, where the clocks change, you're

01:05:24 --> 01:05:26 talking after 11pm for you. But if you're in

01:05:26 --> 01:05:29 Northern Europe, the Geminid radiant never

01:05:29 --> 01:05:31 sets. So where I grew up in the uk, as soon

01:05:31 --> 01:05:33 as it got dark I could see them. The rate

01:05:33 --> 01:05:35 still got better through the night. Similarly

01:05:35 --> 01:05:37 for the Perseids in particular. Perseids are

01:05:37 --> 01:05:40 a northern hemisphere only thing. It's light

01:05:40 --> 01:05:41 until quite late, certainly for the high

01:05:41 --> 01:05:43 northern latitudes like the uk, but as soon

01:05:43 --> 01:05:45 as it gets dark you can see them. So they're

01:05:45 --> 01:05:48 the showers that uh, are well worth going out

01:05:48 --> 01:05:50 to look at as a beginner and you just sit out

01:05:50 --> 01:05:52 there. I would figure out where the radiant

01:05:52 --> 01:05:55 is and look 30 or 40 degrees to the left or

01:05:55 --> 01:05:57 right of it to get the best balance between a

01:05:57 --> 01:06:00 lot of meteors but decent ones to see and

01:06:00 --> 01:06:03 just get a comfy chair, lie back, wrap up

01:06:03 --> 01:06:05 warm m with the people you love and tell

01:06:05 --> 01:06:07 stories and relax and occasionally you'll see

01:06:07 --> 01:06:08 something good and it's quite addictive. You

01:06:08 --> 01:06:10 think, you know, I'll go to bed, but I just

01:06:10 --> 01:06:12 want to see one more and then, well, that's

01:06:12 --> 01:06:14 rubbish. So uh, I want to see another one

01:06:14 --> 01:06:16 that's actually good. You've then got like

01:06:16 --> 01:06:19 the mid tier showers which can be decent but

01:06:19 --> 01:06:21 you need to be a bit more dedicated for these

01:06:21 --> 01:06:23 are the ones where you might see 10 or 15 an

01:06:23 --> 01:06:26 hour instead of 50 an hour. And I, um,

01:06:26 --> 01:06:27 wouldn't recommend people who were beginners

01:06:27 --> 01:06:29 go out and see them because it's, there's not

01:06:29 --> 01:06:32 enough happening. And that's why I worry

01:06:32 --> 01:06:34 about coverage for the April Lyrids, even in

01:06:34 --> 01:06:36 the Northern Hemisphere, because they're just

01:06:36 --> 01:06:39 not that good. If you're someone who's really

01:06:39 --> 01:06:41 keen, you'll enjoy them. But for most people

01:06:41 --> 01:06:43 there'll be a letdown and you don't want to

01:06:43 --> 01:06:45 turn people off the subject. Then there are

01:06:45 --> 01:06:48 the minor showers that you frankly need to be

01:06:48 --> 01:06:49 very obsessive to follow. And I've seen

01:06:49 --> 01:06:52 stories of a lot of the science of this has

01:06:52 --> 01:06:54 been done by amateur astronomers and, um,

01:06:54 --> 01:06:56 quite often by people who are quite obsessive

01:06:56 --> 01:06:59 about the topic. And I

01:06:59 --> 01:07:02 saw one guy who was in North America where it

01:07:02 --> 01:07:04 gets brutal, brutal cold in the winter,

01:07:05 --> 01:07:08 who built himself a, an insulated coffin with

01:07:08 --> 01:07:10 an incredibly transparent glass lid that he

01:07:10 --> 01:07:12 would carry out with him that was big enough

01:07:12 --> 01:07:14 for him to have a notebook and write down the

01:07:14 --> 01:07:17 details of every meteor he saw. He could lie

01:07:17 --> 01:07:19 out in minus 40 degrees and I think

01:07:19 --> 01:07:21 that's, um, units ambivalent. I think

01:07:21 --> 01:07:23 Fahrenheit and Centigrade are very similar at

01:07:23 --> 01:07:26 that point. But he's in an insulated box that

01:07:26 --> 01:07:28 keeps him warm and he'd lie out all night

01:07:28 --> 01:07:31 recording 2 meters, 3 meters an hour. That

01:07:31 --> 01:07:34 isn't for me, but it is for some people. But

01:07:34 --> 01:07:36 when you see a meteor shower with a ZHR of

01:07:36 --> 01:07:38 less than about 20, I'd probably leave that

01:07:38 --> 01:07:41 unless you're really keen. If it's got a zhr

01:07:41 --> 01:07:44 of 50 plus, well worth looking out for. But

01:07:44 --> 01:07:46 look for when the time of maximum is for most

01:07:46 --> 01:07:49 meteor showers, they've got what we call a

01:07:49 --> 01:07:51 full width half maximum of about 24 hours.

01:07:51 --> 01:07:54 What that means is that, uh, the rate only

01:07:54 --> 01:07:56 stays above half of the peak rate for about

01:07:56 --> 01:07:59 24 hours for 48 hours, then it'd stay above

01:07:59 --> 01:08:01 a quarter of the rate and so on. For the

01:08:01 --> 01:08:03 Quadrantids, it's full width at quarter

01:08:03 --> 01:08:06 maximum of about 12 hours. So that means

01:08:06 --> 01:08:08 if you're six hours away from the peak, the

01:08:08 --> 01:08:10 rate is already down to a quarter of that

01:08:10 --> 01:08:12 peak. It's a very sharp peak and if you're

01:08:12 --> 01:08:14 looking at the wrong time, the show won't be

01:08:14 --> 01:08:16 as good as you'd like it to be and you'll be

01:08:16 --> 01:08:17 disappointed.

01:08:18 --> 01:08:20 Andrew Dunkley: So much to consider, Jonti, but fascinating.

01:08:20 --> 01:08:22 Uh, copper and meteors.

01:08:22 --> 01:08:24 Um, there's so much to talk about and we

01:08:24 --> 01:08:27 probably didn't really cover absolutely

01:08:27 --> 01:08:29 everything. Although we did, uh, we did hit

01:08:29 --> 01:08:31 on quite a fair bit of info. And of course,

01:08:31 --> 01:08:34 we do welcome questions and comments. So, uh,

01:08:34 --> 01:08:36 please, um, go to our website and,

01:08:36 --> 01:08:39 um, click that little AMA button at

01:08:39 --> 01:08:41 the top and you can send us, uh, questions

01:08:41 --> 01:08:44 and comments, uh, in text and audio form.

01:08:44 --> 01:08:46 Don't forget to tell us who you are and where

01:08:46 --> 01:08:47 you're from, but we're going to wrap it up

01:08:47 --> 01:08:49 there. Jonti, thank you so much. We'll catch

01:08:49 --> 01:08:50 you on the next show.

01:08:50 --> 01:08:51 Jonti Horner: Thank you very much.

01:08:52 --> 01:08:54 Andrew Dunkley: Professor Jonti Horner, professor of

01:08:54 --> 01:08:57 Astrophysics at the University of Southern

01:08:57 --> 01:08:59 Queensland, our, uh, special, uh, guest

01:08:59 --> 01:09:02 commentator. While Fred's, uh, on the other

01:09:02 --> 01:09:04 side of the planet looking at meteors. And,

01:09:04 --> 01:09:07 uh, just a special word for, uh, for Huw in

01:09:07 --> 01:09:10 the studio. He's been a little unwell lately.

01:09:10 --> 01:09:12 Huw, get well soon, mate. We're all thinking

01:09:12 --> 01:09:15 of you. And from me, Andrew Dunkley. Thanks

01:09:15 --> 01:09:16 for your company. We'll catch you on the next

01:09:16 --> 01:09:18 episode of Space Nuts.

01:09:19 --> 01:09:21 Jonti Horner: You'll be listening to the Space Nuts

01:09:21 --> 01:09:24 podcast, available at

01:09:24 --> 01:09:26 Apple Podcasts, Spotify,

01:09:27 --> 01:09:29 iHeartRadio or your favorite podcast

01:09:29 --> 01:09:31 player. You can also stream on

01:09:31 --> 01:09:33 demand@bytes.com.

01:09:33 --> 01:09:35 Andrew Dunkley: this has been another quality podcast

01:09:35 --> 01:09:37 production from bytes.com.