Space Chronicles: Blue Origin’s Boom, The Case for Primordial Black Holes | Space Nuts:...
Space News TodayJune 12, 202600:38:1134.96 MB

Space Chronicles: Blue Origin’s Boom, The Case for Primordial Black Holes | Space Nuts:...

Sponsor Link:

This episode of Space Nuts is brought to you by NordVPN , your reliable partner for online security. To take advantage of our exclusive offer, including four extra months for free , visit www.nordvpn.com/spacenuts (https://www.nordvpn.com/spacenuts) .


Space Exploration: Blue Origin's Explosive Test and the Mysteries of the Universe In this thrilling episode of Space Nuts , hosts Andrew Dunkley and Professor Fred Watson reunite to discuss a range of captivating topics, including the recent explosive test of Blue Origin's New Glenn rocket, primordial black holes, and the ongoing debate around dark energy. Buckle up as we delve into the cosmos and explore these fascinating themes.

Episode Highlights:

- Blue Origin's Test Launch: The episode kicks off with an analysis of the dramatic Blue Origin test that resulted in an explosive incident at Cape Canaveral, raising questions about the future of the Artemis programme and the implications for upcoming lunar missions.

- Primordial Black Holes: Andrew and Fred Watson discuss a recent microlensing event observed in the Large Magellanic Cloud, exploring the possibility that the mysterious object, dubbed Phoebe, could be a primordial black hole, a concept first proposed by Stephen Hawking.

- Gravitational Microlensing Explained: The hosts break down the phenomenon of gravitational microlensing, illustrating how invisible objects can magnify the light of distant stars and what this means for our understanding of dark matter and the universe.

- Dark Energy: A Possible Furphy? A thought-provoking discussion ensues about the nature of dark energy, with insights from a recent paper suggesting that our current model of the universe may be oversimplified, raising the possibility that dark energy may not be necessary at all.


For more Space Nuts, including our continuously updating newsfeed and to listen to all our episodes, visit our website. (https://www.spacenutspodcast.com/) Follow us on social media at SpaceNutsPod on Facebook, Instagram, and more. We love engaging with our community, so be sure to drop us a message or comment on your favourite platform.

If you’d like to help support Space Nuts and join our growing family of insiders for commercial-free episodes and more, visit spacenutspodcast.com/about (https://www.spacenutspodcast.com/about) .

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


Become a supporter of this podcast: https://www.spreaker.com/podcast/space-nuts-astronomy-insights-cosmic-discoveries--2631155/support (https://www.spreaker.com/podcast/space-nuts-astronomy-insights-cosmic-discoveries--2631155/support?utm_source=rss&utm_medium=rss&utm_campaign=rss) .


- Blue Origin's Explosive Test

- Understanding Primordial Black Holes

- Gravitational Microlensing Phenomenon

- The Debate Around Dark Energy

- Implications for Future Space Exploration

Episode link: https://play.headliner.app/episode/33758087?utm_source=youtube

Kind: captions Language: en
00:00:02 --> 00:00:04 Hello again. Thank you for joining us.

00:00:04 --> 00:00:06 This is Space Nuts, where we talk

00:00:06 --> 00:00:09 astronomy and space science. My name is

00:00:09 --> 00:00:10 Andrew Dunley. Great to have your

00:00:10 --> 00:00:12 company. Well, you've probably been

00:00:12 --> 00:00:15 listening to Jonty for the last few

00:00:15 --> 00:00:18 weeks with Fred overseas, gallivanting

00:00:18 --> 00:00:22 as he does. He loves to gallivant. And

00:00:22 --> 00:00:24 he's back. And what we're going to talk

00:00:24 --> 00:00:26 about today, uh, all sorts of things.

00:00:26 --> 00:00:28 The Blue Origin blowout. You've probably

00:00:28 --> 00:00:31 seen the footage. Wow. Uh, primordial

00:00:31 --> 00:00:33 black holes, gravitational micro

00:00:33 --> 00:00:36 lensing, and is dark matter a fury.

00:00:36 --> 00:00:38 We'll deal with all of that today on

00:00:38 --> 00:00:40 Space Nuts.

00:00:40 --> 00:00:44 >> 15 seconds. Guidance is internal. 10 9g

00:00:44 --> 00:00:46 Ignition sequence start.

00:00:46 --> 00:00:47 >> Space nuts.

00:00:47 --> 00:00:52 >> 5 4 3 2 1 2 3 4 5 4 3 2 1

00:00:52 --> 00:00:53 >> Space Nuts.

00:00:53 --> 00:00:56 >> Astronauts report. It feels good.

00:00:56 --> 00:00:59 >> And he's back. and he's looking well.

00:00:59 --> 00:01:01 It's Professor Fred Watson, astronomer

00:01:01 --> 00:01:03 at large. Hello, Fred.

00:01:03 --> 00:01:04 >> Hello, Andrew. You're looking well, too.

00:01:04 --> 00:01:05 It's nice to see you.

00:01:05 --> 00:01:07 >> Yeah, it's good to see you, too. I mean,

00:01:08 --> 00:01:09 it's been a while for both of us

00:01:09 --> 00:01:12 because, uh, we had to do a lot of

00:01:12 --> 00:01:14 catchup episodes, but we didn't quite

00:01:14 --> 00:01:16 have enough time to cover everything, so

00:01:16 --> 00:01:17 we brought Jonty in.

00:01:17 --> 00:01:20 >> Uh, but he and I had to do catchup

00:01:20 --> 00:01:23 episodes to cover an absence of mine.

00:01:23 --> 00:01:26 So, um I haven't actually recorded with

00:01:26 --> 00:01:28 you for quite a while.

00:01:28 --> 00:01:30 >> Yes. Yeah. Must be a couple of months or

00:01:30 --> 00:01:30 so.

00:01:30 --> 00:01:32 >> Yeah, it would be. But it doesn't sound

00:01:32 --> 00:01:34 like that to the audience. Really?

00:01:34 --> 00:01:35 >> No, probably not.

00:01:35 --> 00:01:39 >> Yes. It's all witchery.

00:01:39 --> 00:01:41 >> Well, we Yeah, I think so. I think so.

00:01:41 --> 00:01:42 Yeah, there's at least two or three of

00:01:42 --> 00:01:43 them.

00:01:43 --> 00:01:44 >> Yeah. Okay, good.

00:01:44 --> 00:01:47 >> So, where did where did you go? You you

00:01:47 --> 00:01:48 were all over the place.

00:01:48 --> 00:01:51 >> Uh yes. So it was uh a conference in

00:01:51 --> 00:01:53 Germany that took me up to Europe and

00:01:53 --> 00:01:56 that that actually wasn't really

00:01:56 --> 00:01:59 interesting um because in fact I was

00:01:59 --> 00:02:01 going to Scotland before that. I had a

00:02:01 --> 00:02:03 week with my daughters in Scotland and

00:02:03 --> 00:02:05 then off to Germany. But the trip there

00:02:05 --> 00:02:08 of course um we can't fly through the

00:02:08 --> 00:02:10 Middle East at the moment because of the

00:02:10 --> 00:02:15 war going on there. And so my flight via

00:02:15 --> 00:02:17 via Dubai, they were long cancelled, but

00:02:17 --> 00:02:20 Marley managed to pull me a flight up to

00:02:20 --> 00:02:24 Seoul in Korea. And then on thin air

00:02:24 --> 00:02:27 from Soul over the North Pole, and I've

00:02:27 --> 00:02:29 actually got a certificate to prove that

00:02:29 --> 00:02:32 I've been over the North Pole. It's over

00:02:32 --> 00:02:34 there. I can't go and grab it, but

00:02:34 --> 00:02:36 >> uh and then into into Helsinki, and then

00:02:36 --> 00:02:40 yes, it was cold. Then then um uh across

00:02:40 --> 00:02:42 to Edinburgh. So the the polar flight

00:02:42 --> 00:02:43 was really interesting because we

00:02:43 --> 00:02:47 started off in Seoul in Korea uh and

00:02:47 --> 00:02:50 then you know took off uh with with Vin

00:02:50 --> 00:02:53 Air and I expected us to head towards

00:02:53 --> 00:02:56 the towards the west cuz that's what you

00:02:56 --> 00:02:59 do. Uh but no, we headed to the east.

00:02:59 --> 00:02:59 Wow.

00:03:00 --> 00:03:03 >> And we actually went up between Russia

00:03:03 --> 00:03:06 and America. So up the Bearing Straight.

00:03:06 --> 00:03:07 Wow.

00:03:07 --> 00:03:09 >> So, it went far enough east that you

00:03:09 --> 00:03:11 could turn north right up the bearing

00:03:11 --> 00:03:12 straight. So, you got Russia on one

00:03:12 --> 00:03:14 side, America on the other, and then

00:03:14 --> 00:03:17 over the North Pole uh with with a

00:03:17 --> 00:03:19 little Polar certificate to prove it.

00:03:19 --> 00:03:21 Nice touchdown in Helsinki. Yeah.

00:03:21 --> 00:03:23 >> Uh an hour or so there, then a nice

00:03:23 --> 00:03:25 flight over to Edinburgh. And there was

00:03:25 --> 00:03:28 with my daughter directly. It was great.

00:03:28 --> 00:03:31 >> Yeah. Fantastic. Um I've got an Arctic

00:03:31 --> 00:03:33 Circle certificate, I think.

00:03:33 --> 00:03:34 >> Yes, you will have. Yeah, I've got one

00:03:34 --> 00:03:35 of those as well, a North Cape

00:03:35 --> 00:03:36 certificate, in fact.

00:03:36 --> 00:03:38 >> Oh, yeah.

00:03:38 --> 00:03:40 >> Yeah. Um, but the conference I went to

00:03:40 --> 00:03:43 in Germany, uh, was, um, it was the 60th

00:03:44 --> 00:03:46 birthday conference of a colleague with

00:03:46 --> 00:03:48 whom I've worked very closely, uh, on

00:03:48 --> 00:03:50 the rave survey, which we've talked

00:03:50 --> 00:03:51 about before, the radio velocity

00:03:51 --> 00:03:54 experiment. Uh, Matias Steinmet's hair,

00:03:54 --> 00:03:57 Dr. Professor Matias Steinmets, uh, very

00:03:57 --> 00:03:59 senior German astronomer now. He, uh,

00:04:00 --> 00:04:01 led the project. I was the project

00:04:01 --> 00:04:03 manager. So we worked very closely

00:04:03 --> 00:04:05 together with a team of people most of

00:04:05 --> 00:04:07 whom were at the conference to celebrate

00:04:07 --> 00:04:10 his 60th birthday. So I was the sole

00:04:10 --> 00:04:12 Australian representative so they made a

00:04:12 --> 00:04:14 bit of a fuss of me which was nice. Uh I

00:04:14 --> 00:04:17 got the the kickoff talk and uh and they

00:04:17 --> 00:04:19 they looked after me. Uh so it was very

00:04:19 --> 00:04:21 very good and I I picked up a lot of

00:04:21 --> 00:04:24 what's happening currently in the field

00:04:24 --> 00:04:25 of science that we're doing. Well we

00:04:25 --> 00:04:26 might mention some of that a bit later

00:04:26 --> 00:04:27 on in the show.

00:04:27 --> 00:04:30 >> Sounds good. Uh my trip uh was a little

00:04:30 --> 00:04:32 closer to home, only a 9-hour flight

00:04:32 --> 00:04:35 away. We went to uh Vietnam for two and

00:04:35 --> 00:04:37 a half weeks. And uh people jokingly

00:04:37 --> 00:04:40 said to me, "Don't mention the war." But

00:04:40 --> 00:04:42 don't mention the war. M

00:04:42 --> 00:04:44 >> it's uh it's still very sensitive

00:04:44 --> 00:04:46 subject and and imagine

00:04:46 --> 00:04:48 >> what blew my mind and this will be of

00:04:48 --> 00:04:51 interest to um I suppose American

00:04:51 --> 00:04:53 listeners because of America's

00:04:53 --> 00:04:55 involvement in the Vietnam War but um

00:04:55 --> 00:04:57 there is still strong division between

00:04:58 --> 00:04:59 North and South

00:04:59 --> 00:05:02 >> and it hasn't been forgotten even 50

00:05:02 --> 00:05:05 years after it ended there's still very

00:05:05 --> 00:05:08 much focused on the aftermath of of that

00:05:08 --> 00:05:11 conflict

00:05:11 --> 00:05:12 >> I suppose just because it had it was

00:05:12 --> 00:05:14 such a defining time in their history.

00:05:14 --> 00:05:17 And uh I mean the Vietnam War was only a

00:05:17 --> 00:05:18 part of what they dealt with. They

00:05:18 --> 00:05:21 they'd been dealing with colonialism

00:05:21 --> 00:05:25 prior to that from France for for

00:05:25 --> 00:05:27 decades and decades.

00:05:27 --> 00:05:30 >> Uh so it's quite extraordinary. There

00:05:30 --> 00:05:34 was a a great uh documentary series I

00:05:34 --> 00:05:36 think it was on SPS in Australia called

00:05:36 --> 00:05:39 The Birth of a Nation. And uh one of our

00:05:39 --> 00:05:41 guides actually mentioned it and said,

00:05:41 --> 00:05:43 "We'd love to see it over here, but

00:05:43 --> 00:05:45 we're not allowed."

00:05:45 --> 00:05:46 >> Oh, interesting.

00:05:46 --> 00:05:49 >> So, I watched it and um I'm going to try

00:05:49 --> 00:05:50 and figure out how to get it to him, but

00:05:50 --> 00:05:52 I don't know. I don't know.

00:05:52 --> 00:05:52 >> We'll see.

00:05:52 --> 00:05:56 >> You could get You could run a foul of uh

00:05:56 --> 00:05:58 diplomatic nicities if you tried that.

00:05:58 --> 00:05:59 Who knows?

00:05:59 --> 00:06:01 >> Could do. Could do. Anyway,

00:06:01 --> 00:06:02 >> especially if you talk about it on a

00:06:02 --> 00:06:03 public podcast.

00:06:03 --> 00:06:07 >> Yeah, maybe like you are doing now. Am

00:06:07 --> 00:06:08 I?

00:06:08 --> 00:06:09 >> They're probably not allowed to watch

00:06:09 --> 00:06:11 this over in Vietnam either.

00:06:11 --> 00:06:13 >> Maybe not. Maybe not.

00:06:13 --> 00:06:14 >> It was funny though cuz I was posting

00:06:14 --> 00:06:17 posting uh some little videos. I like

00:06:17 --> 00:06:18 like to do little videos while I'm away

00:06:18 --> 00:06:20 and I was posting them on Tik Tok. I

00:06:20 --> 00:06:24 picked up 140 Vietnamese followers.

00:06:24 --> 00:06:26 >> Oh, that's fantastic.

00:06:26 --> 00:06:27 >> Yeah, I thought it was cool.

00:06:27 --> 00:06:29 >> There you go. That at least I can watch

00:06:29 --> 00:06:30 your Tik Tok stuff.

00:06:30 --> 00:06:33 >> Yeah. Yeah. Uh particularly the one I

00:06:33 --> 00:06:35 did at uh Harong Bay. It's beautiful

00:06:35 --> 00:06:37 part of the world. And I only did a

00:06:37 --> 00:06:40 60-second sort of 360 degree scan of the

00:06:40 --> 00:06:43 the place. But uh for some reason that

00:06:43 --> 00:06:45 video's gone nuts. It's uh at last count

00:06:45 --> 00:06:48 had 14 and a half thousand views.

00:06:48 --> 00:06:49 >> Whoa.

00:06:50 --> 00:06:52 >> I don't understand it, but uh yeah, that

00:06:52 --> 00:06:54 was nice.

00:06:54 --> 00:06:55 >> And we did all the other stuff. Train

00:06:55 --> 00:06:57 Street, you know, where the train runs

00:06:57 --> 00:06:59 next to the cafes in in um

00:06:59 --> 00:07:01 >> No, I didn't. Yeah. Yeah. It's very

00:07:01 --> 00:07:01 popular.

00:07:02 --> 00:07:03 >> Somewhere I should go.

00:07:03 --> 00:07:05 >> Yeah. uh up in Hanoi and uh many other

00:07:05 --> 00:07:07 places. I won't I won't bore people to

00:07:07 --> 00:07:09 tears with it. We got to get down to

00:07:09 --> 00:07:12 business. Uh our first topic, Fred, is

00:07:12 --> 00:07:16 very explosive. This is the um the the

00:07:16 --> 00:07:19 Blue Origin not launch that happened the

00:07:19 --> 00:07:21 other day. Uh in fact, I don't even

00:07:21 --> 00:07:23 think it got an inch off the ground

00:07:23 --> 00:07:25 before it went up in a beautiful um

00:07:26 --> 00:07:27 nuclear plume.

00:07:27 --> 00:07:29 >> It was very like a nuclear plume. And

00:07:29 --> 00:07:31 no, it wasn't actually meant to get off

00:07:31 --> 00:07:33 the ground. This was a fire test. So it

00:07:33 --> 00:07:35 was fired. All right.

00:07:35 --> 00:07:39 >> Yeah, it did. Uh it was um um Yes.

00:07:39 --> 00:07:42 Basically testing out the engines for

00:07:42 --> 00:07:44 for a launch that was forthcoming that

00:07:44 --> 00:07:47 was going to take a whole lot of sat uh

00:07:47 --> 00:07:50 telecommunication satellites

00:07:50 --> 00:07:53 uh up uh into orbit. Uh they were

00:07:53 --> 00:07:56 fortunately not on the rocket. Um I

00:07:56 --> 00:07:59 think there were uh the Amazon Leo uh

00:07:59 --> 00:08:01 satellites which is the what used to be

00:08:01 --> 00:08:04 called Kiper uh and is perhaps the

00:08:04 --> 00:08:07 principal com competitor potentially to

00:08:07 --> 00:08:10 Starink. Um uh anyway the satellites

00:08:10 --> 00:08:15 were not on the on the booster uh and uh

00:08:16 --> 00:08:19 it's basically was to test fire it seven

00:08:19 --> 00:08:21 engines. This is the new Glenn booster

00:08:21 --> 00:08:24 which is Blue Origin's heavy lift

00:08:24 --> 00:08:27 booster. It's not as heavy lift as the

00:08:27 --> 00:08:31 SpaceX uh super heavy uh booster that

00:08:31 --> 00:08:32 takes the Starship up.

00:08:32 --> 00:08:34 >> It's not lifting anything now, is it?

00:08:34 --> 00:08:38 >> Uh it's not. No. And uh what's it it's

00:08:38 --> 00:08:41 got sort of serious ramifications

00:08:41 --> 00:08:43 because not only did they blow up the

00:08:44 --> 00:08:45 rocket, they also blew up the launch

00:08:45 --> 00:08:48 pad. Uh effectively there's a lot of

00:08:48 --> 00:08:51 damage uh to the launchpad which is if I

00:08:51 --> 00:08:53 remember right, it is at Cape Canaveral.

00:08:53 --> 00:08:57 >> Yeah, I think so. Uh and um that uh

00:08:57 --> 00:08:59 explosion has caused damage that people

00:08:59 --> 00:09:02 are now talking about several months if

00:09:02 --> 00:09:05 not a year or so to repair. Uh and

00:09:06 --> 00:09:07 that's bad because that's the only

00:09:07 --> 00:09:09 facility in the world that can launch

00:09:09 --> 00:09:11 the new Glenn booster.

00:09:11 --> 00:09:13 >> And the new Glen booster is needed for

00:09:13 --> 00:09:17 the Arteimus program. Uh uh in

00:09:17 --> 00:09:20 particular uh later this year there was

00:09:20 --> 00:09:24 supposed to be a test launch of the

00:09:24 --> 00:09:27 their Blue Moon lander. This is Blue

00:09:27 --> 00:09:31 Origins Luna lander um which is the uh

00:09:31 --> 00:09:35 the um basically uh the competition if I

00:09:36 --> 00:09:38 can put it that way with the SpaceX

00:09:38 --> 00:09:41 Starship. So NASA contracted both SpaceX

00:09:41 --> 00:09:44 and Blue Origin to develop a lander,

00:09:44 --> 00:09:47 Luna lander for the moon. SP X has

00:09:47 --> 00:09:51 theirs based on the Starship. Um this

00:09:51 --> 00:09:53 what is it 4 to 50 m tall? It's

00:09:53 --> 00:09:54 colossal.

00:09:54 --> 00:09:56 >> Uh to land that on a rough surface on

00:09:56 --> 00:09:59 the moon, I'm not sure I'd be that keen

00:09:59 --> 00:10:02 on that, but never mind. uh the uh the

00:10:02 --> 00:10:06 Blue Origin version, the Blue uh Blue

00:10:06 --> 00:10:08 Moon as it's called. Uh that is only

00:10:08 --> 00:10:12 eight stories high. Uh so it's it's uh

00:10:12 --> 00:10:15 shorter. Uh but these two are both in

00:10:15 --> 00:10:17 the running to land the first astronauts

00:10:17 --> 00:10:20 on the lunar surface in 2028. Yeah. Uh

00:10:20 --> 00:10:23 so um there was going to be a test of uh

00:10:23 --> 00:10:27 the the U New Glenn heavy lifter lifting

00:10:27 --> 00:10:32 up a blue moon um landing vehicle uh a

00:10:32 --> 00:10:35 prototype landing vehicle uh into into

00:10:35 --> 00:10:36 orbit and actually to touch it down on

00:10:36 --> 00:10:38 the moon and that was supposed to happen

00:10:38 --> 00:10:40 this year. That's clearly off the agenda

00:10:40 --> 00:10:43 now. Yeah. Uh and so um it's not going

00:10:43 --> 00:10:44 to happen. Actually, it's a little bit

00:10:44 --> 00:10:47 sad because I've just read today that

00:10:47 --> 00:10:50 that Luna lander um which of course

00:10:50 --> 00:10:51 wasn't on board the rocket when it

00:10:51 --> 00:10:53 exploded has just passed with flying

00:10:53 --> 00:10:56 colors its environmental test. There's

00:10:56 --> 00:10:58 an environmental test that everything

00:10:58 --> 00:11:00 goes through. is in a huge vacuum

00:11:00 --> 00:11:04 chamber um which is a NASA facility

00:11:04 --> 00:11:08 uh and you can you can change the uh the

00:11:08 --> 00:11:11 temperature to match those huge extremes

00:11:11 --> 00:11:12 of temperature that you would get on the

00:11:12 --> 00:11:15 moon. Uh so there the their prototype

00:11:15 --> 00:11:18 lunar lander the blue moon mark1 which

00:11:18 --> 00:11:21 is called endurance which is a great

00:11:21 --> 00:11:23 name because that's not what's happened

00:11:23 --> 00:11:25 to the booster but endurance has passed

00:11:25 --> 00:11:27 with flying colors. Sadly, at the

00:11:27 --> 00:11:28 moment, there's nothing to take it into

00:11:28 --> 00:11:31 space. So, we'll have to see how that

00:11:31 --> 00:11:31 evolves.

00:11:31 --> 00:11:35 >> Yeah, I think you you and I spoke about

00:11:35 --> 00:11:37 NASA looking at other options other than

00:11:37 --> 00:11:40 SpaceX um not long before you you went

00:11:40 --> 00:11:45 away and um and and now this is kind of,

00:11:45 --> 00:11:47 >> for one of a better term, blown up in

00:11:47 --> 00:11:49 Blue Origin's face because that takes

00:11:49 --> 00:11:51 them off the table, doesn't it? Uh it

00:11:51 --> 00:11:54 seems to for a while unless they can do

00:11:54 --> 00:11:58 some very rapid repairs to the launch

00:11:58 --> 00:12:01 vehic uh the sorry the launch site

00:12:01 --> 00:12:03 >> uh the launch facility. So yeah it could

00:12:03 --> 00:12:06 push back. So the idea was that late

00:12:06 --> 00:12:09 next year uh there would be the Optimus

00:12:09 --> 00:12:12 3 flight which would consist of these

00:12:12 --> 00:12:15 two potential lunar landing vehicles. Um

00:12:16 --> 00:12:18 the Starship on Space X's side, the Blue

00:12:18 --> 00:12:21 Moon on Blue Origin side. They were both

00:12:21 --> 00:12:23 going to be launched into Earth orbit uh

00:12:24 --> 00:12:27 to have um rendevous tests uh to

00:12:27 --> 00:12:29 demonstrate that their viability. Uh

00:12:29 --> 00:12:32 when you link them to the space launch

00:12:32 --> 00:12:34 system, the the basically the Orion

00:12:34 --> 00:12:36 spacecraft, which is what took the

00:12:36 --> 00:12:38 Arteimus 2 astronauts around the moon,

00:12:38 --> 00:12:41 that will take Artemis 3, beg you

00:12:41 --> 00:12:44 pardon, Otimus 4 astronauts to the moon,

00:12:44 --> 00:12:46 but to land they've got to transfer into

00:12:46 --> 00:12:48 another spacecraft and land on the lunar

00:12:48 --> 00:12:52 surface. So all that I think is being

00:12:52 --> 00:12:54 thrown into question uh with this

00:12:54 --> 00:12:56 explosion. We will wait to see. It's

00:12:56 --> 00:12:57 still too early. We don't even know what

00:12:58 --> 00:13:01 caused it yet. Uh it's it was only uh

00:13:01 --> 00:13:04 less than a week ago as we as we speak.

00:13:04 --> 00:13:07 Uh it was so we don't actually know what

00:13:07 --> 00:13:09 the consequences are likely to be, but

00:13:09 --> 00:13:11 they could be quite serious for the

00:13:12 --> 00:13:13 Otimus program.

00:13:13 --> 00:13:16 >> Yeah. Uh, I mean, uh, I think Elon Musk

00:13:16 --> 00:13:19 calls these things, um, successful

00:13:19 --> 00:13:22 failures. I I don't know.

00:13:22 --> 00:13:24 >> A rapid unscheduled disintegration.

00:13:24 --> 00:13:26 >> Yes. I don't know what Jeff Bezos calls

00:13:26 --> 00:13:29 them, but um,

00:13:29 --> 00:13:30 >> yeah, hopefully they can get down to the

00:13:30 --> 00:13:32 bottom of it, but it Yeah, it does throw

00:13:32 --> 00:13:34 a spanner into the works. Maybe it was a

00:13:34 --> 00:13:35 spanner thrown into the works that

00:13:35 --> 00:13:38 caused the explosion. Who who knows? The

00:13:38 --> 00:13:40 the one good news story part of the

00:13:40 --> 00:13:43 story is nobody was injured.

00:13:43 --> 00:13:45 Yeah. Wow. Because it, you know, when

00:13:45 --> 00:13:46 you, as you said, it looked like a

00:13:46 --> 00:13:49 nuclear explosion. It was incredible.

00:13:49 --> 00:13:52 >> Uh, and um the so there was huge

00:13:52 --> 00:13:54 potential for injury there, but but

00:13:54 --> 00:13:55 everybody was accounted for.

00:13:56 --> 00:13:59 >> I I actually read today that some people

00:13:59 --> 00:14:02 who watched the explosion

00:14:02 --> 00:14:03 um this this sort of demonstrates how

00:14:03 --> 00:14:08 big and powerful it was took 37 seconds

00:14:08 --> 00:14:11 to feel the shock wave.

00:14:11 --> 00:14:13 >> Really? So they must have been a long

00:14:13 --> 00:14:13 way away.

00:14:13 --> 00:14:15 >> Yeah. But they could see it quite

00:14:15 --> 00:14:17 clearly. It was such a big explosion.

00:14:17 --> 00:14:19 But the shock wave took 37 seconds to

00:14:20 --> 00:14:20 reach

00:14:20 --> 00:14:23 >> there. That's amazing.

00:14:23 --> 00:14:26 >> Yeah. All right. Um so uh yeah, it it

00:14:26 --> 00:14:28 does sort of throw into question the

00:14:28 --> 00:14:31 future of Blue Origin um partnering with

00:14:31 --> 00:14:35 NASA for Artimus 3, but uh never write

00:14:35 --> 00:14:39 these people off. I've I've discovered

00:14:39 --> 00:14:42 >> we're not doing that. Um they will rise

00:14:42 --> 00:14:44 phoenix-l like from the ashes but it the

00:14:44 --> 00:14:46 question is how soon and what it will do

00:14:46 --> 00:14:47 to NASA's schedule.

00:14:47 --> 00:14:49 >> Exactly with Artemis. Yeah.

00:14:49 --> 00:14:51 >> More to come on that and you can read

00:14:51 --> 00:14:54 about it uh at the conversation website.

00:14:54 --> 00:14:56 This is Space Nuts. Andrew Dunley with

00:14:56 --> 00:15:00 Professor Fred Watson.

00:15:00 --> 00:15:01 Let's take a short break from the show

00:15:01 --> 00:15:04 to tell you about our sponsor NordVPN

00:15:04 --> 00:15:07 and to discuss your online privacy.

00:15:07 --> 00:15:09 Because let's face it, these days,

00:15:09 --> 00:15:11 whether you're browsing at home or

00:15:11 --> 00:15:14 jumping onto public Wi-Fi at a cafe or

00:15:14 --> 00:15:17 an airport or wherever, your data is

00:15:17 --> 00:15:19 constantly at risk. Hackers, trackers,

00:15:19 --> 00:15:21 even companies you've never heard of.

00:15:22 --> 00:15:23 They're all trying to get a piece of

00:15:23 --> 00:15:26 your digital life. And that's where

00:15:26 --> 00:15:30 NordVPN comes in. Uh our sponsor is

00:15:30 --> 00:15:32 fantastic. It's it's one I've been using

00:15:32 --> 00:15:35 for many years now myself and I have

00:15:36 --> 00:15:39 absolute faith in their product. NordVPN

00:15:39 --> 00:15:41 encrypts your internet connection, hides

00:15:41 --> 00:15:44 your IP address, and keeps your personal

00:15:44 --> 00:15:47 information safe from prying eyes. It's

00:15:47 --> 00:15:50 like uh putting an entire online world

00:15:50 --> 00:15:53 inside a secure tunnel. They've got over

00:15:53 --> 00:15:57 7 servers worldwide. You can browse

00:15:57 --> 00:16:01 fast, safely, and without restrictions.

00:16:01 --> 00:16:03 Plus, features like threat protection

00:16:03 --> 00:16:06 and ultraast speeds with Nord Links mean

00:16:06 --> 00:16:09 you're not sacrificing performance for

00:16:09 --> 00:16:12 security. You get both. Right now, you

00:16:12 --> 00:16:15 can grab our special space nuts deal and

00:16:15 --> 00:16:17 get 4 months extra for free. Plus,

00:16:17 --> 00:16:20 there's a 30-day money back guarantee.

00:16:20 --> 00:16:22 So, it's completely risk-f free to try.

00:16:22 --> 00:16:25 Just head along to our special URL,

00:16:25 --> 00:16:29 nordvpn.com/spacenuts.

00:16:29 --> 00:16:32 That's nordvpn.com/spacenuts.

00:16:32 --> 00:16:34 And don't forget to use the code

00:16:34 --> 00:16:41 spacenuts. That's nordvpn.com/spacenuts.

00:16:41 --> 00:16:45 Stay safe, stay private with nordvpn,

00:16:46 --> 00:16:47 our sponsor.

00:16:47 --> 00:16:49 >> Okay, we checked all four systems and

00:16:50 --> 00:16:50 with the go.

00:16:50 --> 00:16:51 >> Space Nuts

00:16:51 --> 00:16:55 >> now. And next story, Fred, uh, has a lot

00:16:55 --> 00:16:57 of moving parts as well. Nothing

00:16:57 --> 00:17:00 explosive, but uh, we're we're talking

00:17:00 --> 00:17:02 what primordial black holes and

00:17:02 --> 00:17:04 gravitational microlensing. Is that is

00:17:04 --> 00:17:05 that

00:17:05 --> 00:17:06 >> what it's about?

00:17:06 --> 00:17:08 >> It it's uh certainly the gravitational

00:17:08 --> 00:17:11 microlensing. Uh, what it means for

00:17:11 --> 00:17:14 primordial black holes, we remains to be

00:17:14 --> 00:17:16 seen, but uh, it's a good opportunity to

00:17:16 --> 00:17:18 talk about it and talk about the latest

00:17:18 --> 00:17:20 research on this. So, what's the story?

00:17:20 --> 00:17:23 Um on the night of the 18th of December

00:17:24 --> 00:17:26 2019,

00:17:26 --> 00:17:30 uh there was uh a microlensing event

00:17:30 --> 00:17:33 observed with a star in the large

00:17:33 --> 00:17:35 Melanic cloud, the the the nearest of

00:17:35 --> 00:17:38 our sort of largeish galactic neighbors,

00:17:38 --> 00:17:41 the um the the the satellite galaxy of

00:17:41 --> 00:17:44 our Milky Way, 165 light years away

00:17:44 --> 00:17:47 as the crow flies as far as I remember.

00:17:47 --> 00:17:50 So um what's a microlensing event? Well,

00:17:50 --> 00:17:53 something passes in front of a star. Uh,

00:17:53 --> 00:17:55 you can't actually see the something

00:17:55 --> 00:17:57 because it's too faint. You can see the

00:17:57 --> 00:18:00 light of the star. And you might think

00:18:00 --> 00:18:01 there's something passing in front of a

00:18:01 --> 00:18:04 star, it would dim the light of the

00:18:04 --> 00:18:07 star. But actually, if the geometry is

00:18:07 --> 00:18:08 right, in other words, if the if there's

00:18:08 --> 00:18:10 something that passes between you and

00:18:10 --> 00:18:12 the star is far enough away from the

00:18:12 --> 00:18:15 star, you get the opposite effect. the

00:18:15 --> 00:18:17 um distortion of the space around the

00:18:17 --> 00:18:20 invisible object uh actually acts as a

00:18:20 --> 00:18:23 magnifying glass and so you get a

00:18:23 --> 00:18:25 brightening of the light of the distant

00:18:25 --> 00:18:28 star. Uh and this is a phenomenon known

00:18:28 --> 00:18:30 as gravitational microlensing. It's well

00:18:30 --> 00:18:32 established, well observed. Uh there's a

00:18:32 --> 00:18:35 team in New Zealand which um is very

00:18:35 --> 00:18:38 very adept at these microlensing

00:18:38 --> 00:18:43 observations. Uh so um what we see when

00:18:43 --> 00:18:45 that happens is a rise in the brightness

00:18:45 --> 00:18:48 of the star and then a fall in the

00:18:48 --> 00:18:51 brightness of the background star uh

00:18:51 --> 00:18:54 which you we call a excuse me we call a

00:18:54 --> 00:18:56 light curve. It's the way the light

00:18:56 --> 00:18:58 changes over time. You can plot it out

00:18:58 --> 00:19:00 as a graph and it's got a very

00:19:00 --> 00:19:02 characteristic shape. It's a bit like a

00:19:02 --> 00:19:05 a rather elongated volcano. It's got a

00:19:05 --> 00:19:09 steady rise to a peak and then a rapid

00:19:09 --> 00:19:11 fall that falls away very like the

00:19:11 --> 00:19:14 flanks of a a volcano. So that's the

00:19:14 --> 00:19:17 sort of shape. So this uh was the event

00:19:17 --> 00:19:20 that was observed on the 18th of

00:19:20 --> 00:19:21 December.

00:19:21 --> 00:19:23 Can't remember which telescope it was

00:19:23 --> 00:19:27 used. Uh but we have a group of

00:19:27 --> 00:19:30 Australians who are directly involved

00:19:30 --> 00:19:35 with this. Uh so they the question is

00:19:35 --> 00:19:38 what was the object that passed in front

00:19:38 --> 00:19:39 of the star?

00:19:39 --> 00:19:41 >> Guess

00:19:41 --> 00:19:43 >> maybe a primordial black hole.

00:19:44 --> 00:19:47 >> Well that's that's the perhaps the most

00:19:47 --> 00:19:52 um provocative explanation. Uh they've

00:19:52 --> 00:19:53 given it a name this thing. They've

00:19:53 --> 00:19:55 called it Phoebe which is I think a

00:19:55 --> 00:19:59 lovely name actually. Um but uh the

00:19:59 --> 00:20:05 issue is it is kind of too small to be

00:20:05 --> 00:20:10 anything normal if you put it that way.

00:20:10 --> 00:20:15 >> Um so what are the possibilities? One is

00:20:15 --> 00:20:18 a what we sometimes call a rogue planet

00:20:18 --> 00:20:21 or a an orphan planet. Better known

00:20:21 --> 00:20:23 perhaps as a free floating planet. In

00:20:23 --> 00:20:26 other words, a planetary sized object.

00:20:26 --> 00:20:28 maybe something that's been ejected from

00:20:28 --> 00:20:31 its solar system or something that never

00:20:31 --> 00:20:33 gained enough mass to become a star and

00:20:33 --> 00:20:36 it's just sort of wandering uh through

00:20:36 --> 00:20:38 the galaxy. Uh there we know there are

00:20:38 --> 00:20:41 many of these things. Uh so that could

00:20:41 --> 00:20:44 be one of the uh one of the explanations

00:20:44 --> 00:20:48 for it. But uh the the issue is this

00:20:48 --> 00:20:53 thing has basically got a very very

00:20:53 --> 00:20:56 small mass. Uh it's only about three

00:20:56 --> 00:20:57 times the mass of the moon.

00:20:58 --> 00:20:58 >> Oh.

00:20:58 --> 00:21:01 >> Uh and that's kind of small for a

00:21:01 --> 00:21:06 planet. Uh so it suggests it's an object

00:21:06 --> 00:21:10 that is, you know, not a dwarf planet or

00:21:10 --> 00:21:11 sorry, a rogue planet or an orphan

00:21:12 --> 00:21:15 planet. Um and it points towards this

00:21:15 --> 00:21:19 much more exotic notion of a primordial

00:21:19 --> 00:21:22 black hole. Uh which you've kind of, you

00:21:22 --> 00:21:24 know, you've already flagged. Uh, and

00:21:24 --> 00:21:26 that's where it gets really exciting.

00:21:26 --> 00:21:29 So, primordial black holes, we've talked

00:21:29 --> 00:21:32 about them before. They were predicted

00:21:32 --> 00:21:36 by Steven Hawking. Um, they were

00:21:36 --> 00:21:38 predicted by him to have been a

00:21:38 --> 00:21:41 byproduct of the big bang. In other

00:21:41 --> 00:21:43 words, these are things that don't form

00:21:44 --> 00:21:46 from collapsing stars like the stellar

00:21:46 --> 00:21:50 mass black holes that we see, but from

00:21:50 --> 00:21:54 um well, basically um fluctuations in

00:21:54 --> 00:21:58 the density uh in the first few

00:21:58 --> 00:22:01 milliseconds after the big bang, the

00:22:01 --> 00:22:03 density of that hot medium. Uh, in other

00:22:03 --> 00:22:05 words, you know, if you could get these

00:22:05 --> 00:22:07 little spots that collapse

00:22:07 --> 00:22:10 instantaneously to become a black hole,

00:22:10 --> 00:22:12 what you'll produce in the big bang is

00:22:12 --> 00:22:15 not just time and space, but you litter

00:22:15 --> 00:22:18 it with these primordial black holes.

00:22:18 --> 00:22:21 And I think it's from Hawking's work

00:22:22 --> 00:22:24 that we assume that they can be any size

00:22:24 --> 00:22:27 you like. Um they can be you know

00:22:27 --> 00:22:30 perhaps uh super massive black holes

00:22:30 --> 00:22:31 which we know are the centers of

00:22:31 --> 00:22:36 galaxies uh or smaller than stellar mass

00:22:36 --> 00:22:38 black holes. And so by a stellar mass

00:22:38 --> 00:22:40 black hole we mean one that has a mass

00:22:40 --> 00:22:43 of about not too different from a star.

00:22:43 --> 00:22:45 In fact typically about five times the

00:22:45 --> 00:22:48 mass of the sun. Um and they are thought

00:22:48 --> 00:22:50 to have been caused by a star exploding

00:22:50 --> 00:22:52 at the end of its life. The core

00:22:52 --> 00:22:54 collapses. uh nothing will stop the

00:22:54 --> 00:22:55 collapse and it goes into becoming a

00:22:55 --> 00:22:58 black hole. But for a star to behave

00:22:58 --> 00:23:01 like that, it's got to be massive. It's

00:23:01 --> 00:23:03 got to be at least well five to 10 times

00:23:03 --> 00:23:06 the mass of the sun. Um so that does not

00:23:06 --> 00:23:09 account for things that are three times

00:23:09 --> 00:23:13 the mass of the moon. Uh but if you can

00:23:13 --> 00:23:16 have um if you can have primordial black

00:23:16 --> 00:23:21 holes of any mass then that makes Phoebe

00:23:21 --> 00:23:26 a very distinct candidate for a a

00:23:26 --> 00:23:28 primordial black hole. Um I might

00:23:28 --> 00:23:31 mention that the researchers who've done

00:23:31 --> 00:23:34 this uh work are at Swimburn University

00:23:34 --> 00:23:37 in Melbourne uh an university very

00:23:37 --> 00:23:40 active in its studies of actually most

00:23:40 --> 00:23:43 phenomena to do with our galaxy. Uh

00:23:43 --> 00:23:45 they've got some extremely talented

00:23:45 --> 00:23:46 scientists there some of whom I know

00:23:46 --> 00:23:47 quite well.

00:23:47 --> 00:23:51 >> Um so uh it's it's definitely a

00:23:51 --> 00:23:53 microlensing event. Something has caused

00:23:53 --> 00:23:56 this phenomenon. Uh the question is what

00:23:56 --> 00:23:57 is it?

00:23:58 --> 00:24:01 So let me um

00:24:01 --> 00:24:05 segue if I may to one of the talks at

00:24:05 --> 00:24:07 the conference that I was at in Germany.

00:24:07 --> 00:24:08 >> Yeah.

00:24:08 --> 00:24:11 >> Uh given by people who are well in this

00:24:11 --> 00:24:13 case it was a black hole specialist

00:24:13 --> 00:24:18 >> and he was saying that the the evidence

00:24:18 --> 00:24:24 for primordial black holes is growing.

00:24:24 --> 00:24:26 Uh and this is just one more example of

00:24:26 --> 00:24:29 it. this the the example of Phoebe here.

00:24:29 --> 00:24:32 Uh but he also said he thought this was

00:24:32 --> 00:24:36 the next big thing in black hole science

00:24:36 --> 00:24:40 uh to actually determine the reality of

00:24:40 --> 00:24:42 primordial black holes whether they are

00:24:42 --> 00:24:44 there or whether they're just a a wild

00:24:44 --> 00:24:48 prediction of of Professor Hawking. Um

00:24:48 --> 00:24:51 but he also made the comment the comment

00:24:51 --> 00:24:54 sorry not the comet he made the comment

00:24:54 --> 00:24:58 that uh it was his belief that the next

00:24:58 --> 00:25:00 Nobel Prize in astronomy or physics is

00:25:00 --> 00:25:03 is the way it goes would be the

00:25:03 --> 00:25:07 discovery of a primordial black hole. In

00:25:07 --> 00:25:08 other words

00:25:08 --> 00:25:11 finding absolutely rocksolid evidence

00:25:11 --> 00:25:13 that primordial black holes exist. Now,

00:25:13 --> 00:25:16 Phoebe is not that rockolid evidence

00:25:16 --> 00:25:18 because we've got multiple theories.

00:25:18 --> 00:25:20 >> Uh, yeah, multiple theories. It could

00:25:20 --> 00:25:24 even be uh, you know, a a lost satellite

00:25:24 --> 00:25:26 of a planet that's been chucked out of

00:25:26 --> 00:25:28 its solar system.

00:25:28 --> 00:25:30 >> So, it could be an object like the moon

00:25:30 --> 00:25:32 or Mercury or something like that.

00:25:32 --> 00:25:35 >> But that seems unlikely. Um, but and in

00:25:35 --> 00:25:38 fact, the um the, you know, the the

00:25:38 --> 00:25:40 primordial mass black hole idea I think

00:25:40 --> 00:25:43 is much more interesting. It's one that

00:25:43 --> 00:25:46 I'm sure will be looked at in detail.

00:25:46 --> 00:25:48 The problem with these gravitational

00:25:48 --> 00:25:50 micro lenting events, Andrew, is you

00:25:50 --> 00:25:52 only get one shot at it. You never see

00:25:52 --> 00:25:55 the object again. So Phoebe's basically

00:25:55 --> 00:25:57 never going to be seen again. All we've

00:25:57 --> 00:25:59 seen is the effect of it passing in

00:25:59 --> 00:26:00 front of a star.

00:26:00 --> 00:26:04 >> Yeah. Um, so, uh, what we've got to look

00:26:04 --> 00:26:07 for is other perhaps other similar

00:26:07 --> 00:26:10 phenomena, uh, or something that is an

00:26:10 --> 00:26:12 unequivocally a black hole but has a

00:26:12 --> 00:26:14 mass less than the sun. And we did talk

00:26:14 --> 00:26:18 about a candidate object uh, before we

00:26:18 --> 00:26:20 both went on our various surn. Uh, we

00:26:20 --> 00:26:22 did talk about an object like that. I'd

00:26:22 --> 00:26:24 need to look it up to find out what it

00:26:24 --> 00:26:26 was. But if, you know, if we can nail

00:26:26 --> 00:26:28 one of these things and say that is

00:26:28 --> 00:26:31 definitely what it is. Um, in fact, the

00:26:31 --> 00:26:33 object we talked about was the result of

00:26:33 --> 00:26:35 a, I think, a collision that was

00:26:35 --> 00:26:37 measured with gravitational waves. So,

00:26:37 --> 00:26:40 all this is perhaps pointing to the idea

00:26:40 --> 00:26:42 of primordial mass black holes. Somebody

00:26:42 --> 00:26:44 will nail it before too long and they'll

00:26:44 --> 00:26:47 probably get the Nobel Prize. Well, I

00:26:47 --> 00:26:49 suppose we shouldn't be surprised

00:26:49 --> 00:26:52 because in the past we've had theories

00:26:52 --> 00:26:54 about things existing and voila,

00:26:54 --> 00:26:57 suddenly we find an exoplanet and now we

00:26:57 --> 00:26:59 found thousands and thousands of them.

00:26:59 --> 00:27:01 So, it stands to reason that this is

00:27:01 --> 00:27:02 just another progression in that regard.

00:27:02 --> 00:27:04 We're

00:27:04 --> 00:27:06 >> the evidence is stacking up. We haven't

00:27:06 --> 00:27:09 confirmed one yet, but it sounds like

00:27:09 --> 00:27:12 it's going to happen. Yeah, I think

00:27:12 --> 00:27:14 that's right. I think we're on the track

00:27:14 --> 00:27:20 of uh a whole new regime of physics. And

00:27:20 --> 00:27:23 of course, uh primordial black holes are

00:27:23 --> 00:27:26 one potential candidate for dark matter.

00:27:26 --> 00:27:27 Mhm.

00:27:27 --> 00:27:33 >> Um, which was ruled out in the 1990s,

00:27:33 --> 00:27:35 maybe prematurely. It was ruled out

00:27:35 --> 00:27:38 because we didn't see a whole lot of

00:27:38 --> 00:27:40 these microlending events, which you'd

00:27:40 --> 00:27:42 expect to see if there was a lot of

00:27:42 --> 00:27:45 primordial mass black holes. Maybe it's

00:27:45 --> 00:27:46 just that we weren't looking hard enough

00:27:46 --> 00:27:47 that we missed them.

00:27:48 --> 00:27:48 >> Maybe.

00:27:48 --> 00:27:49 >> Um, yeah,

00:27:49 --> 00:27:51 >> I never look hard enough for anything.

00:27:51 --> 00:27:51 No.

00:27:51 --> 00:27:54 >> Well, well, that's cuz you're a you're a

00:27:54 --> 00:27:57 male. Yeah, you're a bloke and we don't

00:27:57 --> 00:27:59 we we look at something and we just

00:27:59 --> 00:28:00 don't see it.

00:28:00 --> 00:28:03 >> No. No.

00:28:03 --> 00:28:06 >> Which is, you know, not real good for

00:28:06 --> 00:28:07 human history because weren't we the

00:28:07 --> 00:28:09 hunters? Like we were supposed to be

00:28:09 --> 00:28:12 able to see stuff that quite

00:28:12 --> 00:28:15 >> Oh dear. Uh it's a a really fascinating

00:28:15 --> 00:28:18 story and I venture to say there'll be

00:28:18 --> 00:28:20 more on this in the not too distant

00:28:20 --> 00:28:21 future, but you can read about it uh

00:28:21 --> 00:28:23 great article about it on the

00:28:23 --> 00:28:25 universetoday.com

00:28:25 --> 00:28:28 website. You're listening to and

00:28:28 --> 00:28:30 possibly viewing space nuts with Andrew

00:28:30 --> 00:28:35 Dunley and Professor Fred Watson.

00:28:35 --> 00:28:37 >> Roger. Also,

00:28:37 --> 00:28:39 >> Space Nuts. Now, final story, Fred,

00:28:39 --> 00:28:42 intrigues me for one very good reason.

00:28:42 --> 00:28:44 It's one of the pet topics of our

00:28:44 --> 00:28:45 audience. We get a lot of questions

00:28:45 --> 00:28:50 about dark energy. But this s story pers

00:28:50 --> 00:28:53 the question, did we actually invent

00:28:53 --> 00:28:55 dark energy for nothing? Why are they

00:28:55 --> 00:28:58 suggesting that?

00:28:58 --> 00:28:59 >> Um,

00:28:59 --> 00:29:03 yeah, it's all mathematics.

00:29:03 --> 00:29:06 And I'd like just to refer uh listeners

00:29:06 --> 00:29:09 and viewers uh at the outset to a very

00:29:09 --> 00:29:14 nice article uh on this uh from um our

00:29:14 --> 00:29:17 much admired Universe Today uh website

00:29:17 --> 00:29:21 that's kind of an old friend of of um of

00:29:21 --> 00:29:23 Space Nuts, an article written by Mark

00:29:23 --> 00:29:27 Thompson uh which really very eloquently

00:29:27 --> 00:29:30 puts this story into perspective. And

00:29:30 --> 00:29:32 I'm I'm going to quote Mark. I hope he

00:29:32 --> 00:29:34 won't mind me doing that. Um it because

00:29:34 --> 00:29:37 he he introduces this uh this article by

00:29:37 --> 00:29:40 saying stand a pencil on its end and

00:29:40 --> 00:29:43 mathematically speaking it's perfectly

00:29:43 --> 00:29:44 balanced. Every force is accounted for

00:29:44 --> 00:29:47 and the equations are satisfied. And yet

00:29:47 --> 00:29:49 you already know what happens next, the

00:29:49 --> 00:29:51 slightest disturbance and it topples. A

00:29:51 --> 00:29:54 solution that exists on paper but can

00:29:54 --> 00:29:58 never survive contact with reality. In

00:29:58 --> 00:30:01 other words, um something that's stable

00:30:01 --> 00:30:05 but only stable briefly. Uh I think I'm

00:30:05 --> 00:30:07 paraphrasing what he's getting at with

00:30:07 --> 00:30:09 that. Yeah. Uh but just to read a little

00:30:09 --> 00:30:11 bit further uh from Mark's article,

00:30:11 --> 00:30:13 that's the image Blake Temple, a

00:30:13 --> 00:30:14 mathematician at the University of

00:30:14 --> 00:30:17 California, Davis, uses to describe our

00:30:17 --> 00:30:19 best model of the universe. And it's a

00:30:19 --> 00:30:22 deeply uncomfortable one. And so I think

00:30:22 --> 00:30:26 the way this story evolves is that yes

00:30:26 --> 00:30:28 we've uh for 30 years almost 30 years

00:30:28 --> 00:30:30 it's 1998

00:30:30 --> 00:30:33 when the accelerated expansion of the

00:30:33 --> 00:30:35 universe was discovered.

00:30:35 --> 00:30:36 >> Yeah.

00:30:36 --> 00:30:40 >> Uh by uh my colleague um Bradmitt and

00:30:40 --> 00:30:44 his uh uh his actually competitors over

00:30:44 --> 00:30:47 over the Pacific Soul Pul Muta and his

00:30:47 --> 00:30:49 team. uh they they jointly won the Nobel

00:30:49 --> 00:30:53 Prize in 2011 for that discovery that

00:30:53 --> 00:30:56 the um the accelerate the expansion of

00:30:56 --> 00:30:59 the universe is accelerating and so um

00:30:59 --> 00:31:02 the issue was to try and explain that

00:31:02 --> 00:31:05 and that's why dark energy was

00:31:05 --> 00:31:08 introduced as a as a concept uh an

00:31:08 --> 00:31:10 invisible

00:31:10 --> 00:31:13 outward pressure um that is part of

00:31:13 --> 00:31:16 space uh just pushes space and

00:31:16 --> 00:31:20 everything in it apart. part. Um and so

00:31:20 --> 00:31:23 that's where we get our idea of dark

00:31:23 --> 00:31:27 energy from. But um this um

00:31:27 --> 00:31:31 mathematician uh Blake Temple has said

00:31:32 --> 00:31:36 okay maybe we're taking too simplistic a

00:31:36 --> 00:31:41 view of all this. Uh and uh I think it's

00:31:41 --> 00:31:44 a group of uh of mathematicians led by

00:31:44 --> 00:31:46 Dr. Temple. uh they've got a paper in

00:31:46 --> 00:31:48 the proceedings of the Royal Society.

00:31:48 --> 00:31:49 You don't get papers in there if they're

00:31:49 --> 00:31:51 rubbish. So, no.

00:31:51 --> 00:31:52 >> Uh there's something to think about

00:31:52 --> 00:31:55 there. And they've actually uh

00:31:55 --> 00:31:58 mathematically demonstrated

00:31:58 --> 00:32:03 that our u model of the expansion of the

00:32:03 --> 00:32:07 universe with dark energy in it is

00:32:07 --> 00:32:11 unstable. Uh it's something that can't

00:32:11 --> 00:32:12 survive.

00:32:12 --> 00:32:16 Um and that's

00:32:16 --> 00:32:21 almost uh means that you can rule it out

00:32:21 --> 00:32:24 uh in the world of physics. Uh if you've

00:32:24 --> 00:32:27 got a solution that's unstable uh then

00:32:27 --> 00:32:30 it shouldn't it shouldn't happen. And so

00:32:30 --> 00:32:34 um what u uh Dr. Temple and his

00:32:34 --> 00:32:37 associates are proposing is that we've

00:32:37 --> 00:32:41 got it wrong. uh and that uh the model

00:32:41 --> 00:32:45 of the universe that we that we have

00:32:45 --> 00:32:49 which assumes that matter is basically

00:32:49 --> 00:32:50 spread throughout the universe. You know

00:32:50 --> 00:32:53 that the universe isotropic. It's the

00:32:53 --> 00:32:57 same in all directions. Uh is suggesting

00:32:57 --> 00:33:01 that that is also unstable.

00:33:01 --> 00:33:04 um and that really we have to take into

00:33:04 --> 00:33:06 account the fact that the universe isn't

00:33:06 --> 00:33:12 the same everywhere. Um it's uh it's I

00:33:12 --> 00:33:14 can't really go in deeply to the

00:33:14 --> 00:33:16 mathematics because I'm actually looked

00:33:16 --> 00:33:20 at the the the original paper. Um and so

00:33:20 --> 00:33:23 I haven't followed the mathematical

00:33:23 --> 00:33:26 um steps in the process. And between you

00:33:26 --> 00:33:28 and me, Andrew, I probably couldn't

00:33:28 --> 00:33:31 anyway even if I looked at the paper.

00:33:31 --> 00:33:33 I do remember what some of the equations

00:33:34 --> 00:33:36 that uh that govern this sort of thing

00:33:36 --> 00:33:37 look like. And I do remember the

00:33:37 --> 00:33:41 emotional response that my my psyche

00:33:41 --> 00:33:44 gets to them. But basically um what

00:33:44 --> 00:33:49 they're saying is that uh

00:33:49 --> 00:33:52 that accelerated expansion

00:33:52 --> 00:33:57 um is actually part of what Einstein

00:33:57 --> 00:34:01 suggested in the first place um without

00:34:01 --> 00:34:05 the need to invoke dark energy. Uh and

00:34:05 --> 00:34:09 it it's it's it's I'm simplifying I

00:34:09 --> 00:34:13 guess uh what um Mark the the author of

00:34:13 --> 00:34:15 this this article has written. Uh but

00:34:15 --> 00:34:19 the bottom line is that um our our um

00:34:19 --> 00:34:21 view of the universe on its largest

00:34:22 --> 00:34:26 scale is probably naive. It's probably

00:34:26 --> 00:34:29 we've perhaps oversimplified it and as a

00:34:29 --> 00:34:31 result of that we've come out with the

00:34:31 --> 00:34:34 wrong answer. Um, I might just

00:34:34 --> 00:34:36 >> That's a really big call though, isn't

00:34:36 --> 00:34:36 it?

00:34:36 --> 00:34:39 >> It's a huge call. Absolutely huge call.

00:34:39 --> 00:34:41 Uh,

00:34:41 --> 00:34:44 I I Let me just wind up with the last

00:34:44 --> 00:34:45 paragraph that uh

00:34:45 --> 00:34:47 >> Yeah, I was just looking at that myself

00:34:48 --> 00:34:49 >> because that's the Yeah, that Mark

00:34:49 --> 00:34:51 Thompson's written. I think it really

00:34:51 --> 00:34:54 sums it up. Dark energy has never felt

00:34:54 --> 00:34:56 entirely comfortable to many scientists.

00:34:56 --> 00:34:58 Einstein himself introduced something

00:34:58 --> 00:34:59 very like it, which he called his

00:34:59 --> 00:35:02 cosmological constant. then subsequently

00:35:02 --> 00:35:04 called it his biggest blunder. It was

00:35:04 --> 00:35:06 quietly resurrected in the 1990s when

00:35:06 --> 00:35:08 the data demanded it. That's when the

00:35:08 --> 00:35:11 accelerated expansion was discovered.

00:35:11 --> 00:35:13 Now the mathematics might be telling us

00:35:13 --> 00:35:15 it was never needed in the first place.

00:35:15 --> 00:35:17 The universe, it turns out, may be s

00:35:17 --> 00:35:21 stranger and simpler than we thought,

00:35:21 --> 00:35:23 only both at the same time. It's a great

00:35:23 --> 00:35:25 article. I encourage all our listeners

00:35:26 --> 00:35:27 to have a look at it. Yes, it's at the

00:35:28 --> 00:35:29 universitytoday.com

00:35:29 --> 00:35:32 website or you can read the paper at the

00:35:32 --> 00:35:34 proceedings of the Royal Society. But uh

00:35:34 --> 00:35:36 I dare say we haven't heard the last of

00:35:36 --> 00:35:38 this.

00:35:38 --> 00:35:39 >> Uh and what if what if we have got it

00:35:40 --> 00:35:43 wrong? What if dark energy is a fury? Um

00:35:43 --> 00:35:45 that that's the that's the big question.

00:35:45 --> 00:35:48 But uh they they seem to be

00:35:48 --> 00:35:50 >> ing towards the probability that it that

00:35:50 --> 00:35:52 it is in fact a fury.

00:35:52 --> 00:35:57 >> That that's right. Um, you know, uh,

00:35:57 --> 00:36:02 I suspect that, um, this theory, uh, if

00:36:02 --> 00:36:04 you, if you eliminate the need for dark

00:36:04 --> 00:36:06 energy, you might well eliminate the

00:36:06 --> 00:36:08 need for dark matter as well.

00:36:08 --> 00:36:11 >> Uh, or it might turn out to be

00:36:11 --> 00:36:12 primordial black holes. Look, we're

00:36:12 --> 00:36:16 we've covered two potential uh,

00:36:16 --> 00:36:18 solutions to the dark matter problem in

00:36:18 --> 00:36:21 this in this episode. Uh, nobody can

00:36:21 --> 00:36:23 accuse us of not addressing the big

00:36:23 --> 00:36:24 questions, Andrew.

00:36:24 --> 00:36:26 >> Absolutely. We just don't give them the

00:36:26 --> 00:36:26 big answers.

00:36:26 --> 00:36:28 >> We don't give them the answers. No,

00:36:28 --> 00:36:28 that's right.

00:36:28 --> 00:36:30 >> Leave that to somebody else

00:36:30 --> 00:36:31 >> because we don't know.

00:36:31 --> 00:36:33 >> No, we don't. No, we don't. But, uh, no,

00:36:33 --> 00:36:35 fascinating, fascinating story. Couple

00:36:35 --> 00:36:38 of fascinating stories. Uh, and it all

00:36:38 --> 00:36:39 started with a big bang called Blue

00:36:39 --> 00:36:40 Origin. Um,

00:36:40 --> 00:36:43 >> yes, it did. That's right. It was a huge

00:36:43 --> 00:36:43 bang.

00:36:43 --> 00:36:46 >> It was. Uh, that brings us to the end.

00:36:46 --> 00:36:48 Fred, thank you very much.

00:36:48 --> 00:36:50 >> It's a pleasure, Andrew. Always good to

00:36:50 --> 00:36:52 have a chat and uh bring to the

00:36:52 --> 00:36:54 forefront exactly what's happening in

00:36:54 --> 00:36:56 the deep depths of the universe.

00:36:56 --> 00:36:58 >> Indeed. And good to have you back too.

00:36:58 --> 00:37:00 Thank you. Professor Fred Watson,

00:37:00 --> 00:37:01 astronomer at large. Uh don't forget to

00:37:01 --> 00:37:04 visit us online at our website if you so

00:37:04 --> 00:37:06 desire. Uh spaceodcast.com.

00:37:06 --> 00:37:09 You can click on the AMA link at the top

00:37:09 --> 00:37:12 and ask us anything or ask u anybody

00:37:12 --> 00:37:14 anything really, but we always make

00:37:14 --> 00:37:15 comments. Uh you can sign up for the

00:37:16 --> 00:37:19 astron astronomy daily feed. Uh you can

00:37:19 --> 00:37:20 become a supporter if you so desire. And

00:37:20 --> 00:37:23 don't forget to leave uh reviews at your

00:37:23 --> 00:37:25 favorite podcasting platform. Wherever

00:37:25 --> 00:37:27 you listen to us, reviews are really

00:37:27 --> 00:37:29 useful, unless they're bad. But then

00:37:29 --> 00:37:30 again, there are some people who like

00:37:30 --> 00:37:32 bad because they want to see what all

00:37:32 --> 00:37:34 the fuss is about. Uh but don't do it.

00:37:34 --> 00:37:36 Don't you want to? I'm not going to tell

00:37:36 --> 00:37:38 you what to do. Um but anyway, that's

00:37:38 --> 00:37:41 it. And thanks to Hugh in the studio who

00:37:41 --> 00:37:42 couldn't be with us today because he's a

00:37:42 --> 00:37:44 fury. And from me, Andrew Dunley, thanks

00:37:44 --> 00:37:46 for your company on this edition. and

00:37:46 --> 00:37:48 we'll catch you on the next episode of

00:37:48 --> 00:37:50 Space Nuts. Bye-bye.

00:37:50 --> 00:37:51 >> Space Nuts.

00:37:51 --> 00:37:53 >> You've been listening to the Space Nuts

00:37:53 --> 00:37:56 podcast

00:37:56 --> 00:37:59 >> available at Apple Podcasts, Spotify,

00:37:59 --> 00:38:01 iHeart Radio, or your favorite podcast

00:38:01 --> 00:38:04 player. You can also stream on demand at

00:38:04 --> 00:38:06 bites.com. This has been another quality

00:38:06 --> 00:38:11 podcast production from byes.com.