Cosmic Winds, Nebula Secrets & the Mysteries of Neptune | Space Nuts: Exploring the Cosmos
Space News TodayApril 03, 202500:46:0442.18 MB

Cosmic Winds, Nebula Secrets & the Mysteries of Neptune | Space Nuts: Exploring the Cosmos

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Space Nuts Episode 509: Neptune's Secrets, Lunar Dust Shields, and the Helix Nebula

In this exciting episode of Space Nuts, fill-in host Heidi Campo joins astronomer Fred Watson to explore some of the cosmos' most intriguing phenomena. From the latest discoveries about Neptune's atmosphere to innovative solutions for lunar dust challenges, and the mysteries of the Helix Nebula, listeners are in for a treat filled with cosmic insights and engaging discussions.

Episode Highlights:

- Neptune's Atmosphere: Heidi and Fred dive into the recent observations made by the James Webb Space Telescope, revealing the presence of auroras on Neptune and discussing its unique atmospheric conditions, including record-breaking winds and intriguing cloud formations.

- Lunar Dust Shield Innovations: The duo explores NASA's new Electrodynamic Dust Shield, designed to repel lunar regolith, and its potential applications for future lunar missions and even everyday life on Earth.

- Helix Nebula Mysteries: The episode wraps up with a discussion about the Helix Nebula, its stunning visuals, and the fascinating theory surrounding the remnants of a planet that was destroyed as its star transitioned into a white dwarf.

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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.

(00:00) Welcome to Space Nuts with Heidi Campo and Fred Watson

(01:40) Discussion on Neptune's auroras and atmospheric conditions

(11:20) The innovative Electrodynamic Dust Shield for lunar missions

(22:15) Exploring the Helix Nebula and its planetary ghost

(30:00) Final thoughts and reflections on space exploration

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Episode link: https://play.headliner.app/episode/26428218?utm_source=youtube

Kind: captions Language: en
00:00:00 --> 00:00:04 welcome to Space Nuts my name is Heidi

00:00:04 --> 00:00:06 Compo and I'm here with Fred Watson

00:00:06 --> 00:00:09 astronomer at large and I bet many of

00:00:09 --> 00:00:11 you are wondering who is this lady why

00:00:11 --> 00:00:14 is she here where is Andrew i can assure

00:00:14 --> 00:00:16 you he is just fine and probably having

00:00:16 --> 00:00:19 the time of his life i am here filling

00:00:19 --> 00:00:22 in helping him out while he is on a

00:00:22 --> 00:00:26 little break and I I found safe space

00:00:26 --> 00:00:28 originally from just being a listener

00:00:28 --> 00:00:31 myself i also have a podcast Reality

00:00:31 --> 00:00:33 Check: The Science of Fiction where I

00:00:33 --> 00:00:35 talk to subject matter experts about the

00:00:35 --> 00:00:39 plausibility of sci-fi concepts and I am

00:00:39 --> 00:00:42 a graduate student here in space city

00:00:42 --> 00:00:45 Houston Texas and I'm focusing on

00:00:45 --> 00:00:48 spaceflight human optimization and

00:00:48 --> 00:00:51 performance so I have a very interesting

00:00:51 --> 00:00:54 segue into the space world i'm really

00:00:54 --> 00:00:57 interested in a lot of the I guess the

00:00:57 --> 00:01:00 sci-fi concepts that integrate into

00:01:00 --> 00:01:02 space science and all the new

00:01:02 --> 00:01:04 discoveries that Fred knows so much

00:01:04 --> 00:01:08 about and I'm excited to be here as your

00:01:08 --> 00:01:11 fillin host for this episode 15 seconds

00:01:11 --> 00:01:15 guidance is internal 10 9 ignition

00:01:15 --> 00:01:20 sequence start space nets 5 4 3 2 1 2 3

00:01:20 --> 00:01:24 4 5 5 4 3 2 1 Space nuts astronauts

00:01:24 --> 00:01:27 report it feels good fred thanks for

00:01:27 --> 00:01:30 having me uh you're very welcome Heidi

00:01:30 --> 00:01:33 uh it's a delight to welcome you to the

00:01:33 --> 00:01:37 Space Nuts team uh it's very appropriate

00:01:37 --> 00:01:38 I think that we should be beaming

00:01:38 --> 00:01:41 beaming out from Houston Texas uh and

00:01:41 --> 00:01:44 what better person to fit into Andrew's

00:01:44 --> 00:01:46 empty shoes at the moment than yourself

00:01:46 --> 00:01:49 uh it's uh lovely to have you and I'm

00:01:49 --> 00:01:51 really looking forward to our our next

00:01:51 --> 00:01:53 few sessions when we can chat together

00:01:53 --> 00:01:56 behind Andrew's back

00:01:56 --> 00:01:59 no this is going to be great so we have

00:01:59 --> 00:02:02 some really interesting topics this week

00:02:02 --> 00:02:04 i was looking over them um we're going

00:02:04 --> 00:02:07 to be talking about the blue ghost uh

00:02:07 --> 00:02:10 sojourn on Mars or sorry on the moon and

00:02:10 --> 00:02:13 that looked really interesting to me the

00:02:13 --> 00:02:14 other thing we're going to be talking

00:02:14 --> 00:02:17 about is some of the activity with the

00:02:17 --> 00:02:21 James Webb telescope about Neptune so

00:02:21 --> 00:02:23 that's a planet we really don't talk as

00:02:23 --> 00:02:26 much about neptune is really kind of the

00:02:26 --> 00:02:28 ignored stepchild of the solar system so

00:02:28 --> 00:02:30 I'm excited to hear what you have to say

00:02:30 --> 00:02:32 about that activity and then the last

00:02:32 --> 00:02:34 thing we'll be talking today about today

00:02:34 --> 00:02:39 is the Helix Nebula and some really

00:02:39 --> 00:02:42 exciting new discoveries going on with

00:02:42 --> 00:02:46 that so I think that I would be

00:02:46 --> 00:02:49 interested in just jumping right in with

00:02:49 --> 00:02:54 the Neptune story

00:02:54 --> 00:02:57 excellent um a good planet to start with

00:02:57 --> 00:03:00 Heidi uh and you're absolutely right um

00:03:00 --> 00:03:04 Neptune has only been visited by once by

00:03:04 --> 00:03:07 um you know a human-built spacecraft

00:03:07 --> 00:03:09 maybe there were alien spacecraft that

00:03:09 --> 00:03:11 have visited it but only one human built

00:03:11 --> 00:03:15 one uh which was Voyager 2 uh and um so

00:03:15 --> 00:03:18 what we know about it really comes very

00:03:18 --> 00:03:20 much from the images that were taken

00:03:20 --> 00:03:23 when Voyager 2 flew by Neptune that was

00:03:23 --> 00:03:27 in the 80s uh but Neptune of course is a

00:03:27 --> 00:03:30 world that has an active atmosphere it's

00:03:30 --> 00:03:31 an ice giant one of the two ice giants

00:03:32 --> 00:03:34 in the uh in the outer solar system and

00:03:34 --> 00:03:37 and that term refers to the fact that we

00:03:37 --> 00:03:40 believe there are solid ices as a kind

00:03:40 --> 00:03:43 of haze in the atmosphere of Neptune um

00:03:43 --> 00:03:45 so it's slightly different from the

00:03:45 --> 00:03:49 other two gas giants uh Jupiter uh and

00:03:49 --> 00:03:52 Saturn which are they they don't have

00:03:52 --> 00:03:53 those icy hazes because their

00:03:53 --> 00:03:56 temperature is just slightly warmer uh

00:03:56 --> 00:03:59 being nearer the sun um so the really

00:03:59 --> 00:04:02 interesting thing was when uh the flyby

00:04:02 --> 00:04:06 uh with Voyager 2 took place um Neptune

00:04:06 --> 00:04:09 looked very boring uh it had a you know

00:04:09 --> 00:04:12 it was just like a a pale blue green

00:04:12 --> 00:04:15 disc with not much happening uh and I

00:04:15 --> 00:04:17 think that probably did it a disservice

00:04:17 --> 00:04:19 because we've you know we thought of

00:04:20 --> 00:04:22 this planet as having rather

00:04:22 --> 00:04:24 uninteresting atmospherics although

00:04:24 --> 00:04:26 subsequent measurements made from earth

00:04:26 --> 00:04:30 actually uh demonstrated that it does

00:04:30 --> 00:04:33 have high winds in its atmosphere uh and

00:04:33 --> 00:04:36 just a mention to uh the the the system

00:04:36 --> 00:04:39 of moons of Neptune because uh some of

00:04:39 --> 00:04:41 those are particularly interesting as

00:04:41 --> 00:04:44 well triton is its largest moon it may

00:04:44 --> 00:04:47 well be one of these ice worlds with a

00:04:47 --> 00:04:50 uh with a rocky core an overlying ocean

00:04:50 --> 00:04:53 a global ocean and ice on top but that's

00:04:53 --> 00:04:55 not what we're talking about today uh so

00:04:56 --> 00:04:59 so uh what's the story why is Neptune in

00:04:59 --> 00:05:02 the news well it it's because as you

00:05:02 --> 00:05:04 might expect it has been a subject of

00:05:04 --> 00:05:08 observation by uh basically astronomy's

00:05:08 --> 00:05:12 new toy still new after 3 years I guess

00:05:12 --> 00:05:15 now uh the James Web Space Telescope um

00:05:15 --> 00:05:18 with its marvelous infrared cameras uh

00:05:18 --> 00:05:21 and very very sensitive spectroscopic

00:05:21 --> 00:05:26 systems so what has been uh detected by

00:05:26 --> 00:05:29 the web is something that we've known

00:05:30 --> 00:05:33 about uh maybe hinted at uh by earlier

00:05:33 --> 00:05:37 observations over a long period of time

00:05:37 --> 00:05:39 uh probably since those the the Voyager

00:05:39 --> 00:05:43 flyby uh that um it has aurori or

00:05:43 --> 00:05:46 auroras if you want to be less uh pick

00:05:46 --> 00:05:49 um picky about your Latin uh aurori um

00:05:49 --> 00:05:51 northern and southern light like we have

00:05:51 --> 00:05:54 on Earth like the other gas giants

00:05:54 --> 00:05:57 themselves have uh but the problem is

00:05:57 --> 00:06:00 you know uh hints are fine but what you

00:06:00 --> 00:06:03 really want is a kind of signature of

00:06:03 --> 00:06:05 these things in the spectrum the the

00:06:05 --> 00:06:09 sort of rainbow of colors that we see uh

00:06:09 --> 00:06:11 when we split the light up uh into into

00:06:11 --> 00:06:14 those components and that as we've

00:06:14 --> 00:06:16 discussed many times on space nuts those

00:06:16 --> 00:06:20 spectra are crossed by a kind of almost

00:06:20 --> 00:06:24 like a a you know a supermarket barcode

00:06:24 --> 00:06:26 uh of information which we can read and

00:06:26 --> 00:06:29 detect what gases are involved with

00:06:29 --> 00:06:33 these with these spectral colors so uh

00:06:33 --> 00:06:36 yes the James Web has thrown its might

00:06:36 --> 00:06:39 behind observations of Neptune and sure

00:06:39 --> 00:06:43 enough we have found strong emission uh

00:06:43 --> 00:06:47 of the the kind of telltale elements uh

00:06:47 --> 00:06:50 that indicate auroral activity and

00:06:50 --> 00:06:53 remember uh aurora are caused by the the

00:06:53 --> 00:06:55 the solar particles the subatomic

00:06:55 --> 00:06:57 particles that come from the sun

00:06:57 --> 00:06:59 interacting with the atmosphere of a

00:06:59 --> 00:07:01 planet that's what causes the glow and

00:07:01 --> 00:07:02 that's why it has characteristic colors

00:07:02 --> 00:07:05 because the glow itself comes from the

00:07:05 --> 00:07:08 elements in the atmosphere so yes aurori

00:07:08 --> 00:07:12 on Neptune uh and very similar to the

00:07:12 --> 00:07:15 phenomenon on earth but different colors

00:07:15 --> 00:07:17 uh because it's different elements that

00:07:17 --> 00:07:20 are being excited the green in in Aurori

00:07:20 --> 00:07:22 here on Earth comes from oxygen uh which

00:07:22 --> 00:07:25 isn't there on Neptune so the colors are

00:07:26 --> 00:07:27 coming from they're actually coming from

00:07:27 --> 00:07:29 hydrogen

00:07:29 --> 00:07:30 yeah it's absolutely beautiful i'm

00:07:30 --> 00:07:32 looking at these images right now it

00:07:32 --> 00:07:34 reminds me of one of those uh mood rings

00:07:34 --> 00:07:36 that were really popular in the '9s

00:07:36 --> 00:07:39 where it starts to change color it's uh

00:07:39 --> 00:07:41 really spectacular to see and I'm seeing

00:07:41 --> 00:07:43 in this image so you you just described

00:07:43 --> 00:07:46 that the greenish color comes from um

00:07:46 --> 00:07:50 hydrogen i'm seeing also spots of white

00:07:50 --> 00:07:53 cuz if you look at the images of Hubble

00:07:53 --> 00:07:55 which it's pretty much just blue all the

00:07:55 --> 00:07:58 way across and then the image of the web

00:07:58 --> 00:08:00 um there's some big white spots is that

00:08:00 --> 00:08:05 part of the aura um I suspect um some of

00:08:05 --> 00:08:08 those are clouds uh which are also now

00:08:08 --> 00:08:11 visible in the infrared we see similar

00:08:11 --> 00:08:13 things on uh in the atmosphere of Uranus

00:08:13 --> 00:08:17 white spots which are um very extensive

00:08:17 --> 00:08:20 areas of cloud in the atmosphere um the

00:08:20 --> 00:08:23 the atmospheric circulation um you know

00:08:23 --> 00:08:26 on on both those ice giants Uranus and

00:08:26 --> 00:08:29 Neptune is relatively slow in terms of

00:08:30 --> 00:08:33 the uh the changes in the atmosphere and

00:08:33 --> 00:08:34 that's partly because the temperature

00:08:34 --> 00:08:39 there is - 214° C at the surface but

00:08:39 --> 00:08:41 that doesn't um necessarily mean that

00:08:41 --> 00:08:43 you don't get high winds and in fact um

00:08:43 --> 00:08:48 it I think uh the winds on Neptune uh

00:08:48 --> 00:08:50 are the record-breaking winds in the

00:08:50 --> 00:08:51 atmosphere of a planet in the solar

00:08:51 --> 00:08:55 system up to 2 kilometers per hour

00:08:55 --> 00:08:59 um that's what's that that's about 18 uh

00:08:59 --> 00:09:03 1 miles hour so it's that's very

00:09:03 --> 00:09:04 fast i'm thinking of it in hurricane

00:09:04 --> 00:09:07 terms yeah it's super hurricane that's

00:09:07 --> 00:09:10 right um and I think um that there is

00:09:10 --> 00:09:14 also uh on Neptune there is a something

00:09:14 --> 00:09:17 that's sort of related to the great red

00:09:17 --> 00:09:21 spots on Jupiter a storm a long lived

00:09:21 --> 00:09:23 storm and maybe that's what's showing up

00:09:23 --> 00:09:26 as the some of the white spots or at

00:09:26 --> 00:09:27 least one of the white spot i'm just

00:09:27 --> 00:09:29 looking for them now there is a big

00:09:29 --> 00:09:31 white spot in the middle of the um the

00:09:31 --> 00:09:35 JWST images uh but I think the poles is

00:09:35 --> 00:09:38 the aurora and you've just reminded me

00:09:38 --> 00:09:39 though looking at those pictures one of

00:09:40 --> 00:09:40 the

00:09:40 --> 00:09:43 peculiarities of Neptune is that we

00:09:43 --> 00:09:45 think it's

00:09:45 --> 00:09:48 magnetic axis that the two magnetic

00:09:48 --> 00:09:52 poles um are tilted well over to sort of

00:09:52 --> 00:09:54 middle latitudes unlike here on Earth

00:09:54 --> 00:09:57 where they they don't exactly align

00:09:57 --> 00:09:58 magnetic north is not the same as

00:09:58 --> 00:10:00 geographic north but the the magnetic

00:10:00 --> 00:10:02 poles more or less align with the

00:10:02 --> 00:10:06 rotation of the planet uh and that's

00:10:06 --> 00:10:08 probably to do with the fact that we

00:10:08 --> 00:10:09 think these that the earth's magnetism

00:10:10 --> 00:10:13 is generated by uh the circulation of

00:10:13 --> 00:10:17 the iron uh and nickel core uh which is

00:10:17 --> 00:10:19 in two parts and it sort of acts like a

00:10:19 --> 00:10:21 dynamo and that generates a magnetic

00:10:21 --> 00:10:24 field um Neptune and probably the other

00:10:24 --> 00:10:26 gas giants have something similar we

00:10:26 --> 00:10:27 really don't understand the origin of

00:10:27 --> 00:10:29 their magnetism we don't know whether

00:10:29 --> 00:10:31 there's a solid core or not in the gas

00:10:31 --> 00:10:33 giants we suspect there must be in order

00:10:33 --> 00:10:35 for them to have these strong magnetic

00:10:35 --> 00:10:37 fields but on Neptune the magnet the

00:10:37 --> 00:10:39 magnetic field is tilted over at quite a

00:10:40 --> 00:10:42 considerable angle to the rotation of

00:10:42 --> 00:10:45 the planet uh which is why the aurori

00:10:45 --> 00:10:47 appear at mid latitudes on Neptune

00:10:48 --> 00:10:50 rather than near the poles as they do

00:10:50 --> 00:10:52 here on Earth as I know well from my

00:10:52 --> 00:10:56 sojun up in the Arctic two months ago

00:10:56 --> 00:11:00 yeah so I I have heard there's something

00:11:00 --> 00:11:03 going on with Neptune's orbit it's

00:11:03 --> 00:11:05 either wobbly or it changes or something

00:11:05 --> 00:11:06 like that would that have anything to do

00:11:06 --> 00:11:10 with this tilt um it it is possible you

00:11:10 --> 00:11:14 know the two may be related um usually

00:11:14 --> 00:11:18 the rotation of a planet and its

00:11:18 --> 00:11:24 orbit are fairly decoupled um and you've

00:11:24 --> 00:11:26 only to look at Uranus which you know as

00:11:26 --> 00:11:29 you know is tilted over nine degrees I

00:11:29 --> 00:11:31 think it's nine degrees below below the

00:11:32 --> 00:11:33 uh the what you might call the

00:11:33 --> 00:11:36 horizontal the plane of its orbit uh and

00:11:36 --> 00:11:39 um Uranus has a reasonably

00:11:39 --> 00:11:42 well sort of well- behaved orbit um

00:11:42 --> 00:11:45 Neptune's interesting because it's in

00:11:45 --> 00:11:48 modern parliament it represents the the

00:11:48 --> 00:11:51 outermost planet of the solar system uh

00:11:51 --> 00:11:54 and it does affect the orbits of the

00:11:54 --> 00:11:56 many myriads of objects that we know lie

00:11:56 --> 00:11:58 beyond that the so-called trans

00:11:58 --> 00:12:00 neptunian objects which include things

00:12:00 --> 00:12:02 in the Kiper belt and things called

00:12:02 --> 00:12:04 resonant objects like Plutos plutos are

00:12:04 --> 00:12:07 resonant objects because it resonates in

00:12:07 --> 00:12:09 its orbital period with Neptune and the

00:12:09 --> 00:12:11 and the scattered disc objects as they

00:12:11 --> 00:12:14 called way beyond that uh so it it could

00:12:14 --> 00:12:16 be um that Neptune's orbit is

00:12:16 --> 00:12:17 interacting with those although a big

00:12:17 --> 00:12:20 planet like Neptune it takes a lot to

00:12:20 --> 00:12:23 shift its orbit to to per perturb it so

00:12:23 --> 00:12:25 I I haven't seen those reports that

00:12:25 --> 00:12:27 you've mentioned and um everything

00:12:27 --> 00:12:29 you've just heard is complete waffle but

00:12:29 --> 00:12:31 that's the way it works when you're

00:12:31 --> 00:12:32 talking about things you've not seen

00:12:32 --> 00:12:35 before right and I think there's just so

00:12:35 --> 00:12:39 much of that with space it's uh the the

00:12:39 --> 00:12:42 I was at a NASA tech talk last week and

00:12:42 --> 00:12:43 one of the they were me they were

00:12:43 --> 00:12:45 talking about SANS which is an ocular

00:12:46 --> 00:12:48 syndrome that the astronauts experience

00:12:48 --> 00:12:50 or they have issues with their eyes and

00:12:50 --> 00:12:51 for those of you listening my little dog

00:12:52 --> 00:12:53 spiking for attention in the corner

00:12:53 --> 00:12:55 we're just going to ignore them play

00:12:55 --> 00:12:58 time when we're done recording but um

00:12:58 --> 00:13:01 the the uh presenter he brought he was a

00:13:01 --> 00:13:03 flight surgeon and he brought up so many

00:13:03 --> 00:13:06 funny headlines and articles it's NASA

00:13:06 --> 00:13:08 scientists say this and this he's like I

00:13:08 --> 00:13:10 cannot find these experts yes if anybody

00:13:10 --> 00:13:12 knows these experts that this headline

00:13:12 --> 00:13:14 is claiming to talk about please let me

00:13:14 --> 00:13:16 know because this is all wrong so I

00:13:16 --> 00:13:17 think there's a lot of that in the space

00:13:17 --> 00:13:19 industry

00:13:19 --> 00:13:21 so that that's a really interesting

00:13:21 --> 00:13:23 syndrome isn't it because that's one of

00:13:23 --> 00:13:26 the potential longived um u consequences

00:13:26 --> 00:13:30 of of um long-term space flight that

00:13:30 --> 00:13:33 you've got these ocular effects um my

00:13:33 --> 00:13:35 Sorry we've we're way off topic here

00:13:35 --> 00:13:38 Heidi but that's all right

00:13:38 --> 00:13:41 um hello i've forgotten your dog simba

00:13:41 --> 00:13:43 like the Lion King you know he's wagging

00:13:43 --> 00:13:46 his tail he's He's trying as hard as he

00:13:46 --> 00:13:49 can to be as cute as possible

00:13:49 --> 00:13:52 he's doing a fine job the tail wager he

00:13:52 --> 00:13:54 thinks if he's cuter I'll stop recording

00:13:54 --> 00:13:57 and go play with him yeah I I know the

00:13:57 --> 00:14:01 syndrome um so this what I've read is

00:14:01 --> 00:14:04 that it may be caused by the fact that

00:14:04 --> 00:14:05 you know the circulation in the body the

00:14:05 --> 00:14:08 blood circulation in the body changes in

00:14:08 --> 00:14:10 microgravity and that you might well

00:14:10 --> 00:14:15 have uh pressures in the cranium that

00:14:15 --> 00:14:17 might affect the eyes in a way that we

00:14:17 --> 00:14:19 don't have on Earth is that the thinking

00:14:19 --> 00:14:21 or am I just making that up you're

00:14:21 --> 00:14:23 absolutely spot on yeah it's it's has

00:14:23 --> 00:14:25 everything to do with fluid so when the

00:14:25 --> 00:14:28 fluid changes in the body we normally

00:14:28 --> 00:14:30 have gravity pulling that fluid away

00:14:30 --> 00:14:32 from the head but when we're in space

00:14:32 --> 00:14:35 the fluid tends to you know pull up

00:14:35 --> 00:14:38 towards our head and shift in places

00:14:38 --> 00:14:40 that we don't necessarily want it so

00:14:40 --> 00:14:43 there that is a leading issue um and

00:14:43 --> 00:14:45 causing that pressure and then there

00:14:45 --> 00:14:47 were you know there were so many other

00:14:47 --> 00:14:49 points and tangents with that but um

00:14:49 --> 00:14:51 we're learning so much more about it now

00:14:51 --> 00:14:53 and one of the really interesting things

00:14:53 --> 00:14:55 with space medicine and human

00:14:55 --> 00:14:57 performance in space is when we're

00:14:57 --> 00:14:58 looking at the research we'll have like

00:14:58 --> 00:15:01 an N of eight and for those of you

00:15:01 --> 00:15:03 non-science people N is your subject

00:15:03 --> 00:15:06 number so you know when we're looking at

00:15:06 --> 00:15:08 you know cancer research that can be in

00:15:08 --> 00:15:11 the hundreds or thousands of data points

00:15:11 --> 00:15:12 that we're looking at but when we're

00:15:12 --> 00:15:14 talking about astronaut health it's just

00:15:14 --> 00:15:17 a handful of people so there's really

00:15:17 --> 00:15:20 there's as much as we know about it is

00:15:20 --> 00:15:22 with the people that have been to space

00:15:22 --> 00:15:24 already and that's one reason why I'm so

00:15:24 --> 00:15:27 excited about what some of these other

00:15:27 --> 00:15:29 companies are doing like Blue Origin

00:15:29 --> 00:15:31 Axiom Virgin that are getting more and

00:15:31 --> 00:15:33 more people into space so that we can

00:15:33 --> 00:15:36 learn more about space health which does

00:15:36 --> 00:15:39 influence health on Earth

00:15:39 --> 00:15:41 there's so much we've learned about

00:15:41 --> 00:15:43 space medicine that has helped improve

00:15:43 --> 00:15:45 life on Earth

00:15:45 --> 00:15:48 which is remarkable and um and and great

00:15:48 --> 00:15:50 news and one of the you know the many

00:15:50 --> 00:15:54 many many benefits of space exploration

00:15:54 --> 00:15:57 uh we've got another commercial flight

00:15:57 --> 00:15:59 about to launch I think within the next

00:15:59 --> 00:16:00 few days is that right the Framm 2

00:16:00 --> 00:16:03 mission oh they are going all the time i

00:16:03 --> 00:16:05 uh don't I can't even keep up with all

00:16:05 --> 00:16:08 of them sometimes yeah that's what

00:16:08 --> 00:16:13 um you should listen to this show for

00:16:13 --> 00:16:15 so I have another Depune question and I

00:16:15 --> 00:16:18 want to segue this in with the humans in

00:16:18 --> 00:16:20 the people part i love that are you

00:16:20 --> 00:16:23 familiar with the book it's a book and a

00:16:23 --> 00:16:25 TV series called The Expanse are you

00:16:25 --> 00:16:30 familiar with it um um no um and um I um

00:16:30 --> 00:16:34 I apologize for that um because I I

00:16:34 --> 00:16:35 there's so much going on out there that

00:16:35 --> 00:16:38 I simply don't have time to read or look

00:16:38 --> 00:16:41 at and understand yeah I rely on I

00:16:41 --> 00:16:43 certainly rely on Andrew uh keeping

00:16:43 --> 00:16:45 keeping me honest in regards to science

00:16:45 --> 00:16:47 fiction and I'm sure the same is going

00:16:47 --> 00:16:48 to be true with you but no I don't know

00:16:48 --> 00:16:52 about the So in the expanse they have um

00:16:52 --> 00:16:55 they have populated the solar system

00:16:55 --> 00:16:57 there's people living on Earth Mars and

00:16:57 --> 00:16:59 there are also people living out in the

00:16:59 --> 00:17:02 asteroid belts they call them belters

00:17:02 --> 00:17:05 and these people are multigenerations

00:17:05 --> 00:17:07 born in space so they have phys

00:17:07 --> 00:17:10 physiologically adapted to life in space

00:17:10 --> 00:17:12 so they have become physically different

00:17:12 --> 00:17:14 from people born on earth because of the

00:17:14 --> 00:17:16 gravities and the systems there so I

00:17:16 --> 00:17:18 want to segue this back into talking

00:17:18 --> 00:17:20 about Neptune because we have ice we

00:17:20 --> 00:17:24 have wind and from what I do know about

00:17:24 --> 00:17:27 greenhouse gases um and thinking about

00:17:27 --> 00:17:30 the expanse there has been some chatter

00:17:30 --> 00:17:34 about putting some

00:17:34 --> 00:17:37 industrial factories and whatnot on Mars

00:17:37 --> 00:17:39 eventually to help generate greenhouse

00:17:39 --> 00:17:42 gases to help increase atmosphere on

00:17:42 --> 00:17:46 Mars is this something because I always

00:17:46 --> 00:17:47 like to think about what we're looking

00:17:47 --> 00:17:49 at and seeing with these auroras and

00:17:49 --> 00:17:50 space and everything we're learning and

00:17:50 --> 00:17:53 what does it mean for future generations

00:17:53 --> 00:17:57 could could Neptune potentially be um a

00:17:57 --> 00:18:00 big power generating planet with these

00:18:00 --> 00:18:04 winds if we could harvest these winds

00:18:04 --> 00:18:07 what a lovely idea um um wind turbines

00:18:07 --> 00:18:12 on Neptune now that's really a really um

00:18:12 --> 00:18:16 expansive idea if I can um use the joke

00:18:16 --> 00:18:21 there uh it's um so um it the the

00:18:21 --> 00:18:25 likelihood is that um with as with so

00:18:25 --> 00:18:28 many things that people talk about doing

00:18:28 --> 00:18:32 in space it's actually easier not to uh

00:18:32 --> 00:18:36 to find alternative sources uh of

00:18:36 --> 00:18:38 whatever it is you're trying to generate

00:18:38 --> 00:18:42 um and the the the the winds on Neptune

00:18:42 --> 00:18:44 colossal winds as we've said you know up

00:18:44 --> 00:18:46 to maybe approaching 2 miles per

00:18:46 --> 00:18:48 hour

00:18:48 --> 00:18:52 uh how you would generate them it's hard

00:18:52 --> 00:18:55 to know what might be interesting though

00:18:55 --> 00:18:57 is if you could use them sorry how you

00:18:58 --> 00:19:00 could use how you could use those winds

00:19:00 --> 00:19:03 to generate power it's hard to know but

00:19:03 --> 00:19:05 if you could um use those winds to

00:19:05 --> 00:19:08 facilitate exploration of the planet's

00:19:08 --> 00:19:10 atmosphere and that something I could

00:19:10 --> 00:19:12 well imagine you know people dropping um

00:19:12 --> 00:19:15 balloons into the atmosphere of of

00:19:15 --> 00:19:17 Neptune uh to watch the circulation to

00:19:18 --> 00:19:21 do what we do here on Earth with uh um

00:19:21 --> 00:19:25 our multiple capacity for for uh

00:19:25 --> 00:19:28 measuring and predicting the weather so

00:19:28 --> 00:19:29 weather on Neptune might be something

00:19:29 --> 00:19:31 that turns out to be quite interesting i

00:19:32 --> 00:19:36 think um a more in some ways a more

00:19:36 --> 00:19:39 uh what's the word opposite maybe is the

00:19:39 --> 00:19:42 right word uh world uh to be interested

00:19:42 --> 00:19:44 in in the Neptune system is is moon

00:19:44 --> 00:19:47 Triton because that could turn out to be

00:19:47 --> 00:19:49 you know one of the places like Europa

00:19:49 --> 00:19:51 and Enteladus that has the potential for

00:19:51 --> 00:19:53 perhaps living organisms beneath the

00:19:53 --> 00:19:57 surface and that is very exciting very

00:19:57 --> 00:19:59 exciting and it really just comes down

00:19:59 --> 00:20:02 to the human ingenuity the engineering

00:20:02 --> 00:20:03 and all the new breakthroughs that we're

00:20:03 --> 00:20:05 making it seems like every single day

00:20:05 --> 00:20:07 there's more stuff that we're coming up

00:20:07 --> 00:20:10 with to get us out there

00:20:10 --> 00:20:12 okay let's take a quick break from the

00:20:12 --> 00:20:15 show to give a shout out to our sponsor

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00:21:45 --> 00:21:47 nordvpn.com/spacenuts all right let's

00:21:47 --> 00:21:50 get back to the show

00:21:50 --> 00:21:52 space nuts which I think is kind of a

00:21:52 --> 00:21:58 good segue into our next story um so

00:21:58 --> 00:22:02 NASA's created this new dust shield and

00:22:02 --> 00:22:05 it's going to help repel the lunar

00:22:05 --> 00:22:09 regalith which is very important uh the

00:22:09 --> 00:22:11 regalith is

00:22:11 --> 00:22:15 very fine it's very sticky it can be

00:22:15 --> 00:22:18 kind of dangerous if this is getting in

00:22:18 --> 00:22:20 their um analoges and their facilities

00:22:20 --> 00:22:22 and where they're living so tell me more

00:22:22 --> 00:22:24 about this this is quite the interesting

00:22:24 --> 00:22:27 story

00:22:27 --> 00:22:31 that's um that that's Jordy

00:22:31 --> 00:22:33 um let let me just check what's

00:22:34 --> 00:22:35 happening because it's he does sound

00:22:35 --> 00:22:38 like a chicken yeah jordy jordy jordy

00:22:38 --> 00:22:40 johnny

00:22:40 --> 00:22:42 uh I do apologize he does sound like a

00:22:42 --> 00:22:44 chicken he does doesn't he yeah he's

00:22:44 --> 00:22:46 just like a rooster he doesn't know that

00:22:46 --> 00:22:49 he thinks he sounds like a big Just calm

00:22:49 --> 00:22:52 down Jordy it's all right there's um

00:22:52 --> 00:22:54 there's a dog that he hates that its

00:22:54 --> 00:22:57 owner occasionally brings it near our

00:22:57 --> 00:23:00 property to take they know better

00:23:00 --> 00:23:03 yeah all right Jordy calm down good boy

00:23:03 --> 00:23:06 good boy good boy um okay so the Luna

00:23:06 --> 00:23:08 Regal is

00:23:08 --> 00:23:09 back to the moon from the sublime to the

00:23:10 --> 00:23:13 ridiculous or the other way around uh we

00:23:13 --> 00:23:15 Yes you're absolutely right that the the

00:23:15 --> 00:23:18 soil on the moon is such an interesting

00:23:18 --> 00:23:21 thing it's different from anything we

00:23:21 --> 00:23:23 have on Earth uh and that's because it

00:23:24 --> 00:23:27 has been formed not by wind and water

00:23:27 --> 00:23:29 erosion like the soil on Earth has but

00:23:29 --> 00:23:32 by um bombardment by these subatomic

00:23:32 --> 00:23:34 particles the wind of particles that

00:23:34 --> 00:23:36 constantly blows from the sun probably a

00:23:36 --> 00:23:38 few micrometeorites banging into the

00:23:38 --> 00:23:40 surface as well and so what we've got is

00:23:40 --> 00:23:43 a soil that is very very fine and very

00:23:43 --> 00:23:46 angular uh so it's got sharp edges all

00:23:46 --> 00:23:48 the way around it and exactly as you've

00:23:48 --> 00:23:49 said that's why it gets into all the

00:23:49 --> 00:23:52 nooks and cran crannies all the crevices

00:23:52 --> 00:23:55 the the basically the clothing of

00:23:55 --> 00:23:59 astronauts um there is one recorded case

00:23:59 --> 00:24:00 uh and you probably know more about this

00:24:00 --> 00:24:03 than I do Heidi one of the Apollo

00:24:03 --> 00:24:04 missions and I can't remember which one

00:24:04 --> 00:24:08 it was but so much dust was brought into

00:24:08 --> 00:24:11 the uh into the lunar module by one of

00:24:11 --> 00:24:14 the astronauts that uh it pervaded the

00:24:14 --> 00:24:16 whole return trip back to Earth and gave

00:24:16 --> 00:24:19 that person the first case of lunar hay

00:24:19 --> 00:24:21 fever because he was sneezing all the

00:24:21 --> 00:24:23 time because of this dust i can't

00:24:23 --> 00:24:24 remember who it was

00:24:24 --> 00:24:26 i I do remember hearing about this and I

00:24:26 --> 00:24:28 also can't remember who it was but yeah

00:24:28 --> 00:24:30 it could be quite the problem it's just

00:24:30 --> 00:24:33 this sticky fine mess

00:24:33 --> 00:24:37 so um NASA in their wisdom are looking

00:24:37 --> 00:24:40 at ways to mitigate the effects of that

00:24:40 --> 00:24:43 and um as part of the Blue Ghost mission

00:24:43 --> 00:24:46 that was a spacecraft that commercial

00:24:46 --> 00:24:48 spacecraft landed on the moon

00:24:48 --> 00:24:50 successfully uh I don't know a month ago

00:24:50 --> 00:24:53 I guess it's it's not very long ago um

00:24:53 --> 00:24:57 uh which was part of NASA's program for

00:24:57 --> 00:24:59 I think it's called the commercial lunar

00:24:59 --> 00:25:02 payloads program in other words getting

00:25:02 --> 00:25:05 um the commercial world to actually do

00:25:05 --> 00:25:07 some of the leg work in preparing for

00:25:08 --> 00:25:10 the Opimus uh flights to the moon later

00:25:10 --> 00:25:13 in the decade uh and one of the

00:25:13 --> 00:25:16 experiments carried on board Blue Ghost

00:25:16 --> 00:25:19 was indeed about how you can reduce the

00:25:19 --> 00:25:23 effects of this lunar dust uh it has a

00:25:23 --> 00:25:26 name it is called the EDS uh the

00:25:26 --> 00:25:30 electronamic dust shield and um

00:25:30 --> 00:25:34 basically it uh is a way of removing uh

00:25:34 --> 00:25:36 the the the contamination of dust and

00:25:36 --> 00:25:40 dirt from uh whatever surfaces you

00:25:40 --> 00:25:43 you've got on the moon probably uh it's

00:25:43 --> 00:25:45 more like spacecraft surfaces than

00:25:45 --> 00:25:47 clothing although this it might lend

00:25:47 --> 00:25:50 itself to that eventually uh and um it

00:25:50 --> 00:25:52 seems to have worked very very well

00:25:52 --> 00:25:56 there is uh a pair of images which are

00:25:56 --> 00:25:58 pretty easy to find on the web um I'm

00:25:58 --> 00:26:01 looking actually at the NASA uh uh

00:26:01 --> 00:26:03 website itself for the press release

00:26:03 --> 00:26:05 which is entitled NASA's dust shield

00:26:05 --> 00:26:08 successfully repels lunar regalith on

00:26:08 --> 00:26:11 moon uh and you can see a before and

00:26:11 --> 00:26:13 after with this uh with this device

00:26:13 --> 00:26:18 activated um I I suspect it works well

00:26:18 --> 00:26:21 it's called an electro electronamic uh

00:26:21 --> 00:26:25 dust shield uh but um that electronamic

00:26:25 --> 00:26:27 usually means moving electrons so

00:26:27 --> 00:26:30 there's a current flowing uh but um it's

00:26:30 --> 00:26:32 I suspect that the basic mechanism is

00:26:32 --> 00:26:35 electrostatic it's a repulsion of the of

00:26:35 --> 00:26:39 the you know the slightly charged uh

00:26:39 --> 00:26:41 soil particles that that exist on the

00:26:41 --> 00:26:43 moon they they are they are electrically

00:26:43 --> 00:26:45 charged so if you can give them an

00:26:45 --> 00:26:47 opposite charge they'll be repelled and

00:26:47 --> 00:26:48 that looks as though it's what's

00:26:48 --> 00:26:50 happening and it's been met with success

00:26:50 --> 00:26:53 so perhaps it's a step forward in

00:26:53 --> 00:26:55 cleaning up our voyages to the moon and

00:26:55 --> 00:26:56 not bringing back a whole lot of

00:26:56 --> 00:26:58 unwanted moon dust when you come back to

00:26:58 --> 00:27:01 Earth absolutely and I'm just thinking

00:27:01 --> 00:27:03 again of the implications for Earth

00:27:03 --> 00:27:04 because I think sometimes there's a

00:27:04 --> 00:27:06 little bit of like I said earlier

00:27:06 --> 00:27:07 there's a little bit of a disconnect you

00:27:07 --> 00:27:10 know thinking space and how it's not

00:27:10 --> 00:27:12 related to Earth and it's so so related

00:27:12 --> 00:27:14 to everything we do here on Earth i mean

00:27:14 --> 00:27:17 GPS NASA gave us GPS nasa gave us water

00:27:17 --> 00:27:20 purification nasa gave us

00:27:20 --> 00:27:23 um Oh man i'm totally mindbling the big

00:27:23 --> 00:27:25 machine that you go into that scans you

00:27:25 --> 00:27:27 if you go to the hospital yeah an MRI

00:27:27 --> 00:27:29 mri machine yes that should be the one

00:27:29 --> 00:27:31 that I know but yeah I mean so much of

00:27:31 --> 00:27:33 this has come from space science and I'm

00:27:33 --> 00:27:34 thinking of something that would make my

00:27:34 --> 00:27:37 life easier even just on the simplest

00:27:37 --> 00:27:40 level if the surfaces in my house my

00:27:40 --> 00:27:43 tables and everything repelled dust and

00:27:43 --> 00:27:45 I don't know if we are just that much

00:27:45 --> 00:27:48 closer to inventing dust repelling

00:27:48 --> 00:27:50 surfaces and that just makes everybody's

00:27:50 --> 00:27:53 life that much easier that much safer

00:27:53 --> 00:27:54 because then you're not using cleaning

00:27:54 --> 00:27:56 agents and chemicals to clean your house

00:27:56 --> 00:27:59 you just have a surface that just repels

00:27:59 --> 00:28:00 that dust automatically and that just

00:28:00 --> 00:28:02 could that could even have really good

00:28:02 --> 00:28:04 implications in sterile environments

00:28:04 --> 00:28:07 like computer um places where they're

00:28:07 --> 00:28:09 building computer or hospital settings

00:28:09 --> 00:28:12 so this is actually very very exciting

00:28:12 --> 00:28:14 that they're doing this and the article

00:28:14 --> 00:28:16 is quite short it's just a blur but the

00:28:16 --> 00:28:19 implications of this you know we don't

00:28:19 --> 00:28:21 know how this is going to improve life

00:28:21 --> 00:28:23 down the road exactly that's right it's

00:28:23 --> 00:28:27 um you know the the sky Well the sky's

00:28:27 --> 00:28:29 is the limit really isn't it in terms of

00:28:29 --> 00:28:33 what we can do with space technology um

00:28:33 --> 00:28:35 technology perfected for space i I do

00:28:35 --> 00:28:37 worry you know if you if you press a

00:28:38 --> 00:28:39 button and all the dust leaps off all

00:28:39 --> 00:28:41 the surfaces in your house you might

00:28:41 --> 00:28:44 need an extractor fan to take them away

00:28:44 --> 00:28:45 so they don't wind up somewhere where

00:28:45 --> 00:28:49 you don't want them yes

00:28:49 --> 00:28:53 the next segue

00:28:53 --> 00:28:55 okay we checked all four systems and

00:28:55 --> 00:28:58 keying with the space nets speaking of

00:28:58 --> 00:29:01 the sky being the limit our last article

00:29:02 --> 00:29:06 that we're looking at there was a

00:29:06 --> 00:29:10 um big nebula explosion and there's a

00:29:10 --> 00:29:15 glow left over from it uh the title is a

00:29:15 --> 00:29:17 nebula's x-ray glow may come from a

00:29:17 --> 00:29:21 destroyed giant planet

00:29:21 --> 00:29:23 and that's quite dramatic

00:29:23 --> 00:29:26 but we are excited about these images

00:29:26 --> 00:29:30 because it tells us about history

00:29:30 --> 00:29:33 that's right um and in fact everything

00:29:33 --> 00:29:35 in the universe tells you about history

00:29:35 --> 00:29:36 which is great because you're always

00:29:36 --> 00:29:39 looking back in time uh we're we're

00:29:39 --> 00:29:41 looking back in this case I think it's

00:29:41 --> 00:29:42 about

00:29:42 --> 00:29:46 670 650 light years it's a very very

00:29:46 --> 00:29:50 well-known object uh called the Helix

00:29:50 --> 00:29:53 Nebula um and in fact first captured in

00:29:53 --> 00:29:56 full color by my colleague and friend

00:29:56 --> 00:29:59 David Merlin who um was the person who

00:29:59 --> 00:30:01 essentially developed a technique in the

00:30:01 --> 00:30:04 1970s and 80s uh to put true color into

00:30:04 --> 00:30:08 celestial images by taking three sets of

00:30:08 --> 00:30:10 photographic plates as we used in those

00:30:10 --> 00:30:13 days through red green and blue filters

00:30:13 --> 00:30:16 um and he he became very well known for

00:30:16 --> 00:30:18 that he was totally fastidious and still

00:30:18 --> 00:30:20 is actually about getting the color

00:30:20 --> 00:30:22 balance right so that what we saw in

00:30:22 --> 00:30:25 these images was what uh what we would

00:30:25 --> 00:30:27 be able to see if our eyes were millions

00:30:27 --> 00:30:29 of times more sensitive now segue from

00:30:30 --> 00:30:33 that to the present time when that

00:30:33 --> 00:30:35 lovely color image uh of the Helix

00:30:35 --> 00:30:39 Nebula became very very famous uh um

00:30:39 --> 00:30:41 that was what we see in visible light

00:30:41 --> 00:30:44 but it's now been observed at many other

00:30:44 --> 00:30:47 wavelengths of light as well um and

00:30:47 --> 00:30:51 ranging from uh infrared to X-rays in

00:30:51 --> 00:30:53 fact put it that way around or X-rays to

00:30:53 --> 00:30:56 infrared um and it's the X-ray radiation

00:30:56 --> 00:30:58 that is the most exciting and it's the

00:30:58 --> 00:31:01 reason why we've got this story so the

00:31:01 --> 00:31:02 the Helix Nebula just to give the

00:31:02 --> 00:31:04 backstory is what we call a planetary

00:31:04 --> 00:31:06 nebula uh and and it's nothing to do

00:31:06 --> 00:31:09 with planets except in the way that

00:31:09 --> 00:31:11 we'll come to in a minute uh it was

00:31:11 --> 00:31:13 called that by William

00:31:13 --> 00:31:16 Herschel an astronomer back in the early

00:31:16 --> 00:31:19 19th century who saw these things uh

00:31:19 --> 00:31:21 which were clearly not planets because

00:31:21 --> 00:31:24 they were in the deep sky they they were

00:31:24 --> 00:31:26 not they were moving with the stars

00:31:26 --> 00:31:28 rather than with with planets so they

00:31:28 --> 00:31:30 weren't in the solar system but they had

00:31:30 --> 00:31:32 a slightly planetary appearance they

00:31:32 --> 00:31:34 looked circular uh so he called them

00:31:34 --> 00:31:37 planetary nebula and what we discovered

00:31:37 --> 00:31:40 in the early 20th century is that what

00:31:40 --> 00:31:42 we're seeing there is the outer layers

00:31:42 --> 00:31:46 of a star which has reached old age and

00:31:46 --> 00:31:49 u is not massive enough to explode like

00:31:49 --> 00:31:51 a supernova

00:31:51 --> 00:31:53 an exploding star that detonates and

00:31:53 --> 00:31:56 blows itself to pieces you need to be

00:31:56 --> 00:31:57 more than about three or four times the

00:31:57 --> 00:32:00 mass of the sun to do that um in fact 10

00:32:00 --> 00:32:03 times is probably a better bet uh the

00:32:03 --> 00:32:05 star like the sun gets to the end of its

00:32:06 --> 00:32:08 life and basically the instabilities

00:32:08 --> 00:32:10 that are caused by the fact that it's

00:32:10 --> 00:32:12 used up most of its hydrogen fuel it

00:32:12 --> 00:32:14 causes the outer atmosphere to to

00:32:14 --> 00:32:18 basically to be shed gently uh and um

00:32:18 --> 00:32:22 that produces a a cloud of gas often

00:32:22 --> 00:32:24 spherical in form sometimes they're

00:32:24 --> 00:32:26 hourglass shaped they've got all kinds

00:32:26 --> 00:32:29 of different shapes but the Helix Nebula

00:32:29 --> 00:32:30 in the southern hemisphere sky is the

00:32:30 --> 00:32:34 classic example of uh of a of a a

00:32:34 --> 00:32:36 planetary nebula a star at the end of

00:32:36 --> 00:32:37 its life it shed its outer layers

00:32:38 --> 00:32:40 they're glowing because what's left of

00:32:40 --> 00:32:42 the star is a remnant called a white

00:32:42 --> 00:32:46 dwarf uh which is uh a a an object the

00:32:46 --> 00:32:48 size of our planet size of the earth but

00:32:48 --> 00:32:50 with the mass of a star so it's very

00:32:50 --> 00:32:52 very dense um now white dwarfs are

00:32:52 --> 00:32:55 interesting creatures in their own right

00:32:55 --> 00:32:58 but the Helix Nebula has one that is

00:32:58 --> 00:33:01 even more interesting than normal

00:33:01 --> 00:33:05 because it radiates copiously in X-rays

00:33:05 --> 00:33:07 and X-rays we have to get above the

00:33:07 --> 00:33:09 Earth's atmosphere to detect because the

00:33:09 --> 00:33:11 atmosphere fortunately absorbs X-rays

00:33:12 --> 00:33:14 very um very effectively uh but there

00:33:14 --> 00:33:17 have been a number of space satellites

00:33:17 --> 00:33:19 uh mostly satellites around the earth

00:33:19 --> 00:33:21 spacecraft that have been essentially

00:33:22 --> 00:33:26 used to uh survey the the sky in X-ray

00:33:26 --> 00:33:29 emission uh and the Helix Nebula of

00:33:29 --> 00:33:31 course has been one of the things that

00:33:31 --> 00:33:34 uh uh have been looked at with X-rays

00:33:34 --> 00:33:36 with a whole series of different

00:33:36 --> 00:33:39 satellites um through the you know

00:33:39 --> 00:33:42 through the ages uh it it was

00:33:42 --> 00:33:46 um actually uh first detected by back in

00:33:46 --> 00:33:49 the early 1980s by NASA's Einstein

00:33:49 --> 00:33:50 Observatory which is an an X-ray

00:33:51 --> 00:33:53 satellite and there was another one

00:33:53 --> 00:33:55 called Rossat i guess it comes from

00:33:55 --> 00:33:59 Rentgun the German word for X-rays after

00:33:59 --> 00:34:02 Professor Rengun who discovered them um

00:34:02 --> 00:34:05 Rosat in the 19 early 1990s both of

00:34:05 --> 00:34:09 those spacecraft detected X-rays from uh

00:34:09 --> 00:34:11 from the Helix Nebula which weren't

00:34:11 --> 00:34:14 really understood uh now those have been

00:34:14 --> 00:34:17 followed up um couple of decades later

00:34:17 --> 00:34:20 NASA's Chandra X-ray Observatory in 1999

00:34:20 --> 00:34:22 and XMM Newton which is a European Space

00:34:22 --> 00:34:26 Agency spacecraft in 2002 have recorded

00:34:26 --> 00:34:28 these copious quantities of X-rays

00:34:28 --> 00:34:31 coming from the Helix Nebula what is it

00:34:31 --> 00:34:33 all about where do they come from how do

00:34:33 --> 00:34:35 you get something that shouldn't be

00:34:35 --> 00:34:37 producing X-rays but has you know sort

00:34:37 --> 00:34:41 of 30 years uh well 20 years anyway of

00:34:41 --> 00:34:44 of e of strong X-ray emission and so the

00:34:44 --> 00:34:46 people who think deeply about these

00:34:46 --> 00:34:48 things the theoretical astronomers and

00:34:48 --> 00:34:50 some of these uh astronomers in this

00:34:50 --> 00:34:54 case uh some are in uh the United States

00:34:54 --> 00:34:58 but some are also in Mexico um they they

00:34:58 --> 00:35:01 have deduced that what's happening is

00:35:01 --> 00:35:05 probably a Jupiter sized planet uh maybe

00:35:05 --> 00:35:09 a bit more than Jupiter uh was uh

00:35:09 --> 00:35:12 orbiting the star as it reached the end

00:35:12 --> 00:35:15 of its life carried on orbiting the

00:35:15 --> 00:35:17 white dwarf but because of the forces

00:35:17 --> 00:35:19 involved with the collapse of the star

00:35:19 --> 00:35:21 to a white dwarf at the end of its life

00:35:22 --> 00:35:23 uh that the planet was shredded

00:35:23 --> 00:35:26 basically and formed a ring of disc

00:35:26 --> 00:35:30 sorry a disc of material not a ring of

00:35:30 --> 00:35:32 disc that doesn't make sense a disc of

00:35:32 --> 00:35:35 material around the the around the white

00:35:35 --> 00:35:39 dwarf which is accelerated to very very

00:35:39 --> 00:35:40 high velocities the gravitational field

00:35:40 --> 00:35:42 of a white dwarf is a bit like a black

00:35:42 --> 00:35:45 hole not quite as extreme but very

00:35:45 --> 00:35:46 strong and so you got So this is the

00:35:46 --> 00:35:49 ghost of a planet exactly yes the debris

00:35:49 --> 00:35:51 of a planet planetary ghost i love the

00:35:51 --> 00:35:55 term um it's uh but it it's all it's you

00:35:55 --> 00:35:58 know it's basically it's dismembered

00:35:58 --> 00:36:00 remains are whizzing around this white

00:36:00 --> 00:36:04 dwarf at high orbital velocity and that

00:36:04 --> 00:36:08 creates X-rays because of the heating

00:36:08 --> 00:36:10 effect of this turbulence that is in the

00:36:10 --> 00:36:13 dis of material and that's the theory at

00:36:13 --> 00:36:14 the moment and it's the best one that

00:36:14 --> 00:36:17 we've got as to why the Helix Nebula is

00:36:17 --> 00:36:20 so copiously emitting X-rays that it's

00:36:20 --> 00:36:23 got an unfortunate planet that didn't

00:36:23 --> 00:36:26 survive the collapse uh and is radiating

00:36:26 --> 00:36:29 violently in the X-ray wavelengths so

00:36:29 --> 00:36:32 rather intriguing story let me see if I

00:36:32 --> 00:36:34 understand this correctly so I'm looking

00:36:34 --> 00:36:37 at this image and it's got kind of a red

00:36:37 --> 00:36:39 dot in the middle for those listening if

00:36:39 --> 00:36:41 you don't see the image you guys can

00:36:41 --> 00:36:43 look up the Helix Nebula it's a very

00:36:43 --> 00:36:45 famous photo and you'll see what I'm

00:36:45 --> 00:36:47 describing it almost looks like a kind

00:36:47 --> 00:36:49 of like an eye so it's got this red like

00:36:49 --> 00:36:51 the Terminator it's got this red dot in

00:36:51 --> 00:36:53 the middle and then it almost looks like

00:36:53 --> 00:36:55 an iris and then it keeps expanding out

00:36:55 --> 00:36:57 it actually does look exactly like an

00:36:57 --> 00:37:00 eye now that I look at it but so the

00:37:00 --> 00:37:02 planet got sucked into the red which is

00:37:02 --> 00:37:05 the dwarf and then spun apart like a

00:37:05 --> 00:37:08 centuge and cuz it looks like it

00:37:08 --> 00:37:10 exploded from inside out but what's

00:37:10 --> 00:37:12 happening is it's spinning apart and

00:37:12 --> 00:37:15 that's why it's surrounding this red and

00:37:15 --> 00:37:17 it's spinning and so the gravity is like

00:37:17 --> 00:37:19 the debris is coming apart from the

00:37:19 --> 00:37:23 center rather than getting pulled into

00:37:23 --> 00:37:24 the center is that what I'm am I

00:37:24 --> 00:37:25 understanding this correctly that's

00:37:26 --> 00:37:30 right yes that's right so so the the the

00:37:30 --> 00:37:33 X- radiation is um it you know it's it's

00:37:34 --> 00:37:36 sort of pervading the whole of the of

00:37:36 --> 00:37:38 the nebula you've got X-rays coming from

00:37:38 --> 00:37:41 every part of it uh or or appearing to

00:37:41 --> 00:37:44 but but they're being emitted by this

00:37:44 --> 00:37:47 object which is actually within it's not

00:37:47 --> 00:37:49 visible the disc itself is not visible

00:37:49 --> 00:37:52 the dis of material that was this planet

00:37:52 --> 00:37:55 uh that's too near the white dwarf the

00:37:55 --> 00:37:58 white dwarf itself uh is is visible in

00:37:58 --> 00:38:00 visible in optical images visible light

00:38:00 --> 00:38:03 images but not in the X-ray image so uh

00:38:03 --> 00:38:06 it's a matter of inference along the

00:38:06 --> 00:38:08 lines that you've just described Heidi

00:38:08 --> 00:38:10 so maybe you already explained this

00:38:10 --> 00:38:12 because this doesn't make sense to me

00:38:12 --> 00:38:14 why so if the gravity is strong enough

00:38:14 --> 00:38:17 to be keeping these bits and parts

00:38:17 --> 00:38:19 within its gravity why are why is it

00:38:20 --> 00:38:22 still spreading out

00:38:22 --> 00:38:26 so the the um the the the the gaseous

00:38:26 --> 00:38:30 envelope of the star itself

00:38:30 --> 00:38:34 uh is that was basically emitted over

00:38:34 --> 00:38:37 many millions probably tens of millions

00:38:37 --> 00:38:39 hundreds of millions of years before the

00:38:40 --> 00:38:42 star collapsed into a white dwarf so

00:38:42 --> 00:38:45 that's far enough away that um it's not

00:38:45 --> 00:38:48 feeling that intense gravity in the you

00:38:48 --> 00:38:50 know the the the region near to the

00:38:50 --> 00:38:51 white dwarf itself

00:38:52 --> 00:38:54 um it's it's basically drifting off uh

00:38:54 --> 00:38:57 as uh you know the distances are

00:38:57 --> 00:38:59 measured in light years they're not

00:38:59 --> 00:39:00 they're not measured in millions of

00:39:00 --> 00:39:02 kilometers they're very very large

00:39:02 --> 00:39:05 distances so um yes it's a great

00:39:05 --> 00:39:07 question though um that so so it's all

00:39:08 --> 00:39:09 the stuff that is really within the

00:39:09 --> 00:39:11 immediate vicinity of the white dwarf

00:39:11 --> 00:39:14 that's feeling that acceleration and and

00:39:14 --> 00:39:17 undergoing that intense orbital uh

00:39:17 --> 00:39:20 motion around the white dwarf

00:39:20 --> 00:39:23 is this your favorite nebula um uh it it

00:39:23 --> 00:39:25 probably is actually that's a really

00:39:25 --> 00:39:27 good question too because I've never

00:39:27 --> 00:39:29 sort of thought about that there is a

00:39:29 --> 00:39:30 well-known one in the northern sky which

00:39:30 --> 00:39:32 will be visible from Houston called the

00:39:32 --> 00:39:36 Ring Nebula uh but the Helix Nebula I

00:39:36 --> 00:39:37 think is a little bit more glamorous

00:39:38 --> 00:39:39 because it's got a bit more structure to

00:39:39 --> 00:39:41 it it's it's got this it's called the

00:39:41 --> 00:39:43 Helix Nebula because it's it looks a bit

00:39:44 --> 00:39:47 like a a sort of unwound spring um and

00:39:47 --> 00:39:48 you can see you're probably having a

00:39:48 --> 00:39:50 look at the Ring Nebula as we speak

00:39:50 --> 00:39:52 looking it up oh yeah it's absolutely

00:39:52 --> 00:39:55 beautiful that's just stunning

00:39:55 --> 00:39:58 so I think maybe this will be a topic

00:39:58 --> 00:40:02 for um a Q&A or another session but I

00:40:02 --> 00:40:04 definitely want to understand more of

00:40:04 --> 00:40:07 the um the the technology that you said

00:40:07 --> 00:40:09 your friend developed his name was also

00:40:09 --> 00:40:12 Fred uh no david actually is Fred his

00:40:12 --> 00:40:15 middle name is Frederick frederick okay

00:40:15 --> 00:40:19 david david Mail yeah so he um just

00:40:19 --> 00:40:20 briefly

00:40:20 --> 00:40:24 uh when the Anglo Australian telescope

00:40:24 --> 00:40:26 it's the largest visible light telescope

00:40:26 --> 00:40:31 on Australian soil uh with a 3.9 m 156

00:40:31 --> 00:40:34 in mirror um and he and I both worked

00:40:34 --> 00:40:36 there i was the astronomer in charge for

00:40:36 --> 00:40:40 20 years in fact but uh before that he

00:40:40 --> 00:40:42 in fact when the telescope was brand new

00:40:42 --> 00:40:45 he was taken on board on the stuff he he

00:40:45 --> 00:40:47 speaks a lot like me because he comes

00:40:47 --> 00:40:49 from the north of England uh went to

00:40:49 --> 00:40:52 Australia and perfected this technique

00:40:52 --> 00:40:55 in those days um imaging of astronomical

00:40:55 --> 00:40:56 objects was done with photographic

00:40:56 --> 00:40:58 plates and I'm talking about 1975 that's

00:40:58 --> 00:41:02 when he went to Australia um and um

00:41:02 --> 00:41:05 apart from a few experiments with color

00:41:05 --> 00:41:08 emulsions normal color film which really

00:41:08 --> 00:41:10 didn't work well for astronomical

00:41:10 --> 00:41:13 objects because color film is designed

00:41:13 --> 00:41:15 for a very short exposure you know

00:41:15 --> 00:41:17 you're in a camera you press a button

00:41:17 --> 00:41:19 shutter opens and closes again in a 50th

00:41:19 --> 00:41:22 of a second and you record the image uh

00:41:22 --> 00:41:25 astronomers spend hours exposing their

00:41:25 --> 00:41:27 photographic plates as we did in those

00:41:27 --> 00:41:31 days and the the whole you know optical

00:41:31 --> 00:41:33 chemical process that makes color

00:41:33 --> 00:41:35 photography just didn't work and so he

00:41:35 --> 00:41:38 designed this technique it actually goes

00:41:38 --> 00:41:41 back a couple of hundred years um to you

00:41:41 --> 00:41:43 know way people thought you can perhaps

00:41:43 --> 00:41:45 replicate with the red green and blue

00:41:45 --> 00:41:47 you can replicate a color image and it's

00:41:47 --> 00:41:50 true you can but it took David's skills

00:41:50 --> 00:41:53 and hard work to perfect that and the

00:41:53 --> 00:41:55 result was uh twofold it made the

00:41:55 --> 00:41:58 telescope very famous because his images

00:41:58 --> 00:42:01 found their way onto the front covers of

00:42:01 --> 00:42:04 magazines and album covers and books uh

00:42:04 --> 00:42:06 they were all over the world in the 19

00:42:06 --> 00:42:09 uh 80s early 1980s it made the telescope

00:42:09 --> 00:42:11 famous and it made him very famous as

00:42:11 --> 00:42:14 well uh and he still um is interested in

00:42:14 --> 00:42:17 this he's now retired he uh doesn't

00:42:17 --> 00:42:19 really do any frontline photography

00:42:19 --> 00:42:23 anymore but occasionally uh we end up in

00:42:23 --> 00:42:25 involved in scientific discussions about

00:42:25 --> 00:42:27 all kinds of things so he's still very

00:42:27 --> 00:42:30 active well it's it's I mean I think

00:42:30 --> 00:42:32 nebulas I think are probably one of the

00:42:32 --> 00:42:34 most beautiful beautiful things in space

00:42:34 --> 00:42:36 and these images are just breathtaking

00:42:36 --> 00:42:38 and to think of the it's it's almost

00:42:38 --> 00:42:40 impossible to comprehend the scale of a

00:42:40 --> 00:42:42 nebula because we just see them on our

00:42:42 --> 00:42:44 desktop as a beautiful picture but to

00:42:44 --> 00:42:45 think of the size and the magnitude is

00:42:45 --> 00:42:48 quite amazing and the contributions of

00:42:48 --> 00:42:51 the field are really quite incredible

00:42:51 --> 00:42:54 it's uh it's it's quite astonishing to

00:42:54 --> 00:42:56 think of the um conspiracy theorists and

00:42:56 --> 00:42:58 how they think that these are just you

00:42:58 --> 00:43:00 know computerenerated images and they're

00:43:00 --> 00:43:02 like "Oh the scientists are just

00:43:02 --> 00:43:03 painting the photos to make them look

00:43:03 --> 00:43:05 like how they want." And then you're

00:43:05 --> 00:43:06 telling us stories of how how your

00:43:06 --> 00:43:08 friend and you put 20 years into just

00:43:08 --> 00:43:12 developing these technologies yeah yeah

00:43:12 --> 00:43:13 that's

00:43:13 --> 00:43:16 right um look conspiracy theorists are

00:43:16 --> 00:43:19 another breed uh we could talk endlessly

00:43:19 --> 00:43:24 about them but um uh yes uh you know the

00:43:24 --> 00:43:27 the the the work that David did was

00:43:27 --> 00:43:29 really very rigorous to try and make

00:43:29 --> 00:43:31 sure that what we were seeing was what

00:43:31 --> 00:43:33 we would see if our eyes were more

00:43:33 --> 00:43:35 sensitive uh the the the the downside of

00:43:35 --> 00:43:38 that Heidi is that um whenever David

00:43:38 --> 00:43:40 went anywhere to give give a talk and he

00:43:40 --> 00:43:44 did that all the time um especially in

00:43:44 --> 00:43:47 the digital era as things moved on he

00:43:47 --> 00:43:49 got very upset if the color balance on

00:43:49 --> 00:43:53 the projector was not to his liking um

00:43:53 --> 00:43:55 and indeed he started all his talks and

00:43:55 --> 00:43:58 I do now too with a with a basically a

00:43:58 --> 00:44:00 color chart you know a color diagram and

00:44:00 --> 00:44:02 if it wasn't to his liking he would

00:44:02 --> 00:44:04 start tinkering with a projector to try

00:44:04 --> 00:44:07 and make it so and once in a while he

00:44:07 --> 00:44:09 would refuse to give the talk because it

00:44:09 --> 00:44:11 would not show his pictures in the true

00:44:11 --> 00:44:12 colors that he'd worked so hard to

00:44:12 --> 00:44:14 create

00:44:14 --> 00:44:17 talk about a perfectionist and it's

00:44:17 --> 00:44:19 things like that you really It just

00:44:19 --> 00:44:21 makes the conspiracy theorist sound just

00:44:21 --> 00:44:24 that much more silly they think they

00:44:24 --> 00:44:25 have something figured out because they

00:44:25 --> 00:44:29 watched a YouTube video yes there you go

00:44:29 --> 00:44:32 not to end on a negative note with the

00:44:32 --> 00:44:34 conspiracy theorists and we'll we'll

00:44:34 --> 00:44:35 take it as we're ending on a positive

00:44:35 --> 00:44:37 talking about these beautiful beautiful

00:44:37 --> 00:44:39 nebulas and these incredible

00:44:39 --> 00:44:42 contributions to the field and I just

00:44:42 --> 00:44:44 want to I don't know inspire and

00:44:44 --> 00:44:47 encourage listeners to if you're a space

00:44:47 --> 00:44:50 enthusiast to keep considering all these

00:44:50 --> 00:44:52 possibilities and if you are someone who

00:44:52 --> 00:44:55 works in the field you never know what

00:44:55 --> 00:44:57 you know you're going to be producing 20

00:44:57 --> 00:44:59 years from now and what your work is

00:44:59 --> 00:45:02 going to do and contribute to humanity

00:45:02 --> 00:45:04 and what kind of neuroticism you'll

00:45:04 --> 00:45:06 develop if you'll never be able to look

00:45:06 --> 00:45:08 at a projector the same way or if you're

00:45:08 --> 00:45:10 just going to become the person who is

00:45:10 --> 00:45:12 so obsessed with doing this one thing

00:45:12 --> 00:45:14 because you've put 20 30 40 years into

00:45:14 --> 00:45:17 studying something so incredibly niche

00:45:17 --> 00:45:20 um Fred do you have anything else you

00:45:20 --> 00:45:24 want to add uh not to that story uh just

00:45:24 --> 00:45:26 to say this has been a wonderful uh

00:45:26 --> 00:45:30 session i think it's uh episode 509 that

00:45:30 --> 00:45:32 we've just done

00:45:32 --> 00:45:34 wow thanks and it's been great talking

00:45:34 --> 00:45:36 to you Heidi and um I look forward to

00:45:36 --> 00:45:39 our next chat excellent again thank you

00:45:39 --> 00:45:41 so much for having me and you have been

00:45:41 --> 00:45:44 listening to Space Nuts space Nuts

00:45:44 --> 00:45:46 you've been listening to the Space Nuts

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