Jan. 30, 2025
Extreme Winds, Martian Clays & Hidden Stars: #491 - The Interstellar Exploration
Space Nuts Episode 491: The Windiest Planet, Martian Mysteries, and Light Pollution Concerns
Join Andrew Dunkley and Professor Jonti Horner in this captivating episode of Space Nuts, where they explore some of the most fascinating cosmic discoveries...
Space Nuts Episode 491: The Windiest Planet, Martian Mysteries, and Light Pollution Concerns
Join Andrew Dunkley and Professor Jonti Horner in this captivating episode of Space Nuts, where they explore some of the most fascinating cosmic discoveries of our time. From the extraordinary winds of a distant exoplanet to intriguing geological findings on Mars, and the looming threat of light pollution on astronomical observations, this episode is packed with insights that will expand your cosmic perspective.
Episode Highlights:
- The Windiest Planet: Discover Wasp 127B, the exoplanet with astonishing wind speeds reaching up to 33,000 kilometers per hour. Andrew and Jonti delve into the implications of these extreme weather conditions and what they reveal about the planet's atmosphere and energy dynamics.
- Martian Terrain Discovery: A new study uncovers a fascinating area on Mars that suggests the presence of permanent liquid water in the planet's ancient past. Jonti explains the significance of the clay deposits found in the northern lowlands and how they relate to the theory of a Martian ocean.
- Protostar Insights: Learn about T Tauri North, a protostar set to fade from view as it moves behind a thick disk of material in a triple star system. Andrew and Jonti discuss the scientific opportunities this presents for studying the formation of stars and planets in such systems.
- Light Pollution Threat: The Extremely Large Telescope, built in one of the darkest places on Earth, faces potential light pollution from a nearby renewable energy project. Explore the challenges this poses to astronomical research and the delicate balance between development and preservation of dark skies.
For more Space Nuts, including our continually updating newsfeed and to listen to all our episodes, visit our website. Follow us on social media at SpaceNutsPod on Facebook, X, YouTube Music Music, Tumblr, Instagram, and TikTok. We love engaging with our community, so be sure to drop us a message or comment on your favorite 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
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 - Introduction to the episode and topics
02:15 - Discussion on Wasp 127B and its extreme winds
10:30 - Insights into Martian clay deposits and ancient oceans
18:00 - The fading protostar T Tauri North and its implications
26:45 - Light pollution concerns for the Extremely Large Telescope
30:00 - Closing thoughts and listener engagement
✍️ Episode References
Wasp 127B Discovery
https://exoplanetarchive.ipac.caltech.edu/
Mars Clay Deposits
https://mars.nasa.gov/
T Tauri Stars
https://en.wikipedia.org/wiki/T_Tauri_star
Extremely Large Telescope
https://www.eso.org/public/teles-instr/elt/
Become a supporter of this podcast: https://www.spreaker.com/podcast/space-nuts--2631155/support.
Join Andrew Dunkley and Professor Jonti Horner in this captivating episode of Space Nuts, where they explore some of the most fascinating cosmic discoveries of our time. From the extraordinary winds of a distant exoplanet to intriguing geological findings on Mars, and the looming threat of light pollution on astronomical observations, this episode is packed with insights that will expand your cosmic perspective.
Episode Highlights:
- The Windiest Planet: Discover Wasp 127B, the exoplanet with astonishing wind speeds reaching up to 33,000 kilometers per hour. Andrew and Jonti delve into the implications of these extreme weather conditions and what they reveal about the planet's atmosphere and energy dynamics.
- Martian Terrain Discovery: A new study uncovers a fascinating area on Mars that suggests the presence of permanent liquid water in the planet's ancient past. Jonti explains the significance of the clay deposits found in the northern lowlands and how they relate to the theory of a Martian ocean.
- Protostar Insights: Learn about T Tauri North, a protostar set to fade from view as it moves behind a thick disk of material in a triple star system. Andrew and Jonti discuss the scientific opportunities this presents for studying the formation of stars and planets in such systems.
- Light Pollution Threat: The Extremely Large Telescope, built in one of the darkest places on Earth, faces potential light pollution from a nearby renewable energy project. Explore the challenges this poses to astronomical research and the delicate balance between development and preservation of dark skies.
For more Space Nuts, including our continually updating newsfeed and to listen to all our episodes, visit our website. Follow us on social media at SpaceNutsPod on Facebook, X, YouTube Music Music, Tumblr, Instagram, and TikTok. We love engaging with our community, so be sure to drop us a message or comment on your favorite 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
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 - Introduction to the episode and topics
02:15 - Discussion on Wasp 127B and its extreme winds
10:30 - Insights into Martian clay deposits and ancient oceans
18:00 - The fading protostar T Tauri North and its implications
26:45 - Light pollution concerns for the Extremely Large Telescope
30:00 - Closing thoughts and listener engagement
✍️ Episode References
Wasp 127B Discovery
https://exoplanetarchive.ipac.caltech.edu/
Mars Clay Deposits
https://mars.nasa.gov/
T Tauri Stars
https://en.wikipedia.org/wiki/T_Tauri_star
Extremely Large Telescope
https://www.eso.org/public/teles-instr/elt/
Become a supporter of this podcast: https://www.spreaker.com/podcast/space-nuts--2631155/support.
WEBVTT
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Hi there, thanks for joining us, and welcome to a
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fresh episode of Space Nuts.
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My name is.
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Andrew, Uncle, your host. It's always good to have your company.
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Coming up, we are going to look at the windiest
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planet ever discovered. This is planet Baked Beans. No it's not,
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it's called something else, but yeah, it's it's quite extraordinary.
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The numbers will blow your mind. A strange area of
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terrain has been identified in Mars, which tells a very
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interesting tale about the planet's history. We're going to look
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at a protostar that we won't be able to look
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at soon and it's also part of a triple star system,
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and time permitting, we are going to bring up that
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old chestnut again, light pollution. That's all coming up on
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this episode of Space Nuts. Fifteen second, Channel ten nine
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ignition Space Nuts or three two one Space Nuts. But
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it meels good, indeed it is now. Fred's still away
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gallivanting around with reindeer in the Northern Hemisphere somewhere, and
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joining us in his place is Professor John D. Horner,
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Professor of astrophysics at the University of Southern Queensland.
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Hi, joundy, how are you going good?
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Good and you.
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Getting that slowly, a little bit sniffy. We're having the
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joys of summer around herese It's been nice and dry
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and warm for the last few dar I saw the
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plants have been getting too excited, and I think couple
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are a little bit from their excitement.
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Our plants are very unexcited because we're going to hit
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forty two celsius today and I've got the air conditioning
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on and it usually cuts itself off pretty quickly this
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time of the day because you know, it equalizes through
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the thermostep. It has been running NonStop for forty five
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minutes now because it cannot keep the temperature down.
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Because it's so hot outside right right at the moment.
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One of the beauties of the Darling Downs is that
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our heat wears don't get quite that extreme. I think
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further west they do, but this area around to One
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was just really lovely. So our summers are pretty much
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thirty to thirty five most days, but gets cool enough
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at night. Sleep still a very rare that we'll get
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up near to forty. I think in the couple of
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years I've been in this house, we've not hit forty yet,
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and yet we don't have all the humidity that make
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Brisbane the kind of world's armpit. The sound of it, Johnny, Yeah, well,
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I tell you who likes this kind of weather. It's
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the local snake population. I drove into our we live
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in a gated estate. We drove in.
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I drove in yesterday and saw what I thought was
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a piece of plastic hose on the road. It wasn't.
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It was a five foot Eastern brown snake crossing the
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road mining its own business. But that's the third time
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we've seen one this summer. If you want to have
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a look at it, I've put photos of it on
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Instagram and TikTok. So yeah, it's it was a big one.
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I let him go, I let you go, or the
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old sayings say, you know, they're not scared of you
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than you are of them. Out of the Australian But
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when I moved out here from the UK, everybody was
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kind of oh, no, you're going. All the animals will
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kill you. You know, the drop pay will get you
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all this. And so I got a book called Australia's
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Most Dangerous Animals, which is only a little one. Turns
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out the most dangerous animal in Australia have gone to
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that book is not sharks or snakes. I mean, obviously
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it's people. But aside from people, it's European honeybee because
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people would allergic to them and they are in and
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that really puts it in perspective. It's the case that
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Australia has all these animals that can be dangerous, but
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they're also nearly all cowards, so they'll typically get out
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of your way. It's not like the you know, rattlesnakes
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in the US, or I think is it cobra's in
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the subcontinent, where they'll actually aggressively defend themselves, but they
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just want to run away. It's tail between the legs,
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shoot off.
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Yes, if they had legs, I could probably do that.
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Yep.
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Now we should get on with it because we've got
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a lot to talk about. We're going to focus firstly
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on the windiest planet ever discovered, planet Baked Beans. It's
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not it's it's WASP one two seven B tell us
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all about it.
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The joys of catalog numbers that do exactly what they're
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saying on that in incidentally, for those who are not
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sucking on the catalog numbers that are given to exoplanets,
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which are really useful to astronomers, but not really good
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for everybody's imagination. The International Astronomical Union are slowly naming
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planets and their stars, and they're doing it in a
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very kind of democratic, global community type fashion. And this
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one hasn't yet been named, but it may well be
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in the future, so names coming soon. Probably people will
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nominate make beans given this story, but we'll just have
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to see how that ends out. What's one twenty seven Bees,
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a planet that was found using the transit methods. So
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the WASP program is a wide angle search for planets,
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and they've got this array of essentially pretty good the
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SLR cameras with wide angle lenses all strapped together that
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have been staring at the same patch of the night
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sky whenever it's above the horizon for a long long time.
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And they have a couple of stations around the world.
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And what this lets them do is monitor the brightness
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of all the stars in that field of view and
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look for any of them that periodically winked us. And
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this is the same technique that NASA's Kepler mission used
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that the Test mission uses as well, and they find
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planets by looking at the planets passing between us and
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the star blocking out some of that light and causing
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the star to dimm and then brighten. And it's a
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technique that is really effective, but it's very biased towards
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finding planets that are big because a bigger planet blocks
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more light, and finding planets that are nearer to the
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star because the planet that's nearer to the star goes
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around more quickly, so you get more winks in a
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given period of time. And that's very true of this planet.
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This is a planet that's big. It's one and a
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third times larger than Jupiter in terms of diameter. It's
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also quite light. It's less massive than Saturn. It's about
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a fifth of Jupiter's mass, which means it's one of
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the least planets we know. People describe it as a
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super puff. But because it's big, it's got this big diameter,
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it blocks quite a big chunk of its stars like,
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making it relatively obvious for people to detect. And it
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goes around every four days, so this star winks at
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as every four days or so, and that's how this
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planet was discovered. Now, because it's big, because it stars
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quite bright, it's a really prime target for people to
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look at to see if they can learn more about it.
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We want to develop the tools to study the atmospheres
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of planets around other stars and learn more about them,
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so not to just know that they're there, but actually
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characterize them, and that helps us understand how planets form,
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what the diversity of planets is, and all the rest
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of it. And this has been a prime target for
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that kind of work for a few years. The new
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results that have come out are the results of people
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trying to study the atmosphere of this planet. They used
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a very large telescope which is remarkably imaginatively named, and
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they were getting oblimations with this huge ground based telescope
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to study the spectra of this planet. So to take
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the light that we get from the planet separately from
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the star, break it into its component colors and look
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at what spectral lines are in there. Because the spectral
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lines give you the fingerprint of the competition of the atmosphere.
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They also tell you things like how quickly the atmosphere
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is moving, how hot it is, and with enough information
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you can even start inferring things about the structure where
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the clouds are, things like that. Now this is really
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cutting edge, So even with the biggest telescopes in the world.
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We can only really do it for big, fluffy planets
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that are very near their starts. We know when they're
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being able to do it for planets like Earth yet,
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but it's a step on that journey. So that's the
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background here. What happened with this planet is that the
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observations when they got the spectrum, it revealed something really
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weird for the different things in the atmosphere. Instead of
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having a single peak in the spectrum that said, hey, okay,
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we've got hydrogen or whatever, they found two peaks quite
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close together but certainly quite separate from one another, distinctly separate.
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Are this puzzle for a little bit, And there was
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a bit of a continuum between them as well, So
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it wasn't just like one narrow spike and a gap
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in another narrows bike. But what they realized was that,
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thanks to the Dopper effect, just exactly the same kind
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of thing we use for the radial velocity measurements that
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we do have starts to measure their wobbles. If you've
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got gas that's coming towards here, light that it emits
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and light that it absorbs, that light will be blue shifted.
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The wavelength will be shorter than it would be if
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that was stationary. If that gas is moving away from us,
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the light stretched out, and so the light's red shifted,
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And the degree to which the light is blue or
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red shifted tells you the speed. The quicker it's moving,
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the bigger the shifts. You know, this is the same
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thing you get if a police carra and ambulance comes past.
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You know, you hear the siren when it's approaching, and
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it's high pitched and fast, you like n n no Nino.
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And then it goes past and it's going away in here,
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Nino Nino. And the fact that it's going the bigger
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the shifted. So when they're in a real hurry, it's
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really distinct. That allows them to figure out what's going
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on here. So it turns out that this planet is
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the victim of incredibly high wind speeds. There's extreme weather
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going on, and what they think it is best described
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as is like an equatorial jet, where we've got winds
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going around the planet at ridiculously high speed. Now, this
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is a planet that goes around its star every four days.
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Its surface temperature of the cloud tops is like eleven
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hundred degrees sea, so it's really extreme anyway. But the
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wind speed to explain these two peaks, must be about
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thirty three thousand kilometers per hour, so that's nine kilometers
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per second, which is just ridiculous. And you've got the
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blue shifted peaks on one side of the planet the
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wind's coming towards us, and yeah, the red shifted peak
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because on the other side of the planet, on the
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other edge of the planet, the wind's going away from us.
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So you get this peak to peak with about eighteen
196
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kilometers a second, between nine kilometers a second towards us
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and nine kilometers per second away. Putting that in scale,
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that is sixteen to faster than the fastest winds we've
199
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ever seen in the Solar System, which are the two
200
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hundred kilometers per hour winds on net Tune, and is
201
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therefore something like one hundred and sixty one hundred and
202
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fifty times stronger than the strongest wing gust ever recorded
203
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on Earth. So that's just insane remarkable wind speed, and
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it tells us a lot about the properties of the atmosphere.
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There's going to be a lot we learn about it
206
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in terms of how energy is moved from the daylight
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side to the nighttime side, because this planet should be
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tidally locked, so it should keep one side facing towards
209
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the style, one side facing away, and these winds are
210
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probably what's transferring the heat from the daytime side, which
211
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is super hot, rather to the night side, which is.
212
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Called I was going to get to that. Yeah, that
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makes perfect sense. So you get getting superheated on one side,
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and it's just yeah, around and around, absolutely and a.
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Bit more than anybody would have expected to find. But
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that's the natural of this kind of exploration. We I
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always think it's true of most things in astronomy that
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the also you are to the conditions that are in
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your room right now, the better we understand it. So
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the further we go away from standard temperature, room temperature,
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room pressure, the less understanding we have, the more we
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have to learn. Now we've got guideposts in our Soul system,
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so we've learned a bit about planets that are like
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the Solar System planets. But when it comes to something
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like this super hot, super puffy planet around this star
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that is similar to but a bit bigger and a
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bit hotter than the Sun, it's totally different to anything
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we've ever seen and experienced and therefore you get results
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you don't expect, and in understanding those we get a
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better handle of how planets work.
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Yes, fascinating. How does it compare to the guest giants
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in our Solar System? I mean, they've much further away
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from the star, so further away, but.
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There's still a lot of interesting things happening. Energy wise.
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We've got a lot of data for Jupiter and Saturin
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and more limited data from the Voyager spacecraft that went
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to your inner selection. We've basically been to Jupiter and
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Saturn more often. But the highest speeds that we've ever
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observed in the Solar System of those on Neptune, which
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were about two thousand kilometers per hour. Now, that is
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pretty impressive from an Earth based point of view and
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was a big surprise because Neptune is so far from
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the Sun, it's got so little energy that that was
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