Cosmic Queries: Understanding Black Holes, Galactic Centres, and Mars Days | Space Nuts:...
In this engaging Q&A episode of Space Nuts, join host Andrew Dunkley and astronomer Fred Watson Watson as they tackle a variety of fascinating questions from listeners. From the peculiarities of Martian days to the mysteries of black holes and the galactic centre, this episode is filled with enlightening discussions that are sure to spark curiosity about the cosmos.
In this episode:
- John asks about the implications of Mars' longer day length on human biology and potential adaptations for future colonists.
- Dan inquires about the growth of black holes, exploring how quickly they can develop into supermassive entities and what happens when there’s nothing left to consume.
- Young Thomas, just 11 years old, poses several intriguing questions about the galactic centre, including whether it can swallow all stars and planets in the galaxy, and the limits of a black hole's gravitational reach.
- Paul reflects on historical discoveries in astronomy, specifically how Harlow Shapley determined our Sun's position within the Milky Way, challenging the long-held belief that it was at the centre.
Join Andrew and Fred Watson as they explore these thought-provoking questions and more, encouraging listeners to continue their journey of exploration and discovery in the universe.
Become a supporter of this podcast: https://www.spreaker.com/podcast/space-nuts-astronomy-insights-cosmic-discoveries--2631155/support (https://www.spreaker.com/podcast/space-nuts-astronomy-insights-cosmic-discoveries--2631155/support?utm_source=rss&utm_medium=rss&utm_campaign=rss) .
(00:00) This is a Q and A edition where we take audience questions
(02:16) When and if Mars is populated with humans, how would we work with longer day
(08:50) Andrew: How astronauts deal with gravity when they land on Earth
(11:47) Dan from the Gold coast has some questions about black holes
(12:51) Fred: How fast do black holes grow? Dan asks fundamental astrophysics question
(18:17) Fred asks five questions about black holes from Thomas Reid, 11
(22:03) Thomas asks if black holes can swallow up all stars and planets
(24:31) Final question comes from Paul from Las Vegas
(26:42) It was actually 1919 when that discovery was made
(34:24) We continue to receive great questions from great listeners and long may it continue
Episode link: https://play.headliner.app/episode/34693771?utm_source=youtube
Kind: captions
Language: en
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Hello again and thank you for joining us
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on another episode of Space Nuts. This
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is a Q&A edition where we take audience
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questions, we put them on paper, and
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then we put them on a roll that goes on
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a little thing in a bathroom.
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Or we could answer them. We can do that.
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Uh coming up today, we have uh questions
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uh from John about Martian days. The
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length of a Martian day. It's close, but
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is it close enough to Earth's standard?
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We'll discuss that. Uh, the growth of a
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black hole has been uh brought up again.
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Uh, we've got a um a uh question from an
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11-year-old named Thomas. Hi, Thomas. He
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wants to talk about the galactic center.
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And Paul is asking our uh about our
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galactic location. So, we'll deal with
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all of that today on this episode of
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Space Nuts.
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>> 15 seconds. Guidance is internal. 10 9
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ignition sequence start. Space Nuts.
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>> 5 4 3 2
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>> 1 2 3 4 5 5 4 3 2 1
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>> Space Nuts.
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>> Astronauts report. It feels good.
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>> Joining us again to sort all of that out
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is Professor Fred Watson, astronomer at
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large. Hello, Fred.
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>> Hello, Andrew. Good to see you again.
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>> Good to see you, too.
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>> Yes. Despite the hole in my head.
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>> Yeah. Yeah. It doesn't look any better
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than the last time I show you.
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>> It doesn't, does it?
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>> No. I mean, you know, it's only been
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minutes. You'd think it would have
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improved by now.
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>> That's what happens when you walk into a
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when you walk into a closed screen door.
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>> Yeah.
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>> In the dark,
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>> it hurts.
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>> Now, that's why they have stuff um on on
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glass sliding doors. You know, that
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that's a standard safety standard
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required these days so that you know the
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door is there.
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>> Yeah.
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But when it's nighttime and it's a
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screen door, not not many excuses left
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there, Fred. Really?
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>> Only stupidity, I think, is the is the
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last one. But that's that's my excuse
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many, many times.
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>> Yeah. Well, like I said before, we've
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all done it.
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>> Uh shall we try and answer these
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questions?
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>> We should.
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>> Okay, let's go to question one. This one
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comes from John. Uh we know that the
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Martian day is 39 minutes longer than an
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Earth Day. That's about 4 and 1/2 hours
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a week. Uh when and if Mars is populated
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with humans, how would we work with the
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longer day/week?
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Would human biology tend to keep to the
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24-hour day or would we adapt to a
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longer dayight cycle? Thanks. Love the
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show and have been a listener since you
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started. Wow, you've got a lot of spare
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time, John. Uh thank you so much uh for
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sending your question in and hope all is
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well. Uh I love this question because it
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you've got a planet that is close enough
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for us to get to in the not too distant
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future. Probably
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not a permanent settlement, but a
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rotating settlement of some kind will be
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the initial stages of humans being on
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Mars.
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and yet you've got an extra 39 minutes a
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day to deal with. What is going to be
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the impact?
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>> Um I think we've already
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>> have um a lot of data on this because
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the
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>> we've already talked about this once
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before in the dead dark past came up
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again. Yeah.
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>> Yeah. because of the the um um rover
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drivers.
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>> Uh they um people the people who are uh
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in command of if I can put it that way
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because they don't actually drive them
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directly but in command of the the
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rovers on Mars and the two active NASA
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ones at the moment are Curiosity and
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Perseverance.
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uh they adapt to a 20 to 24 hours 39
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minutes day uh and do it quite
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successfully as far as I've been able to
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work out.
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>> Well, I hope so.
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>> Yeah. Otherwise, there might be a pile
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up on Mars. Um, and in fact, the reason
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why I said they don't actually drive
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them is because the the rovers
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themselves have got to be to some extent
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autonomous because of the the the delay
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in in signal time to get between Mars
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and the Earth. You can't have video
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coming back from your rover and a
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steering wheel so that you respond to
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that because you'd have a sort of 20 or
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30 minute delay probably before
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>> uh before um you you turn before the
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wheels turned on on the rover.
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>> I would I would imagine that the the
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manual driving of a rover from Earth on
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Mars would be damn near impossible
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because even your images would be out of
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sync with
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>> everything's out of sync. That's right.
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So you see, oh, there's a rock coming
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up. That was 40 minutes ago.
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>> I'll turn left now.
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>> Oops.
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>> Yeah. Um so so the the rovers drive
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themselves basically uh with a lot of um
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assistance and monitoring from Earth uh
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in order to see what's coming up and see
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what the onboard computers are doing in
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terms of what route they're taking
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through the rocks and debris on Mars.
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uh and um so but those people as I
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understand it do go on to uh this 24
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hours and 39 minutes day length uh I
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think it's near enough to our 24 hours
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that I think they adapt quite quickly
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from my recollection of our previous
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conversation about this Andrew
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>> yeah I if I remember rightly we were
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talking about the fact that if you're
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going to stay on Mars long term you
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would have to adapt
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um you wouldn't adapt naturally
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at all. You you'd have to take catnaps
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or something like that to to catch up um
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or something to that effect.
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>> Well, it Yes. So, your circadian rhythms
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would they'd be under stress. They
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they'd change.
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>> Um um and I suppose you'd have a
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permanent feeling of jet lag probably.
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Probably what it feels like.
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>> It would be tough. I read an article uh
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last weekend which I I found fascinating
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and it was um detailing how the 8hour
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night cycle that humans have like going
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to bed for 8 hours is a myth.
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>> Yes.
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>> And that um it was it was actually
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something invented by a mattress company
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back in 1938. Have you heard this?
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>> No. Yes.
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>> I I I do know that we used to sleep
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twice in the night with it.
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>> That's right. So, you go to bed at like
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9:00
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>> and you'd sleep for 4 hours and then
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you'd get up for 2 hours and you'd do
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stuff
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>> like stuff we can't talk about on this
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podcast, but other stuff like um
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>> they cited a couple of um famous people
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um whose names have dropped straight out
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of my head. Um, William Shakespeare
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>> uh apparently wrote a lot of his famous
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works between 1 and 3 in the morning
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when he got up and then he go back to
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bed for 4 hours. And Bethovven did the
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same thing with some of his symphonies.
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He wrote some of the best works that he
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ever created at 3:00 in the morning um
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during his wake time between his two
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sleeps. Yeah. So the 8hour sleep
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that we have at night was an invention
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apparently to sell mattresses.
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That's what I'm told. I look I haven't
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confirmed or denied that but it seems it
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seems possible I suppose. Well, yes. I I
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think I think we have we've I think um
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there's been evidence from, you know,
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the earliest times,
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uh the times when people truly were
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ancient peoples back thousands of years
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ago, uh that that's how they lived their
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lives, exactly as you've said. And maybe
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there were the last vestigages of that
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were
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>> keeping going in Shakespeare's time and
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then in Beethoven's time. Um
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there weren't that many clocks around
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then. There were some, but not that
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many. It wasn't like you had a
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smartwatch by your bedside or anything
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like that. So, uh it would be a natural
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rhythm that they would use uh to, you
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know, to to sleep and wake up.
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>> Yes. And if you're natural,
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modernization certainly messed us up,
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hasn't it?
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>> Yeah. Yeah, that's right. I think in
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that case it has.
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>> And I think uh on Mars it will be um it
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will be a pretty difficult thing. I I
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imagine
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>> it may be. So, um maybe I can just
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sidestep here slightly, Andrew, because
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um I would very much like to know uh
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what answer one of our listeners would
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give to that. And that's Dr. Heidi
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Deblock, who's I think based in Houston,
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if I remember rightly, who is a
00:09:07.600 --> 00:09:11.590
basically a space medic. Uh and um it
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will be very interesting to hear her
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take on how humans will adapt to that.
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And if I may, she was in touch with us
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recently to comment on one of our
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earlier questions. Would it be all right
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if I read that?
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>> And that was when we were talking about
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how people deal with um gravity when
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they get back on Earth after being out
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in space for a while.
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>> Correct. Yes, that's right.
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>> Uh she says, um, "I just finished the
00:09:37.760 --> 00:09:40.150
July 5th Space Nuts and wanted to help
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answer the question about how the
00:09:41.360 --> 00:09:43.030
astronauts feel when they land back on
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Earth. Of course, I haven't experienced
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it in person, but have worked with
00:09:47.279 --> 00:09:49.269
plenty of astronauts at landing in
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particular. All of our physiology
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changes in space as we are designed for
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1G. Some astronauts are pretty good when
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they land, especially those who are on
00:09:58.640 --> 00:10:01.269
the shuttle and in space for short time
00:10:01.279 --> 00:10:04.550
for a sorry a 4A short time. Some had
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significant problems. They stem from the
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orthostatic hypotension as a result from
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the cardiovascular changes. Some of the
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changes in the inner ear with balance
00:10:14.959 --> 00:10:16.870
and knowing where you physically are,
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some mild weaknesses, etc. These changes
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are more exaggerated with long duration
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flight in the International Space
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Station. The vision problems are called
00:10:26.480 --> 00:10:30.069
SANS, SNS, which is an acronym for
00:10:30.079 --> 00:10:33.190
spaceflight associated neuroccular
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syndrome. Our lab is studying that as
00:10:36.320 --> 00:10:38.550
well. That's a whole other fascinating
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issue.
00:10:40.399 --> 00:10:42.470
I could tell you some fun stories about
00:10:42.480 --> 00:10:44.470
astronauts and how weird some of them
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feel when they get back. Maybe we need
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to get Heidi on the show.
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>> Maybe we do.
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>> Yeah. No, that's um that's uh she has
00:10:52.720 --> 00:10:54.389
another interesting comment actually
00:10:54.399 --> 00:10:57.350
about the uh about the uh Voyager Golden
00:10:57.360 --> 00:10:59.110
Record, but we might talk about that
00:10:59.120 --> 00:11:00.150
another time.
00:11:00.160 --> 00:11:01.670
>> Fair enough. Yeah. All right. Thank you,
00:11:01.680 --> 00:11:03.990
Heidi. That was fascinating. Yeah. Um
00:11:04.000 --> 00:11:05.990
what a what an amazing job working with
00:11:06.000 --> 00:11:08.710
all those incredible people
00:11:08.720 --> 00:11:10.230
trying to figure out how to deal with
00:11:10.240 --> 00:11:13.190
the zerog problem. But uh on Mars the
00:11:13.200 --> 00:11:15.990
gravity will also be an issue. So um
00:11:16.000 --> 00:11:17.829
there's there's a heck of a lot that
00:11:17.839 --> 00:11:21.590
needs to be sorted out before we um
00:11:21.600 --> 00:11:24.230
>> put people down there because it it it's
00:11:24.240 --> 00:11:25.829
so such a long trip to get there. It's
00:11:25.839 --> 00:11:27.350
not like you can go ah no this is no
00:11:27.360 --> 00:11:28.790
good and come straight back. It's not
00:11:28.800 --> 00:11:30.069
going to be that simple.
00:11:30.079 --> 00:11:31.430
>> No, that's right. Once you're on your
00:11:31.440 --> 00:11:33.030
way, you're on your way. And the only
00:11:33.040 --> 00:11:35.110
way back is to keep going.
00:11:35.120 --> 00:11:37.430
>> Yeah, exactly. Thanks for the question,
00:11:37.440 --> 00:11:40.310
John. Uh, well asked. And, uh, yeah,
00:11:40.320 --> 00:11:42.389
it's not going to be a snack, that's for
00:11:42.399 --> 00:11:44.870
sure. Let's, uh, move on to our next
00:11:44.880 --> 00:11:48.470
question from Dan. Hello, gentlemen. Dan
00:11:48.480 --> 00:11:50.870
from the Gold Coast here. Uh, now, I
00:11:50.880 --> 00:11:53.910
know you've been asked a million
00:11:53.920 --> 00:11:56.310
questions about black holes. Uh, but I
00:11:56.320 --> 00:11:57.990
do have a quick two-parter, and I'm
00:11:58.000 --> 00:11:59.269
hoping it's something you've never had
00:11:59.279 --> 00:12:02.069
to answer before. really quickly from
00:12:02.079 --> 00:12:05.190
the point when a black hole is born,
00:12:05.200 --> 00:12:06.710
birth, created, whatever you want to
00:12:06.720 --> 00:12:09.269
call it. Uh how quickly is that growing
00:12:09.279 --> 00:12:11.509
to become a let's say super massive
00:12:11.519 --> 00:12:12.790
black hole or just something a lot
00:12:12.800 --> 00:12:16.949
bigger? Um or is that not how black
00:12:16.959 --> 00:12:18.550
holes work and I'm not understanding it
00:12:18.560 --> 00:12:22.310
properly? two, uh, hypothetically, if
00:12:22.320 --> 00:12:24.949
there's no matter or energy or anything
00:12:24.959 --> 00:12:28.150
surrounding the black hole to take in
00:12:28.160 --> 00:12:31.509
and let's say eat, uh, is the black hole
00:12:31.519 --> 00:12:33.509
still going to grow? Is there more to
00:12:33.519 --> 00:12:36.470
the black hole growing than I
00:12:36.480 --> 00:12:39.269
understand? Um, yeah, hopefully that
00:12:39.279 --> 00:12:40.550
made sense and hopefully it's worth
00:12:40.560 --> 00:12:43.190
answering. Love the show. Love you guys
00:12:43.200 --> 00:12:45.509
work. Cheers. Bye.
00:12:45.519 --> 00:12:47.509
>> Thank you, Dan. Uh, nice to hear from
00:12:47.519 --> 00:12:50.470
you. Uh yeah, a couple of questions in
00:12:50.480 --> 00:12:52.710
that one. Um we never talk about black
00:12:52.720 --> 00:12:55.750
holes, but we will today. Uh speed of
00:12:55.760 --> 00:12:59.590
growth. Um that's an interesting one. Uh
00:12:59.600 --> 00:13:01.910
given that we're starting to think that
00:13:01.920 --> 00:13:06.470
there were some absolutely enormous
00:13:06.480 --> 00:13:09.430
um black holes in the early universe.
00:13:09.440 --> 00:13:13.350
Um and and that they're looking for more
00:13:13.360 --> 00:13:14.790
and more evidence to see what was going
00:13:14.800 --> 00:13:17.590
on early on. Um, but we've got some
00:13:17.600 --> 00:13:21.030
gargantuan ones still around. Uh, so how
00:13:21.040 --> 00:13:24.150
fast did they get that big? And I I I'm
00:13:24.160 --> 00:13:26.310
starting to think, Fred, it wouldn't be
00:13:26.320 --> 00:13:28.870
a stock standard approach.
00:13:28.880 --> 00:13:31.269
Maybe not. Maybe not. Uh, but well, I
00:13:31.279 --> 00:13:34.069
mean, Dan's asking uh one of the
00:13:34.079 --> 00:13:35.910
fundamental questions of astrophysics at
00:13:35.920 --> 00:13:37.829
the moment. This is a very hot topic.
00:13:37.839 --> 00:13:39.750
Yeah. And what set the cat among the
00:13:39.760 --> 00:13:41.590
pigeons and made it a hot topic is the
00:13:41.600 --> 00:13:44.790
James Web Space Telescope because um
00:13:44.800 --> 00:13:48.629
until that came along, the idea was that
00:13:48.639 --> 00:13:51.350
as basically as Dan suggests, black
00:13:51.360 --> 00:13:54.949
holes were formed in the early universe
00:13:54.959 --> 00:13:58.389
by exploding stars that um collapsed at
00:13:58.399 --> 00:14:00.470
the end of their lives to to form a
00:14:00.480 --> 00:14:02.470
black hole. the core would collapse to a
00:14:02.480 --> 00:14:05.750
black hole and that then over over
00:14:05.760 --> 00:14:07.990
billions of years that black hole would
00:14:08.000 --> 00:14:10.790
grow and eventually in our own epoch
00:14:10.800 --> 00:14:13.670
today 13.8 billion years after the after
00:14:13.680 --> 00:14:16.470
the big bang uh you have super massive
00:14:16.480 --> 00:14:17.990
black holes at the center of every
00:14:18.000 --> 00:14:21.110
galaxy. That was the old wisdom. But the
00:14:21.120 --> 00:14:22.710
James Webb telescope has turned that
00:14:22.720 --> 00:14:25.590
completely on its head because we have
00:14:25.600 --> 00:14:28.230
serious evidence of super massive black
00:14:28.240 --> 00:14:32.230
holes within the first 500 million years
00:14:32.240 --> 00:14:34.949
of the universe's existence. And that's
00:14:34.959 --> 00:14:39.110
too quick for or too short a time for
00:14:39.120 --> 00:14:42.389
this um you know the this slow accretion
00:14:42.399 --> 00:14:46.389
of of stuff uh as being the um the the
00:14:46.399 --> 00:14:49.110
the growth mechanism for black holes. Uh
00:14:49.120 --> 00:14:50.949
it's too too short a time for that to be
00:14:50.959 --> 00:14:55.910
the case. Uh so either our ideas of how
00:14:55.920 --> 00:14:59.350
fast they gobble up matter is wrong and
00:14:59.360 --> 00:15:01.269
they gobble up faster matter a lot
00:15:01.279 --> 00:15:02.870
faster than we thought. And we actually
00:15:02.880 --> 00:15:05.030
covered a story on this I think about
00:15:05.040 --> 00:15:07.670
four or five episodes ago because there
00:15:07.680 --> 00:15:10.069
are some scientists who came to
00:15:10.079 --> 00:15:11.990
conclusion that one of the things that
00:15:12.000 --> 00:15:15.189
we thought limited how fast a black hole
00:15:15.199 --> 00:15:17.509
can gobble stuff up uh was actually
00:15:17.519 --> 00:15:20.470
invalid under certain circumstances.
00:15:20.480 --> 00:15:23.750
>> So that's that's one avenue of research
00:15:23.760 --> 00:15:26.310
that's come from the James Web telescope
00:15:26.320 --> 00:15:28.150
showing us that we've got these super
00:15:28.160 --> 00:15:29.430
massive black holes in the early
00:15:29.440 --> 00:15:31.509
universe. But the other one is the the
00:15:31.519 --> 00:15:33.910
idea of the little pink dots or the
00:15:33.920 --> 00:15:35.990
little red dots as they're called. And
00:15:36.000 --> 00:15:39.829
these are thought to be basically just
00:15:39.839 --> 00:15:43.189
clouds of gas, hydrogen gas, which are
00:15:43.199 --> 00:15:46.150
directly feeding a black hole that may
00:15:46.160 --> 00:15:48.310
have been formed in the Big Bang. In
00:15:48.320 --> 00:15:49.910
other words, you didn't have to have
00:15:49.920 --> 00:15:52.870
star formation and then stars blowing up
00:15:52.880 --> 00:15:55.030
to create back black holes in order to
00:15:55.040 --> 00:15:57.350
kick this process off. the big bang
00:15:57.360 --> 00:15:59.110
itself might have kicked off the process
00:15:59.120 --> 00:16:00.949
of black hole formation by producing
00:16:00.959 --> 00:16:03.189
these things that we call primordial
00:16:03.199 --> 00:16:07.749
black holes. Um and they may have turned
00:16:07.759 --> 00:16:10.629
out to be able to grow very quickly uh
00:16:10.639 --> 00:16:13.749
by immersing themselves simply in big
00:16:13.759 --> 00:16:15.990
clouds of hydrogen and gobbling it all
00:16:16.000 --> 00:16:16.550
up.
00:16:16.560 --> 00:16:20.470
>> Yeah. Of course uh when they run out of
00:16:20.480 --> 00:16:23.189
stuff they can't grow. Is that right?
00:16:23.199 --> 00:16:25.269
>> That's right. So, that's part two of
00:16:25.279 --> 00:16:28.150
Dan's question. Uh, what happens when
00:16:28.160 --> 00:16:29.509
there's nothing there for them to eat?
00:16:29.519 --> 00:16:31.430
And they become what we call quiescent
00:16:31.440 --> 00:16:33.910
black holes. They they they don't do
00:16:33.920 --> 00:16:36.389
anything. They're there. Uh, and they're
00:16:36.399 --> 00:16:39.430
still things that um if if a cloud of
00:16:39.440 --> 00:16:42.389
hydrogen strayed by, they they might
00:16:42.399 --> 00:16:44.150
seize it by their own gravity and pull
00:16:44.160 --> 00:16:45.189
it in. Yeah.
00:16:45.199 --> 00:16:47.749
>> But, um, they're not going to go out
00:16:47.759 --> 00:16:49.910
roaming through the um roaming through
00:16:49.920 --> 00:16:51.990
the universe looking for stuff to
00:16:52.000 --> 00:16:53.590
accrete. In other words, looking for a
00:16:53.600 --> 00:16:54.310
snap.
00:16:54.320 --> 00:16:56.790
>> Yeah. I used to work with a guy whose
00:16:56.800 --> 00:16:58.629
nickname was queercent black hole. He
00:16:58.639 --> 00:17:03.189
was there, but he didn't do anything.
00:17:03.199 --> 00:17:08.390
>> Yes, I think I know who you mean.
00:17:08.400 --> 00:17:11.110
Yeah. Anyway, quent black holes are
00:17:11.120 --> 00:17:13.829
basically what what Dan has described.
00:17:13.839 --> 00:17:15.750
But the first part of his question is
00:17:15.760 --> 00:17:17.829
absolutely asking the same questions
00:17:17.839 --> 00:17:20.069
that today's astrophysicists are. It's
00:17:20.079 --> 00:17:22.630
one whose answer we don't know. But the
00:17:22.640 --> 00:17:24.549
contentus will emerge over the next
00:17:24.559 --> 00:17:26.309
probably not very long because we're
00:17:26.319 --> 00:17:28.230
getting so much data from the James Webb
00:17:28.240 --> 00:17:29.430
telescope
00:17:29.440 --> 00:17:30.870
>> uh that I think it'll be quite soon
00:17:30.880 --> 00:17:32.710
before this whole issue is resolved.
00:17:32.720 --> 00:17:34.630
>> I would think sorry
00:17:34.640 --> 00:17:36.470
>> I was just going to say when when there
00:17:36.480 --> 00:17:38.630
is hard evidence of a primordial black
00:17:38.640 --> 00:17:40.549
hole being discovered, one that was
00:17:40.559 --> 00:17:43.430
created in the Big Bang, then that'll be
00:17:43.440 --> 00:17:45.669
Nobel Prizewinning science when we get
00:17:45.679 --> 00:17:47.270
to that stage.
00:17:47.280 --> 00:17:48.310
>> But it won't be us.
00:17:48.320 --> 00:17:50.630
>> Indeed. I was going to suggest that um
00:17:50.640 --> 00:17:53.029
black holes are probably like humans.
00:17:53.039 --> 00:17:54.710
Consumption will decide how big they
00:17:54.720 --> 00:17:56.070
get.
00:17:56.080 --> 00:17:57.510
>> Maybe that's right.
00:17:57.520 --> 00:17:58.549
>> Yeah. Yeah.
00:17:58.559 --> 00:18:01.029
>> We'll have to wait and see. All right,
00:18:01.039 --> 00:18:03.029
Dan. Uh hopefully we covered that for
00:18:03.039 --> 00:18:05.590
you adequately. Thanks for sending in
00:18:05.600 --> 00:18:07.669
the question. This is Space Nuts with
00:18:07.679 --> 00:18:12.710
Andrew Dunley and Professor Fred Watson.
00:18:12.720 --> 00:18:15.510
>> Three, two, one.
00:18:15.520 --> 00:18:18.950
>> Space nuts. Our next question, Fred,
00:18:18.960 --> 00:18:21.830
comes from Thomas Reed. Thomas is 11
00:18:21.840 --> 00:18:23.909
years old. He says, "Something has been
00:18:23.919 --> 00:18:25.750
troubling me in books I've read. They
00:18:25.760 --> 00:18:28.390
say that the centers of galaxies are
00:18:28.400 --> 00:18:30.789
very big black holes, and I have a few
00:18:30.799 --> 00:18:32.870
questions about them, but I'm only an
00:18:32.880 --> 00:18:35.110
11year-old kid, so the questions might
00:18:35.120 --> 00:18:36.870
sound silly, but here they are. Now, we
00:18:36.880 --> 00:18:38.950
got five questions, Fred, so we can be
00:18:38.960 --> 00:18:41.029
brief on them on them, unless you want
00:18:41.039 --> 00:18:43.750
to sit here another couple of hours. Um,
00:18:43.760 --> 00:18:45.510
if Jy was here, we would be a couple of
00:18:45.520 --> 00:18:46.710
hours.
00:18:46.720 --> 00:18:49.510
Um, can the galactic centers swallow all
00:18:49.520 --> 00:18:51.909
the stars and planets in the galaxy? How
00:18:51.919 --> 00:18:54.230
big are the galactic centers or do we
00:18:54.240 --> 00:18:56.710
not know? Uh, if they can swallow up all
00:18:56.720 --> 00:18:59.270
the stars and planets, is there a limit?
00:18:59.280 --> 00:19:01.990
If there is a limit, what is it? And if
00:19:02.000 --> 00:19:04.230
there is a limit, what happens when the
00:19:04.240 --> 00:19:06.390
limit is reached? Thank you for taking
00:19:06.400 --> 00:19:08.150
the time to read this. And I would love
00:19:08.160 --> 00:19:09.990
it if you could reply. Well, we are
00:19:10.000 --> 00:19:13.750
going to reply right now, Thomas. Um,
00:19:13.760 --> 00:19:15.909
yeah, it's uh it's great that uh
00:19:15.919 --> 00:19:18.230
somebody so young is is taking a keen
00:19:18.240 --> 00:19:20.470
interest in something so mysterious as a
00:19:20.480 --> 00:19:23.270
as a black hole. Uh we want to start at
00:19:23.280 --> 00:19:25.029
the top. Can the galactic center swallow
00:19:25.039 --> 00:19:27.430
all the stars and planets in the galaxy?
00:19:27.440 --> 00:19:30.230
>> Well, so the answer is no. Um so the
00:19:30.240 --> 00:19:32.549
galaxies are very big. Um ours is about
00:19:32.559 --> 00:19:35.270
100,000 light years across. Uh, black
00:19:35.280 --> 00:19:38.549
holes have a a kind of sphere of
00:19:38.559 --> 00:19:41.510
influence um, which gravitationally
00:19:41.520 --> 00:19:43.430
stretches to the edge of the galaxy, but
00:19:43.440 --> 00:19:45.510
by the time you get there, the gravity
00:19:45.520 --> 00:19:47.270
of the black hole is very very weak
00:19:47.280 --> 00:19:50.630
indeed. Uh, and so it's only in the
00:19:50.640 --> 00:19:53.350
central region of a galaxy where you
00:19:53.360 --> 00:19:55.909
could get material being swallowed up
00:19:55.919 --> 00:19:58.470
uh, to create this activity that we talk
00:19:58.480 --> 00:19:59.830
about when we talk about active black
00:19:59.840 --> 00:20:03.029
holes. uh where there's uh an accretion
00:20:03.039 --> 00:20:05.270
disc, a disc of material swirling around
00:20:05.280 --> 00:20:08.070
it and these jets that point basically
00:20:08.080 --> 00:20:09.750
at right angles to the accretion disc.
00:20:09.760 --> 00:20:11.510
Jets of material traveling at nearly the
00:20:11.520 --> 00:20:13.590
speed of light. Quite extraordinary.
00:20:13.600 --> 00:20:16.549
>> So, um that's all great and a black hole
00:20:16.559 --> 00:20:18.390
is like a factory or a furnace doing
00:20:18.400 --> 00:20:20.870
that, but it's it stretch is not very
00:20:20.880 --> 00:20:24.070
far. Uh it's measured in light years,
00:20:24.080 --> 00:20:25.590
but not in hundreds of thousands of
00:20:25.600 --> 00:20:27.669
light years, which you'd have to be to
00:20:27.679 --> 00:20:29.669
to grab everything in the galaxy. So the
00:20:29.679 --> 00:20:32.310
answer is no. Uh the galactic center
00:20:32.320 --> 00:20:34.630
black hole cannot swallow all the stars
00:20:34.640 --> 00:20:36.630
and planets in the galaxy.
00:20:36.640 --> 00:20:39.190
>> So So Thomas can sleep well tonight. Um
00:20:39.200 --> 00:20:41.350
how big are the galactic centers? Do we
00:20:41.360 --> 00:20:43.830
know how big?
00:20:43.840 --> 00:20:47.270
>> We do. Yes, we do because we can measure
00:20:47.280 --> 00:20:50.470
we can measure the uh the speed of
00:20:50.480 --> 00:20:54.070
rotation of stuff swirling around a
00:20:54.080 --> 00:20:56.310
black hole if it's an active one.
00:20:56.320 --> 00:20:58.470
>> Yeah. And that directly tells you the
00:20:58.480 --> 00:21:01.830
mass of the black hole. Um because the
00:21:01.840 --> 00:21:03.510
bigger the black hole the faster the
00:21:03.520 --> 00:21:07.110
stuff is going. And so um in terms of
00:21:07.120 --> 00:21:10.549
you know if the if if by big Thomas
00:21:10.559 --> 00:21:13.669
means what's their mass uh we can we can
00:21:13.679 --> 00:21:16.070
measure them quite accurately. Now
00:21:16.080 --> 00:21:18.310
because we can measure their mass we can
00:21:18.320 --> 00:21:20.870
also work out their event horizon
00:21:20.880 --> 00:21:24.310
diameter or radius. The event horizon is
00:21:24.320 --> 00:21:26.870
that sort of imaginary sphere around a
00:21:26.880 --> 00:21:29.510
black hole beyond which light cannot
00:21:29.520 --> 00:21:32.230
escape and so it would appear as a dark
00:21:32.240 --> 00:21:35.029
sphere. Um so the event horizon is the
00:21:35.039 --> 00:21:36.950
point of no return for anything going
00:21:36.960 --> 00:21:39.110
into a black hole and it's also the
00:21:39.120 --> 00:21:42.870
point of no escape for for light waves.
00:21:42.880 --> 00:21:45.270
Uh so we can knowing the mass of a black
00:21:45.280 --> 00:21:48.310
hole we can calculate how big that event
00:21:48.320 --> 00:21:50.390
horizon would be. And some of the super
00:21:50.400 --> 00:21:52.950
massive ones are really very big.
00:21:52.960 --> 00:21:55.029
They're measured in light years, tens of
00:21:55.039 --> 00:21:56.310
light years perhaps for the super
00:21:56.320 --> 00:21:57.510
massive black holes.
00:21:57.520 --> 00:22:00.230
>> Yeah, that it's it's a level of enormity
00:22:00.240 --> 00:22:01.990
that you just struggle to get your head
00:22:02.000 --> 00:22:02.630
around.
00:22:02.640 --> 00:22:04.390
>> Yeah. I suppose in terms of the rest of
00:22:04.400 --> 00:22:06.630
Thomas's questions, you've basically
00:22:06.640 --> 00:22:08.710
answered it with the answer to the first
00:22:08.720 --> 00:22:10.390
question cuz he's asking if they can
00:22:10.400 --> 00:22:12.310
swallow all the stars and planets. Is
00:22:12.320 --> 00:22:14.390
there a limit? If there is a limit, what
00:22:14.400 --> 00:22:17.110
is it? Uh and if there is a limit, what
00:22:17.120 --> 00:22:19.190
happens when the limit is reached? Well,
00:22:19.200 --> 00:22:23.430
the limit is probably the local area of
00:22:23.440 --> 00:22:25.590
the center of the galaxy and what's
00:22:25.600 --> 00:22:27.029
available to eat.
00:22:27.039 --> 00:22:28.950
>> Yes, that's right. So the the limit the
00:22:28.960 --> 00:22:33.669
limiting factor is um basically the the
00:22:33.679 --> 00:22:35.110
what you might call the grasp of the
00:22:35.120 --> 00:22:37.830
black hole. How how far it can reach to
00:22:37.840 --> 00:22:40.870
pull something in. And that is dependent
00:22:40.880 --> 00:22:43.510
on how fast the objects are moving. So
00:22:43.520 --> 00:22:45.270
you can have some stars and there are
00:22:45.280 --> 00:22:47.190
some we've observed them uh with
00:22:47.200 --> 00:22:50.310
infrared radiation that are comfortably
00:22:50.320 --> 00:22:54.789
in orbit uh around the the black hole at
00:22:54.799 --> 00:22:56.870
the center of our own galaxy which are
00:22:56.880 --> 00:22:58.710
not being pulled in. They're orbiting
00:22:58.720 --> 00:23:00.390
and that's because their speed is enough
00:23:00.400 --> 00:23:02.470
to keep them out of the out of the grasp
00:23:02.480 --> 00:23:05.270
of the black hole. um their distances
00:23:05.280 --> 00:23:07.510
from the black hole are measured, you
00:23:07.520 --> 00:23:09.510
know, in not two dissimilar units from
00:23:09.520 --> 00:23:11.430
the from the solar system, sort of half
00:23:11.440 --> 00:23:14.230
a light day or something like that, you
00:23:14.240 --> 00:23:17.430
know, light light day. That's that's the
00:23:17.440 --> 00:23:18.789
sort of measures that we're talking
00:23:18.799 --> 00:23:19.830
about.
00:23:19.840 --> 00:23:22.870
>> Um which probably denies what I just
00:23:22.880 --> 00:23:25.270
said a few minutes ago about um some
00:23:25.280 --> 00:23:27.750
black hole event horizons being tens of
00:23:27.760 --> 00:23:29.110
light years. I don't think they are. I
00:23:29.120 --> 00:23:30.390
think they're smaller than that.
00:23:30.400 --> 00:23:32.390
>> Okay. I've thought of a way to explain
00:23:32.400 --> 00:23:34.470
it to Thomas. say, "Uh, Thomas, you've
00:23:34.480 --> 00:23:37.510
won a competition and you can go to
00:23:37.520 --> 00:23:40.549
McDonald's and eat everything you want."
00:23:40.559 --> 00:23:43.029
Absolutely. Just keep eating until you
00:23:43.039 --> 00:23:45.830
know the cows come home. However, you
00:23:45.840 --> 00:23:47.830
aren't allowed to move from wherever
00:23:47.840 --> 00:23:49.510
you're standing and you can only eat
00:23:49.520 --> 00:23:52.230
what's within reach.
00:23:52.240 --> 00:23:54.870
Once you run out of food, you stop
00:23:54.880 --> 00:23:57.270
growing. And you're the black hole, by
00:23:57.280 --> 00:23:59.350
the way. How's that for an analogy?
00:23:59.360 --> 00:24:00.630
>> It's a nice one. I like it.
00:24:00.640 --> 00:24:03.270
>> Yes. Yeah. Because the your reach is the
00:24:03.280 --> 00:24:04.549
sort of gravitational
00:24:04.559 --> 00:24:04.950
>> Yeah.
00:24:04.960 --> 00:24:06.470
>> force that you can exert. Yeah, it's a
00:24:06.480 --> 00:24:07.750
good way of putting it, Andrew. Well
00:24:07.760 --> 00:24:08.950
done. You should be on the reach.
00:24:08.960 --> 00:24:11.110
>> I try to think on 11y old level, but I'm
00:24:11.120 --> 00:24:12.789
I'm thinking Thomas was probably much
00:24:12.799 --> 00:24:15.430
brighter at 11 than I was.
00:24:15.440 --> 00:24:17.669
>> Struggle to get to 11. So do I.
00:24:17.679 --> 00:24:19.990
>> Yes. Thanks, Thomas. That was really
00:24:20.000 --> 00:24:21.750
terrific. Thanks for sending it in. And
00:24:21.760 --> 00:24:25.830
uh keep on listening.
00:24:25.840 --> 00:24:27.830
>> Swiftity
00:24:27.840 --> 00:24:30.390
base here. The angle has landed. Space
00:24:30.400 --> 00:24:31.430
Nuts.
00:24:31.440 --> 00:24:35.190
>> Final question, Fred, comes from Paul.
00:24:35.200 --> 00:24:37.269
Hello, Space Nuts. Paul here from sunny
00:24:37.279 --> 00:24:38.630
Bris Vegas, where it's currently
00:24:38.640 --> 00:24:40.950
bucketing down in what is being
00:24:40.960 --> 00:24:45.269
described as a rare rain occurrence.
00:24:45.279 --> 00:24:47.190
Anyway,
00:24:47.200 --> 00:24:50.470
I am currently looking through a very
00:24:50.480 --> 00:24:53.510
old book of mine. Guess it's old
00:24:53.520 --> 00:24:56.149
compared to the students I teach. It was
00:24:56.159 --> 00:24:58.549
published back in 1978. I think I got in
00:24:58.559 --> 00:25:01.909
in 1980 from uh an uncle of mine, Uncle
00:25:01.919 --> 00:25:03.510
Jim. Thank you very much. It's called
00:25:03.520 --> 00:25:05.269
Stars and Planets, and it's probably
00:25:05.279 --> 00:25:09.110
what got me into the whole field of
00:25:09.120 --> 00:25:11.510
astronomy in the first place, at least
00:25:11.520 --> 00:25:16.070
my interest in astronomy, obviously. Uh
00:25:16.080 --> 00:25:18.870
very very grateful. I'm on the page
00:25:18.880 --> 00:25:20.870
where it's talking about how the
00:25:20.880 --> 00:25:24.870
American astronomer Harlo Shepley
00:25:24.880 --> 00:25:28.950
used the 1.5 m reflector on top of Mount
00:25:28.960 --> 00:25:31.750
Wilson in California
00:25:31.760 --> 00:25:35.510
to work out that our sun is not at the
00:25:35.520 --> 00:25:37.590
center of our galaxy as was previously
00:25:37.600 --> 00:25:39.990
thought, but is about 2/3 of the way to
00:25:40.000 --> 00:25:43.909
the edge. Could you please give us some
00:25:43.919 --> 00:25:48.789
idea how he actually managed to do that?
00:25:48.799 --> 00:25:52.230
Was it something about the density of
00:25:52.240 --> 00:25:55.269
stars? I mean, how many stars in the
00:25:55.279 --> 00:25:57.350
field of view uh when you point it one
00:25:57.360 --> 00:25:59.669
way compared to the other? How did he do
00:25:59.679 --> 00:26:01.909
it? I'm really curious. And I know I
00:26:01.919 --> 00:26:03.750
could Google it, but I'd rather hear it
00:26:03.760 --> 00:26:07.029
from you guys. So, thanks in advance.
00:26:07.039 --> 00:26:10.870
love the show and dare I say, keep up
00:26:10.880 --> 00:26:13.510
the good work. Cheers.
00:26:13.520 --> 00:26:15.430
>> Cheers, Paul. Thanks for sending that
00:26:15.440 --> 00:26:18.549
in, uh, sending the question in and, uh,
00:26:18.559 --> 00:26:21.669
we don't know the answer. So,
00:26:21.679 --> 00:26:24.710
but we're going to Google it. No. Um,
00:26:24.720 --> 00:26:28.149
1978, Stars and Planets. Uh, I tried to
00:26:28.159 --> 00:26:30.710
look it up. There are teen books named
00:26:30.720 --> 00:26:31.830
Stars and Planets.
00:26:31.840 --> 00:26:32.230
>> Yeah.
00:26:32.240 --> 00:26:34.390
>> So, I haven't been able to, you know,
00:26:34.400 --> 00:26:36.310
distinguish one from the other as yet.
00:26:36.320 --> 00:26:39.590
So um uh yeah, you'll have to do some
00:26:39.600 --> 00:26:41.830
fishing to find the book that Paul was
00:26:41.840 --> 00:26:44.789
talking about. But he wanted to know
00:26:44.799 --> 00:26:48.470
about the man who decided or discovered
00:26:48.480 --> 00:26:50.470
that the sun was not the center of
00:26:50.480 --> 00:26:53.990
everything. Uh which was a common belief
00:26:54.000 --> 00:26:55.830
back in the day.
00:26:55.840 --> 00:26:58.470
>> It was um it was actually 1919 when that
00:26:58.480 --> 00:26:59.909
discovery was made. Um
00:26:59.919 --> 00:27:01.590
>> is it was it that recent?
00:27:01.600 --> 00:27:04.390
>> Yeah. Um I I it's one of my favorite
00:27:04.400 --> 00:27:06.070
astronomical discoveries, which is why I
00:27:06.080 --> 00:27:07.830
didn't need to go to Google to look it
00:27:07.840 --> 00:27:11.990
up. Um so it goes back to the time of
00:27:12.000 --> 00:27:16.070
William Hershel, uh who was a
00:27:16.080 --> 00:27:19.269
German turned British astronomer,
00:27:19.279 --> 00:27:22.070
worked late in the 18th century and
00:27:22.080 --> 00:27:23.750
early in the 19th century. He discovered
00:27:23.760 --> 00:27:26.710
the planet Uranus in 1781.
00:27:26.720 --> 00:27:28.470
But what he was doing when he discovered
00:27:28.480 --> 00:27:30.789
Uranus was actually mapping the Milky
00:27:30.799 --> 00:27:34.630
Way. He was observing uh the the Milky
00:27:34.640 --> 00:27:36.950
Way in a very systematic way with a
00:27:36.960 --> 00:27:39.350
relatively small telescope. So he sort
00:27:39.360 --> 00:27:42.870
of counting stars in the field of view
00:27:42.880 --> 00:27:44.710
of his telescope and then moving the
00:27:44.720 --> 00:27:46.549
telescope a bit further along the Milky
00:27:46.559 --> 00:27:48.789
Way. Counting stars again, how many he
00:27:48.799 --> 00:27:51.110
could see in the field of view and doing
00:27:51.120 --> 00:27:52.870
that and doing it. He couldn't do it all
00:27:52.880 --> 00:27:54.149
the way around the Milky Way because
00:27:54.159 --> 00:27:55.590
there's parts of it that he he could
00:27:55.600 --> 00:27:56.630
never see because they're in the
00:27:56.640 --> 00:27:58.870
southern hemisphere. But he got round
00:27:58.880 --> 00:28:01.430
most of it. And what he discovered was
00:28:01.440 --> 00:28:04.950
that the star counts are pretty even all
00:28:04.960 --> 00:28:06.789
the way around.
00:28:06.799 --> 00:28:09.909
>> And so that led him to build the
00:28:09.919 --> 00:28:12.470
hypothesis that the stars are in a sort
00:28:12.480 --> 00:28:15.110
of flattened disc, which is correct, uh,
00:28:15.120 --> 00:28:17.029
but that we're very near the middle,
00:28:17.039 --> 00:28:20.710
which is not correct. And the reason why
00:28:20.720 --> 00:28:23.269
he got that erroneous answer was that
00:28:23.279 --> 00:28:25.269
when you look through a I think it was a
00:28:25.279 --> 00:28:28.149
7-in telescope if I remember rightly a
00:28:28.159 --> 00:28:30.710
telescope of that size at the Milky Way,
00:28:30.720 --> 00:28:33.430
the stars that you see are all
00:28:33.440 --> 00:28:36.549
relatively nearby. They're perhaps a
00:28:36.559 --> 00:28:38.070
thousand light years away or something
00:28:38.080 --> 00:28:40.630
like that, maybe a bit more, maybe a
00:28:40.640 --> 00:28:42.310
couple of thousand light years away in
00:28:42.320 --> 00:28:44.470
the plane of the Milky Way. And that's
00:28:44.480 --> 00:28:46.389
partly because the Milky Way is very
00:28:46.399 --> 00:28:48.549
dusty. Uh there's a lot of dust
00:28:48.559 --> 00:28:50.070
everywhere. It's probably better
00:28:50.080 --> 00:28:52.389
described as smoke, but we call it dust
00:28:52.399 --> 00:28:54.870
in the world of astronomy. And so that
00:28:54.880 --> 00:28:57.750
dust limits how far you can see. And so
00:28:57.760 --> 00:28:59.669
when you look at the Milky Way, it does
00:28:59.679 --> 00:29:01.909
look generally relatively even. There's
00:29:01.919 --> 00:29:03.430
one bit in the constellation of
00:29:03.440 --> 00:29:05.830
Sagittarius where it's it's brighter and
00:29:05.840 --> 00:29:07.430
that's because you are looking towards
00:29:07.440 --> 00:29:09.830
as we now know the galactic center. But
00:29:09.840 --> 00:29:12.789
um Hershel um he couldn't see that very
00:29:12.799 --> 00:29:13.990
well from the northern hemisphere
00:29:14.000 --> 00:29:16.870
anyway. But he did sort of discount that
00:29:16.880 --> 00:29:19.990
uh he said by and large it's the same
00:29:20.000 --> 00:29:21.830
count all the way around. So we must be
00:29:21.840 --> 00:29:25.590
in the middle. Uh roll on the the years
00:29:25.600 --> 00:29:28.710
and in 1919 Harlo Shappley a very gifted
00:29:28.720 --> 00:29:30.310
American astronomer although he did get
00:29:30.320 --> 00:29:33.350
one thing one big thing wrong. Uh but
00:29:33.360 --> 00:29:36.389
what he did was he was interested in
00:29:36.399 --> 00:29:38.630
objects that we call globular clusters.
00:29:38.640 --> 00:29:40.389
And so these are in fact they were named
00:29:40.399 --> 00:29:42.149
by William Hershel. He gave them that
00:29:42.159 --> 00:29:44.310
name clusters of stars that appear like
00:29:44.320 --> 00:29:49.110
a globe. Uh and uh her halos Shappley
00:29:49.120 --> 00:29:52.230
was uh obser he like he was interested
00:29:52.240 --> 00:29:54.149
in globular clusters. He noticed there
00:29:54.159 --> 00:29:59.350
were a lot of them in our skies. Uh they
00:29:59.360 --> 00:30:02.230
tended to be different sizes.
00:30:02.240 --> 00:30:04.549
Uh and he didn't know whether that was
00:30:04.559 --> 00:30:06.230
cuz they were all the same size and some
00:30:06.240 --> 00:30:08.070
were nearer than others or whether they
00:30:08.080 --> 00:30:10.549
were intrinsically different sizes. But
00:30:10.559 --> 00:30:12.789
what he did notice was that there's a
00:30:12.799 --> 00:30:15.990
concentration of them in the southern
00:30:16.000 --> 00:30:19.350
hemisphere sky. Uh he was observing from
00:30:19.360 --> 00:30:21.590
California, so he could see a fair swath
00:30:21.600 --> 00:30:23.909
of the southern hemisphere sky. But he
00:30:23.919 --> 00:30:26.230
he noticed that they were concentrated
00:30:26.240 --> 00:30:28.389
in that direction and that made him
00:30:28.399 --> 00:30:32.310
wonder if that was where the center of
00:30:32.320 --> 00:30:34.310
the galaxy lay rather than us being near
00:30:34.320 --> 00:30:38.149
the center. Uh but then his other step
00:30:38.159 --> 00:30:41.110
was that he recognized that within these
00:30:41.120 --> 00:30:43.590
globular clusters were something called
00:30:43.600 --> 00:30:46.710
clust they called them cluster variables
00:30:46.720 --> 00:30:49.430
stars that varied in a certain way on a
00:30:49.440 --> 00:30:52.470
with a periodicity of about a day. Uh
00:30:52.480 --> 00:30:55.110
today we call them rli variables and I
00:30:55.120 --> 00:30:56.549
actually started my astronomical
00:30:56.559 --> 00:30:58.710
research back in the 70s studying these
00:30:58.720 --> 00:31:03.669
things. uh rlari variables uh and they
00:31:03.679 --> 00:31:07.750
they are good because they've got a
00:31:07.760 --> 00:31:11.269
basically a known distance uh if you if
00:31:11.279 --> 00:31:13.830
you can see an RLI variable and identify
00:31:13.840 --> 00:31:16.149
it as one you know how intrinsically
00:31:16.159 --> 00:31:19.110
bright it is uh and then from that you
00:31:19.120 --> 00:31:21.750
can work out how far away it is. And so
00:31:21.760 --> 00:31:24.149
he found these variable stars in the
00:31:24.159 --> 00:31:27.269
globular clusters and recognized that he
00:31:27.279 --> 00:31:29.830
could draw a chart with the the globular
00:31:29.840 --> 00:31:32.310
clusters all at their correct distance
00:31:32.320 --> 00:31:34.230
on it, make a kind of three-dimensional
00:31:34.240 --> 00:31:37.590
map of the sky. And sure enough, um they
00:31:37.600 --> 00:31:40.710
concentrated around the galactic center
00:31:40.720 --> 00:31:43.190
around a point. Uh he actually got the
00:31:43.200 --> 00:31:45.269
answer wrong because his magnitude, his
00:31:45.279 --> 00:31:47.509
brightness that he had for the uh
00:31:47.519 --> 00:31:50.310
cluster variables was incorrect. uh and
00:31:50.320 --> 00:31:51.990
I can't remember what answer he got, but
00:31:52.000 --> 00:31:55.909
in modern parliament it's about 25,000
00:31:55.919 --> 00:31:58.870
light years. The cluster, the globular
00:31:58.880 --> 00:32:00.870
clusters themselves cluster around a
00:32:00.880 --> 00:32:03.830
point about 25,000 light years away,
00:32:03.840 --> 00:32:05.750
which is deeply hidden by the dust
00:32:05.760 --> 00:32:08.230
clouds in Sagittarius. So
00:32:08.240 --> 00:32:10.149
>> he figured out that that's where the
00:32:10.159 --> 00:32:12.149
center of the galaxy was. A brilliant
00:32:12.159 --> 00:32:14.149
piece of detective work. We know he was
00:32:14.159 --> 00:32:17.350
right. Uh what he was wrong about was uh
00:32:17.360 --> 00:32:21.830
he had a big discussion I think in 1923
00:32:21.840 --> 00:32:24.310
just before Hubble recognized that
00:32:24.320 --> 00:32:26.389
galaxies were big things a long way
00:32:26.399 --> 00:32:28.549
away. Uh Shappley was arguing that
00:32:28.559 --> 00:32:31.029
galaxies lie within our own Milky Way
00:32:31.039 --> 00:32:32.950
that they're small objects in our own
00:32:32.960 --> 00:32:36.389
Milky Way. And he was um arguing it was
00:32:36.399 --> 00:32:37.990
a public debate actually between
00:32:38.000 --> 00:32:40.870
Chappley and a guy called Hea Curtis. Uh
00:32:40.880 --> 00:32:42.389
Curtis had the answer right. He said
00:32:42.399 --> 00:32:44.789
they're big and a long way off. Uh
00:32:44.799 --> 00:32:46.470
Shappley said, "No, they're small and
00:32:46.480 --> 00:32:48.630
nearby." And it was very soon after that
00:32:48.640 --> 00:32:50.070
that Hubble produced that they're big
00:32:50.080 --> 00:32:52.470
and a long way proved that they're big
00:32:52.480 --> 00:32:53.669
and a long way off.
00:32:53.679 --> 00:32:54.070
>> Yeah.
00:32:54.080 --> 00:32:55.430
>> So Shappley was wrong in that, but he
00:32:55.440 --> 00:32:57.830
was right about the Galactic Center.
00:32:57.840 --> 00:33:00.950
Fantastic. Gee whiz. Um great question,
00:33:00.960 --> 00:33:04.389
Paul. And um yeah, if people are looking
00:33:04.399 --> 00:33:06.710
for that uh that book, Stars and
00:33:06.720 --> 00:33:09.190
Planets, uh it is out there. Uh, look,
00:33:09.200 --> 00:33:10.870
I've I've found a couple that were
00:33:10.880 --> 00:33:13.029
actually published around that time that
00:33:13.039 --> 00:33:15.430
Paul mentioned, but um not sure if
00:33:15.440 --> 00:33:17.110
they're the ones I I can't remember the
00:33:17.120 --> 00:33:19.350
author now um that he said, but
00:33:19.360 --> 00:33:20.950
>> I don't think he mentioned an author,
00:33:20.960 --> 00:33:21.269
did he?
00:33:21.279 --> 00:33:22.870
>> I thought he did, but uh No, he might
00:33:22.880 --> 00:33:25.190
have mentioned an uncle
00:33:25.200 --> 00:33:27.430
mention
00:33:27.440 --> 00:33:28.070
it.
00:33:28.080 --> 00:33:30.710
>> But um
00:33:30.720 --> 00:33:32.789
um so yeah, thanks Paul. Thanks for the
00:33:32.799 --> 00:33:34.950
the question. And um yeah, it's it's a
00:33:34.960 --> 00:33:37.590
fascinating um history in astronomy as
00:33:37.600 --> 00:33:39.269
we discover these things. I think one of
00:33:39.279 --> 00:33:40.950
my favorite
00:33:40.960 --> 00:33:43.509
>> moments I suppose in in astronomical
00:33:43.519 --> 00:33:45.669
history was when they discovered that
00:33:45.679 --> 00:33:48.630
our sun was a star.
00:33:48.640 --> 00:33:50.630
>> Yeah, that was a long long time ago.
00:33:50.640 --> 00:33:51.190
>> Yeah.
00:33:51.679 --> 00:33:53.990
>> But for a while there we didn't think of
00:33:54.000 --> 00:33:54.389
it like that.
00:33:54.399 --> 00:33:55.430
>> Thought it was something else. That's
00:33:55.440 --> 00:33:57.909
right. Something bit special.
00:33:57.919 --> 00:34:00.950
>> Yeah. Um, and and I I saw that on a BBC
00:34:00.960 --> 00:34:02.630
documentary many years ago, and I sat
00:34:02.640 --> 00:34:05.669
there and went, "Wow, I never thought
00:34:05.679 --> 00:34:07.430
about that cuz I've always known it to
00:34:07.440 --> 00:34:10.629
be a star, but for generations, they
00:34:10.639 --> 00:34:12.550
didn't."
00:34:12.560 --> 00:34:14.869
Quite quite intriguing. And why would
00:34:14.879 --> 00:34:16.790
you? It doesn't look like a star.
00:34:16.800 --> 00:34:20.389
>> That's That's right. Uh, it's uh it's
00:34:20.399 --> 00:34:24.069
clearly quite different from a star.
00:34:24.079 --> 00:34:25.669
>> Incredible. Thanks, Paul. Thanks for
00:34:25.679 --> 00:34:27.349
sending that in. And if you have a
00:34:27.359 --> 00:34:29.190
question for a thanks to all our
00:34:29.200 --> 00:34:31.510
senderiners, I've always wanted to say
00:34:31.520 --> 00:34:33.430
that uh for their questions. And if you
00:34:33.440 --> 00:34:34.950
would like to send a question, go to our
00:34:34.960 --> 00:34:37.109
website spaceenutspodcast.com
00:34:37.119 --> 00:34:39.190
or spacenuts.io
00:34:39.200 --> 00:34:42.149
and there's a little AMA tab at the top
00:34:42.159 --> 00:34:44.710
which stands for ask me anything. Not me
00:34:44.720 --> 00:34:48.629
personally, it's the royal me. And um
00:34:48.639 --> 00:34:50.710
just put your uh question in there. It
00:34:50.720 --> 00:34:52.629
can be text or audio. Don't forget to
00:34:52.639 --> 00:34:53.829
tell us who you are and where you're
00:34:53.839 --> 00:34:55.109
from and have a look around while you're
00:34:55.119 --> 00:34:57.829
there. Don't forget to leave a review at
00:34:57.839 --> 00:35:00.550
your favorite podcasting platform. We're
00:35:00.560 --> 00:35:02.150
all done. Thanks, Fred.
00:35:02.160 --> 00:35:05.030
>> A great pleasure, Andrew. We um we uh
00:35:05.040 --> 00:35:07.349
continue to get great questions from
00:35:07.359 --> 00:35:09.109
great listeners and long may it
00:35:09.119 --> 00:35:09.990
continue. Thank you.
00:35:10.000 --> 00:35:12.310
>> Yes, indeed. We we continue to solve and
00:35:12.320 --> 00:35:13.829
evolve.
00:35:13.839 --> 00:35:15.430
Um maybe not.
00:35:15.440 --> 00:35:18.069
>> I'm not evolving.
00:35:18.079 --> 00:35:20.390
>> When once you reach a certain certain
00:35:20.400 --> 00:35:22.630
age, evolving just is not part of the
00:35:22.640 --> 00:35:23.270
program.
00:35:23.280 --> 00:35:24.069
>> That's right.
00:35:24.079 --> 00:35:26.630
>> Yeah. Ask my mom in the internet. Uh,
00:35:26.640 --> 00:35:28.390
thanks Fred. We'll see you soon.
00:35:28.400 --> 00:35:29.750
>> Sounds great. Thanks.
00:35:29.760 --> 00:35:31.430
>> Professor Fred Watson, astronomer at
00:35:31.440 --> 00:35:32.950
large. And thanks to Hugh in the studio.
00:35:32.960 --> 00:35:35.990
He's just turned up. Um, we started 39
00:35:36.000 --> 00:35:38.790
minutes ago. And and um, Hugh set his
00:35:38.800 --> 00:35:41.109
clock to a Martian day. So that's why
00:35:41.119 --> 00:35:43.750
he's 39 minutes late. Boom. Boom. And
00:35:43.760 --> 00:35:45.349
from me, Andrew Dunley, thanks for your
00:35:45.359 --> 00:35:46.950
company. We'll see you on the next
00:35:46.960 --> 00:35:48.950
episode of Space Nuts. Bye-bye.
00:35:48.960 --> 00:35:51.270
>> Space Nuts. You've been listening to the
00:35:51.280 --> 00:35:54.310
Space Nuts podcast. Missing complete
00:35:54.320 --> 00:35:57.270
>> available at Apple Podcasts, Spotify,
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iHeart Radio, or your favorite podcast
00:35:59.920 --> 00:36:02.310
player. You can also stream on demand at
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00:36:05.200 --> 00:36:09.720
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