Cosmic Questions, Solar Mysteries & Lunar Dreams: #492 - The Great Space Q&A | Space Nuts
Space Nuts Episode 492: Tidal Locking, Solar Mysteries, and Moon Travel
Join Andrew Dunkley and Professor Jonti Horner in this engaging Q&A edition of Space Nuts, where they tackle a variety of cosmic questions from our curious listeners. From the complexities of tidal locking in celestial systems to the intriguing heat discrepancies in the Sun's layers, and even how to get to the Moon, this episode is filled with fascinating insights that will deepen your understanding of the universe.
Episode Highlights:
- Tidal Locking Explained: Jake from Tennessee asks about the possibility of tidal locking between stars and their orbiting planets. Jonti dives into the mechanics of tidal interactions, using examples from our own solar system, including the Earth-Moon relationship and Pluto's moons.
- Solar Mysteries: Clint from Georgia raises a thought-provoking question about the Sun's corona, which is millions of degrees hotter than its surface. Andrew and Jonti explore the latest theories on how gravitational interactions and magnetic fields could contribute to this phenomenon.
- How to Get to the Moon : Emily from Melbourne wants to know how humans travel to the Moon. Jonti breaks down the journey, explaining the rocket science behind space travel, the challenges of exiting Earth's atmosphere, and the exciting prospects of future lunar missions.
- Listener Engagement: Andrew and Jonti encourage listeners to submit their own questions, highlighting the importance of curiosity in the scientific community.
For more Space Nuts, including our continually updating newsfeed and to listen to all our episodes, visit our website (https://www.spacenutspodcast.com/about)
Stay curious, keep looking up, and join us next time for more stellar insights and cosmic wonders. Until then, clear skies and happy stargazing.
00:00 - Introduction to the episode and topics
02:15 - Discussion on tidal locking and celestial mechanics
10:30 - Insights into the Sun's corona and heat discrepancies
18:00 - How to travel to the Moon explained
26:45 - Listener Ash engagement and questions
30:00 - Closing thoughts and future episodes
✍️ Episode References
NASA's Lunar Missions
Tidal Locking
https://en.wikipedia.org/wiki/Tidal_locking
Solar Corona Studies
https://www.nasa.gov/solar-system/
Become a supporter of this podcast: https://www.spreaker.com/podcast/space-nuts--2631155/support (https://www.spreaker.com/podcast/space-nuts--2631155/support?utm_source=rss&utm_medium=rss&utm_campaign=rss) .
Episode link: https://play.headliner.app/episode/25385855?utm_source=youtube
00:00 - Introduction to the episode and topics
02:15 - Discussion on tidal locking and celestial mechanics
10:30 - Insights into the Sun’s corona and heat discrepancies
18:00 - How to travel to the Moon explained
26:45 - Listener Ash engagement and questions
30:00 - Closing thoughts and future episodes
Kind: captions
Language: en
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hi there Andrew Dunley here and you're
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listening to Space Nuts Q&A Edition glad
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to have your company once again uh on
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this episode we will be uh answering an
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array of questions on very different
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topics uh Jake is asking us about tidal
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lock uh that's not something to hold
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back the water in the temps River no uh
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something completely different uh Clint
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wants to talk about the heat of the sun
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uh Emily uh sand daughter in Melbourne
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wants to get to the moon and we're going
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to tell her how and Fenton has asked a
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vast array of questions which could
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probably fill an episode on their own
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about the radiation of Jupiter that's
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all coming up on this edition of Space
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Nuts 15 seconds guidance is internal 10
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9 ignition sequence start space Nets 5 4
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3 2 1 2 3 4 5 5 4 3 2 1 Space Nuts asut
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reported feels good and joining me once
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again is not Professor Fred Watson
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because he is overseas looking at the
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sky up in the northern hemisphere uh but
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with us is Professor johy Horner
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professor of astrophysics at the
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University of Southern Queensland jonty
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hello hey how you going I am well we're
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working on getting you your own intro
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but with we we're we're in a time of
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year where all the radio stations in
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Australia uh want new jingles and our um
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Studio producer who does all that work
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is um is flat out at the moment so we've
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been put on the back burner I think but
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you can understand why all the radio
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stations want to ramp up how they sound
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so that they can get new audience I
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worked in radio for 40 years I'm pretty
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sure changing the jingle doesn't
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actually do much but just my just my
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observation in proba get it just in time
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for Fred to get back yes yes I think
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that's exactly what I was about to say
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they stole my joke never
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mind but what we'll do right now is uh
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look at some audience questions I love
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this this particular um episode every
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week because uh it's the audience's
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chance to to get involved and we've got
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a few audio questions coming up uh but
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our first one comes from Jake who
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actually sent this question via Facebook
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Messenger which we don't often catch
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because we don't monitor it as much as
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we as we probably should but we just
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haven't got the person power but I just
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happened to be sort of on my uh iPad the
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other day and went oh hang on a minute
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there's a little one there uh greetings
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from Tennessee USA it's Tennessee home
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of the Titans um I I know that several
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two body uh systems are in various
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stages of tidal locking I was wondering
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if a star or planet with several
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orbiting bodies can even become tidally
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locked with a particular one for example
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can the sun become tidy locked to one of
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our planets likewise can Jupiter become
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tidy locked to one of its moons I assume
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that if such tidal lock can occur the
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larger body becomes locked with its most
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gravitationally attractive orbiting body
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but if that's the case how are the other
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orbiting bodies affected love the show
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and that was a question from Jake Tyler
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I got a feeling that he's going to some
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the things he said in the question are
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the reality yes so there's a lot of
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complex to this it's a really really
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good question now we familiar with tidal
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loing anytime we look up at the annoying
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source of light pollution in our sky
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that is the moon you know that keeps one
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face pointed towards us all the time
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with a little bit of rock and roll
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because it's being nudged by everything
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else it's not on a perfectly circular
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orbit but it essentially keeps an a side
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of the moon FES towards it The Far Side
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FES away it rotates once on its axis and
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exactly the same time it take to go
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around the earth essentially so it's
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turning as it goes the Earth is slowing
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down in its rotation as the Moon is
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getting nudged away there's this tidal
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interaction between them that I always
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visualized essentially as being the
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result of the tidal bugers the moon res
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on the earth so we get high tide and low
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tide every day and I view those a bit
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like brake blocks on a wheel they're
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kind of applying friction to the Earth
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because the Earth is turning under them
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once every 24 hours or so but those
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tidle buers are doing one la
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every 27 28 days because they are tied
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to the location of the Moon and the Sun
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so those bulges are dragged Along by the
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friction of the earth they're pulled
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slightly away from that line between the
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moon and the sun which means that they
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are then pulling a little bit on the
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moon and causing the moon to speed up
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which means it moves away so they've got
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this transfer of energy and momentum
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between the rotation of the Earth on the
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orbit of the moon so the Earth's spin is
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slowing down and the Moon is moving
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further away now in theory if we could
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carry on for long enough that would
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eventually slow the earth rotation down
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such that it matched the orbital period
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of the
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Moon there is some debate though a that
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will not happen quick enough for it to
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happen within the age of the solar
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system that's left but there's also some
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debate as to whether that would happen
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before the moon gets far enough away to
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escape the Earth's gravity so in the
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case of the Earth Moon system it's not
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going to happen but illustrates that it
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could so move out further out in the Sol
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system to Pluto the dwarf planet and we
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talked about Pluto a couple of weeks ago
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having this big companion called karon
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yeah Pluto actually though has about
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five minutes it's got PL got karon which
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is huge and then it's got four little
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ones in Kerberos Nick sticks and Hydra I
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think they're called and then smaller
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ones further out now Pluto and Kon are
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tily locked Kon spins once in the time
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it takes to orbit the center of Mass
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between Pluto and karon once so it
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always keeps the same side facing
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towards Pluto in just the same way that
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the moon does going around the Earth but
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Pluto has also tily locked with karon so
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Pluto keeps a same face pointing towards
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karon all the time so that's a prime
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example of the kind of system Jake was
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asking about a case where the biggest
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body has locked to the second biggest
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body and they're both locked together
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and there are other things in the system
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when it comes to plant system
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and when it comes to the more generality
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of it it gets a bit more complicated so
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there's a few things going on it's not
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necessarily the most massive body going
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around a star that would be the one that
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it tidally locked to because the
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distance is important as well and tidal
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forces fall off incredibly rapidly as a
00:06:48.560 --> 00:06:50.189
function of distance much more quickly
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than the r squ fall off of the
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gravitational attraction I think it's
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either an R cubed or an R to the power 4
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setup which means that the closer you
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get to the star the much more strongly
00:07:01.280 --> 00:07:03.710
you tidally interact now we see this
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with EXO planets we can see that EXO
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planets that are very close to the stars
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are tidally locked the ones that are
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further away are probably not but we
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also see it in the form of tidal
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circularization of orbits so you get a
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planet that is flung onto an elongated
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orbit where the closest point to the
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star is very near the
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star because of the degree to which
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tidal forces varies a function of
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distance that means the St will interact
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much more strongly with the planet in a
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tidal sense when it's near the closest
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approach and when it's far away that
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means that you will get a you'll get an
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attempt to tily lock the planet so the
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planet's rotation will be getting mged
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into a rotation period that matches the
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orbital period but at the same time you
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get this dissipation of energy that
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tries to make the orbit more circular
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and that dissipation of energy is
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happening at the per apps of the orbit
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the point of the orbit where it's
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closest to the South so the result of
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this is that that orbit gets more and
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more circular by bringing the Appo apps
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the furthest point from the Star closer
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to the star so it ends up being
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circularized at that closest approach
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distance and that happens more quickly
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than the tidal locking process and
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that's a result of the fact that the
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tidal forces fall off much more strongly
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as a function of
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distance we haven't yet found any stars
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that we think are definitely tily locked
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to their planet now part of this is down
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to the m difference so the small thing
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will tidle lock much more quickly than
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its bigger companion that's what we're
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seeing with the Earth and the moon yeah
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but it's not beyond the bounds of
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possibility and there are suggestions
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that tidal interactions between really
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massive planets planets a lot bigger
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than Jupiter and stars when the planets
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are really close in can have a
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significant impact on the spin of those
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stars and also the energy dynamics of
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what's going on in their Interiors not
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totally my area of expertise I've got to
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flag that but this is something that
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that people are having to think about
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when they come to looking at ways of
00:09:02.519 --> 00:09:04.949
measuring the age of stars now there's a
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few ways you can do this I've got
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colleagues at unq who work on asteros
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seismology they're looking at how Stars
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wobble and Wibble ringing like bells
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that have been struck and you can look
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at the different frequencies at which
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they're wobbling and wibbling to learn a
00:09:18.519 --> 00:09:20.910
lot about their interior and that kind
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of study can give you an estimate of the
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ages that's really quite accurate but
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it's really resource intensive you need
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to stare at us s for a long time doing a
00:09:29.160 --> 00:09:29.910
lot of
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observations if you're trying to just
00:09:31.640 --> 00:09:33.230
get the age of stars in general there's
00:09:33.240 --> 00:09:35.630
a technique called gyro chronology or
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Gyro chronology which is essentially
00:09:38.160 --> 00:09:40.949
measuring the rotation speed of the star
00:09:40.959 --> 00:09:42.910
and using that to get a first estimate
00:09:42.920 --> 00:09:44.430
of its age which will have quite big
00:09:44.440 --> 00:09:45.829
uncertainties but seems to do a
00:09:45.839 --> 00:09:48.350
reasonably good job and the idea here is
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that when Stars Are Born they're born
00:09:49.839 --> 00:09:52.150
from Material collapsing in which spins
00:09:52.160 --> 00:09:54.069
faster and faster so typically a newly
00:09:54.079 --> 00:09:56.350
born star will spin quite quickly every
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day or two but over billions of years
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all the m it's losing through the
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Stellar Wind will kind of act as a break
00:10:03.399 --> 00:10:05.550
on the St rotation taking away that
00:10:05.560 --> 00:10:07.630
angular momentum causing it spin to slow
00:10:07.640 --> 00:10:10.069
down over time so if you know the degree
00:10:10.079 --> 00:10:12.630
to which stars slow down as a function
00:10:12.640 --> 00:10:14.190
of time and you measure how quick a
00:10:14.200 --> 00:10:15.670
Stars spinning it gives you an estimate
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of its age because an old star will spin
00:10:17.880 --> 00:10:20.509
slower than a young star but if that
00:10:20.519 --> 00:10:22.069
star's got a really close in Planet
00:10:22.079 --> 00:10:23.550
that's interfering with it tily that
00:10:23.560 --> 00:10:26.430
will impact that process yeah so there's
00:10:26.440 --> 00:10:28.069
a lot of aspects to this I'm I
00:10:28.079 --> 00:10:29.470
appreciate I'm going a little bit off
00:10:29.480 --> 00:10:31.870
topic from Jake's question but it shows
00:10:31.880 --> 00:10:33.389
you the complexity of it and it's why
00:10:33.399 --> 00:10:35.030
it's such a good question because it's
00:10:35.040 --> 00:10:37.430
something that we don't know the final
00:10:37.440 --> 00:10:39.269
answer to it's going to depend very much
00:10:39.279 --> 00:10:41.790
on each individual system for the Earth
00:10:41.800 --> 00:10:43.949
and the moon we're probably not never
00:10:43.959 --> 00:10:45.870
going to get fully Tiddly locked to the
00:10:45.880 --> 00:10:48.110
moon but we know that when the dinosaurs
00:10:48.120 --> 00:10:49.590
walked the Earth the Earth was spinning
00:10:49.600 --> 00:10:52.069
quicker and we've had independent
00:10:52.079 --> 00:10:53.870
verification of that not only do we know
00:10:53.880 --> 00:10:55.389
that from the tidal motion of the Moon
00:10:55.399 --> 00:10:57.550
moving away we can measure the speed of
00:10:57.560 --> 00:11:00.150
the moon's moving away but also
00:11:00.160 --> 00:11:01.310
measurements that have been made of
00:11:01.320 --> 00:11:03.389
Fossil Beds that show that they were
00:11:03.399 --> 00:11:07.230
about 380 390 days a year back in the
00:11:07.240 --> 00:11:09.509
crous now the Earth orbital period
00:11:09.519 --> 00:11:11.310
hasn't changed as measured in the number
00:11:11.320 --> 00:11:13.550
of seconds so how do you get more days
00:11:13.560 --> 00:11:15.509
in a year you get more days in a year by
00:11:15.519 --> 00:11:18.389
making the day shorter so that's the
00:11:18.399 --> 00:11:21.829
direct outcome of that tidal reaction
00:11:21.839 --> 00:11:23.990
between the Earth and the Moon Pluto is
00:11:24.000 --> 00:11:26.949
a stage further along that's full opta
00:11:26.959 --> 00:11:28.269
you've got an interesting case in our
00:11:28.279 --> 00:11:30.150
soul system of Merc which is trapped in
00:11:30.160 --> 00:11:32.870
a 3 to2 spin orbit resonance so it's
00:11:32.880 --> 00:11:34.430
tidally locked but it's not locked in
00:11:34.440 --> 00:11:37.069
one: one and the only reason that works
00:11:37.079 --> 00:11:39.069
is that mercury is on an elongated orbit
00:11:39.079 --> 00:11:41.030
and is also not a perfectly spherical
00:11:41.040 --> 00:11:44.389
object gets quite complicated yeah but
00:11:44.399 --> 00:11:46.150
this gets orderer than while you study
00:11:46.160 --> 00:11:47.629
it basically and there's a lot of depth
00:11:47.639 --> 00:11:50.030
to it so it makes it a fabulous question
00:11:50.040 --> 00:11:53.110
yeah certainly is uh thank you Jake um a
00:11:53.120 --> 00:11:54.430
question popped into my head while you
00:11:54.440 --> 00:11:56.030
were talking you talk about the uh the
00:11:56.040 --> 00:11:58.990
effect of the moon on Earth's oceans the
00:11:59.000 --> 00:12:03.710
you the tides uh would it be too an
00:12:03.720 --> 00:12:06.550
extreme too extreme a thought to suggest
00:12:06.560 --> 00:12:09.269
that the um the tides are actually just
00:12:09.279 --> 00:12:11.870
a slow motion tidal
00:12:11.880 --> 00:12:14.110
wave you could possibly think of it that
00:12:14.120 --> 00:12:15.990
way I never have done before but it it's
00:12:16.000 --> 00:12:17.590
an interesting one because the the
00:12:17.600 --> 00:12:20.509
phrase tidal wave in itself is quite
00:12:20.519 --> 00:12:23.430
misleading because they're not really
00:12:23.440 --> 00:12:25.110
waves in the same sense as the waves we
00:12:25.120 --> 00:12:27.310
see on the beach so this is where when
00:12:27.320 --> 00:12:29.430
you see disaster movies and you get this
00:12:29.440 --> 00:12:31.910
toll breaking wave that's not really
00:12:31.920 --> 00:12:33.790
what a tidal wave is like a tidal wave
00:12:33.800 --> 00:12:36.310
is a a huge body of water rising and
00:12:36.320 --> 00:12:37.790
falling so it's more like the surface of
00:12:37.800 --> 00:12:40.030
the ocean getting higher or lower and
00:12:40.040 --> 00:12:41.389
it's only when it gets really close to
00:12:41.399 --> 00:12:43.670
the coast that that then breaks I know
00:12:43.680 --> 00:12:45.870
people who are into geophysics and ocean
00:12:45.880 --> 00:12:48.590
Dynamics who get grumpy at disaster
00:12:48.600 --> 00:12:50.350
movies for getting title Wars totally
00:12:50.360 --> 00:12:53.470
totally wrong but in that sense our
00:12:53.480 --> 00:12:55.870
tides are very much like that it's the
00:12:55.880 --> 00:12:57.829
same kind of process of water rising and
00:12:57.839 --> 00:13:00.470
falling and huge body of water doing
00:13:00.480 --> 00:13:02.269
that means it slushes around a bit as
00:13:02.279 --> 00:13:04.870
well a very similar thing and tied into
00:13:04.880 --> 00:13:06.389
this of course when the moon was closer
00:13:06.399 --> 00:13:09.230
to us which it had to be in the past
00:13:09.240 --> 00:13:11.150
when the days were shorter the tides
00:13:11.160 --> 00:13:12.790
were higher and more extreme and that's
00:13:12.800 --> 00:13:15.150
tied into arguments people have had
00:13:15.160 --> 00:13:17.670
about the origin of Life suggesting that
00:13:17.680 --> 00:13:19.430
the origin of Life happened in the inter
00:13:19.440 --> 00:13:21.990
tidal region on the Cur which would have
00:13:22.000 --> 00:13:23.590
been larger when the tides were higher
00:13:23.600 --> 00:13:24.750
but the tides were happening more
00:13:24.760 --> 00:13:26.910
quickly as well so the inundation and
00:13:26.920 --> 00:13:28.629
drying out happened on a quicker time
00:13:28.639 --> 00:13:29.629
scale
00:13:29.639 --> 00:13:33.150
so the move yeah it's quite yeah it's
00:13:33.160 --> 00:13:36.430
intriguing it's it's amazing site uh
00:13:36.440 --> 00:13:38.350
thank you again Jake great question glad
00:13:38.360 --> 00:13:40.750
I um happened to cross it the other day
00:13:40.760 --> 00:13:42.629
this is Space Nuts Andrew Dunley here
00:13:42.639 --> 00:13:45.670
with Professor johy
00:13:45.680 --> 00:13:48.350
hoer okay we checked all four systems
00:13:48.360 --> 00:13:51.550
and It Go Space Nuts uh let's go to our
00:13:51.560 --> 00:13:55.150
next question uh which comes from Clint
00:13:55.160 --> 00:13:58.509
hi Fred hi Andrew this is Clint from
00:13:58.519 --> 00:14:02.389
Rome Georgia USA love the show Happy New
00:14:02.399 --> 00:14:05.030
Year my question though comes from uh
00:14:05.040 --> 00:14:07.550
the sun uh we know the surface of the
00:14:07.560 --> 00:14:10.670
Sun is around 6,000 de C but the corona
00:14:10.680 --> 00:14:13.310
is much hotter millions of degrees I
00:14:13.320 --> 00:14:14.910
know scientists are still puzzled with
00:14:14.920 --> 00:14:17.629
this phenomena but my question is could
00:14:17.639 --> 00:14:19.269
this be due to the gravitational
00:14:19.279 --> 00:14:22.189
pullback towards the Sun that is causing
00:14:22.199 --> 00:14:24.069
some kind of friction on leaving matter
00:14:24.079 --> 00:14:26.590
that the sun is losing or projecting
00:14:26.600 --> 00:14:28.110
just a thought I have when reading how
00:14:28.120 --> 00:14:30.470
the Parker solar probe came its closest
00:14:30.480 --> 00:14:34.629
to the Sun earlier uh last year or this
00:14:34.639 --> 00:14:36.870
year depending on when you're listening
00:14:36.880 --> 00:14:40.749
to this um and use they use its own
00:14:40.759 --> 00:14:43.230
gravity to uh Power it quickly through
00:14:43.240 --> 00:14:46.389
uh the surface of that Corona just a
00:14:46.399 --> 00:14:48.310
quick question I had while exploring
00:14:48.320 --> 00:14:51.990
that thank you okay uh thanks Clint uh
00:14:52.000 --> 00:14:54.550
love the accent um now I know the sun
00:14:54.560 --> 00:14:58.670
isn't your main area but uh I'm I'm
00:14:58.680 --> 00:14:59.990
guessing you've done your homework on
00:15:00.000 --> 00:15:02.030
this question a little bit it's it's
00:15:02.040 --> 00:15:03.389
actually a real head scratcher because
00:15:03.399 --> 00:15:04.870
it's pushing the boundaries of what we
00:15:04.880 --> 00:15:06.310
know and that's what I really love so
00:15:06.320 --> 00:15:08.110
you know the first thing for me to say
00:15:08.120 --> 00:15:09.389
here and I think it's always important
00:15:09.399 --> 00:15:10.829
to acknowledge this is that I don't know
00:15:10.839 --> 00:15:13.389
the answer here fully um I'm not an
00:15:13.399 --> 00:15:16.069
expert but part of the be of science is
00:15:16.079 --> 00:15:17.470
asking questions we don't know the
00:15:17.480 --> 00:15:18.629
answer to that's what makes the
00:15:18.639 --> 00:15:20.110
scientists if we already knew the answer
00:15:20.120 --> 00:15:21.550
to everything it'd be really really
00:15:21.560 --> 00:15:24.269
boring and the the Suns coron room by
00:15:24.279 --> 00:15:26.389
extension the coroni of all the stars
00:15:26.399 --> 00:15:29.990
that we see is a so problem so exactly
00:15:30.000 --> 00:15:32.509
as you say the Photosphere the visible
00:15:32.519 --> 00:15:35.230
surface of the Sun that area of the sun
00:15:35.240 --> 00:15:39.350
is about 5,8 6,000 degrees C Centigrade
00:15:39.360 --> 00:15:43.790
Celsius roughly not precise but it's
00:15:43.800 --> 00:15:45.790
high density so that's
00:15:45.800 --> 00:15:48.069
essentially the final surface you can
00:15:48.079 --> 00:15:49.749
see before light gets scattered so the
00:15:49.759 --> 00:15:51.550
analogy I often use here is like looking
00:15:51.560 --> 00:15:54.230
at a fog Bank a fog bank is not solid
00:15:54.240 --> 00:15:56.189
but when you on a foggy or a misty day
00:15:56.199 --> 00:15:57.829
people measure the distance that you can
00:15:57.839 --> 00:16:00.949
see and the the fog is the shorter that
00:16:00.959 --> 00:16:03.110
distance is of course you're looking at
00:16:03.120 --> 00:16:04.189
particles and essentially the
00:16:04.199 --> 00:16:05.870
Photosphere of the sun is the last
00:16:05.880 --> 00:16:08.829
surface of which your average Photon of
00:16:08.839 --> 00:16:10.350
light would hit a particle and be
00:16:10.360 --> 00:16:12.550
scattered so once it reaches this point
00:16:12.560 --> 00:16:14.350
it can escape space and so that gives us
00:16:14.360 --> 00:16:16.749
this illusion of a solid surface when in
00:16:16.759 --> 00:16:18.230
fact you're just get into a denser piece
00:16:18.240 --> 00:16:21.350
of gas so the gas in the Photosphere is
00:16:21.360 --> 00:16:23.509
quite dense on a huge amount of
00:16:23.519 --> 00:16:25.629
radiation comes out from it so when
00:16:25.639 --> 00:16:27.069
people look at the sun in the sky and
00:16:27.079 --> 00:16:28.629
there's always the usual caveat hair of
00:16:28.639 --> 00:16:30.629
pleas don't do that because it's a very
00:16:30.639 --> 00:16:31.910
good way of damaging your eyes
00:16:31.920 --> 00:16:34.110
permanently yeah but when you see the
00:16:34.120 --> 00:16:36.710
sun when you see a photograph of the Sun
00:16:36.720 --> 00:16:38.110
that surface you're seeing is because
00:16:38.120 --> 00:16:39.829
there's a high density so there's a huge
00:16:39.839 --> 00:16:42.189
amount of radiation coming in coming out
00:16:42.199 --> 00:16:43.670
of it when we get in the total eclipse
00:16:43.680 --> 00:16:45.389
of the sun we suddenly see this
00:16:45.399 --> 00:16:48.910
beautiful diaphanous very variable area
00:16:48.920 --> 00:16:51.590
around us and we call the Corona and
00:16:51.600 --> 00:16:54.389
that's a much whiter Bluer light when
00:16:54.399 --> 00:16:56.629
you get color photos which is indicative
00:16:56.639 --> 00:16:59.189
of a much higher temperature
00:16:59.199 --> 00:17:00.430
and you think well it's a higher
00:17:00.440 --> 00:17:02.590
temperature the amount of energy that
00:17:02.600 --> 00:17:04.870
you get from a photon is related to the
00:17:04.880 --> 00:17:07.470
temperature to the power four really
00:17:07.480 --> 00:17:09.870
incredible more energy so shouldn't the
00:17:09.880 --> 00:17:11.390
corona be brighter than the surface of
00:17:11.400 --> 00:17:13.829
the Sun why don't we see it and the
00:17:13.839 --> 00:17:15.870
answer is because the individual photons
00:17:15.880 --> 00:17:18.390
are much more energetic but there's far
00:17:18.400 --> 00:17:21.270
far far far less gas there so there's
00:17:21.280 --> 00:17:22.829
much less
00:17:22.839 --> 00:17:25.829
flux you've got higher energy photons
00:17:25.839 --> 00:17:27.590
but a lot less of them so you can only
00:17:27.600 --> 00:17:29.830
see it when the sun's blocked out out
00:17:29.840 --> 00:17:31.310
but the corona is incredibly hot it's
00:17:31.320 --> 00:17:33.630
like a million 2 million degrees this
00:17:33.640 --> 00:17:36.029
incredibly tenuous gas hot enough that
00:17:36.039 --> 00:17:39.549
the individual atoms the individual
00:17:39.559 --> 00:17:41.350
nuclei are traveling quick enough that
00:17:41.360 --> 00:17:42.630
they'll escape the Sun's gravity and
00:17:42.640 --> 00:17:45.909
flood out into the space so Corona links
00:17:45.919 --> 00:17:47.750
in with the solar wind they're
00:17:47.760 --> 00:17:50.470
connected and it's been an outstanding
00:17:50.480 --> 00:17:52.870
really long-term question of how on the
00:17:52.880 --> 00:17:54.990
Corona is heated to those temperatures
00:17:55.000 --> 00:17:59.430
what on Earth's going on now the gravity
00:17:59.440 --> 00:18:02.070
idea the idea of friction there will be
00:18:02.080 --> 00:18:03.590
a little bit of friction so any
00:18:03.600 --> 00:18:05.909
particles entering into the corona that
00:18:05.919 --> 00:18:08.110
are colliding with things will transfer
00:18:08.120 --> 00:18:10.590
energy to the to the atoms and nuclei
00:18:10.600 --> 00:18:12.950
that they're impacting and you can get
00:18:12.960 --> 00:18:14.470
some degree of frictional heating there
00:18:14.480 --> 00:18:16.430
but that's going to be a very very very
00:18:16.440 --> 00:18:18.430
small amount it's not going to be
00:18:18.440 --> 00:18:19.950
anywhere near enough to do this but
00:18:19.960 --> 00:18:22.110
you're right it will probably contribute
00:18:22.120 --> 00:18:23.909
a bit of energy to this and we know for
00:18:23.919 --> 00:18:26.750
well that there is continually dust a
00:18:26.760 --> 00:18:29.230
material falling into the Sun the must
00:18:29.240 --> 00:18:30.669
spectacular example of that are the
00:18:30.679 --> 00:18:32.669
sungrazing Comets that go in and fall
00:18:32.679 --> 00:18:35.270
apart and fragment dumping hu a huge
00:18:35.280 --> 00:18:37.029
amount of dust and gas into that coroner
00:18:37.039 --> 00:18:40.230
in a localized event now the thing that
00:18:40.240 --> 00:18:43.310
to me from a Science Education
00:18:43.320 --> 00:18:45.390
background from the way I've been
00:18:45.400 --> 00:18:48.630
trained to think about problems to say
00:18:48.640 --> 00:18:51.190
that Clint's idea doesn't quite work
00:18:51.200 --> 00:18:52.950
would be to look at the distribution of
00:18:52.960 --> 00:18:55.669
temperature in the corona so the bulk of
00:18:55.679 --> 00:18:57.430
the mass entry into the corona would be
00:18:57.440 --> 00:18:59.390
the rarer events like the cover for sun
00:18:59.400 --> 00:19:01.750
gring comic you get a 100 meter sized
00:19:01.760 --> 00:19:03.310
object breaking into dust and that would
00:19:03.320 --> 00:19:04.950
inject a lot of material in one
00:19:04.960 --> 00:19:06.990
particular place yeah so if the
00:19:07.000 --> 00:19:09.230
mechanism Clint was suggesting was the
00:19:09.240 --> 00:19:11.470
main one you'd expect that one bit of
00:19:11.480 --> 00:19:13.190
the corona to then become much hotter
00:19:13.200 --> 00:19:15.190
and much brighter than the rest and we
00:19:15.200 --> 00:19:17.789
don't observe that so that to me is a
00:19:17.799 --> 00:19:19.710
very big Telltale that it's not in
00:19:19.720 --> 00:19:21.830
Falling material heating it up because
00:19:21.840 --> 00:19:23.750
INF falling material will be episodic
00:19:23.760 --> 00:19:26.110
and localized and so you get one bit of
00:19:26.120 --> 00:19:27.710
the corona bright then another bit then
00:19:27.720 --> 00:19:29.430
another bit and and instead the corona
00:19:29.440 --> 00:19:32.110
seems to be uniformly hot it shape and
00:19:32.120 --> 00:19:33.870
structure changes are through the solar
00:19:33.880 --> 00:19:35.470
cycle and that's tied to the magnetic
00:19:35.480 --> 00:19:37.990
fields and that seems to be a hint at
00:19:38.000 --> 00:19:40.390
what's actually going on now it's
00:19:40.400 --> 00:19:42.230
absolutely right we don't know the final
00:19:42.240 --> 00:19:43.590
answer but I've been looking around and
00:19:43.600 --> 00:19:45.630
there was a bit of work came out back in
00:19:45.640 --> 00:19:49.350
2023 I think it was that has come up
00:19:49.360 --> 00:19:51.830
with a potential part of the
00:19:51.840 --> 00:19:55.310
answer so the answer here is linked to
00:19:55.320 --> 00:19:57.630
what researchers have called low
00:19:57.640 --> 00:20:01.190
amplitude careless King
00:20:01.200 --> 00:20:03.590
cations right again we're really good at
00:20:03.600 --> 00:20:06.789
naming things um lad I guess if you
00:20:06.799 --> 00:20:10.190
really wanted an Acron acronym there so
00:20:10.200 --> 00:20:12.950
the corona is tied in with the magnetic
00:20:12.960 --> 00:20:15.110
field of the Sun and as the solar cycle
00:20:15.120 --> 00:20:17.510
goes on the magnetic field gets more and
00:20:17.520 --> 00:20:19.590
more tangled up and you get loops and
00:20:19.600 --> 00:20:21.950
Kinks happening near the surface of the
00:20:21.960 --> 00:20:24.230
Sun often tied with sun spots and this
00:20:24.240 --> 00:20:26.029
is all tied in with flares and coronal
00:20:26.039 --> 00:20:29.029
mass injections things like this what
00:20:29.039 --> 00:20:31.430
this is saying I think is that you get
00:20:31.440 --> 00:20:33.430
oscillations in those magnetic field
00:20:33.440 --> 00:20:35.990
lines and the oscillations carry energy
00:20:36.000 --> 00:20:38.350
from the surface into the coron room can
00:20:38.360 --> 00:20:40.470
deposit it there now normally those
00:20:40.480 --> 00:20:41.909
oscillations would be shortlived so
00:20:41.919 --> 00:20:43.310
you'd only have a short period of time
00:20:43.320 --> 00:20:44.950
to deposit energy so they wouldn't be
00:20:44.960 --> 00:20:47.110
very efficient but these studies these
00:20:47.120 --> 00:20:49.750
observations found a kind of oscillation
00:20:49.760 --> 00:20:51.549
on those magnetic field lines that is of
00:20:51.559 --> 00:20:54.029
low frequency so not carrying much
00:20:54.039 --> 00:20:57.230
energy per second but can be long lived
00:20:57.240 --> 00:20:59.230
because they are became pess they're not
00:20:59.240 --> 00:21:00.870
decaying so you get these oscillations
00:21:00.880 --> 00:21:03.029
that set up that keep going for minutes
00:21:03.039 --> 00:21:05.630
or hours and that gives them a long time
00:21:05.640 --> 00:21:07.390
to put energy into the corona so the
00:21:07.400 --> 00:21:10.549
authors of this work are talking about
00:21:10.559 --> 00:21:12.909
the fact that such oscillations which
00:21:12.919 --> 00:21:15.269
seem to be really common from their
00:21:15.279 --> 00:21:17.630
observations could act to deposit a
00:21:17.640 --> 00:21:19.789
large amount of energy in the corona so
00:21:19.799 --> 00:21:21.350
it's a way of transferring energy from
00:21:21.360 --> 00:21:23.029
the magnetic field of the sun into the
00:21:23.039 --> 00:21:25.029
corona which then carries that energy
00:21:25.039 --> 00:21:27.630
away into space which ties into what we
00:21:27.640 --> 00:21:28.870
were talking about before actually in
00:21:28.880 --> 00:21:31.390
the gyro chronology because it's that
00:21:31.400 --> 00:21:32.830
energy that has been lost that is
00:21:32.840 --> 00:21:34.549
transferring angular momentum away into
00:21:34.559 --> 00:21:36.390
space as well and causing the to slow
00:21:36.400 --> 00:21:39.669
down so it is all linked together now
00:21:39.679 --> 00:21:42.110
that study used data from European Space
00:21:42.120 --> 00:21:45.590
Agency solar Orbiter NASA's Sol Dynamics
00:21:45.600 --> 00:21:47.909
Observatory and they found one of these
00:21:47.919 --> 00:21:49.470
oscillations that lasted for four
00:21:49.480 --> 00:21:51.470
minutes now four minutes doesn't sound
00:21:51.480 --> 00:21:54.070
long but a kink a wobble weing off four
00:21:54.080 --> 00:21:55.630
minutes has a lot of time to deposit
00:21:55.640 --> 00:21:58.269
energy into space yeah um read more
00:21:58.279 --> 00:21:59.750
about this you can have a look online it
00:21:59.760 --> 00:22:02.149
was published I think September 12
00:22:02.159 --> 00:22:04.830
2023 in nature Communications with the
00:22:04.840 --> 00:22:07.549
lead author being and and apologies for
00:22:07.559 --> 00:22:09.190
the pronunciation there it's a solop
00:22:09.200 --> 00:22:11.190
physicist at the University of war in
00:22:11.200 --> 00:22:15.830
the UK and it's Valerie nakariakov n a k
00:22:15.840 --> 00:22:19.510
a r i a k RV um you can find the
00:22:19.520 --> 00:22:21.950
findings online in n Communications
00:22:21.960 --> 00:22:23.990
their paper will do an infinitely better
00:22:24.000 --> 00:22:25.710
job of explaining what's going on than I
00:22:25.720 --> 00:22:28.070
just did because they're the experts but
00:22:28.080 --> 00:22:31.390
that seems to be the latest entry in our
00:22:31.400 --> 00:22:34.029
attempt to answer the question of um WTF
00:22:34.039 --> 00:22:35.510
essentially what on Earth is going on
00:22:35.520 --> 00:22:38.750
with the corona how does it work and
00:22:38.760 --> 00:22:40.190
that's how science progresses you know
00:22:40.200 --> 00:22:41.549
we don't know all the answers yet and
00:22:41.559 --> 00:22:42.990
that's why this is such a fabulous
00:22:43.000 --> 00:22:45.149
question and what Clint has done in
00:22:45.159 --> 00:22:47.750
coming up with a potential hypothesis
00:22:47.760 --> 00:22:49.190
for what happens is how scientists
00:22:49.200 --> 00:22:50.870
actually work so we do just what Clint
00:22:50.880 --> 00:22:53.230
did we come up with an idea this I think
00:22:53.240 --> 00:22:54.990
is something that could contribute this
00:22:55.000 --> 00:22:57.149
is how it could work and then what
00:22:57.159 --> 00:23:00.070
happens is that we make predi from that
00:23:00.080 --> 00:23:02.029
which is how I extrapolated it which is
00:23:02.039 --> 00:23:03.909
that if it's linked to INF falling
00:23:03.919 --> 00:23:05.870
material and that's a man driver what
00:23:05.880 --> 00:23:07.630
would we see well we'd see the places
00:23:07.640 --> 00:23:08.990
where you get a big fa in Fall of
00:23:09.000 --> 00:23:10.750
material you get a bright Outburst of
00:23:10.760 --> 00:23:12.909
energy and they would Dominate and we
00:23:12.919 --> 00:23:15.149
don't see that so that theory doesn't
00:23:15.159 --> 00:23:16.750
work we make testable predictions and
00:23:16.760 --> 00:23:19.149
test them and this is just another step
00:23:19.159 --> 00:23:20.630
in the way to working to that answer so
00:23:20.640 --> 00:23:23.149
I think it's a wonderful question it is
00:23:23.159 --> 00:23:24.590
approaching something that we don't have
00:23:24.600 --> 00:23:26.149
all the answers for yet but hopefully my
00:23:26.159 --> 00:23:27.549
answer helps a little bit in
00:23:27.559 --> 00:23:29.190
understanding just what's going on and
00:23:29.200 --> 00:23:31.710
what isn't happening yeah it also shows
00:23:31.720 --> 00:23:35.070
how how complex these these things are I
00:23:35.080 --> 00:23:37.470
mean the sun is the most studied star in
00:23:37.480 --> 00:23:39.269
the universe as far as we're concerned
00:23:39.279 --> 00:23:42.230
and we still haven't figured it out so
00:23:42.240 --> 00:23:43.830
and and there's so many different kinds
00:23:43.840 --> 00:23:46.669
of stars uh and they might not all be
00:23:46.679 --> 00:23:48.470
doing the same thing so yeah there's
00:23:48.480 --> 00:23:50.269
much to learn Clint great question
00:23:50.279 --> 00:23:52.590
thanks for sending it in this is Space
00:23:52.600 --> 00:23:54.470
Nuts Andrew Dunley here with Professor
00:23:54.480 --> 00:23:59.029
johy HOA
00:23:59.039 --> 00:24:03.390
2 one Space Nuts uh johy our next
00:24:03.400 --> 00:24:06.149
question comes from one of our younger
00:24:06.159 --> 00:24:09.549
audience members and I will hand it over
00:24:09.559 --> 00:24:12.590
to Sandy and Emily good day friend
00:24:12.600 --> 00:24:15.549
Andrew it's Sandy from again thank you
00:24:15.559 --> 00:24:17.710
for answering my last question um they
00:24:17.720 --> 00:24:20.909
gag about the asteroids um pretty funny
00:24:20.919 --> 00:24:24.230
um now today um my four-year-old
00:24:24.240 --> 00:24:26.909
daughter Emily wants to ask a question
00:24:26.919 --> 00:24:28.909
um so I'm going to pass it on to her how
00:24:28.919 --> 00:24:32.190
do we go to the mo good job Emy thank
00:24:32.200 --> 00:24:34.230
you um thank you for Andrew hopefully
00:24:34.240 --> 00:24:36.029
you can answer this question for us
00:24:36.039 --> 00:24:39.149
cheers well it won't be Fred um nor
00:24:39.159 --> 00:24:42.149
Andrew it will be jonty um and hi Emily
00:24:42.159 --> 00:24:44.430
and sy's one of our regular contributors
00:24:44.440 --> 00:24:47.870
but great to hear from Emily um a giant
00:24:47.880 --> 00:24:51.310
ladder probably not probably not it's an
00:24:51.320 --> 00:24:52.950
awesome question and a really good one
00:24:52.960 --> 00:24:55.470
Emily so thank you very much for that
00:24:55.480 --> 00:24:58.350
it's difficult is the very short things
00:24:58.360 --> 00:25:00.789
so traveling into space is challenging
00:25:00.799 --> 00:25:03.149
and this is why we never managed it
00:25:03.159 --> 00:25:06.029
until 1957 when they launched Sputnik 1
00:25:06.039 --> 00:25:07.310
which was the first thing that went into
00:25:07.320 --> 00:25:09.669
orbit around the Earth the moon's
00:25:09.679 --> 00:25:11.710
further away the Moon on average is
00:25:11.720 --> 00:25:16.590
about 384,000 km away um what that means
00:25:16.600 --> 00:25:18.110
is if you want to get there in a
00:25:18.120 --> 00:25:19.430
reasonable amount of time you need to
00:25:19.440 --> 00:25:22.110
travel really really quickly if you were
00:25:22.120 --> 00:25:24.470
to travel on the highway you're going at
00:25:24.480 --> 00:25:27.269
100 km an hour it would take you
00:25:27.279 --> 00:25:29.990
something like 3,000 800 hours to drive
00:25:30.000 --> 00:25:32.070
there driving at that speed and I think
00:25:32.080 --> 00:25:33.669
we've all got better things to do than
00:25:33.679 --> 00:25:35.549
that so obviously we can't drive to them
00:25:35.559 --> 00:25:37.310
and even if we had a road or we had a
00:25:37.320 --> 00:25:40.190
ladder what we need to do instead is
00:25:40.200 --> 00:25:42.269
find a way to get to go very very
00:25:42.279 --> 00:25:44.789
quickly and then travel there more
00:25:44.799 --> 00:25:47.070
rapidly and put that in perspective when
00:25:47.080 --> 00:25:49.149
the first people walked on the moon back
00:25:49.159 --> 00:25:51.990
in the late 1960s took them about three
00:25:52.000 --> 00:25:54.110
days to get there so they were traveling
00:25:54.120 --> 00:25:55.549
a lot quicker than you go when you're
00:25:55.559 --> 00:25:57.950
driving to school or driving to work
00:25:57.960 --> 00:26:01.590
andless you got P plates on your car yes
00:26:01.600 --> 00:26:03.230
even with the p plates it's a push I
00:26:03.240 --> 00:26:05.149
mean I wish I could do my commute at
00:26:05.159 --> 00:26:06.630
this kind of speed because it will make
00:26:06.640 --> 00:26:09.590
life a lot easier yes so there's a few
00:26:09.600 --> 00:26:11.470
problems with that you've got to get to
00:26:11.480 --> 00:26:14.470
a very high speed which our cars just
00:26:14.480 --> 00:26:16.310
can't do but you don't want to just get
00:26:16.320 --> 00:26:18.870
to that speed instantaneously because
00:26:18.880 --> 00:26:21.029
the acceleration would be really really
00:26:21.039 --> 00:26:23.350
violent and really really painful and
00:26:23.360 --> 00:26:25.149
you feel this when you feel you know
00:26:25.159 --> 00:26:26.990
somebody driving maybe Sand's driving
00:26:27.000 --> 00:26:29.470
Emily um and they Accelerate from the
00:26:29.480 --> 00:26:31.269
traffic lights the harder they
00:26:31.279 --> 00:26:32.750
accelerate the more you're pushed back
00:26:32.760 --> 00:26:35.149
into your seat and so the more you're
00:26:35.159 --> 00:26:37.870
changing speed the more you feel that
00:26:37.880 --> 00:26:39.510
and this is something fighter pilots
00:26:39.520 --> 00:26:41.630
need to train to practice with because
00:26:41.640 --> 00:26:44.389
when a fighter jet does a really sharp
00:26:44.399 --> 00:26:48.110
turn the pilot can pass out because the
00:26:48.120 --> 00:26:50.070
G forces are so extreme that all the
00:26:50.080 --> 00:26:52.149
blood is pushed out of their brain and
00:26:52.159 --> 00:26:53.830
they kind of fall asleep and that's not
00:26:53.840 --> 00:26:55.389
good so they have special clothes to
00:26:55.399 --> 00:26:57.789
deal with this so what that means is we
00:26:57.799 --> 00:27:00.149
can't accelerate too quickly
00:27:00.159 --> 00:27:01.789
instantaneously because that would be
00:27:01.799 --> 00:27:04.789
bad for the people going in addition
00:27:04.799 --> 00:27:07.029
we've got to get out of the atmosphere
00:27:07.039 --> 00:27:08.510
and the faster you travel through the
00:27:08.520 --> 00:27:11.110
earth's air the air pushes back at you
00:27:11.120 --> 00:27:13.710
so it's really hard to speed up and you
00:27:13.720 --> 00:27:15.230
can see this if you get a sheet of paper
00:27:15.240 --> 00:27:16.590
in your hand and try and push it through
00:27:16.600 --> 00:27:18.269
the air face onto the air if you go
00:27:18.279 --> 00:27:20.430
gently it's not too bad but the harder
00:27:20.440 --> 00:27:22.190
you push it the more the paper will bend
00:27:22.200 --> 00:27:23.510
back against your hand as it's pushed
00:27:23.520 --> 00:27:26.190
back by the air resistance so a big part
00:27:26.200 --> 00:27:27.630
of getting to space is actually getting
00:27:27.640 --> 00:27:30.070
out of the that much feir and the way we
00:27:30.080 --> 00:27:33.110
solved all of these problems is to build
00:27:33.120 --> 00:27:35.070
really really really big Rockets with
00:27:35.080 --> 00:27:37.789
multiple stes and use those to propel
00:27:37.799 --> 00:27:40.710
objects into space and then when the
00:27:40.720 --> 00:27:42.669
first stage is dealt with it falls away
00:27:42.679 --> 00:27:44.149
you get rid of that mass and you get a
00:27:44.159 --> 00:27:46.950
smaller and smaller spacecraft so when
00:27:46.960 --> 00:27:48.990
astronauts went to the moon in the 1960s
00:27:49.000 --> 00:27:50.750
they had this enormous rocket called the
00:27:50.760 --> 00:27:53.230
Saturn 5 rocket you can look at things
00:27:53.240 --> 00:27:55.269
of it when I was a kid we went to
00:27:55.279 --> 00:27:58.310
Florida and we went and I stood next to
00:27:58.320 --> 00:28:02.470
the sa five rocket and it's Bonkers big
00:28:02.480 --> 00:28:05.070
ridiculous like it looks big on TV but
00:28:05.080 --> 00:28:07.310
when you're standing next to it you go
00:28:07.320 --> 00:28:10.029
oh my gosh it is so much bigger than you
00:28:10.039 --> 00:28:11.549
think it's going to be yeah it's long
00:28:11.559 --> 00:28:13.029
enough that an Olympic sprinter would
00:28:13.039 --> 00:28:14.830
take about 10 seconds to run the length
00:28:14.840 --> 00:28:16.710
of it something like that ridiculously
00:28:16.720 --> 00:28:19.269
big so that is the giant firework that
00:28:19.279 --> 00:28:21.549
we built to send astronauts to the room
00:28:21.559 --> 00:28:24.789
to the moon and it launches it the
00:28:24.799 --> 00:28:26.669
rocket engine goes off like firework
00:28:26.679 --> 00:28:28.110
pushing them higher and higher into the
00:28:28.120 --> 00:28:31.070
in the sky speeding up at a speed at an
00:28:31.080 --> 00:28:32.950
acceleration that anything in the top
00:28:32.960 --> 00:28:35.750
could manage so it's uncomfortable and
00:28:35.760 --> 00:28:38.190
you've being pushed back into your seats
00:28:38.200 --> 00:28:40.470
but it's not so extreme it makes you own
00:28:40.480 --> 00:28:43.149
well and that big rocket is made of
00:28:43.159 --> 00:28:45.029
multiple parts so when you get quite
00:28:45.039 --> 00:28:46.830
hope in the atmosphere and all the fuel
00:28:46.840 --> 00:28:49.269
is used up in the first part that falls
00:28:49.279 --> 00:28:51.149
away and you've now got a smaller rocket
00:28:51.159 --> 00:28:52.950
that does the next burn and pushes you
00:28:52.960 --> 00:28:55.549
even faster and faster and eventually
00:28:55.559 --> 00:28:57.269
you get out of the atmosphere and that's
00:28:57.279 --> 00:28:58.430
good because you no longer to have the
00:28:58.440 --> 00:29:01.430
wind resistance against you and you can
00:29:01.440 --> 00:29:03.350
therefore use less energy to move around
00:29:03.360 --> 00:29:04.669
because you're not pushing against the
00:29:04.679 --> 00:29:05.830
wind so once you're out of the
00:29:05.840 --> 00:29:08.470
atmosphere it gets easier what tends to
00:29:08.480 --> 00:29:10.350
happen then is that the rocket will do
00:29:10.360 --> 00:29:12.470
one final boost to get you to a speed
00:29:12.480 --> 00:29:14.590
where you'll travel towards the moon and
00:29:14.600 --> 00:29:16.509
it will take you two or three days to
00:29:16.519 --> 00:29:19.789
get there and you curs you then go into
00:29:19.799 --> 00:29:22.310
Free Fall flirting there just cruising
00:29:22.320 --> 00:29:23.830
along this is a bit like when you've got
00:29:23.840 --> 00:29:25.190
up to speed on the highway and your
00:29:25.200 --> 00:29:26.789
car's just going along at the speed
00:29:26.799 --> 00:29:29.029
limit mining
00:29:29.039 --> 00:29:30.549
neutral and then just put it in neutral
00:29:30.559 --> 00:29:32.789
and you just Cruise a lot and at this
00:29:32.799 --> 00:29:34.350
point you've got a couple of days of the
00:29:34.360 --> 00:29:36.430
astronauts feeling weightless because
00:29:36.440 --> 00:29:37.830
they're moving at the same speed as the
00:29:37.840 --> 00:29:39.870
spacecraft around them and they just
00:29:39.880 --> 00:29:41.470
curse along and then when you get near
00:29:41.480 --> 00:29:44.190
to the Moon you're going too quickly to
00:29:44.200 --> 00:29:45.430
orbit the Moon because you're going at
00:29:45.440 --> 00:29:47.430
the speed you need to do to get there so
00:29:47.440 --> 00:29:49.269
you need to turn around and slow down
00:29:49.279 --> 00:29:51.230
again to slow down enough to get into
00:29:51.240 --> 00:29:53.310
orbit around the moon and so the Rockets
00:29:53.320 --> 00:29:54.830
burn again pushing you in the other
00:29:54.840 --> 00:29:57.269
direction slowing you down until you're
00:29:57.279 --> 00:29:59.230
moving on an orbit around the Moon that
00:29:59.240 --> 00:30:01.549
kind of circular and maybe a few tens of
00:30:01.559 --> 00:30:03.909
kilometers above the moon's surface and
00:30:03.919 --> 00:30:05.470
he sit there for a while and check that
00:30:05.480 --> 00:30:07.669
everything's okay because it's hard work
00:30:07.679 --> 00:30:09.389
and you want to make sure things are
00:30:09.399 --> 00:30:11.710
right but then when the astronuts went
00:30:11.720 --> 00:30:13.509
to the moon the final part was that two
00:30:13.519 --> 00:30:15.590
of the astronauts on the mission climbed
00:30:15.600 --> 00:30:17.950
into this small Landing module and the
00:30:17.960 --> 00:30:20.029
third one stayed piloting the Orbiter
00:30:20.039 --> 00:30:21.549
they stayed above the Moon and didn't go
00:30:21.559 --> 00:30:23.750
down to the surface but the landing
00:30:23.760 --> 00:30:25.669
module separated from the orbitor got
00:30:25.679 --> 00:30:28.230
nudged away and then used its own small
00:30:28.240 --> 00:30:30.430
little Rockets to boost and slow down
00:30:30.440 --> 00:30:32.669
and boost and slow down until it touched
00:30:32.679 --> 00:30:35.110
down landed safely at a specific point
00:30:35.120 --> 00:30:37.269
on the moon and the pilot had to watch
00:30:37.279 --> 00:30:38.549
up what they were doing they were kind
00:30:38.559 --> 00:30:40.190
of looking out at the ground below to
00:30:40.200 --> 00:30:42.430
pick the best place to land and with the
00:30:42.440 --> 00:30:44.269
very first landing when Neil arong and
00:30:44.279 --> 00:30:46.470
buz Aldren landed on the moon they kept
00:30:46.480 --> 00:30:47.950
going and kept going and nearly run out
00:30:47.960 --> 00:30:49.950
of fuel they only had a few seconds left
00:30:49.960 --> 00:30:51.950
before they would have to abort and
00:30:51.960 --> 00:30:54.029
boost back up because when you land on
00:30:54.039 --> 00:30:56.190
the moon you've got to get back so they
00:30:56.200 --> 00:30:57.990
land on the moon they do all their fun
00:30:58.000 --> 00:31:00.470
things they bounce around like kangaroos
00:31:00.480 --> 00:31:02.430
but then to get back to Earth they've
00:31:02.440 --> 00:31:03.950
got to get back in this small Landing
00:31:03.960 --> 00:31:06.190
module which is probably not got much
00:31:06.200 --> 00:31:07.789
more room in it to be honest in the
00:31:07.799 --> 00:31:11.029
interior of your car strap themselves in
00:31:11.039 --> 00:31:13.629
and then the top of the module detaches
00:31:13.639 --> 00:31:15.789
leaving the legs behind and the rocket
00:31:15.799 --> 00:31:18.070
pushes them back up so they can get into
00:31:18.080 --> 00:31:20.950
orbit around the Moon they dock and
00:31:20.960 --> 00:31:23.990
reconnect with the parent spacecraft
00:31:24.000 --> 00:31:25.629
that the pilot was sad in Waiting for a
00:31:25.639 --> 00:31:27.509
couple of days on their own then they
00:31:27.519 --> 00:31:29.070
turn on their rockets and they come back
00:31:29.080 --> 00:31:31.669
to the Earth same thing they boost up up
00:31:31.679 --> 00:31:34.029
to a high speed then they Cruise along
00:31:34.039 --> 00:31:35.389
floating there for a couple of days
00:31:35.399 --> 00:31:37.549
until they get near the Earth then they
00:31:37.559 --> 00:31:39.549
boost their Rockets again to slow down
00:31:39.559 --> 00:31:42.389
fall into the atmosphere and land again
00:31:42.399 --> 00:31:44.990
so it's a big long dramatic Journey now
00:31:45.000 --> 00:31:46.590
we've got better technology now so we
00:31:46.600 --> 00:31:48.549
can do it more effectively and that's
00:31:48.559 --> 00:31:51.070
why NASA are hoping to send people back
00:31:51.080 --> 00:31:53.870
to the moon in the next few years now
00:31:53.880 --> 00:31:55.990
everybody who went to the moon so far
00:31:56.000 --> 00:31:58.070
all 12 people who walked on the moon
00:31:58.080 --> 00:31:59.629
were people who looked a bit like me and
00:31:59.639 --> 00:32:01.789
Andrew and Fred they were older white
00:32:01.799 --> 00:32:05.230
men and that was it that it and you know
00:32:05.240 --> 00:32:06.590
these were all people who trained as
00:32:06.600 --> 00:32:09.110
test pilots and stuff like this with the
00:32:09.120 --> 00:32:10.590
next people landing on the moon they're
00:32:10.600 --> 00:32:13.909
going to be mon you know a wider variety
00:32:13.919 --> 00:32:16.070
of people so the hope is that in a few
00:32:16.080 --> 00:32:17.590
years time we'll see the first woman
00:32:17.600 --> 00:32:19.669
walk on the moon and the third person
00:32:19.679 --> 00:32:21.549
who isn't white to walk on the moon as
00:32:21.559 --> 00:32:23.509
well and that'll be really good because
00:32:23.519 --> 00:32:25.029
it's important to know that this is
00:32:25.039 --> 00:32:27.509
something anybody can do everybody could
00:32:27.519 --> 00:32:29.070
learn to be an astronaut it's very
00:32:29.080 --> 00:32:31.509
competitive and really hard but if you
00:32:31.519 --> 00:32:33.149
only ever see people who look like me
00:32:33.159 --> 00:32:34.549
and Andrew do it you'll think they're
00:32:34.559 --> 00:32:36.750
the only kind of people who can so it's
00:32:36.760 --> 00:32:39.350
really important to have everybody
00:32:39.360 --> 00:32:40.830
represented in this and I think it's
00:32:40.840 --> 00:32:43.310
really exciting that in a few years time
00:32:43.320 --> 00:32:44.870
we won't just talk about men walking on
00:32:44.880 --> 00:32:46.669
the moon but we'll talk about men and
00:32:46.679 --> 00:32:47.990
women walking on the moon that's going
00:32:48.000 --> 00:32:50.909
to be really cool yes it is I I grew up
00:32:50.919 --> 00:32:54.990
in the pionering era of uh space flight
00:32:55.000 --> 00:32:57.509
and and going to the moon and I was
00:32:57.519 --> 00:33:00.190
quite Young when Neil Armstrong put his
00:33:00.200 --> 00:33:01.870
foot on the surface and was followed by
00:33:01.880 --> 00:33:04.310
buz Aldren I was so very lucky to meet
00:33:04.320 --> 00:33:07.149
buz Aldren many many years later and I
00:33:07.159 --> 00:33:08.669
got to interview him for the Australian
00:33:08.679 --> 00:33:10.590
Broadcasting Corporation that was
00:33:10.600 --> 00:33:12.509
probably one of the highlights of my
00:33:12.519 --> 00:33:14.509
career to be honest to to meet someone
00:33:14.519 --> 00:33:16.350
so famous one of the most famous people
00:33:16.360 --> 00:33:18.470
in the world because of what he did but
00:33:18.480 --> 00:33:20.190
it's reached a point now where people
00:33:20.200 --> 00:33:22.190
are going up and down all the time into
00:33:22.200 --> 00:33:24.389
space and we'll never know their names
00:33:24.399 --> 00:33:27.350
because it's become so common but as you
00:33:27.360 --> 00:33:29.590
say emis going back to the moon and
00:33:29.600 --> 00:33:31.590
those people setting foot on the surface
00:33:31.600 --> 00:33:35.789
again men and women of multiple Races
00:33:35.799 --> 00:33:39.029
they will again reignite that Fame that
00:33:39.039 --> 00:33:40.549
goes with doing something so
00:33:40.559 --> 00:33:42.509
extraordinary and and Emily I would
00:33:42.519 --> 00:33:45.590
imagine that in your lifetime uh it will
00:33:45.600 --> 00:33:47.190
reach a point where there will be people
00:33:47.200 --> 00:33:50.549
living on the moon I I expect that will
00:33:50.559 --> 00:33:53.990
happen might have happen in my lifetime
00:33:54.000 --> 00:33:55.870
but certainly in yours it'll be very
00:33:55.880 --> 00:33:59.230
different maybe even Mars Emily H uh
00:33:59.240 --> 00:34:01.389
thank you for the question thanks Sandy
00:34:01.399 --> 00:34:03.990
um always great to hear from our younger
00:34:04.000 --> 00:34:06.909
listeners um joty I'm going to make an
00:34:06.919 --> 00:34:08.869
executive decision and I'm going to
00:34:08.879 --> 00:34:11.230
pigeon hole Fenton until next week
00:34:11.240 --> 00:34:13.589
because his question is two hours long
00:34:13.599 --> 00:34:15.990
yeah and I imagine the answer will be
00:34:16.000 --> 00:34:18.589
five times that so um I just don't think
00:34:18.599 --> 00:34:20.869
we can fit it in today but it's a great
00:34:20.879 --> 00:34:22.750
question about the radiation of Jupiter
00:34:22.760 --> 00:34:24.990
we will put that at the top of the tree
00:34:25.000 --> 00:34:27.909
for next week's Q&A episode but thanks
00:34:27.919 --> 00:34:29.270
to everyone who contributed and don't
00:34:29.280 --> 00:34:31.069
forget if you've got questions for us
00:34:31.079 --> 00:34:33.270
jump on our website SPAC nuts
00:34:33.280 --> 00:34:37.750
podcast.com and SPAC nuts. our two URLs
00:34:37.760 --> 00:34:40.270
and uh just click on that little AMA
00:34:40.280 --> 00:34:41.950
Link at the top that's where you send
00:34:41.960 --> 00:34:43.829
you text and audio questions if you've
00:34:43.839 --> 00:34:45.430
got a device with a microphone you're
00:34:45.440 --> 00:34:47.510
all set and have a look around while
00:34:47.520 --> 00:34:48.790
you're there and don't forget our social
00:34:48.800 --> 00:34:51.990
media uh very very active the Space Nuts
00:34:52.000 --> 00:34:54.790
Facebook uh page is our official page
00:34:54.800 --> 00:34:57.230
but we've got the Space Nuts podcast
00:34:57.240 --> 00:35:00.150
group Facebook page where people get
00:35:00.160 --> 00:35:01.829
together and chat and talk and and
00:35:01.839 --> 00:35:04.109
compare photos and notes and yeah it's
00:35:04.119 --> 00:35:06.790
very very active it's a great site and
00:35:06.800 --> 00:35:08.550
thanks to our administrators who look
00:35:08.560 --> 00:35:10.550
after it for us because I haven't got
00:35:10.560 --> 00:35:12.670
time most of the time except when I've
00:35:12.680 --> 00:35:16.710
got time and it's time to go uh thank
00:35:16.720 --> 00:35:19.270
you very much Johnny always great fun
00:35:19.280 --> 00:35:20.990
we'll catch you next week yeah catch you
00:35:21.000 --> 00:35:23.030
later thank you for having me Johnny
00:35:23.040 --> 00:35:25.630
Horner a professor of astrophysics at
00:35:25.640 --> 00:35:29.069
the University of qu Southern Queensland
00:35:29.079 --> 00:35:32.030
uh joining us while Fred is away and
00:35:32.040 --> 00:35:34.870
we'll speak to jonty again next week and
00:35:34.880 --> 00:35:38.109
to here in the studio uh he was awall
00:35:38.119 --> 00:35:40.390
because he's um putting P plates on his
00:35:40.400 --> 00:35:43.550
car so that he can go faster and for me
00:35:43.560 --> 00:35:45.109
Andrew Dunley thanks for your company
00:35:45.119 --> 00:35:47.190
we'll catch you on the very next episode
00:35:47.200 --> 00:35:50.950
of Space Nuts bye-bye Space Nuts you'll
00:35:50.960 --> 00:35:54.030
be listening to the Space Nuts
00:35:54.040 --> 00:35:57.030
podcast available at Apple podcasts
00:35:57.040 --> 00:36:00.109
Spotify by ihart radio or your favorite
00:36:00.119 --> 00:36:02.349
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demand at bites.com this has been
00:36:05.079 --> 00:36:07.470
another quality podcast production from
00:36:07.480 --> 00:36:10.280
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