Ep. 63: Neptune

We’ve reached Neptune, the final planet in our tour through the solar system – but don’t worry! The tour’s not over, but after this week we’ll be all out of planets. Neptune has a controversial story about its discovery, some of the strongest winds in the solar system and some weird moons.

 

  • Episode 63: Neptune (14.7 MB)
  • Jump to Shownotes
  • Jump to Transcript or Download (coming soon!)
  • Shownotes

    Don’t forget to check out the rest of our solar system tour!

    Neptune

    Rings

    Satellites

    Images

     

     

    Transcript: Neptune

    Download the transcript

    Fraser Cain: Now we’ve reached Neptune, the final planet in our tour through the solar system – but don’t worry! The tour’s not over, but after this week we’ll be all out of planets. Neptune has a controversial story about its discovery; it has some of the strongest winds in the solar system and some weird moons. There’s plenty of interesting stuff to talk about Neptune.
     
    Should we talk about the discovery first?

    Dr. Pamela Gay: Seems like as good a place as any to begin.

    Fraser: I think it’s a cool story.

    Pamela: (laughing) I tend to agree.
     
    So, Neptune is actually the very first planet discovered strictly thanks to math. It was first seen by Galileo, but he totally missed the fact that it’s a planet because it was just entering retrograde when he observed it so it really wasn’t moving relative to the stars.

    Fraser: That happened with Uranus too – they saw it, didn’t know what it was and moved on. Or thought it was a star, put it in a catalogue, moved on.

    Pamela: Right, so that really doesn’t count. Yeah, he did see it, but he didn’t discover it.
     
    So once Uranus had been discovered, people were looking at its orbit, mapping its orbit, and they realised its orbit made no sense. They could explain its orbit if there was another planet, another large planet, out beyond Uranus.
     
    So there was a British mathematician, Adams, who threw out all sorts of different possible places for Neptune to be. He’s throwing out ideas, doing calculations, pre-calculator, pre-computer – it’s not easy to do, but you can still do it accurately. H e just didn’t.

    Fraser: If he had better math, he could’ve come up with the right number, he just had bad math or bad observations?

    Pamela: Well, Adams was a theorist, so he’s working purely with mathematics. You have to be careful and make sure you take everything into account, and it’s a lot of detailed mathematics. He didn’t always do it perfectly. So he threw out multiple possible locations for where Neptune could be located. There was no planet name at that point – it was the mystery planet pulling on Uranus. It was never found.
     
    Then, Urbain Le Verrier, in 1846, he did very careful mathematics, came through, got an answer, and tried to get an observer to look.
     
    Then one day in September of 1846, he pointed out “hey, we have these great hand-drawn maps of this one area of the sky.� He got Johann Gottfried Galle to go and look in the area of the sky the maps already existed for, that his mathematics indicated Neptune should be located in. the very first night they went out and looked, they were able to compare the maps with the actual sky and find Neptune as the object that wasn’t there when the maps were drawn.

    Fraser: Okay, so because Neptune moves so slowly, if they just looked in the region of the sky, they’d only see a bunch of stars and wouldn’t be able to tell from one night to the next if something was moving. Especially because it wasn’t like they had photography and a way to capture an image each night. They just had to look and remember and draw some pictures. So they found an old map that showed where all the stars were and then saw something that shouldn’t be there.

    Pamela: It was really cool. His calculations were within one degree of the actual location. Considering all the positions of all of the planets were based on visual estimates, which means you’re going to introduce a fair amount of error as you’re looking through the telescope at the sky and drawing pictures of things relative to one another. They did have good etchings on some of the eyepieces that allowed them to calibrate things, but you’re still going to have errors cropping up. One degree is a really good error.
     
    The thing was, one of Adams’ many calculations was actually within ten degrees of where Neptune was found.

    Fraser: Uh oh.

    Pamela: So here’s Adams in England, and Verrier in France – two countries that didn’t exactly like each other in the 1800s. Adams is going, “I predicted it too!â€? and stomping up and down and England is stomping up and down with him and there’s of course all sorts of international intrigue and they’re arguing over what the thing should be named and they’re trying to give it nationalistic naming… and now, we’re thinking more and more that Adams was not right.
     
    The thing is, all the papers regarding Adams’ calculations sort of haven’t been around for people to consult for a while. There’s an astronomer, Olin J. Eggen – O.J. Eggen, the breakfast astronomer – really good astronomer, did some excellent work, and somehow in the process of his lifetime of research, he scooped up Adams’ papers. It wasn’t until after he died in 1998 that people were going through his papers and found all of the records for what Adams’ had done.
     
    When all this intrigue had initially happened, it was finally decided to jointly give credit to Adams and Verrier and allow to both countries to stand there and go, “we discovered this new planet.� Now it’s looking like England might need to take a step back and say, “okay this time France is actually the country that can claim the person who made the correct calculations.�

    Fraser: Yeah, I’m sure that’ll happen.

    Pamela: Yeah… no. But at least the history is starting to get it sorted out.
     
    The name Neptune was actually sort of settled upon by a Russian astronomer, so this really was a full international affair to get from the point of starting the mathematics, doing the mathematics correctly, and saying we’re going to name it Neptune. Neptune is another Roman God, and it sort of fits in with the rest of the planets, most of which had been named in ancient times. What’s kind of cool is since it’s a modern naming, pretty much all nations have some form of the God of the Sea as the name for this particular planet.

    Fraser: That’s cool. I didn’t know that.

    Pamela: Yeah.

    Fraser: I think it’s funny to hear how, around that time, it was quite an age of scientific discovery. In the 1800’s, they put a lot of emphasis on it. There are so many stories on it, about that time. I remember there was the planetary transit of Venus across the surface of the Sun, and the search for elementary particles. A lot of these things are very similar – there were countries competing to get to the bottom of this. In many cases a lot of the stories all worked out kind of the same way – they’re racing to the same discovery at the same time. It’s neat to hear Neptune was part of that.
     
    Okay, so what do we know about Neptune?

    Pamela: We’ve finally been able to start getting detailed observations of it thanks to first the Voyager 2 mission in 1989 and now we also have observations from the Hubble Space Telescope and the Very Large Telescope down in the southern hemisphere.
     
    Unlike Uranus, Neptune isn’t just a big blue blob. It actually has some of the most fascinating storms in the entire solar system. Its winds are practically supersonic. They’re whipping along at upwards of 2000km/s. so we have these extremely high-speed winds.

    Fraser: Hold on. Neptune has weirder storms, higher wind speeds than Uranus, but it’s further away? How is this possible?

    Pamela: That’s actually one of the things people have struggled with. How do you end up with this crazy set of storms going on? What it appears to be is Neptune’s core is still much warmer. It has a several thousand-degree core – its centre is about the same temperature as the surface of the sun (which is true of pretty much all the planets except Uranus, which has a cooler core). It’s the temperature difference between how hot it is in Neptune’s core and how cold it is on Neptune’s surface that helps to drive all these amazing wind storms that are going on.

    Fraser: I actually did an article (this is way out of left field), about a year and a half ago, about the possibility that there are liquid oceans in Neptune or Neptune-type objects in extrasolar planetary systems. You could have the right combination of warm core and pressures that water could end up being oceans. You could move down through the planet, hit ocean, and move further down and hit super hot compressed water that wouldn’t be good for life. But you could actually hit a reasonable spot somewhere in between.

    Pamela: What’s so neat about these worlds is yeah – we call them ice giants because the type of stuff their inner layers are made of is stuff that for whatever reason (even if it’s not frozen solid) we refer to as ice (so it has water, ammonia, etc). They are, just like you said, heated so much and under so much pressure, that they’re either acting like liquids or they’re actually starting to be at that point where they’re so hot they would be gases if it wasn’t for the amount of pressure they’re under. So there’s really weird, cool fluid dynamics going on in the different layers of this object.
     
    Neptune’s just a funky system geologically, thanks to this neat combination of high internal heat, cold temperatures on the surface, and it’s just out there generating storms. It had a giant dark spot for a while that was likened very much to Jupiter’s Red Spot. It’s had dark spots. The storms appear to come and go over time. It has seasons, and because it is tilted so much we can see the seasons change from one pole getting more heat to the other pole getting more heat.
     
    All these different changes really cause weird things to happen. In fact, right now the south pole of Neptune is about ten degrees Celsius warmer than the rest of Neptune. That slight difference is just enough to make the methane gas in the atmosphere change from icy crystals to gas. So methane gas is coming out the south pole of Neptune, which is just a cartoon waiting to happen.

    Fraser: (laughing) Yeah, you thought you giggled when you talked about Uranus.

    Pamela: But this isn’t the pronunciation! This is actually what Neptune is doing. Neptune is blowing gas out its pole.
     
    [laughter]
     
    You have to laugh, it’s real though – it’s what the science is showing us.

    Fraser: Well it’s real… but it’s what you’re focusing on that’s…
     
    [laughter]
     
    Let’s talk about the winds again, because that’s crazy. Up to 2000km/hr, right?

    Pamela: Yeah, near supersonic speeds.

    Fraser: The only other place we see winds that strong are around extrasolar planets that are hot Jupiters. They’re right up close to their parent star, they’re tidally locked, they’re experiencing thousands of degree differences of temperatures from one face to the other, and that severe temperature difference is causing the supersonic winds to whip around the planet to stabilise things out. Neptune… you’ve got a few degree difference from the feeble Sun… but how can it be whipped up to those kinds of temperatures?

    Pamela: You have a core that’s 7000 degrees and a surface that is -200 degrees Celsius. So here it’s instead of having strictly winds going from the dark side of the planet to the light side of the planet, instead you have churning that is going from the lower layers of the atmosphere out to the outer layers of the atmosphere. Combined with rotation rates and the day and night cycles… all these different things combine to give these multi-thousand kilometre per hour winds.

    Fraser: Wouldn’t it be even? It would be working on all directions at the same time, so it should even out.

    Pamela: You end up getting convective cells.

    Fraser: Right.

    Pamela: It’s the same sort of bulk motion of the hot stuff in the centre rising to the surface, cools off, and flows back down. This can end up driving entire weather systems.

    Fraser: All right. I’m going to chalk it up as a great big mystery and move on. We don’t know.
     
    Now, let’s talk about observations. Before the 1980’s, all we had was a tiny little blue dot.

    Pamela: Yeah.

    Fraser: Now, with Voyager 2 and with Hubble, we’ve got a much better view. What did Voyager see?

    Pamela: Voyager saw these amazing storms on it. That was the first thing that was noticed as Voyager started to approach Neptune. First it had this giant darker storm. They named a cluster of these little white storms Scooters. That’s just kind of cutesy. So there were these little whiter storms moving around faster than the dark storm.
     
    After how boring Uranus had been, it was amazing to see this planet with these high speed storms and all these little wispy features all over its surface.

    Fraser: Rings? Does Neptune have rings?

    Pamela: It has a few of some of the wussiest rings in the entire solar system, but they actually behave differently than any of the other rings.
     
    In general, dynamically we expect that if you get a chunk of something falling apart in a ring, very quickly it will end up spreading itself evenly out around the ring. When we look at Neptune’s rings, we actually find these arcs in the rings where when you look at one particular ring, you’ll see little tiny sections of the ring that seem to be much thicker and much brighter than other sections. These arcs are something we haven’t seen anywhere else. We think these arcs are actually due to different resonances with one of Neptune’s moons. So in this case, it’s Galatea who’s in a 43:42 resonance (which is a really crazy-small resonance).

    Fraser: What do you mean, though? The rings go around 43 times for every 42 orbits…?

    Pamela: Right. So these random times they line up, one goes around 43 times and the other goes around 42 times and they line up with each other… is just enough to end up creating little acrlets inside the ring where the material is a little bit thicker.

    Fraser: Okay, it’s almost like it builds up. It’s like a wobble on the ring that clumps together and piles up each time Galatea comes around, so we’re able to see them as arcs.

    Pamela: Exactly. That leads to a feature that we just haven’t seen anywhere else in the solar system. So it has these rings, they’re very wussy rings, but they still have some really neat features that we haven’t seen anywhere else in the solar system.

    Fraser: Now, I remember, back in the day when I was a kid, there was a sort of historic moment where Neptune became the most distant planet, passing the orbit of Pluto. Now of course, with Pluto not being a planet, that distinction doesn’t matter anymore, but let’s talk about that switching.

    Pamela: Back when we thought Pluto was a planet, Pluto and Neptune’s orbits are such that they intersect each other. Mathematically, they’re never going to run into each other. It’s timed just right that the two of them are never in the same place at the same time. Not only that, but because of the tilts of the orbits, their physical orbits don’t actually cross one another either.

    Fraser: Right, but if you look at it from up above, it would look like they’re crossing.

    Pamela: Yeah.

    Fraser: But in three dimensions, they don’t actually get that close to each other.

    Pamela: Even if we’re only limiting it to looking at the crossing points, they never end up at the crossing point at the same time.

    Fraser: They have a resonance.

    Pamela: Yeah. This resonance, Pluto and Charon aren’t the only things in that resonance. This leads to a lot of people saying, “wait… the International Astronomical Union says one of the definitions of a planet is that you’ve cleared out your orbit in the solar system.� Pluto is in Neptune’s orbit. Charon is in Neptune’s orbit. All these other things are in Neptune’s orbit… so how has it cleared out is orbit?
     
    The IAU definition actually refers more to has it cleared its orbit of other things the same size. Is it the gravitationally dominant object in its orbit. If you look at how big Neptune is, there’s nothing near its size in its orbit.

    Fraser: There aren’t other Neptunes orbiting in the same place.

    Pamela: Right. So Neptune is the biggest thing in its orbit, the same way the Earth and the Moon are the biggest things in their orbit. There are lots of near-Earth objects crossing our orbit all the time. We don’t question if Earth is a planet or if Jupiter (which has lots of things sharing its orbit) is a planet.

    Fraser: We already covered what’s a planet, back in our very first episode, and I’m sure we’ll bring it back up again with the Pluto conversation – yes, we’ll still go to Pluto on the tour.
     
    But I wonder if there was another Neptune, would that be… anyway. We could go on forever.
     
    So does Neptune have a roughly circular orbit, and it’s Pluto that has the really elliptical one?

    Pamela: It’s Pluto that has the crazy-elliptical orbit. The eccentricity of Neptune’s orbit is 0.01, which basically means it’s a circle.

    Fraser: It’s a circle. Right.

    Pamela: So it has this really nice, pretty much circular orbit. The difference between its furthest point and its nearest points is only 100 million kilometres. When it’s 4 billion kilometres away, that’s not that big a difference. So yeah, it’s basically a circular orbit.

    Fraser: Let’s talk about its moons.

    Pamela: It actually has one of the cooler moons in the solar system. Its moon Triton (which somehow works well with Neptune) goes the wrong way around the planet.

    Fraser: Wha?!

    Pamela: Yeah.
     
    So you have Neptune happily doing its I’m-going-to-spin-on-my-axis thing going one way, and that’s the direction it lines up with the entire rest of the solar system.
     
    Triton is basically fighting against the current in a purely retrograde motion.

    Fraser: So if you looked at it from above, the Earth, Jupiter, Saturn, Mars, even Neptune… they’re all rotating in the same direction. All the moons are all going in the same direction as well, around their parent planets?

    Pamela: All the major moons.

    Fraser: So there are other retrograde moons out there.

    Pamela: But none of them are big! They’re little tiny things that you know were captured. Triton’s a nice, big moon. It’s actually the 7th largest moon of all the moons in the solar system. So the fact that it’s going in reverse says it didn’t actually form where it’s located. What we’re now thinking is it’s a captured Kuiper Belt Object.
     
    So once upon a time, just like Pluto, Sedna or Charon, it was out orbiting by itself. It was probably actually orbiting with a second Kuiper Belt Object – it was probably in a binary dwarf planet system. Somehow there was a 3-body interaction with Neptune, Triton and this other object (we don’t know where it went). In the interaction, Triton was carefully captured, it’s now in an almost exactly circular orbit, and it was captured such that it’s now going the wrong way around Neptune.

    Fraser: Can you explain the concept of the 3-body interaction? I think that’s pretty important.

    Pamela: There are a lot of different ways that things can gravitationally interact. The 3-body problem is perhaps one of the most complicated mathematics to try and sort out that is still solvable in a few cases.

    Fraser: All right, I think our listeners are going to want to do the math in front of them – so everyone get a piece of paper and a pen…

    Pamela: Um…

    Fraser: I was kidding.

    Pamela: Yeah – no. I like our listeners too much to do that to them.

    Fraser: All right. We’ll just go with… generalities.

    Pamela: There’s only really one complete solution to a 3-body problem, and that was figured out by Victor Zebehe. You can, with computer modelling, chew through 3-body problems and see if you have these two small objects come in and they get disrupted in this way, one gets flung out violently in one direction and the other can get captured.

    Fraser: It’s almost like how we shoot spacecraft at planet through gravitational assist, but because of the dynamics between the three objects, one gets slingshotted out, and one has to stay.

    Pamela: This happens all the time in the universe. We have binary systems in globular clusters where one of the stars gets pulled off of the binary and the other one rejoins another star or the entire binary gets disrupted. It looks like it happened with Triton and another object. We can see different places where it looks like a binary system was disrupted.
     
    In this particular case, the disruption led to Triton being nice and gracefully captured. Since it’s going the wrong way, it’s constantly getting stuff slamming into its face – which makes it somewhat interesting geologically because it’s been resurfaced very recently.

    Fraser: So, because it’s going the wrong way, it acts like a vacuum cleaner?
     
    [laughter]

    Pamela: Pretty much. If you look at the nose of Triton, for lack of a better way to describe it, the part that’s leading through its orbit, looking at that area and out in a circular pattern around it, you start finding all these large craters from where things have slammed into it. These craters are concentrated around the nose that it’s putting forward as it orbits. If these craters were randomly distributed over the surface of Triton, we might be able to figure out some where swept up from things orbiting Neptune, others were Kuiper Belt Objects that hit Triton… but it looks like the majority of the craters are coming from things that Triton probably swept up that were orbiting Neptune (in the correct direction) that it slammed face-first into.

    Fraser: So what does the future hold for Triton?

    Pamela: It’s actually slowly spiralling in toward its doom.

    Fraser: Uh oh.

    Pamela: Yeah, yeah… this is what happens when you go the wrong way around your planet. Its orbit is actually decaying such that it’s getting a little bit closer in every year, and it looks like in about three and a half billion years (not that we need to worry about it real soon), it’s going to get close enough that it will get tidally disrupted and it’s going to end up adding to the ring system around Neptune.

    Fraser: So it’s going to go through the Roche limit.

    Pamela: It’s going to go through the Roche limit. It’s going to get disrupted. It’s going to become rings.

    Fraser: So it won’t be able to hold itself together gravitationally, the gravity of Neptune will tear it apart, and it will have a ring. I wonder what kind of ring that would be? It would probably be the biggest ring in the solar system, wouldn’t it? It’d be crazy!

    Pamela: It doesn’t have a whole lot of mass, so I’d actually need to look up the numbers to see if the mass of Triton is greater than the mass in the rings of Saturn. I’m not sure how the masses add up. It would be a really shiny ring, because Triton does have a lot of ices, a lot of water ice in it. All of these shiny liquids, once it breaks apart… it has frozen nitrogen/dry ice… these things reflect light really well. So when it breaks apart, it’s going to create all these shiny ice chunks that are going to very readily reflect sunlight back toward observers, wherever they happen to be observing from.

    Fraser: In 3.5 billion years, the Sun won’t be destroyed yet, but it will be a lot brighter, so it might actually be a really pretty view.

    Pamela: It just might be. So in the future, there will be some pretty, shiny, highly reflective rings around Neptune.

    Fraser: Are there any spacecraft headed to Neptune for the future?

    Pamela: Not right now. There have been people who’ve put forward the idea of doing a Cassini-style mission – go, explore, see what the moons have to offer, study the storm systems… but it’s far out. It’s expensive to get to. So right now, there’s nothing concrete other than firm desire to go out and take a look.

    Fraser: It’s interesting – Neptune is more interesting than Uranus, from a science point of view.

    Pamela: Yeah, and that boils down to it has more interesting weather because it’s a lot hotter on the inside.

    Fraser: Right. Okay. I think that wraps up all our planets, but there’s still some more solar system left. The tour isn’t over yet – we’ll keep going.

    Pamela: We have a whole lot of ice.

    Fraser: There’s ice, the Oort Cloud, the Heliopause, Heliosphere and interactions with the rest of our galaxy – there’s still a little ways to go.

    Pamela: So maybe we’ll wrap it up by Christmas. We’ll see.

    Fraser: And then maybe we’ll just tour through the Milky Way… I don’t know.

    This transcript is not an exact match to the audio file. It has been edited for clarity.

    5 Responses to Ep. 63: Neptune

    1. chance April 3, 2008 at 10:07 am #

      it helped me with my school work,THANKS!!!!!!!

    2. Submitter April 11, 2008 at 9:30 pm #

      The pdf transcript is an empty file (0 kb).

    3. B.s.d January 6, 2009 at 3:11 pm #

      ok i dont get this website

    4. Me March 7, 2013 at 5:24 am #

      confusing but helpful with homework!

    5. Sólver July 16, 2014 at 7:52 am #

      Fuzzy shoulder imp again: The transcript needs little revision. While explaining the extreme wind on Neptune it was misspoken 2000km/s instead of 2000m/s: “They’re whipping along at upwards of 2000km/s. so we have these extremely high-speed winds.”

    Leave a Reply

    Powered by WordPress. Designed by WooThemes