, The eight planets and their dozens of moons trace out orbits that have remained basically the same for billions of years. But astronomers. Believe things were not always. This calm. Models suggest that, as the solar system formed four and a half billion years ago, objects movements were way more erratic., Unfortunately proving that hypothesis has been difficult because the passage of billions of years has done away with most of the evidence.. But recently scientists found a possible new clue. In a paper published last week in the Astrophysical Journal Letters a team of astronomers describe two unusual asteroids that may hint at our solar systems tumultuous past. The two asteroids called 203 Pompeja and 269 Justitia orbit in the main Asteroid belt that lies between the paths of Mars and Jupiter.. Both were actually discovered way back in the late 1800s, but scientists are still tracking them today. And during one recent observation of Pompeja researchers picked up on something they hadnt noticed before. Pompeja is far redder than other asteroids.. In fact, after searching through a catalog of past observations, the astronomers could only identify one similarly, red object out of all the known asteroids in the main belt Justitia.. Now its not like these rocks are tomatoes floating through space. To an astronomer. An asteroid is considered red if it reflects more light from the red end of the spectrum than from the blue end and its considered blue. If the reverse is true., It can be a subtle distinction, but it has major implications.

For a solar system. Object. Redness often indicates the presence of organic material on its surface. And its a trait that is almost always found in the outer solar system. Where objects are icy. Thats because, as radiation from the Sun strikes ice, it drives chemical reactions that end with the production of reddish organic matter.. So the process of forming organic molecules starts with an icy surface., But in the inner solar system, its just not cold enough to make icy bodies. And, as a result, there isnt much redness there either.. So astronomers are pretty certain that Pompeja and Justitia are not native to the inner solar system.. They look much more like the objects in the neighborhood of Pluto., And that raises the question of how Pompeja and Justitia got to the asteroid belt. If they didnt form there., And the authors suspect that the answer comes down to that turbulence in the early solar system., If the giant outer planets moved in their orbits, the way astronomers think they did, their gravity would have pushed some outer. Solar system objects, inward and launched others out., And today these two asteroids could be direct evidence of that upheaval. Billions of years ago. Theres, not yet enough evidence to seal the deal, but it lends some weight to a hypothesis that has so far been really hard to prove.. In other solar system news last week, planetary scientists also shared new insights about Jupiters largest moon Ganymede.. Ganymede has long interested astronomers because its pretty exceptional among moons.

, Its bigger than the planet, Mercury – it has its own permanent magnetic field and its icy surface may hide an ocean of liquid water larger than any on Earth., But that might not be all. According to a New paper published in the journal Nature, Astronomy, Ganymede, may also have an atmosphere containing water. Vapor. Researchers drew this conclusion from observations by NASAs Hubble Space Telescope, which has been keeping an eye on Ganymede since the 1990s.. In fact, last weeks, paper incorporated Hubble data going all the way back to its very first picture of the moon in 1998., And it helped answer a question that that first picture raised. See. This was an ultraviolet image that showed evidence of auroras on the moon.. Auroras are emissions of light that form as charged solar particles following magnetic field lines collide into atmospheric gases, such as oxygen in the case of Ganymede.. So this was exciting because it suggested that Ganymede had a magnetic field., But, as Hubble took more images. Astronomers noticed that the auroras always seemed brighter on one side of the moon than the other.. That asymmetry got them wondering what was going on. At the time they thought. Maybe it was because there were more single oxygen atoms in some areas than others. Atoms of oxygen. Emit light more efficiently at the wavelength, Hubble was observing than molecules of oxygen, so maybe they were behind the difference in brightness., But in 2018, Hubble used a more sensitive instrument to search for that atomic oxygen and came up mostly empty.

That sent the research team back To the drawing board. And they found another possible answer, water vapor., Like atomic oxygen molecules of water, emit light easily at the wavelength. Hubble was observing.. Now the question was just: Where could the water be coming from With a temperature always more than a hundred degrees? Below freezing Ganymedes surface is solid ice., But in the hottest part of the day, it can get warm enough near the equator, for molecules of water to sublimate off the surface and into the atmosphere., And when researchers examined this possibility, they found that the regions with brighter Auroras were the same regions where water vapor was expected to be in the atmosphere.. So it looks like not only is there liquid water inside Ganymede and solid water on top of Ganymede, but there may also be gaseous water above Ganymede. …, Which is a lot of water., And since water is a key ingredient to life, as we know it. This will be an interesting place to explore.. Fortunately, the European Space Agency is planning to do just that with their mission named JUICE, which will reach Ganymede in the early 2030s. From there, it will have a front row seat for Ganymedes, aurora water, rich atmosphere and who knows what else., Thanks for watching this episode Of SciShow, If you would like to help support the channel, we have a special Patreon just for this channel, which is all about exploring the universe outside of our world, and that Patreon is at Patreon.