Chapter 10,11,12,13 Flashcards
what does the nebular theory tell us about the giant planets?
- Giant planets must form quickly
- Giant planets must form beyond the frost line
- Gas giants should have solid cores of ice and dust. these should be 10 earth masses since this is the threshold for runaway recreation of gas.
Structure of gas planets
top-down: atmosphere crust mantle and core.
high pressure in the interior causes phase of hydrogen to change with depth. At highest pressure, selectrons can stream freely acting like metals
facts about Jupiter
- Jupiter’s core is not dense, solid mass at center
- solid materials mixed with gas out to 1/2 radius
How are mass and pressure linked
more mass compresses the gas making it smaller
What causes colours on Jupiter and Saturn
Ammonia is the highest coldest layer and it reflects all colours hence the white look
Ammonium sulphide clouds reflect red/brown colour and these form at lower altitudes where its hotter.
Wind pattern of gas giants
all four planets have differential rotation but Uranus and Neptune are simpler and more like Earth
Jupiter and storms?
Jupiter has some of the longest-lived storms
How are moons formed?
moon formation is the same as planet formation but smaller
IO and volcanic activity
Io has evidence of volcanic activity due to tidal heating these effects are weaker the further away you go
Europa’s geology?
- Euphora has lots of water ice available during formation
- Tidal heating acts on Europa too but to a lesser extent than Io
- Extra heat allows for liquid water ocean below the surface of Europa.
What two moons have evidence of water?
Both Europa and Ganymede show measurement changes in the magnetic field suggesting both moons have liquid water oceans beneath icy crusts
Titan Saturn’s largest moon
titan is the only moon with an atmosphere and is the second-largest moon in the solar system. that said it is likely covered by Saturn’s magnetosphere since it doesn’t have its own magnetic field
Enceladus (medium moon of Saturn)
ongoing cryovolcanism - eject water vapours and ice particles. Evidence of liquid water below the icy crust
Moons breakdown
see image:
Rings around gas planets
Saturn’s rings are very thin and consist of ice and boulders, these particles collide and sometimes stick together. any particles with incline collide more often also losing their incline. Bright regions have higher particle density whilst darker regions have lower particle density.