Slide 35
Why can’t we make a huge computer simulation to explain everything?
How do you design a computer simulation?
Slide 36
What models would you create?
Slide 37
Slide 38
A model of planets
growing in a disk.
Slide 39
Slide 40
Slide 41
Some things we’ve learned from models:
Our basic theory holds up pretty well, but .
It’s hard to get little particles to stick to each other when
they collide.
It takes a really, really long time to make planets (maybe
too long??)
It’s hard to form planetary systems as flat as ours.
Slide 42
Solar system formation begins because of gravity - most stuff ends up in the sun
A disk is formed because of rotation
Planet cores form in the disk because rocks hit and/or gravitationally attract each other
If there’s ice around (> 5 AU from the star, where it’s cold) the cores are bigger. If big enough, they’ll suck gas out of the disk and form giant planets
Moons form via collision or capture or in mini disks
Theory:
Observations generally agree with theory, but it’s hard to see details. They also
show us that stars and disks are all very different from each other. And, they
gave us the surprising observation of outflows.
Simulations also agree with theory, but they can’t model everything at once, and
there are some problems (things take too long, for one)
Slide 43
Is our solar system unique?
Are there other Earth-like planets, or are we a fluke?
Under what conditions can Earth-like planets form?
Is life common or rare?