Here’s what stars
look like with a
spectrograph.
What would it
look like with
a disk around it?
Slide 27
In reality, disks are very hard to image.
Why do you think this is?
So we usually use spectroscopy to study disks.
Disks produce infrared light (just like planets)
Here’s what stars
look like with a
spectrograph.
What would it
look like with
a disk around it?
Slide 28
Our theory: What do we think now?
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
Slide 29
Ways to Find Out
Look at our own solar system, and think about how it might have formed
Look at other solar systems while they form
Look for and study other solar systems
Create computer models and see if you can produce a solar system
Slide 30
Ways to Find Out
Look at our own solar system, and think about how it might have formed
Look at other solar systems while they form
Look for and study other solar systems
Create computer models and see if you can produce a solar system
Slide 31
http://www.astronomy.ohio-state.edu/~microfun/ob06109/
Slide 32
Slide 33
Ways to Find Out
Look at our own solar system, and think about how it might have formed
Look at other solar systems while they form
Look for and study other solar systems
Create computer models and see if you can produce a solar system
Slide 34
Our theory: What do we think now?
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