1
|
- Today: Finish Chapter
13, Galaxies
-
“Town Meeting”
|
2
|
|
3
|
|
4
|
|
5
|
|
6
|
|
7
|
|
8
|
- Galaxies live in clusters
- Rich clusters: thousands of
galaxies
- Poor clusters: Fewer than a
thousand
|
9
|
|
10
|
- Galaxies live in clusters
- Rich clusters: thousands of
galaxies
- Poor clusters: Few than a
thousand
- Fundamental difference between stars and galaxies:
- Stars live isolated lives:
- They are much smaller than distance between them
- They virtually never collide
- Galaxies are not isolated
- They are only slightly smaller than the distances between them
- The can (and do) collide, and interact with gas within clusters
|
11
|
- Stars pass “through” each other, but orbits around galaxy
disrupted
- Gas clouds collide
- Gas stripped away from stars
- Collisions cause bursts of star formation
- Ellipticals may be those galaxies which have suffered collisions
- Spirals may be those galaxies which have not suffered collisions
- Joshua Barnes (Hawaii) and the Space Telescope Science Institude provide
a simulation of the Antenna Galaxies: http://imgsrc.stsci.edu/op/pubinfo/pr/1997/34/images/anima.mov
|
12
|
|
13
|
|
14
|
- From the Space Telescope Science Institute which also provided the
Cartwheel image in the textbook:
- http://imgsrc.hubblesite.org/hu/discoveries/striking_encounters/graphics/cartwheel.mpg
|
15
|
|
16
|
|
17
|
- Movie simulation of galaxy formation via assembly of small pieces
(courtesy of Space Telescope Science Institute): http://imgsrc.stsci.edu/op/pubinfo/mpeg/galaxies.mpg
|
18
|
- Family of Galaxies
- Properties of Galaxies
- Distance; The Hubble Law
- Size and Luminosity
- Mass (including Dark Matter)
- Evolution of Galaxies
|