|
1.
|
In
the Hubble classification scheme for spiral galaxies, the tightness of the
winding of the spiral arms appears to be related directly to
|
|
|
A)
|
the
age of the galaxy, as determined from the age of its individual stars.
|
|
|
B)
|
the
number of globular clusters in the halo of the galaxy.
|
|
|
C)
|
the
overall intrinsic size of the galaxy, or the diameter across the spiral arms.
|
|
|
D)
|
the
size of the central bulge of the galaxy.
|
|
|
2.
|
The
typical diameter of a spiral galaxy is about
|
|
|
A)
|
107
ly.
|
|
|
B)
|
105
ly.
|
|
|
C)
|
1
ly.
|
|
|
D)
|
100
ly.
|
|
|
3.
|
What
mechanism is believed to produce flocculent spiral galaxies?
|
|
|
A)
|
Satellite
galaxies plunging through the disk of the nuclear spiral galaxy
|
|
|
B)
|
Self-propagating
star formation, where star formation occurs in bursts
|
|
|
C)
|
Shock
waves from explosive star formation in the nuclear bulge
|
|
|
D)
|
Density
waves in the interstellar medium
|
|
|
4.
|
What
mechanism is believed to produce grand-design spiral galaxies?
|
|
|
A)
|
Shock
waves from explosive star formation in the nuclear bulge
|
|
|
B)
|
Density
waves in the interstellar medium
|
|
|
C)
|
Satellite
galaxies plunging through the disk of the nuclear spiral galaxy
|
|
|
D)
|
Self-propagating
star formation, where star formation occurs in bursts
|
|
|
5.
|
What
is the designation given to a galaxy with a large nuclear bulge and tightly
wound arms starting from a bar through the nuclear bulge?
|
|
|
A)
|
Sb
|
|
|
B)
|
SBa
|
|
|
C)
|
SBc
|
|
|
D)
|
Sa
|
|
|
6.
|
How
do most spiral galaxies rotate?
|
|||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||
|
A)
|
The
arms lead as the galaxy rotates (arms point forward).
|
|||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||
|
B)
|
Spiral
galaxies do not rotate; if they did, then the spiral pattern would soon
disappear.
|
|||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||
|
C)
|
We
do not know; they rotate far too slowly for us to have seen any motion in the
time since galaxies were discovered.
|
|||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||
|
D)
|
The
arms trail as the galaxy rotates (arms point backward).
1. D
2. B
3. B
4.B
5. B
6. D
7.C
8. B
9. C
10. A
|
|||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||
No comments:
Post a Comment