Hubble's Galaxy Classification

Quiz
•
Science
•
9th - 12th Grade
•
Hard
Standards-aligned
Yuri Setnik
Used 2+ times
FREE Resource
Student preview

8 questions
Show all answers
1.
MULTIPLE SELECT QUESTION
30 sec • 1 pt
Spiral galaxies are best described as
irregular in shape with random star movement.
regular in shape with mostly orderly star movement.
having a huge round shape with mostly very old stars.
having a galactic bulge with a huge central black hole.
Tags
NGSS.MS-ESS1-2
2.
MULTIPLE CHOICE QUESTION
30 sec • 1 pt
Spiral galaxies also contain massive lanes of gas & dust which leads to
supermassive black holes.
quasars.
large regions of new star formation.
aliens.
3.
MULTIPLE CHOICE QUESTION
30 sec • 1 pt
"Barred" spiral galaxies are called that because
they have very little material at the center.
they are really elliptical in shape.
they have a massive bar of material at the center.
of massive supernovae explosions near the center.
4.
MULTIPLE CHOICE QUESTION
30 sec • 1 pt
Astronomers currently classify the Milky Way as a(n)
circular galaxy
barred spiral galaxy
irregular galaxy
elliptical galaxy
5.
MULTIPLE SELECT QUESTION
30 sec • 1 pt
Elliptical galaxies can be described as having
no spiral arms and mostly very old stars.
a circular or elongated shape.
some spiral structure with lots of gas & dust.
an irregular shape with mostly old stars.
6.
MULTIPLE CHOICE QUESTION
30 sec • 1 pt
Compared to most elliptical galaxies, spiral galaxies are
very large by comparison.
very small by comparison.
about the same size.
are similar in size and shape to irregular galaxies.
7.
MULTIPLE CHOICE QUESTION
30 sec • 1 pt
The formation of giant elliptical galaxies may have been created by
collisions of supermassive black holes.
supernovae explosions and star mergers.
collisions and mergers of small irregular galaxies.
collisions and mergers of spiral galaxies.
8.
MULTIPLE CHOICE QUESTION
30 sec • 1 pt
Irregular galaxies are defined as having
very little star formation.
no real shape and are comparatively very small.
no star formation
supermassive black holes.
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