AStronomy final

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37 Terms

1
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The Milky Way has different populations of stars; the has the oldest stars in a large sphere of
randomly-tilted orbits while the has the youngest stars all orbiting in a plane.

halo; nucleus

2
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How did we first learn the Sun is not at the center of the Milky Way?

by mapping the location of
globular clusters on the sky

3
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Over time the slight amounts of heavier elements in the Milky Way’s gas increase due to

stars forging heavier elements and spreading them when they die

4
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How much of the Milky Way’s total mass is dark matter?

90 percent

5
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In the Milky Way, where do stars usually form?

in the spiral arms of the disk

6
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What are the Milky Way’s spiral arms?

regions of higher density where gas compresses and forms
new stars

7
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Why are high-mass stars only in spiral arms while low-mass stars are everywhere?

high-mass stars
die before leaving the arms but low-mass stars live long enough to drift away

8
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Which lists the order in which the stars of our galaxy formed?

nucleus and halo first, then disk, then
spiral arms

9
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As generations of stars are born and die, what do they do to the rest of the gas in a galaxy?

increase
the metallicity of the gas

10
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A red dwarf just born in a spiral arm would have a red dwarf born billions of years ago in the
nucleus.

higher metallicity

11
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Which galaxy component contains young and old stars, gas, and dust all orbiting in the same plane and
direction?

the disk

12
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Which galaxy component contains invisible mass whose gravity affects orbital speeds?

the dark
matter halo

13
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Which galaxy component contains old stars with tilted orbits and globular clusters?

the stellar halo

14
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Which galaxy component contains old stars with tilted orbits and the Milky Way’s central black hole?

the nucleus

15
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For a spiral galaxy, where are the low-metallicity low-mass stars found?

in the halo

16
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Which galaxy type forms the fewest stars?

elliptical galaxies

17
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What launches the narrow jets in some galaxies detected at radio wavelengths?

a supermassive
black hole’s accretion disk

18
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How do astronomers determine whether something is a small galaxy or a star cluster?

by seeing
whether more mass is required than the stars alone provide

19
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How do astronomers measure the total mass of a galaxy?

by observing orbital motions of stars and
gas

20
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Large elliptical galaxies today formed mostly through what process?

major mergers in massive dark
matter halos

21
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Medium-mass halos that grew slowly and avoided major mergers became what kind of galaxies?

spiral galaxies

22
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Small halos heated by the first stars in larger galaxies became what kind of galaxies?

dwarf irregular
galaxies

23
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Which distance method is used for a nearby star vs. a distant quasar?

parallax for stars; Hubble’s law
for quasars

24
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If light from a galaxy took 10 million years to reach us, how do we see it?

as it was 10 million years
ago

25
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If galaxy light traveled 10 billion years, how far has it likely traveled?

more than 10 billion light years

26
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Which observation helps us learn about the first galaxies?

observing very high-redshift galaxies

27
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Why doesn’t the expansion of the universe pull galaxy clusters apart?

their gravity holds them
together

28
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Between which objects would the expansion of space be greatest?

between the Milky Way and a
distant galaxy

29
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What observations reveal the expansion history of the universe?

supernova brightnesses and
redshifts

30
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What is the theoretical limit to how far we could see without expansion?

about 14 billion light years

31
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What explains why galaxies and clusters contain mass we cannot see?

dark matter

32
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What explains the accelerating expansion of the universe?

dark energy

33
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What explains the universe’s age, composition, and background radiation?

the Big Bang

34
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What test did the Big Bang pass?

predicting the abundance of light elements

35
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What do astronomers know happened before the Big Bang?

nothing is known about what came
before it

36
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How old is the universe?

about 14 billion years

37
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What determines the ultimate fate of the universe?

the balance of gravity and dark energy