Quiz
ASTR 107 Exam 3 Study Guide
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Questions in this quiz (19)
1What does it mean that the universe is homogenous?
- AThe universe looks the same from every perspective
- BGalaxies are generally distributed evenly throughout the universe
- CAll stars in all galaxies have planetary systems just like ours
- DThe universe has looked the same at all times in its history
2What do astronomers mean when they say that the universe is isotropic?
- AMore distant parts of the universe look just like nearby parts
- BIntergalactic gas has the same density everywhere in the universe
- CThe laws of physics apply everywhere in the universe
- DThe universe is the same in every direction
3Cosmological redshifts are calculated from observations of spectral lines from
- Aindividual stars in different galaxies
- Bclouds of dust and gas in different galaxies
- Cspectra of entire galaxies
- Drotations of the disks of distant galaxies
4Astronomers observe that all galaxies are moving away from the Milky Way. According to the cosmological principle, this observation suggests that
- Athe Milky Way is at the center of the universe
- Bthe Milky Way must be at the center of the expansion
- Cthe Big Bang occurred at the current location of the Milky Way
- Dan observer in a distant galaxy would make the same observation
5Some galaxies have redshifts (z) that if equated to Vr/c correspond to velocities greater than the speed of light. Special relativity is not violated
- Abecause of relativistic beaming
- Bbecause it's a trick of the measurement angle
- Cbecause redshifts carry no information
- Dbecause those velocities do not measure motion through space
6The Big Bang theory predicted
- Athe Hubble law
- Bthe cosmic microwave background radiation
- Cthe cosmological principle
- Dthe abundance of helium
- Ethe period-luminosity relationship of Cepheid variables
7The simplest way to estimate the age of the universe is from
- Ausing the slope of Hubble's Law
- Bthe age of Moon rocks
- Cmodels of stellar evolution
- Dmeasurements of the abundances of elements
8The CMB includes information about
- Athe age of the universe
- Bthe temperature of the early universe
- Cthe density of the early universe
- Ddensity fluctuations in the early universe
- Ethe motion of Earth around the center of the Milky Way
9Repeated measurements showing that the current helium abundance is much less than the value predicted by the Big Bang would imply that
- Asome part of the Big Bang theory is incorrect or incomplete
- Bthe current helium abundance is wrong
- Cscientists don't know how to measure helium abundances
10If the density of the universe is higher than the critical density, the universe will
- Aexpand forever
- Bexpand, but gradually slow down
- Ceventually collapse
- Dneither expand nor contract
11Dark energy has been hypothesized to solve which problem?
- Athe universe is expanding
- Bthe cosmic microwave background radiation is too smooth
- Cthe expansion of the universe is accelerating
- Dstars orbit the centers of galaxies too fast
12What problems of cosmology does inflation solve?
- Aflatness
- Bhorizon
- Cfluctuation
- Dsphere
13The first stars formed in the universe had [blank_start]fewer[blank_end] heavy elements and [blank_start]higher[blank_end] mass than the stars formed today.
- Afewer
- Bmore
- Chigher
- Dlower
14We expect the kinds of galaxies that we see at a redshift of z = 4 to be:
- Amuch like we see today
- Bsmaller and much more irregular looking than today
- Cfar more numerous but with more spiral galaxies
- Dlarger versions of what we see today
15Place the following in order of size, from smallest to largest.
[blank_start]a star[blank_end]
[blank_start]star clusters[blank_end]
[blank_start]a galaxy[blank_end][blank_start]the Local Group[blank_end]
[blank_start]Virgo Cluster[blank_end][blank_start]Laniakea[blank_end]
[blank_start]a wall[blank_end]- Aa star
- Bstar clusters
- Ca galaxy
- Dthe Local Group
- EVirgo Cluster
- FLaniakea
- Ga wall
16The dominant force in the formation of galaxies is
- Agravity
- Bangular momentum
- Cthe electromagnetic force
- Dthe strong nuclear force
17Larger galaxies form from the merging of small protogalaxies. That process is similar to the formation of:
- Astars
- Bplanets
- Cmolecular clouds
- Dasteroids
18Which of the following is a characteristic difference between cold and hot dark matter?
- Atemperature
- Bability to emit radiation
- Cthe way they clump under the influence of gravity
- Dmass density
19The dominant factor in the formation of galaxies is the distribution of [blank_start]dark matter[blank_end] in the early universe.
- Adark matter
Information
- Description
- Ch 19-24
- Author
- Roman Jordan
- Language
- English
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