11/ imagine that you have obtained spectra for several
galaxies and have measured the redshift of each one to determine
its speed away from us. Here are your results:
Galaxy 1: recession velocity is 15000 km/s
Galaxy 2: recession velocity is 20000 km/s
Galaxy 3: recession velocity is 25000 km/s
Estimate the distance to each galaxy from Hubble’s Law. Assume
that H0 = 22km/s/Mlyr
A/ The distances are as follows:
Galaxy 1: 0.00147 Mlyr
Galaxy 2: 0.000110 Mlyr
Galaxy 3: 0.00088 Mlyr
B/ The distances are as follows:
Galaxy 1: 1.02 x 10^7 Mlyr
Galaxy 2: 1.82 x 10^7 Mlyr
Galaxy 3: 2.84 x 10^7 Mlyr
C/ The distances are as follows:
Galaxy 1: 31 Mlyr
Galaxy 2: 41 Mlyr
Galaxy 3: 52 Mlyr
D/ The distances are as follows:
Galaxy 1: 682 Mlyr
Galaxy 2: 909 Mlyr
Galaxy 3: 1136 Mlyr
12/ what may have happened to end the GUT era?
A/ the release of an enormous amount of energy, which may have
caused inflation
B/ the annihilation of all antiprotons and almost all
protons
C/ Gravity became distinct from the GUT force
D/ Hydrogen fusion reactions ceased
13/ What happens when a proton collides with an
antiproton?
A/ they “annihilate” and convert into 2 protons
B/ they fuse together
C/ they repel each other
D/ they start to orbit each other
14/ what is the cosmic microwave background?
A/ it is the period of rapid expansion early in the universe’s
history
B/ it is the wallpaper which covers the universe
C/ it is the left-over radiation from the Big Bang
D/ it is the left-over radiation from the first generation of
stars
15/ what type of spectrum does the cosmic microwave background
have?
A/ an absorption line spectrum
B/ an emission line spectrum
C/ a blackbody radiation spectrum
D/ a power law spectrum
16/ what 3 shortcomings of the Big Bang Model does the
Inflation Hypothesis help to solve?
A/
1. Its inability to explain what happened at the end of the
GUT Era
2. Its inability to explain what happened during the
Electroweak Era
3. Its inability to explain why our universe should be
observed to have an energy density equal to the critical energy
density
B/
1. Its inability to explain the origin of the large-scale
structure of matter
2. Its inability to explain the large-scale uniformity of the
universe
3. Its inability to explain where hydrogen and other heavy
elements made in the early universe come from
C/
1. Its inability to explain what happened during the Planck
Era
2. Its inability to explain why there should have been more
particles than antiparticles at the end of the Particle Era
3. Its inability to explain where the CMB comes from
D/
1. Its inability to explain the origin of the large-scale
structure of matter
2. Its inability to explain the large-scale uniformity of the
universe
3. Its inability to explain why our universe should be
observed to have an energy density equal to the critical energy
density