Revision: 6:05 pm, Tuesday, 24 January 2012
Original: 2:50 pm, Friday, January 20, 2012
Test 1, 26 January 2012
Astronomy 123
Winter 2012
Material: Topic 1 (drawn from parts of Chapters 23-27),
Topic 2 (Chapter 23 and part of 24) (as far get in Topic 2)
Old Test
INTRODUCTION
- Cosmology: What is the definition of cosmology? Is cosmology science?
- Contrast Universe and universe. Why does the fact
that we have observations of only 1 universe hinder theory? What is meant by
multiverse?
- What makes a model scientific? Contrast science and philosophy.
Is cosmology a science or is it philosophy? Defend your position.
- Basic Observations of cosmology (which drive the Big Bang Theory):
- The Universe is expanding as implied by Hubble's Law
(24.3). Who initially discovered Hubble's Law? .
What is the naive interpretation
of Hubble's Law? What is the Principle of Mediocrity and how does it
contribute to our
interpretation of Hubble's Law? What is the current interpreration
accepted by most astronomers for Hubble's Law? What is z? What is meant
by redshift? How are redshifts of galaxies determined?
- Cosmic Microwave Background Radiation (CMBR), What is it? When was it
formed? What are we observing when we see the
CMBR? What are the properties of the CMBR? (26.7) (What is its temperature?
Are there deviations from the mean temperature of the CMBR, if so, what are
they and how are they interpreted?) What is horizon problem?
(27.4) What is COBE? What is WMAP?
- Chemical composition of the normal matter in the
Universe is roughly 90 % hydrogen and ~ 10 %
helium (everyting else heavier than helium is referred to as a metal
and makes-up only a small part of the Universe). How is the
chemical composition of the Universe used as a piece of evidence
which strongly supports the
Big Bang theory.
- What is the
make-up of the overall Universe? What is dark matter? What is normal matter?
What is dark energy?
Who first proposed the idea of some sort of dark energy and why?
What fraction of the Universe is normal matter?
Cosmological Principles:
- What is the Principle of Mediocrity?
- What is the Copernican Revolution? What is the significance of
annual trigonometric parallax for the Copernican Revolution?(pp 27-28).
Explain how Hubble's
Law may be explained through uniform expansion of the Universe.
- Are we at the Center of the Galaxy? Describe how Herschel and
Kapteyn, and Shapley (23.2) attempted to find our location in the Galaxy
and the size of the Galaxy. What did Herschel, Kapteyn, and Shapley conclude
about the location of the Sun in the Milky Way galaxy? Who was correct?
Why did the ones who were in error reach their erroneous conclussions (talk
about dust, what is dust?)? How do we currently study the structure of the
Galaxy? What
is the location of the Sun and the true shape of the Milky Way galaxy?
- Cosmological Principle (26.1), what is it? What is meant by
the terms homogeneity
and isotropy? (The Universe is clearly not bland and uniform on all
scales, so why can homogeneity and isotropy of the Universe be useful
assumptions?)
In the Cosmological Principle is the Universe allowed to evolve in time? Could
it be unchanging in time under the Cosmological Principle? What is a nice
example that our Universe is homogeneous and isotropic?
- Perfect Cosmological Principle, what is it? It is not currently used by
astronomers when they model the Universe. What are some reasons why
the Perfect Cosmological Principle is not in favor? What is the Cosmological
Constant? Why did Einstern propose the Cosmological Constant?
Why did Einstein withdraw his
suggestion of a Cosmological Constant?
- Anthropic Principle, What is the Anthropic Principle?
Does Jim like the Anthropic Principle? Why does
Jim like (or dislike) the Anthropic Principle?
- Describe the Big Bang Theory.
Upon what observations is the Big Bang Theory based? Is the Big Bang on
firm observational footing?
Milky Way Galaxy (Chapter 23 and Chapter 24, Hubble galaxy types,
and Hubble Tuning Fork diagram.
- Milky Way Galaxy:
- What is the Hubble classification of the Milky Way galaxy?
- Briefly describe the apparance of the Milky Way galaxy. What are the
three primary regions of the Milky Way galaxy? What are the properties of
these regions? How large are they? What are their stellar populations?
Which contains the largest amount of mass? ... ? What are the overall
properties of the Milky Way galaxy?
- A black hole lives in the center of the Milky Way galaxy.
What is the mass of the black hole at the center of our Galaxy?
Roughly, what is the density of stars near the center of our Galaxy?
- What are Population I stars? What are Population II stars? Where are
each found?
- How is the structure of the Milky Way galaxy determined? What objects are
used to study the structure of the Milky Way galaxy? Why are OB stars, H I
regions, H II regions, Giant Molecular Clouds used to study the spiral arms
of our Galaxy? What is meant by H I? by H II? Why are these particular
objects so important?
- What are galactic rotation curves (what kinds of rotation curves did I
discuss in class)?
How far do rotation curves
extend beyond the visible disk of our Galaxy? Describe how rotation curves
are used to deduce the masses of spiral galaxies. (Describe orbital motion.)
(Note--how fast does the Sun move in its orbit about the center
of the Milky Way galaxy? How large is the orbit of the Sun about the center
of the Milky Way galaxy?)
- What is the significance of the fact that most
rotation curves are nearly flat at large distances from the centers of the
gaalxies (the galaxy spins at nearly the same speed
at large distances as at small distances from its center)? What is the
strength of the gravitational force one feels at the center of the Earth?
Explain your answer. Does a tennis ball or a ping pong ball feel a stronger
force (due to gravity) near the surface of the Earth? Which accelerates
faster?
- How do the mass
estimates from rotation curve affect the question of the amount of Dark Matter
in our Galaxy?
- Sketch the Hubble Tuning Fork diagram, be sure to include schematic
representations of ellipticals, spirals, barred spirals, S0s & SB0s
(lenticulars), and Irregulars, By schmeatic, I mean indicate the flattening of
ellipticals, bulge sizes, and the tightness of the winding of spiral arms.
Hubble Galaxy Classification scheme (24.1)
- Describe Elliptical, Spiral, Barred Spiral, SBO, S0, and Irregulars.
What are Lenticulars (S0s)?
What the differences between Sa, Sb, and Sc galaxies, S and SB galaxies,
E0 to E7 galaxies, Irr I and Irr II galaxies.
- Is the Hubble Tuning Fork diagram an evolutionary sequence? (Do galaxies
evolve from one Hubble class to another?)
What role (if any) do galactic colliions
play in galaxy evolution?