Astro 3 - Key Themes in My Test Bank
This is a generic list. I made this by looking at all the
~ 250 questions in my test bank. Remember that I make my quizzes and finals
fresh each semester, and you'll see roughly 120 questions drawn randomly from
this master test bank. For more help
in studying for your particular questions, refer to the study guide I handed
out and which is on-line for the Monday/Wednesday, and for the Monday evening
classes, which focuses in a different way on your particular exams. Looks
like a lot to learn here, right? But before you get depressed, realize that
your particular exams will only sample a small part of this, and all you need
is a 80% for an "A". You can do it!
Chap 0: Scientific Thinking
- All
of "Chap 0" is important! Read it thoroughly and ask for any clarifications
- The
steps of the scientific method
- The
nature and psychological issues of pseudo-science.
- Occam's
Razor and Sagan's Corollary
- Modes
of representing reality in our minds
- The
fatal flaws with supernaturalism
Our Place in the Universe
- Most
of this material we will cover in more detail later so I have not written
questions on it. But, I do have a few introductory ideas for you to focus
on
- Distances;
definition of a light year, the general distance order of things out
there; planets, stars, galaxies.
- There are 4 forces in Nature, which account for pretty much all we see so far.
Earth and Sky
- How the seasons and the sky look different at different latitudes.
- How
the sun moves across our sky differently during different seasons.
- How to
relate the phases of the moon and time of day to where the moon appears in
the sky.
- The
nature of lunar and solar eclipses; what phase they occur and the nature
of the shadows involved.
- Understand
the cause of retrograde motion.
Gravity, Motion, Relativity
- Know
Kepler's 3 laws and their meaning
- Know
Newton's 3 Laws of Motion and their meaning
- Gravity - stronger with increasing mass and with decreasing separation of the gravitating objects
- Feel the force of gravity and how it would change if you were inside a spherical distribution of mass
- Tides
as more than water at the beach - the cause of tides via gravity and what
aspects of a gravitating system will increase or decrease tidal force
- Spring
tides and neap tides and how they relate to the position of sun, moon.
- The
meaning of angular momentum and conservation of angular momentum
- (Astro 4 only) General
relativity = modern gravity, paths follow curvature of space, determined
by mass, energy density.
Light, Matter
- Photons
as electromagnetic waves in a particle form
- The
two ways to produce photons.
- The
electromagnetic spectrum and the names of the different energy or wavelength
bands in the spectrum. Which bands will pass through earth's atmosphere.
- The
structure of the atom: nucleus and electrons in quantized orbits. Don't
memorize the names of atoms and how many protons! I want concepts.
- Emission
and absorption of photons via electrons changing orbits in atoms, and how
these processes make the spectral "lines" in astronomical objects.
- Absorption
lines: produced by cool gas in front of a hot object
- Emission
lines: produced by gas lit up from the side against a black background.
- The
Doppler effects; photons "redshifted" to longer wavelength if source / observer
are moving apart; "blueshifted" if moving towards each other
- Know
the shape of a thermal spectrum, and the two thermal radiation laws: Hotter
objects are bluer. Hotter objects give off more total light.
Telescopes, Detectors
* Large modern telescopes
are all reflecting telescopes, using mirrors and not lenses
* Imaging is done with
CCD detectors - digital for astronomers
* Only Visible and Radio
bands make it through the earth's atmosphere and can be studied from ground-based
telescopes
* Light gathering is the
most important property of a telescope. Size matters, big!!
Formation of the Solar System
- Know
how we have detected solar systems around other stars
- The
key features of our solar system any theory must explain: ~circular orbits,
co-planar, revolve in same direction, same plane as sun's equator.
- Inner
planets vs. outer planets general properties; rocky, thin atmosphere vs. hydrogen/helium rich giants with small rocky cores.
- The
roll of tides in the formation of our solar system, and the general formation
process, and age.
- The
two regions of comets, Oort Cloud and Kuiper Belt and where they are
- How planets lose their initial atmosphere;
the different processes that govern how a planet's atmosphere evolves.
- The
age of the solar system; 4.6 billion years
The Terrestrial Worlds (Mercury, Venus, Earth, Mars,
the Moon)
- The
origin of planets' interior heat; kinetic energy of collisions.
- The
factors which govern how rapidly a planet loses heat
- How the rate of impacts on planets has
evolved since their formation
- The
nature of the Greenhouse Effect
- Tectonic
activity; nature and logic of why only Earth has it
- History
of Martian water, magnetic field loss allowed solar wind to strip away atmosphere
Earth's Atmosphere
* CO2 history of Earth - overall decline with geologic time. Carbonate rocks created by life pulling CO2 out of atmosphere
* Milankovich orbital cycles and the Ice Ages
* Modern global warming - firmly established to be caused by humans, mainly CO2 from fossil fuel burning
* climate denialism, debunking myths
The Jovian Planets
- Why
Jupiter and Saturn give off more heat than they receive
- Tidal
stretching and friction and its effect on planetary moons
- Planetary
rings; origin and composition
Asteroids, Comets, Meteoroids
- Relation
between comets and meteor showers
- Comets;
dirty snowballs and the two tails that develop
- The
asteroid belt; why did it form? Where is it?
- The
two regions of comets; Kuiper Belt and Oort Cloud; where they are
The Sun
- The
structure of the sun; layers
- Sunspots
and the sunspot cycle
- Stars
- balancing gravity, energy production, pressure. How changing one will
affect the structure of the star
- Aurorae;
relation to the solar corona, magnetic fields
Life in the Universe
- The
Miller-Urey experiment created amino acids out of the chemistry, conditions
of the early Earth
- G,
K main sequence stars most likely to have living planets
- Carbon
- the only element permitted by the laws of physics which can be used to
make complex molecules, why needed for life.
- The
argument for searching for radio communications near the main spectral lines
for water
- mixing dirt and organic chemicals
can produce RNA, precursor to the first life?
- Know basic theory of evolution
by natural selection