We are 100% user supported.
 

Home > Flashcards > Astronomy > Astronomy Final

Details

Title: Astronomy Final

Description: ast301 final

Total Flash Cards: 80

Created: 12/02/2008 20:24:18

New Users: To study from this flashcard set, or to create your own your own study flash cards, REGISTER HERE.

Existing Users: CLICK HERE.

Additional Astronomy Flashcards

Cards in this set:

Term
Why does hydrogen burning keep the Sun in gravitational equilibrium?
Definition
as gravity pushes inward, energy released from fusion maintains the internal gas pressure that pushes outward
Term
Why does it take so long for a photon in the Sun's center to get to us?
Definition
the photon's "random walk"-- plasma in solar interior so dense that photon can't travel far before it interacts with an electron, deflected in another direction
Term
in a visual binary...
Definition
we can see both stars directly
Term
in an eclipsing binary...
Definition
we see a change in brightness (change of light curve of star when one eclipses the other)
Term
in a spectroscopic binary...
Definition
we see a change in radial velocity (doppler shift in star's spectral lines)
Term
if 2 stars have the same temperature and different luminosity, is mass the same?
Definition
no
Term
if 2 stars have different temperatures and the same luminosity, can the mass be the same?
Definition
yes
Term
as luminosity increases...
Definition
...mass increases
Term
H-R diagram of globular cluster is useful because
Definition
it determines the age of cluster at "main-sequence turnoff" point, where hot, short-lived stars have died
Term
Why does a collapsing gas cloud form a disk?
Definition
gas contracts under force of gravity---Conservation of Angular Momentum---gas flattens into spinning disk
Term
stars with mass <.08 solar mass don't fuse H because..
Definition
they can't compress & there is no nuclear burning because degeneracy pressure overcomes gravity
Term
when star burns all H in core, it expands because
Definition
core H exhausted---core shrinks/hears---H shell burning occurs---star expands into a red giant
Term
solar mass stars do not enrich the ISM because...
Definition
they have no helium capture or supernovae explosions
Term
what are the 3 types of "stellar corpses"?
Definition
white dwarf (least massive) neutron star black hole (most massive)
Term
what supports a white dwarf?
Definition
electron degeneracy pressure
Term
what supports a neutron star?
Definition
neutron degeneracy pressure
Term
what supports a black hole?
Definition
nothing; it has collapsed in on itself
Term
what mechanism creates a pulsar?
Definition
(1)iron core collapses into neutron star (2)neutron star spins rapidly (3)has magnetic field misaligned with its spin axis (4)particles trapped in magnetic field, collide with other particles (5)collisions give off light
Term
what causes superbubbles and galactic fountains?
Definition
supernovae explosions
Term
superbubble
Definition
expanding shell of hot gas given off by supernovae explosion
Term
Why does the rotation curve of our Solar System not require dark matter but that of the Milky Way does?
Definition
not enough dark matter enclosed in the solar system to affect it
Term
why are cepheids used as standard candles?
Definition
we can det each cepheid's luminosity by its period
Term
why might we be able to use gamma-ray bursts as standard candles?
Definition
//QUASAR, except all material accretes at once
Term
quasar
Definition
brightest type of active galactic nucleus
Term
active galactic nuclei
Definition
unusually luminous centers of galaxies powered by accretion onto supermassive black holes
Term
how did Hubble discover his law?
Definition
by measuring the redshifts of galaxies & estimating distances, using the brightest obj. in every galaxy as a standard candle
Term
the Universe is expanding but our bodies are not because...
Definition
Hubble's Law applies to big distances, its affect on us negligible
Term
distance ladder fm closest to farthest:
Definition
radar > parallax > main sequence fitting > cepheids > white dwarf supernovae > Hubble's Law
Term
how to det dist to nearby stars?
Definition
parallax
Term
how to det dist to obj in milky way?
Definition
main sequence fitting
Term
how to det dist to nearby/distant galaxies?
Definition
white dwarf supernovae (by way of distant standards)
Term
in theory, halo stars are older than disk stars because...
Definition
halo stars formed before galaxy's gas fell into disk; disk stars formed after collapse
Term
by observation, we know halo stars are older than disk stars because
Definition
new stars only formed in disk (very little (cold) gas in halo) and the halo lacks heavy elements
Term
nature argument in elliptical galaxies
Definition
(1)low spin (2) high star formation efficiency
Term
nurture argument in elliptical galaxies
Definition
(1)collisions/mergers (2)accretions/cannibalism
Term
arguments for "quasars are powered by accretion onto a supermassive black hole"
Definition
because black hole explains quasar's extreme luminosity, its small size, and how massive it is
Term
more quasars in the past because
Definition
black holes have used up fuel, leaving only black hole (because galaxies have already been created)
Term
stars w/ high concentrations of elements other that H and He likely formed in..
Definition
elliptical galaxies
Term
the first estimate of where the center of the Milky Way is came from...
Definition
locations of globular clusters
Term
what causes a pulsar?
Definition
misalignment of the rotation axis and magnetic field axis
Term
galactic fountain is due to
Definition
gravitational pull of the disk
Term
compared to a blue galaxy, a red galaxy has..
Definition
older stars
Term
Where are blue stars?
Definition
on the leading side of a spiral arm
Term
how are heavy elements supplied to the ISM?
Definition
-helium capture -supernova
Term
If the temp of the Sun's core were to increase due to an increase in the rate of fusion..
Definition
the core would expand, reducing the pressure and temperature, and the rate of fusion would decrease back to its original level
Term
physical mechanism responsible for the solar wind?
Definition
magnetic fields get generated in the convective zones. As they make their way to the surface, the fields get released into the corona and eventually break, causing material to shoot away from the Sun.
Term
after sun converts H to He, the remaining H...
Definition
converts to other forms of energy and ultimately emitted in the form of radiation
Term
Annie Cannon and Cecilia Payne-Gasposchkin known for
Definition
understanding stellar spectral classification
Term
what is a red giant?
Definition
when He burning in core
Term
Why is measurement of neutrinos important?
Definition
means that we understand energy mechanism in the Sun
Term
Why is measurement of neutrinos important?
Definition
means that we understand energy mechanism in the Sun
Term
All atoms prominant in biological systems are created...
Definition
in high-mass stars
Term
globular clusters are important to study because
Definition
all stars are about the same age
Term
a star spends about 10% of its life on
Definition
the giant branch
Term
the Sun is mainly composed of
Definition
H
Term
the Proton-Proton chain creates..
Definition
neutrinos, gamma-rays, and positrons
Term
a main sequence star converts
Definition
H --> He
Term
the idea that an explosion that we see on the Sun actually occurred 8.3 minutes ago is known as
Definition
lookback time
Term
we can detect MACHOs by
Definition
gravitational lensing events
Term
a standard candle is
Definition
a light source of known brightness
Term
a flat universe means that
Definition
our universe is at the critical density
Term
galaxies with extremely bright centers are called
Definition
active galactic nuclei
Term
3 facts about bullet cluster
Definition
(1)gas @ diff location than galaxies (2)dark matter at diff location than gas (3)proves dark matter exists
Term
Hubble's law implies that
Definition
the Universe's age is finite
Term
Galactic bulges and halos are called
Definition
spheroids
Term
cepheids are important since they measure distances to
Definition
nearby galaxies
Term
WIMPs are hard to detect because
Definition
they do not have much of an effect on other particles
Term
3 facts about quasars
Definition
(1)inside galaxies (2)more common in the past (3)supermassive black holes actively eating
Term
why is the H-R diagram for globular clusters important?
Definition
the location of the main-sequence turnoff point determines the age of the globular cluster
Term
solar mass stars do not enrich the ISM because
Definition
-no He capture -no supernovae
Term
how pulsar created
Definition
high-mass star goes supernova---neutron star---degeneracy pressure and a lot of spin---misaligned axes
Term
how does a pulsar give off light?
Definition
(1)mag field not align with spin axis (2)particles trapped in mag field collide with other particles
Term
how did Hubble discover Hubble's Law?
Definition
measured period of cepheids in Andromeda
Term
distance ladder
Definition
radar---parallax---cepheids---white dwarf supernova
Term
arguments for why quasars pwrd by accretion onto supermassive black hole:
Definition
quasars= extremely small and massive (mass det by ext. brightness)
Term
3 ways to measure mass of galaxy clusters
Definition
(1)measure radial velocity of galaxies (2)gravitational lensing (3)x-ray to see hot gas--observe temp/luminosity = mass
Term
There were more quasars in the past because
Definition
matter that used to create friction(ENERGY SOURCE) have fallen into the black hole, rendering it invisible
Term
observational evidence for "dark matter outweighs normal matter by 9 to 1"
Definition
(1)rotation curve of our galaxy (2)bullet clusters
Term
why did Einstein create the cosmological constant?
Definition
to represent a repulsive force/energy that might cause universe to accelerate with time; counter gravity keep galaxies from falling in on each other
Term
active galactic nuclei is..
Definition
unusually luminous centers of some galaxies powered by accretion onto supermassive black holes (quasars=brightest type)



Home  ·  Login  ·  myFlashCards  ·  FlashCardDB  ·  Help  ·  Links  ·  Flash Cards by Subject


© 2001-2009 Flash Card Machine, LLC. Privacy Policy / Terms of Use
Design/Development by Madhu