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