Last ditch Flashcards

1
Q

What are the two reasons that a reflecting telescope with a mirror of 2m in diameter is preferable to one with a 1m diameter mirror

A
  1. Smaller diffraction limit, allows objects with smaller angular separation to be clearly resolved
  2. More light gathering capability
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2
Q

What is the most important reason that the Chandra X-ray observatory is located in space, as opposed to being on Earht

A

X-rays are mainly abosorbed by the Earth’s atmosphere

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3
Q

Describe some of the evidence that there is a supermassive black hole at the center of the milky way

A
  • Orbits of stars near galactic center (K’s 3rd law to get a very large mass)
  • Direct radio imaging of event horizon with event horizon telescope
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4
Q

what is a standard candle

A

Distant source of light with known luminosity. Use that to get apparent brightness and inverse law to get distance

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5
Q

Why are type Ia supernova a good standard candle

A

Type Ia supernova have the same luminosity since they all come from the explosion of WD once they reach Chandrasekhar limit. Also so bright they can be seen in distant galaxies

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6
Q

Why are there many more white dwarfs than planetary nebulae

A

Planetary nebulae dissipate rapidly while WDs live very long

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7
Q

What is a red dwarf

A

Smallest star on the main sequence

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8
Q

What is needed to change with the moon in order to change the tides on Earth

A

Mass and distance

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9
Q

What experimental evidence caused scientists to abandon the steady state theory

A

Discovery of the cosmic microwave background radiation

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10
Q

What observations make us believe that the universe is filled with dark energy

A

Observations of distant supernovae show that the universe is accelerating its rate of expansion

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11
Q

How do we know that much of the light from a quasar comes from an extremely small volume

A

Fluctuates on a time scale of days, so it must be smaller than light-days, which is very small compared to a galaxy

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12
Q

Rank the following from smallest to biggest:
- neutron star
- red giant
- sun
- solar system
- singularity of a black hole
- white dwarf

A

singularity (zero size), neutron star, WD, sun, red giant, solar system

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13
Q

Rank the following in order of decreasing contribution to total energy content of the universe
- H
- He
- elements not H and He
- Dark energy
- dark matter

A

Dark energy, dark matter, H, He, elements other than H and He

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14
Q

Put the following in chronological order
-formation of first stars
- cosmis “dark age”
- formation of atoms
- formation of nuclei
- inflation
- formation of protons and neutrons

A

inflation, formation of neutrons and protons, formation of nuclei, formation of atoms, dark ages, first stars

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15
Q

What are the three types of galaxies and which type is the milky way

A

spiral, elliptical, and irregular. Milky way is spiral

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16
Q

What was discovered via radio telescope to be a new kind of celestial object and what are they

A

Pulsars, rapidly rotating neutron stars

17
Q

How does galactic rotation provide evidence for dark matter

A

Galactic rotation curves are plots of rotational velocity vs distance from center of galaxy. If one uses just the visible mass, can predict the amt of mass at smaller radius, and thus this in Kepler’s 3rd law to calculate what rotational speed should be. For most galaxies this fails, proving there is more mass than is visible in the galaxy, and that this mass extend to much large radii than does the visible mass: dark matter

18
Q

Look at picture in study guide. What is it? what do the spots represent? Explain relevance to clusters and superclusters of galaxies

A

Temperature of the CMB. Diff colored spots are slightly hotter and colder regions. Spots will gradually grow and turn into clusters or superclusters of galaxies

19
Q

what are the three scenarios for the future of the universe

A
  1. collapsing: big crunch
  2. flat: right amount of matter to balance
  3. open: expanding universe
20
Q

what is critical density

A

Overall density needed to “win” against gravity. faster expanding universe = more density needed

21
Q

What are Quasars and what is their importance

A

“Quasi-stellar radio source” that are found to be located at the same spot in the sky. Are incredibly red-shifted that they must be receding at a huge speed. So bright that they give us a window into galaxies in the early universe

22
Q

What is the Tully-Fisher Law

A

Luminosity depends on the rotational rate. Spiral galaxies with higher rotational velocities tend to be more luminous.

23
Q

What are the two broad classes of stars and how do they differ

A

Population I stars
- in the disk, orbiting the galactic center
- typically young open clusters
- composed largely of heavy elements (composed of the remnants of other stars)
Population II stars
- mainly in the halo, follow elliptical orbits
- typically very old (11 - 13 billions years)
- Almost entirely H or He

24
Q

What is gravitational lensing

A

When there is a large object between you and a light source, the light will be bent so that you can see it in two places. Can sometimes result in an “Einstein ring” around the object