Astronomy Final Flashcards

(46 cards)

1
Q

What are the standard units for luminosity?

A

Watts

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2
Q

Purpose of adaptive optics

A

Eliminate distorting effects of atmospheric turbulence for telescopes on the ground

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3
Q

How does the sun generate energy?

A

Nuclear Fusion

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4
Q

What observations characterize solar maximum?

A

we see many sunspots on the sun’s surface

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5
Q

When white light passes through a cool cloud of gas, we see

A

an absorption line spectrum

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6
Q

How are wavelength, frequency, and energy related for photons of light?

A

Longer wavelength means lower frequency and lower energy

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7
Q

HR Diagram: Cool and Dim

A

Lower right

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8
Q

Overall fusion reaction by which the sun produces energy

A

4 H -> He + Energy

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9
Q

Thermal Radiation:

A

radiation that depends only on the emitting objects temperature.

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10
Q

Layers of the sun from center outward

A

Core, radiation zone, convection zone, photosphere, chromosphere, corona

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11
Q

What is true of images captured in X-Ray telescopes?

A

Always displayed in false color

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12
Q

What is the closest temperature to the CORE of the sun?

A

10 million K

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13
Q

What is NOT an advantage of the Hubble Telescope over ground-based telescopes?

A

It is closer to the stars

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14
Q

Luminosity

A

Total amount of light that the star radiates each second

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15
Q

Gravitational Equilibrium

A

balance between the outward push of pressure and the inward pull of gravity.

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16
Q

On the main sequence, stars obtain their energy by

A

converting hydrogen to helium

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17
Q

HR Diagram: Largest Radii

A

Upper right

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18
Q

Lowest energy- highest energy:

Different categories of electromagnetic radiation

A

radio, infrared, visible light, ultraviolet, x-ray, gamma

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19
Q

Cluster ages can be determines from

A

main-sequence turnoff

20
Q

Size of the neutron star

21
Q

What temperature can helium fusion occur?

A

100 million K

22
Q

What is the closest in mass to a white dwarf?

23
Q

10-solar mass main-sequence star will produce a:

24
Q

Planetary Nebula

A

expanding shell of gas that is no longer gravitationally held tot he remnant of a low-mass star

25
What's the upper limit to the mass of a white dwarf?
1.4 solar masses
26
How is time affected by gravity?
Time runs slower in places where gravity is stronger
27
Stages of life for a low-mass star:
Protostar, main-sequence, red giant, white dwarf
28
How many helium nuclei fuse together when making carbon?
3
29
How does gravity of an object affect light?
Light from a massive object will be redshifted
30
Pulsar:
an object that emits flashes of light several times per second or more, with near perfect regularity
31
What is the closest in size to a white dwarf?
Earth
32
White dwarfs are called so because
they are both very hot and very small
33
What happens after a helium flash?
the core quickly heats up and expands
34
How far is the sun from the center of the galaxy?
28,000 light-years
35
How did Edwin Hubble measure the distance to the Andromeda Galaxy?
applied the period-luminocity relation to cepheid variables
36
Diameter of the Milky way?
100,000 light-years
37
Why do we cal dark matter "dark"
Emits no or very little radiation of any wavelength
38
Dark Energy
the agent causing the universal expansion to accelerate
39
Methods for determining distance: nearest to farthest
parallax, main-sequence fitting, cepheid variables, Tully-Fisher, Hubble's Law
40
Quasar:
Extremely bright center of a distant galaxy, thought to be powered by a massive black hole.
41
Spectral Sequence in order of decreasing temperature
OBAFGKM
42
Hubble's Law
Recession velocity of a galaxy is directly proportional to its distance from us
43
Most large galaxies are:
Spiral or lenticular
44
Galaxy type most commonly found in large clusters
Ellipticals
45
What happens when a star exhausts its core hydrogen supply?
Its core contracts, but its outer layers expand and the star becomes bigger and brighter
46
How long does it take the sun to orbit the Milky Way Galaxy?
230 million years