astronomy final Flashcards

(55 cards)

1
Q

What is nuclear fusion?

A

The process where two light atomic nuclei combine to form a heavier nucleus, releasing energy

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2
Q

What is lost in nuclear fusion?

A

Mass, which becomes a large amount of energy (E = mc^2)

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3
Q

What element is fused in stars like the Sun?

A

Hydrogen is fused into helium

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4
Q

What does nuclear fusion do in stars?

A

It powers the star and produces light and heat

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5
Q

Where does fusion take place?

A

In the core of stars

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6
Q

It can take energy a long time to escape a star;

A

True, since energy created in the core must make its way to the outside/surface of a star to radiate into space, which can take hundreds of thousands of years

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7
Q

What is the Big Bang theory?

A

The idea that the universe began from a tiny, hot dense point (singularity) that suddenly expanded violently and started cooling and has been expanding for 13.8 billion years

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8
Q

What are the three key pieces of evidence for the Big Bang theory?

A

Nucleosynthesis, the redshift of galaxies, and the cosmic microwave background radiation

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9
Q

What is cosmic microwave background radiation?

A

Leftover heat from the Big Bang. Would have started as visible light, but has been redshifted into microwave lengths. Discovered as a signal-like background noise discovered by radio astronomers in satellite.

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10
Q

What is the redshift of galaxies (besides Andromeda)

A

Since wavelengths are longer on the red end of the visible light spectrum (shorter on the blue end), when distance galaxies were noticed as red in color, they are moving away from each other.

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11
Q

The farther away a galaxy is…

A

the faster it was moving away from us

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12
Q

How is nucleosynthesis evidence of the Big Bang?

A

Once nucleosynthesis was possible in the cooled singularity, isotopes (sane element with same protons but different neutrons) being colliding to form elements. Since the Big Bang only created helium and hydrogen, the light elements, the process stabilized to get a ration of 75% hydrogen and 25% helium in the universe - now,, in the milky way 75% is still hydrogen and 35% is helium. (oxygen, carbon, came overtime in smallest amounts)

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13
Q

spectrum

A

a band of colors produced by separating the components of light

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14
Q

Each element produces a unique and different

A

spectrum

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15
Q

we can determine the composition of stars by inspecting

A

their spectra

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16
Q

What is the first stage in a star’s life cycle?

A

Protostar- spinning cloud of dust and hydrogen contracted by gravity to become very hot, allowing nuclei to collide and fuse (meaning a star is formed)

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17
Q

What is second stage of star’s life?

A

The main sequence - when hydrogen fuses to create helium and energy and the pull of gravity and outward push of fusion create an equilibrium

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18
Q

What is third stage of all stars

A

When hydrogen is almost gone heliumbegins to fuse, getting much larger and brighter as a Red Giant (outer layers expand and cool, core gets hotter, causing an imbalnce)

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19
Q

What determines the lifespan of a star?

A

Mass (high mass live for longer time)

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20
Q

After being red giants low mass stars will

A

experience a nebula when gravity cannot hold the layers (they expand into space)

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21
Q

What is leftover from a nebula?

A

A white dwarf, which is the carbon core left behind. It as a low mass with no fusing elements and is smaller, dimmer, but still hot.

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22
Q

After a white dwarf planets become

A

black dwarfs - none exist now but will be when white dwarf cools and no longer gloss from heat. end of low-mass star’s life

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23
Q

Instead of experiencing a nebula, high mass stars will

A

curse carbon to create other elements working from out it (iron in the center) - the Many different fusion reactions create the super giant stage, where the star is very bright and large .

24
Q

After becoming a super giant, stars will

A

enter the supernova once the iron tries to fuse and the core of the star collapses, causing layers to explode into space

25
What is created by a supernova
Conditions needed for fusion to continue, Colbalt-Uranium is made this way and other heavier elements.
26
What remains after a supernova?
A very dense core called a neutron star, which, if dense enough, becomes a black hole
27
Main sequence on an HR diagram is
stable in shown in the middle of the graph - has energy (from fusion) giving off luminosity. High mass on left, low mass on right.
28
Red Giant on HR diagram is
Much cooler but brighter than main sequence due to expanding and new fusion reactions making it brighter and larger - right and above main sequence.
29
White dwarf on HR diagram is
Very dim ( no more fusion) but still howl, bottom left below the main sequence (not many in this stage)
30
Supergiants on HR diagrams are
above normal giants. Still cooler but much brighter since more fusion and elements fusing.
31
Stars moving away/towards us will be what color shifted?
away is red, towards is blue
32
Who is Edwin Hubble?
First to recognize that far way objects were other galaxies and light was displaced toward the red part of the spectrum.
33
Which galaxy is no redshifted?
Andromeda is blue shifted
34
Why do elements create a spectrum?
The different number of electrons move between energy shells and jump back down, releasing energy at a certain wavelength that corresponds with a visible line on spectrum.
35
Kepler's was
German astronomer who came up with three laws of planetary motion
36
Kepler's first law (Law of Orbits)
the path of each planet around the Sun is an ellipse (never perfect circle) with sun at one of two foci.
37
Paint where planet is closest/farthest from star
Perihelion is closest, Aphelion is father's.
38
Average of Aphelion and perihelion results in
semi-major axis being half of major axis (semi-minor axis half of minor axis)
39
Kepler's second law (Law of Equal Areas)
A line between the Sun and a planet sweeps out equal areas in equal times. A planet has a greater velocity when close to the Sun it inst orbit, slower when furthest from sun (force of gravity responsible for this speed difference)
40
Pull of gravity depends on
the mass to two things and the distance between them
41
Kepler's Third Law (Law of Periods/law of Harmony)
The ratio of the square of the period and the cube of the average distance from the Sun is the same for all planets
42
What does Kepler's Third Law look like written in two equal equations
T = R^ 3/2 T^2 = R^3
43
What was the age of Bombardment like?
Atmosphere was thick, cloudy, earth was pounded with space debris, hot and molten lava surface due to meteorites+comet+volcanoes+CO2
44
Evidence of the age of bombardment
the craters on planets such as Mercury, Mars, the Moon, ad Ganymede (moon of Jupiter) suggest they were hit by debris.
45
what is coeveolution after age of bombardment
Comets (ice) reached Earth more frequently during Age of Bombardment, bringing more water to the planet. As Earth cooled the water could take liquid form, creating oceans allowing for more life - earliest bacteria used CO2 for energy and the atmosphere began to change. Plane cooled allowing more oceans and more life to evolve, changing atmosphere more. less bombardment helped the cooling, and Earth's layers solidified
46
How did plate Tectonics change Earth's cratered, molten surface?
Any rock that would have been subducted with craters were melted and reformed as new rock (melting volcanic activity)
47
Oceans changed the surface by -
wiping away traces of craters on the surface of oceans and some continental land
48
The two properties of a star that are plotted on an HR diagram are
brightness (luminosity, on log scale) and temperature (on a reverse scale) - measured from sun, which is in the middle
49
Most stars are in ___ stage because ___
Main sequence because they are balanced and stable
50
White dwarfs have high temperature but low luminosity because
fusion reactions are no longer taking place
51
Besides ocean and tectonic plates, the two other processes that change Earth's surface include
the atmosphere and erosion
52
the age of Bombardment impacted
many planets and moons in the solar system
53
The Moon preserves more evidence of the Age of Bombardment that earth because
The moon experiences less erosion than Earth
54
The Moon has no atmosphere, so its
craters remain nearly unchanged for billions of years
55
The probable fate of our sun will be
to expand as a red Giant and end as a white dwarf