Exam 3 Flashcards

1
Q

Photosphere

A

The surface of a star, where the plasma is thin enough that light can escape freely into space

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2
Q

Corona

A

A stars upper atmosphere, where thin plasma is heated to millions of Kelvin by the stars magnetic field

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3
Q

Fusion

A

The process where small nuclei are merged to form a heavier element, which can release energy

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4
Q

Envelope

A

The interior part of a star where fusion doesn’t occur and where the composition stays the same since the star was formed

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5
Q

Fission

A

When a heavy unstable nucleus breaks apart to form nuclei of lighter elements, which can release energy

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6
Q

Core

A

The part of the star where energy is generated

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7
Q

The sun shines because it is

A

Hot like a stove

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8
Q

Heat is generated in the suns core by

A

Nuclear fusion of hydrogen into helium

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9
Q

Nuclear ____ involves merging atoms while nuclear ____ involves splitting them

A
Fusion= merge
Fission= split
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10
Q

The sun has been shining for __ years and is..

A

4.5 billion years; halfway through its life

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11
Q

Sometimes the sun throws a ball of plasma and magnetic field out into the solar system. This is called a

A

Coronal mass ejection (CME)

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12
Q

What causes sunspots and solar cycles

A

The suns magnetic field reverses polarity

Fusion powers the core, changes on the surface are c if the magnetic field

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13
Q

There are more sunspots, flares, and CMEs during

A

The middle of a sunspot cycle

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14
Q

Th corona glows in X-rays while the photosphere only glows in visible light, so we know the corona is ___ than the photosphere

A

Hotter

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15
Q

The ___ is heated by fusion while the ___ is heated by magnetic fields

A
Core= fusion
Corona= magnetic fields
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16
Q

If you were to dive into the sun, you would hit a solid surface at the..

A

… actually, the plasma would just get thicker and thicker as you fell in

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17
Q

You can tell the temperature of a star by looking at its

A

Color

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18
Q

Lost the spectral types from hottest to coolest

A

OBAFGKM

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19
Q

How would you tell a K type red giant from a K type red dwarf?

A

The giant is more luminous

20
Q

True or false: as a star loses mass due to the stellar wind, it goes from being a main sequence O star to being a main sequence G star to finally being a main sequence M star

A

False; a star lands somewhere on the main sequence depending on its mass, and doesn’t move from there until it leaves the main sequence entirely

21
Q

On the main sequence compared to low mass stars, high mass stars are hotter

A

More luminous, and have shorter lifetimes

22
Q

High mass stars can fuse carbon but the sun cannot because

A

It’s core is not hot enough

23
Q

Stars on the main sequence range in luminosity and temperature, but they are all

A

Fusing hydrogen into helium in their cores

24
Q

Stars become larger once they leave the main sequence because

A

They are producing more energy, which makes the surface expand more

25
Q

List stellar corpses based on the mass of the star that formed from the lowest to the highest

A

White dwarf, neutron star, black hole

26
Q

When stars become red giants or red supergiants, they turn red because

A

The surface is farther from the center of the star

27
Q

Which kind of star will die by going supernova?

A

A star with more mass than our sun

28
Q

You see a bright star in the night sky. You have enough information to determine:

A

Nothing

29
Q

When a large gas cloud has clumps that form stars, you would tend to find

A

More low mass stars like K and M stars

30
Q

2 stars are the same mass. Star A is fusing hydrogen into helium, star B is fusing hydrogen into helium and helium into carbon and oxygen. Which star is older?

A

B; it’s fusing heavier elements

31
Q

List the stages that a low mass star goes through in chronological order

A

Main sequence, red giant, planetary nebula, white dwarf

32
Q

As a red isn’t the sun will fuse hydrogen in a shell around the core. What phase comes after this?

A

The sun fuses helium in the core and hydrogen in a shell around the core

33
Q

How can you measure the age of a star cluster?

A

Determine what mass the star is just about to leave the main sequence

34
Q

Your friend says, “this thing keeps publishing bright faint bright faint, and is giving me a headache.” What object is this?

A

Neutron star

35
Q

A supernova is when

A

A massive star dies, a white dwarf gains too much mass

36
Q

Parallax allows us to measure a stars

A

Distance

37
Q

You measure the pulsation period of a variable star in a star cluster. You can now estimate the?

A

Clusters distance

38
Q

Over its lifetime and death, a star creates ___ heavier elements than it uses, so it ___ the amount of heavy elements present in a galaxy’s gas

A

More, increases

39
Q

You observe a red supergiant and a red giant. Which is more polluted with heavier elements?

A

Red supergiant

40
Q

A habitable planet is one that

A

Is the right temperature for water to be liquid

41
Q

Why are exoplanets difficult to detect?

A

They’re far from earth, net to bright stars, and dim

42
Q

When we observe an exoplanet using the Doppler shift, the planets signal is

A

.. actually, we never see the planet itself

43
Q

A hot Jupiter exoplanet is a Jovian planet that

A

Is in very small orbit

44
Q

You see a star moving toward and away from you in a periodic manner. Which detection method is this?

A

Radial velocity

45
Q

Most of the planets in the exoplanet database are Jovian planets because

A

Our detection methods are biased toward finding Jovian planets

46
Q

The Drake equation allows us to estimate there are __ alien civilizations whose radio signals we could detect in the Milky Way

A

.. actually, we have no idea how many

47
Q

If you want to detect a planet like earth that is orbiting a star, you should observe it for a minimum of..

A

3 years