astro ch 16 Flashcards

1
Q

Star A is identical to Star B, but Star A is twice as far from us as Star B. Therefore

A

both stars have the same luminosity, but the apparent brightness of Star B is four times that of Star A

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2
Q

All stars are born with the same basic composition, yet stars can differ greatly in appearance. Which two factors are most important in determining the current appearance of a star?

A

mass and stage of life

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3
Q

Why do some of the bright stars (such as the one indicated by the arrow) in this photo have cross-shaped spikes over them?

A

The spikes are an artifact of photography through a telescope.

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4
Q

Which of the following terms is given to a pair of stars that we can determine are orbiting each other only by measuring their periodic Doppler shifts?

A

spectroscopic binary

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5
Q

If the star Alpha Centauri were moved to a distance 10 times farther than it is now, its parallax angle would

A

get smaller

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6
Q

How did astronomers discover the relationship between spectral type and mass for main sequence stars?

A

By measuring the masses and spectral types of main-sequence stars in binary systems.

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7
Q

The total amount of power (in watts, for example) that a star radiates into space is called its

A

luminosity

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8
Q

According to the inverse square law of light, how will the apparent brightness of an object change if its distance to us triples?

A

Its apparent brightness will decrease by a factor of 9.

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9
Q

Suppose our Sun were suddenly replaced by a supergiant star. Which of the following would be true?

A

Earth would be inside the supergiant.

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10
Q

Sirius is a star with spectral type A star and Rigel is a star with spectral type B star. What can we conclude?

A

Rigel has a higher surface temperature than Sirius.

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11
Q

What is Rigel’s surface temperature?

A

10,000 K

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12
Q

Rigel’s luminosity is about _____ times the Sun’s luminosity

A

100,000

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13
Q

Rigel’s radius is about _____ times the Sun’s radius.

A

80

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14
Q

Based on its location on the HR diagram, what can we say about Rigel’s mass and lifetime?

A

Nothing, because it is not on the main sequence.

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15
Q

Which is brighter in our sky, a star with apparent magnitude 2 or a star with apparent magnitude 7?

A

A star with apparent magnitude 2.

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16
Q

Which units are appropriate for measurement of apparent brightness?

A

watts per square meter

17
Q

Compared to a main-sequence star with a short lifetime, a main-sequence star with a long lifetime is

A

less luminous, cooler, smaller, and less massive

18
Q

Compared to a high-luminosity main-sequence star, stars in the upper right of the H-R diagram are

A

cooler and larger in radius

19
Q

Compared to a low-luminosity main-sequence star, stars in the lower left of the H-R diagram are

A

hotter and smaller in radius

20
Q

If star A is closer to us than star B, then Star A’s parallax angle is

A

larger than that of Star B

21
Q

What can we infer, at least roughly, from a star’s luminosity class?

A

its size (radius)

22
Q

A star with a parallax angle of 1/20 arcsecond is

A

20 parsecs (~ 65.2 light-years) away

23
Q

You observe a star and you want to plot it on an H-R diagram. You will need to measure all of the following, except the star’s

A

mass

24
Q

Which of these stars has the coolest surface temperature?

A

a K star

25
Q

What is the common trait of all main-sequence stars?

A

They generate energy through hydrogen fusion in their core

26
Q

Our Sun is a star of spectral type

A

G

27
Q

Star A has an apparent magnitude = 3 and star B has an apparent magnitude = 5. Which star is brighter in our sky?

A

Star A

28
Q

Which of the following must be true if we are to infer (calculate) a star’s luminosity directly from the inverse square law for light?

A

No interstellar gas or dust absorbs or scatters light between us and the star.
We have measured the star’s apparent brightness.
We have measured the star’s distance.

29
Q

What do we mean by a star’s spectral type, and how is spectral type related to surface temperature and color.

A

Spectral types are a way of classifying stars according to their color or what spectral lines we see in their light. The spectral types run OBAFGKM, where O stars are the hottest and M are the coolest. Hotter stars look bluer to us, and cooler stars look redder.

30
Q

Before we can use parallax to measure the distance to a nearby star, we first need to know

A

the Earth-Sun distance

31
Q

Which of the following is a valid way of demonstrating parallax for yourself?

A

Hold up your hand in front of your face, and alternately close your left and right eyes.

32
Q

What is the cause of stellar parallax?

A

Earth’s orbit around the Sun.

33
Q

The more distant a star, the

A

smaller its parallax angle

34
Q

Approximately what is the parallax angle of a star that is 20 light-years away?

A

0.16 arcsecond

35
Q

Suppose that a star had a parallax angle of exactly 1 arcsecond. Approximately how far away would it be, in light-years?

A

3.3 light-years

36
Q

Describe what would happen to the surface temperature of a star if its radius increased by 4 times, but there was no change in luminosity.

A

Luminosity increases both with increasing radius and increasing temperature. Therefore, a lower temperature would be required to maintain the star’s constant luminosity.