Chapter 10 Flashcards

(31 cards)

1
Q

What part of a star’s velocity is measured by the Doppler Effect?

A

Line-of-Sight

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2
Q

What important property of a star do we learn from its spectral class?

A

Temperature

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3
Q

How do we typically determine the radius of a star?

A

Calculation of radius after determining temperature and luminosity

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4
Q

What is NOT useful in constructing a Hertzsprung-Russell (H-R) diagram?

A

Measuring the Star’s size

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5
Q

Why are the most common stars among the most difficult to observe?

A

They have low luminosities

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6
Q

Why does the spectroscopic parallax method only work for main sequence stars?

A

Only main sequence stars have a well-defined relationship between spectral type and luminosity.

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7
Q

What is the full spectral classification of the sun?

A

G2V

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8
Q

What property of stars can be measured only by using the binary-star systems?

A

Mass

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9
Q

From a distance of 1 parsec, the angular size of Earth’s orbit would be

A

2 arc seconds

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10
Q

Compared with a star of absolute magnitude -2 at a distance of 100 pc, a star of absolute magnitude 5 at a distance of 10 pic will appear

A

Fainter

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11
Q

Cool stars can be very luminous if they are very

A

Large

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12
Q

The well known star Barnard’s star must be

A

Larger

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13
Q

The mass of a star may be determined

A

By studying its orbit around a binary composition

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14
Q

A star has a parallax of .05”. It’s distance is

A

20 parsecs

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15
Q

How much brighter will a 4th magnitude star appear than a 6th magnitude star

A

6.25 times

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16
Q

Which of these stars would be the hottest

17
Q

The stars with masses comparable to our sun’s, but sizes like the Earth are

18
Q

If we know the average separation period of revolution for a binary system, we can then measure

A

The total mass of the system

19
Q

According to the stellar spectra classification, Type A stars would have _____ hydrogen features than/as Type B stars.

20
Q

What is the order of the Stella spectra classification today

A

O, B, A, F, G, K, M

21
Q

The order of the Stella spectra classification used today is based on the stars

A

Surface temperature

22
Q

In order to determine a stars luminosity using its apparent magnitude, one must also determine its

23
Q

Most stars in our galaxy are

24
Q

What is the major factor in determining how a star forms, it’s age, how it will die, and its position on the main sequence?

25
On the H-R diagram the white draw region is
Bottom left corner
26
On the H-R diagram the main sequence is
On the line, in center
27
On the H-R diagram the red dwarf region
At the bottom right corner on main sequence line
28
On the H-R diagram the Red giant region is
Above the main sequence in center
29
The majority of bright naked eye stars are blue or white in color. On the H-R diagram, they would lie
In the high luminosity and High temperature region
30
On the H-R diagram, the main sequence runs from
High luminosity, high temperature region to low luminosity, low temperature
31
Which of the following is Not an intrinsic property of a star?
Luminosity DISTANCE Temperature Mass