Unit 8: Characterizing Stars Flashcards

1
Q

Why do stars appear in different colors?

A

because of their temperature

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2
Q

What is an Astronomical Unit

A

The average distance between the earth and sun

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3
Q

What is a Light Year

A

The distance that light travels in a vacuum in one year

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4
Q

What is a Parsec

A

1 pc= 3.26

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5
Q

What is the most convenient measurement for measuring interstellar and inter galaxies distance

A
  • Light year and Parsec
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6
Q

What are the properties of interest of Stars

A
Distance
Visible brightness
luminosity 
surface temperature
size
age
mass
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7
Q

What is the Parallax Method used for?

A

This is a measurement of the distances to nearby stars

  • This method only works for closer and nearby stars
  • not more than 1000 pc away from the earth
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8
Q

The Parallax Method is the only method allowing what?

A

Only method allowing to express distances to stars in terms of diameter of Earth’s orbit.

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9
Q

When was the first parallax measurement made? By who?

A

1838 by Friderich Wilhem Bessel

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10
Q

What is Apparent Magnitude?

A

The brightness of stars without regard to their distances
(m)
the brightness of stars as seen from Earth

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11
Q

Objects which are brighter than first-magnitude stars have apparent magnitudes ______ than 1, even _______ ones.

A
  1. Less

2. Negative

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12
Q

What is the apparent magnitude of Sirius

A

This is the brightest star in the night sky, has a negative apparent magnitude: m= -1.44

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13
Q

What is the apparent magnitude of Venus

A

m= -4.4

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14
Q

What are the Moon and Sun’s apparent magnitudes

A

Moon (-12.6)

Sun (-26.7)

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15
Q

What is the contemporary measurement of an apparent magnitude based on?

A

Electronic devices directly measuring an intensity of light

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16
Q

What us the naked eye limit of apparent magnitude

A

+6.0

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17
Q

What is a star’s absolute magnitude

A

M

The stars apparent magnitude the star would have if it were 10 pc from the Earth

18
Q

What is the range of absolute magnitude

A

Absolute magnitude range from roughly M= -10 for the brightest stars to M= +17 for the dimmest

19
Q

What is Luminosity

A

the total amount of energy radiating from the star’s surface each second

20
Q

The absolute magnitude of a star and its luminosity are _____ _________.

A

directly proportional

21
Q

What is the Harvard Classification Scheme and who created it?

A

The first serious attempt to organize and classify stars based on their temperatures
- Edward Charles Pickering and Annie Jump Cannon

22
Q

What are the Stellar Classes

A

O, B, A, F, G, K, M,
0= coldest (blue violet)
M= hottest (red-orange)

23
Q

What does the Hertzsprung-Russell Diagram show

A

that stars luminosity and surface temperature are correlated

24
Q

What percent of stars belong to the main sequence band

A

over 90%

25
Q

What does the lower right side of the Hertzsprung-Russell Diagram show

A
  • dim and red
26
Q

What does the top left side of the Hertzsprung-Russell Diagram show

A
  • cold and bright
27
Q

Where are White Dwarfs on the Hertzsprung-Russell Diagram

A

bottom left

High mass and low luminosity

28
Q

Where is the sun on the Hertzsprung-Russell Diagram

A

in the main sequence band

29
Q

Where are the super giants on the Hertzsprung-Russell Diagram

A

top right

low temperature, high luminosity

30
Q

What is the Spectroscopic Parallax

A

the indirect method for the measurement of distances to stars.

31
Q

What kind of stars can the Spectroscopic parallax be applied to

A

any main sequence star

~10,000parsec

32
Q

What are Cepheid Variables and what can it be used for

A

Stars which brighten and dim periodically.

- allows them to be used as cosmic yardsticks out to distances of a few thens of millions of LY

33
Q

What are the steps to determine main sequence stars distance

A
  1. Determine the spectro class (line up from the bottom of the chart in line with the start to the main sequence line)
  2. Absolute Magnitude M
  3. Apparent Magnitude m
34
Q

How/when were Cepheid Stars discovered

A

absolute magnitude combined with apparent magnitude = distance

35
Q

What are Optical Doubles/Apparent Binaries

A

Physically far from each other. They are unrelated stars that appear close together thought chance alignment with Earth

36
Q

What are Binary Stars?

A

Stars that are physically close and form the system

- two stars that orbit each other

37
Q

How many stars in the sky are Binary stars

A

1/3 to half of the stars in the sky

38
Q

What are visual binary stars vs Spectroscopic Binary

A

Visual are seen separately by telescopes and spectroscopic are hard to see separately even with telescope

39
Q

What is the Big Dipper Constellation called

A

Ursa Major

- is a binary star

40
Q

What does Keplers Law tell us

A

the combined mass of binary stars

41
Q

More luminous stars are _____?

A

Bigger