Unit 3 Physical Properties of Stars Flashcards

1
Q

What is an optical double star?

A

Two stars that are totally unrelated to one another yet appear to be closely aligned.

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2
Q

What is a binary star system?

A

Where two stars are the same distance from us and orbit the same common centre of mass.

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3
Q

True or false, the stars in a cluster are linked gravitationally.

A

True.

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4
Q

What is magnitude?

A

Brightness of a star.

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5
Q

What is apparent magnitude?

A

It is the brightness of the star as it appears to the observer.

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6
Q

What is absolute magnitude?

A

The brightness of a star when observed from a standard distance of 10 parsecs.

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7
Q

How is magnitude measured?

A

On a scale where each number corresponds to the magnitude being 2.5 times brighter/dimmer than the last.

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8
Q

What factors do apparent magnitude of stars depend upon?

A

Total energy radiated (depends upon size and temperature.
Distance of star.
Amount of interstellar gas and dust.
Amount of light absorbed by the Earth’s atmosphere.

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9
Q

What is the distance modulus formula?

A
It relates apparent and absolute magnitude.
M=m + 5 - 5 log d
When:
M = Absolute Magnitude
m = Apparent Magnitude
d = Distance in parsecs
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10
Q

What is a variable star?

A

A star that’s magnitude can vary.

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11
Q

What are the two types of variable star?

A

Binary star.

Cepheid variables.

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12
Q

How does a binary star vary in magnitude?

A

As the two stars orbit each other if the stars eclipse each other the light intensity will drop.

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13
Q

How does a Cepheid variable star vary in magnitude?

A

The star pulsates as it expands and contracts having a dramatic effect on it’s luminosity.

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14
Q

Why can we not use the radar technique to measure distances to stars?

A

They are so far away it takes to long for the signal to return.
A reflected signal would be so weak we would not be able to distinguish it from the background.
Stars are spheres of gas and do not have hard reflecting surfaces.

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15
Q

What is parallax?

A

The apparent motion of a star against distant objects.

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16
Q

What is heliocentric parallax?

A

The technique used to determine distances to stars by measuring the movement (parallax) of a star over 6 months (when the Earth is farthest from where it was 6 months earlier in its orbit).

17
Q

What is parallax angle?

A

Half the shift in position over the 6 month measuring period of the position of a star.

18
Q

What is the formula that relates distance and parallax angle?

A

d = 1/p
When:
d = distance in parsec
p = seconds of arc (arcsec)

19
Q

What is an arcsec?

A

One degree is 60 minutes of an arc and one minute is 60 seconds of an arc, so one arcsec is one three thousand six hundredth of a degree.

20
Q

What is a parsec?

A

The distance at which a star would have the parallax angle of one arcsec.

21
Q

How can period luminosity law be used to calculate distance?

A

Period luminosity law is the law that links pulsation period to mean absolute magnitude. With this absolute magnitude and an apparent magnitude we can calculate the star’s distance.