Physical Properties of Stars Flashcards

1
Q

Explain the difference between Optical Double stars and True Binary Stars.

A

-True Binary stars are linked together Gravitationally and orbit a common centre of mass. e.g. Castor in Gemini. e.g. Algol in Perseus. -Optical Double stars merely appear nearby but may be light years apart.

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2
Q

How many times brighter is a star with a magnitude of 5 compared with a star with a magnitude of 1?

A

100 times

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3
Q

What is Pogson’s ratio?

A

The difference in magnitudes is the 5th route of 100 which equals 2.51

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4
Q

Give 4 factors that affect the apparent magnitude of a star.

A

-Energy radiated by star ○ Size ○ Temperature -Interstellar gas and dust. -Amount of light absorbed by Earth’s atmosphere. -Distance from Earth

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5
Q

What is the magnitude of the brightest star in the sky?

A

1.5 Sirius (α Cma)

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6
Q

What is the Absolute Magnitude?

A

A measure of Apparent magnitude if observed from a distance of 10pc

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7
Q

Name two types of variable star.

A

-Cepheid Variables -True Binaries

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8
Q

What is a True Binary?

A

Two Stars orbiting around their common centre of mass.

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9
Q

What is a Cepheid Variable?

A

A giant yellow star that regularly expands and contracts in size.

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10
Q

What is an eclipsing binary?

A

If two binary stars orbit each other in a plane along our line of sight, two stars will eclipse each other. e.g. Algol (β Per)

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11
Q

What is the Primary Star?

A

The brighter star in a binary system

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12
Q

In what way is the variability of light intensity of Cepheid Variables different to that of eclipsing binaries?

A

-One is due to the star pulsating (Cepheid) -The other is due to stars eclipsing each other (eclipsing binaries)

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13
Q

Draw the light curve of a Cepheid Variable.

A
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14
Q

Draw the light curve of a Eclipsing Binary.

A
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15
Q

What is Parallax?

A

The apparent motion of near and more distant objects in respect to each other, caused by the motion of an observer.

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16
Q

Describe the method of heliocentric parallax to determine the distance to nearby stars.

A

We measure the angular shift in position of a star from E1 to E2 Half of the angular shift is called the parallax angle (p) Then we use the formula d=1/p Distance (in parsecs) = 1/ Parallax angle

17
Q

What is the definition of a parsec?

A

The distance at which a star would have a parallax angle of one arc-second.

18
Q

Describe how Cepheid Variables can be used to determine stellar distances.

A

-Using the period – luminosity law we can work out the absolute magnitude of the star -Use the distance modulus formula to calculate distance.