3.3 Physical Poperties 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
Dimmer

To work out brightness ratio do

2.5^(the apparent magnitude)

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3
Q

What is Pogson’s ratio?

A

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 apparent magnitude of the brightest star in the sky?

A

-1.5 Sirius (α Cma)

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6
Q

What’s 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 stars

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’s a cepheid variable

A

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

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10
Q

What’s 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’s the primary star

A

The brighter one

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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

It goes up and down like a triangle - check photo of a graph

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14
Q

What’s the equation of absolute magnitude

A

M = m + 5 - 5 log d

1kpc = 1000pc

1Mpc = 1 000 000pc

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15
Q

Draw a light curve of an eclipsing binary

A

Big dip when little star in front

Small dip when small star behind big one

Check photo

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16
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.

17
Q

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

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

18
Q

What is a parsec

A

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

19
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.