Astronomical Distsnces & Brightness Flashcards

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1
Q

What is a Parallax angle?

A

A parallax angle is half the angle moved against distant background stars over 6 months.

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2
Q

What are parallax angles used for?

A

A parallax is used to measure the distance to nearby stars.

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3
Q

What are parallax angles often measured in?

A

Arcseconds

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4
Q

How many arcseconds are the in 1°?

A

3600 arcseconds

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5
Q

If the parallax angle is smaller what does this tell us about the distance of a star?

A

The smaller the parallax angle the more distant the star

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6
Q

What is a parsec?

A

Parsec is a unit of distance.

Is the distance to a star with with a parallex angle of 1 arcsecond.

1 parsec = about 3 light years.

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7
Q

What is the formula for the calculating the distance to a star (in parsecs) ?

A

Distance (pc) = 1 divided by angle (arcsec)

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8
Q

What does a star’s intrinsic brightness depend on?

A

Size
Temperature

The bigger and hotter a star is the more engery it gives out, so the brighter it is.

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9
Q

What would you see if you looked at two stars with the same intrinsic brightness but one was further away?

A

The further away star would be dimmer because the energy reaching you gets less.

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10
Q

If a star has a longer pulse period what can we tell about it’s luminosity?

A

The longer the pulse period, the higher the luminosity.

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11
Q

What factors of a Cepheid variable can an astronomer look at to work out the distance to a Cepheid variable.

A

Comparing the luminosity worked out by the pulse period & the observed brightness

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