Topic 1: Observational Astronomy Flashcards

1
Q

What is the astronomical unit?

A

Is is the average distance between the earth and the sun. It has a value of 1.5x10^11m

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2
Q

What is parallax?

A

Where objects close to the earth move faster compared to objects further away.

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3
Q

What does it mean if a star has a large parallx angle?

What does it mean if a star has a small parallax angle?

A

The star is close to us.

The star is far away from us.

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4
Q

What is a parsec?

A

An object one parsec away will have a parallax angle of one arcsecond (1”)

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5
Q

With regards to parallax, what is 1 degree equal to?
*Arc

A

1 degree is equal to 60” (arcminutes)
Thus it is equal to 3600’ (arcseconds)

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6
Q

What would 1” be equal to?

A

1”= (1/3600) degrees = 0.00028 degress.

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7
Q

Where should a UV, X-ray or gamma ray telescope be placed?

A

Above the earths atmosphere.

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8
Q

Where should visible light and radiowave telescopes be placed?

A

They are usually ground based.

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9
Q

What is a blackbody?

A

When cool, it will absorb all radiation.

When hot, it was emit radiation.

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10
Q

What does Wiens Law let us calculate?
Lambda=b/T

A

This lets us calculate the max wavelength of light emitted from an object given it’s temperature.
Colour is related to temperature.

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11
Q

Why are planets NOT blackbodies?

A

They generate little radiation, however they do reflect sunlight.

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12
Q

What is albedo?

A

This is the (light reflected from a sphere)/(light incident on it)

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13
Q

What does it mean if a galaxy is redshifted?

A

It is moving away from the observer.

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14
Q

What does it mean if a galaxy is blueshifted?

A

It is moving towards the observer.

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15
Q

What does spectroscopy tell us about a star/planet/galaxy?

A

What elements or molecules it is made up of.

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16
Q

How can the frequency and wavelength doppler equations be equated?

A

Flip the signs in the square root.

17
Q

What increases resolving power in a telescope?

A

Increasing the aperture size.

18
Q

What does a larger aperture size cause?

A

Higher resolving power
Finer angular resolution

19
Q

What are the two main types of telescopes?

A

Refractive and reflective

20
Q

What is an issue commonly found with lenses?

A

Chromatic aberration. This is where light at different wavelengths is refracted by different amounts.

21
Q

What makes mirrors more advantageous over lenses?

A

They are not affected by chromatic aberration.

22
Q

What is angular resolution?

A

This is the smallest angular seperation two objects can have before they blur together.

23
Q

What factors affect where a telescope is built?

A

Atmospheric effects
Light pollution
Cloud cover.

This makes the most optimal place for a telescope a mountain-top.

24
Q

What is adaptive optics?

A

This is where a reference beam of light is used to calculate how much a mirror must be deformed to account for atmospheric effects.

25
Q

What is the relationship between angular resolution and resolving power?

A

The smaller the angular resolution, the higher the resolving power.

26
Q

What is the Zenith?

A

This is the point in the sky directly above the observer

27
Q

What is a circumpolar star?

A

A star that doesn’t rise or set. The altitude min “amin” will be =<0

28
Q

What is the difference between solar time and sidereal time?

A

Solar time is the earth relative to the sun

Sidereal time is the earth relative to the stars

29
Q

How many more days are in a sidereal year?

A

1 more than a solar year.