Lecture 5 Flashcards

1
Q

describe a solar eclipse

A

when the moon is b/w the earth and sun

moon blocks light from the sun which casts a shadow on earth

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2
Q

what are the 2 parts of the shadow in a solar eclipse?

A

penumbra: lighter part
umbra: darker part

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3
Q

why don’t we have eclipses more often?

A

b/c moon’s orbital plane is t ilted by 5 deg w/ respect to the ecliptic

can have eclipses only twice per year

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4
Q

why are lunar eclipses more common than solar?

A

the moon’s shadow on earth is much smaller than the earths shadow on the moon

total solar eclipses can only seen on some parts of the earth

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5
Q

___ side of the moon always faces the earth

a) same
b) difference

A

same

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6
Q

what causes tides on earth?

A

b/c of gravitational force due to moon on on side of earth greater than on other

when the moon is further away, tides are weaker

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7
Q

why is there an offset of tidal bulges? what does this cause?

A

tidal bulges don’t point directly at the moon b/c of the earth’s rotation

thus it is 10 degrees off

causes the moon to be pulled ahead in its orbit –> gives E –> spirals outward slowly –> earth/moon distance increases by 3.8cm each year

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8
Q

how can you tell that the moon/earth distance is changing?

A

can bounce radio waves off moon and see how long it takes for it to return

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9
Q

what is spring tide?

A

the largest tide b/c friction b/w earth and oceans makes the earth rotate more slowly

sun in line with earth and moon

at a new and full moon

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10
Q

what is the neap tide?

A

smallest tide

sun at right angle to earth/moon line

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11
Q

describe the moon tide

what does this cause?

A

moon also feels a similar tidal force

but them moon is solid, so the effect is not as pronounced as on earth

can be seen as tide-correlated moonquakes

tide cased a raised bulge in the moon which forces the moon to rotate synchronously. The bulge is alwasy pointing toward to earth

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12
Q

what is stellar parallax?

why is it imp?

A

technique to measure astronomical distance

aka triangulation

very imp because the viewing angle changes the background. The earth’s position in january is different than in june, thus the location of the star will look different

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13
Q

what is 1 arcminute?

what is 1 arcseccond?

A

1 degree (out of 360) is 60 ‘ (arcmin)

1’ = 60’’ (arcseconds)

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