Chapter 2 Flashcards

1
Q

Celestial Sphere

A

A useful, albeit imaginary star map, which plots the stars, planets, and other celestial objects on a sphere reaching out into space with Earth at its center.

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2
Q

What is the difference between the Celestial North Pole and the North Pole.

A

The celestial north pole reaches out from the earth’s surface and extends into space. The North pole is a point on the earth’s surface.

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3
Q

What is declination and how is it measured?

A

Declination is the distance north or south of the celestial equator as measured in degrees (0 degrees to 90 degrees)

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4
Q

What is right ascension and how is it measured

A

Equivalent to longitude. Measured in hours, minutes, seconds of the rotation of the earth.

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5
Q

What is the ecliptic?

A

The sun’s path through the sky throughout the year.

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6
Q

Zenith

A

The point in the sky directly above you. (Imagine meditating on the ground and a line sprouts from your head and extends into the sky)

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7
Q

Explain horizon and meridian

A

As mapped out on the celestial plane the horizon extends perpendicular to the ground in all directions and the meridian slices from north to south in all directions on the celestial sphere..

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8
Q

Nadir

A

The point directly below you.

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9
Q

How do the stars appear in the night directly at the north pole?

A

Stars rotate around polaris like a carousel.

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10
Q

Where is the point on earth where the Zenith remains the same throughout the day?

A

The North Pole, and South Pole (but the stars rotation clockwise)

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11
Q

How does the NCP appear as you move north and south?

A

The NCP is high in the sky in higher altitudes and lower in the sky at lower altitudes until you reach the equator and the NCP is on the horizon.

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12
Q

How long do stars appear in the sky? How does this depend upon your location

A

Depends on your location. Except for at the poles, objects on the celestial equator appear in the sky 12 hours each day. Objects north of the equator, appear for more than 12 hours each day and objects south appear for less than 12 hours each day.

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13
Q

How can you use the north star to calculate the size of the earth?

A

By measuring degree changes in sky from locations north or south from each other. For instance if you travel 290 km north and the north star changes from 33.5 to 36 degrees, this would result in 42,000 when multiplied.

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14
Q

Why do we not feel the earth rotating?

A

It is due to our frame of reference. because we’re traveling at a consistent speed and the direction of the earth changes very slowly, we do not feel the earth rotating.

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15
Q

What is relative motion?

A

The difference in motion between two different frames of motion.

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16
Q

Coriolis Effect

A

The curving motion which results from the difference in rotation speed at different altitudes.

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17
Q

What are the two major factors which create the change in seasons?

A

The tilt of the earth. The angle that the sun’s rays hit the Earth’s surface.

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18
Q

Summer Solstice

A

Sun rises farthest north east and sets farthest north west as it crosses the meridian. June 20th

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19
Q

Winter Solstice

A

December 21st. Furthers south of the equator.

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20
Q

On what two days does the sun cross the celestial equator?

A

The Autumn Equinox on September 22nd and the vernal equinox on March 20th.

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21
Q

When does the equator get the most direct sunlight.

A

The first day of spring and the first day of autumn when the sun passes directly over the equator.

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22
Q

When is the sun above the horizon for 24 hours in the arctic/antarctic circle?

A

During the Summer and Winter Solstice and the days surrounding the solstice

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23
Q

Tripics

A

The band of land between 23.5 degrees north(Tropic of cancer) and 23.5 degrees south (tropic of Capricorn).

24
Q

Procession of equinoxes

A

As the earth wobbles about its axis, the equinoxes where the equator crosses the ecliptic changes as well. as a result the sun is in difference positions in the sky during the first day of summer in different constellation.

25
Q

What is one cycle in the procession of equinoxes?

A

26,000 years.

26
Q

New moon

A

When the moon is between the earth and the sun. Rises and sets with the sun.

27
Q

Waxing Crescent

A

Between new moon and First Quarter.

28
Q

First Quarter Moon

A

Halfway to full moon. right side is fully illuminated. Rises at noon and sets at midnight

29
Q

Waxing Gibbous

A

More than half illuminated on the right side.

30
Q

Full Moon

A

Earth is between the sun and the moon. Rises at sunset, crosses meridian at midnight and sets in the morning as the sun rises.

31
Q

Wanning Gibbous Moon

A

Right side begins to grow dark.

32
Q

Third Quarter Moon

A

Near side is illuminated by the sun (left side). Rises at midnight, crosses meridian at sunrise, and sets at noon.

33
Q

Waning Crescent moon.

A

Left sliver left before new moon.

34
Q

How long is the sidereal period for the moon? Why?

A

How long the moon takes to return to the same location in its orbit in comparison to a distant star. Prod is 27.32 because of the earth’s rotation, this period is over 2 days shorter.

35
Q

What is the synodic period for the moon?

A

29.53 days. Over 2 days more than the sidereal period.

36
Q

Why do we only see one side of the moon?

A

The moon rotates in sync with the earth so that only one side is visible.

37
Q

Tropical year

A

365.242 days.

38
Q

Solar Day

A

24 hours

39
Q

Sidereal Day

A

23 hours 56 minutes.

40
Q

Eclipse

A

Partial or total obscuration of a celestial body by another celestial body.

41
Q

Solar Eclipse

A

When the moon passes between the earth and the sun.

42
Q

What is the difference between a total eclipse and an annular eclipse

A

Depends on the moon’s distance from the earth. If the moon is not close enough to block the sun it results in an annular eclipse.

43
Q

Umbra

A

Darkest inner part of a shadow

44
Q

Penumbra

A

The surrounding less dark portions of a shadow

45
Q

Total eclipse

A

When a location on earth passes through the moons umbra.

46
Q

Partial eclipse

A

When a location on earth passes through the penumbra of the moon. Blocks light from a portion of the sun’s disk.

47
Q

Annular Solar Eclipse

A

Sun appears as a bright ring around the moon. The moon is a bit further away than average.

48
Q

Why is it so hard to see a total solar ecclipese?

A

1) Eclipse is short. Only lasts 7 1/2 minutes. Umbra is only 270 km wide on the earth’s surface vs penumbra which is 7,000 km.

49
Q

Lunar Eclipse

A

Occurs when the moon moves through the Earth’s shadow.

50
Q

What is a total lunar eclipse and how long does it last?

A

Moon is entirely within earth’s shadow. Lasts 1 40 minutes. Moon often appears red.

51
Q

Why is a total lunar eclipse much longer than a total solar eclipse.

A

Because the earth is much larger than the moon, the umbra of the earth is 2 1/2 times the moon’s diameter.

52
Q

Penumbral lunar eclipse

A

When the moon passes through the penumbra of the Earth’s shadow. Results in a partial lunar eclipse.

53
Q

Line of nodes

A

When the orbital planes of the sun andmoon intersect.

54
Q

How long is an eclipse season?

A

38 days. Occurs every 5 months 20 days. Why? Because the moon’s orbit slowly wobbles.

55
Q

How long does it take for the moon to complete one wobble?

A

18.6 years. Amounts to a 20 day regression each year hence why the eclipse season is 5 months 20 days.