Chapter 1 Flashcards

1
Q

The average distance from the Earth to the Sun, 149,600,000 km can be written in shorthand notation as-

A

1.496 x 10 ^8 km

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2
Q

There are 1000 mm in 1 m. This

means that a distance of 10mm is-

A

1 x 10 ^-2 m

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3
Q

10^2 x 10^5 =

A

10,000,000

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4
Q

100 (10 ^0) =

A

1

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5
Q

10^-3 x 10^3 =

A

1

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6
Q

(3 x 10^4)^4=

A

8.1 x 10^17

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7
Q

(.5)^3 =

A

0.125

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8
Q

(8.0 x 10^5) / (2 x 10^3) =

A

400

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9
Q

The ecliptic can be defined as the-

A

Path traced out by the Sun in our sky over one year against the background stars.

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10
Q

In which direction dies the Sun appear to move along the ecliptic over the course of a year, relative to the background stars?

A

East

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11
Q

If we could see background stars in the daytime, the Sun would-

A

Appear to move eastward against them at a rate of 1• per day

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12
Q

The earth would NOT have seasons if-

A

It’s axis of rotation were perpendicular to its orbital plane

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13
Q

Why do we see different phases of the moon?

A

The illuminated half if the moon becomes more or less visible from earth as the moon orbits the earth

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14
Q

The phase if the moon when the sun NAND moon have the same right ascension-

A

New moon

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15
Q

Approximately when dies a full moon rise?

A

Sunset

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16
Q

How often does the moon rotate to keep one face pointed toward the earth at all times?

A

Once per month

17
Q

The total in Ed if eclipses is limited to seven or fewer per year because one condition that must be met for a lunar or solar eclipse is that the-

A

Moon be close to or crossing the ecliptic plane.

18
Q

What is the approximate inclination if the moon’s orbit to the ecliptic plane?

A

5*

19
Q

A solar eclipse occurs in the earth when the

A

Moon casts a shadow in the earth

20
Q

A lunar eclipse does not occur at every full moon because the

A

Plane if the moon’s orbit I’d at an angle to the place of the earth’s orbit.

21
Q

A lunar eclipse is caused by the

A

Moon passing unto the shadow of the earth

22
Q

The difference between an umbral eclipse and a penumbras eclipse is

A

The distance of the moon above or below the ecliptic

23
Q

A total solar eclipse is visible (assuming clear skies everywhere) to

A

Only people in aping narrow path, much smaller than a hemisphere

24
Q

What is the major factor they governs whether a douse eclipse is a total rather than annular when viewed from the center of the eclipse path on earth?

A

Earth-moon distance

25
Q

A person standing in the moon’s penumbra will see a

A

Partial solar eclipse