prequiz Flashcards

1
Q

The model of the sky is called the Celestial Sphere. The point directly overhead on this sphere is called ———

A

zenith

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2
Q

Our Earth’s axis is tilted by an angle of ——— degrees.

A

23.5

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3
Q

If you stood at the Earth’s North Pole, ——– would be seen overhead.

A

north celestial pole

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4
Q

The path that Sun appears to take around the Celestial Sphere every year is called ——–

A

ecliptic

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5
Q

For observers in Continental United States, the star group: Big Dipper ———

A

never sets

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5
Q

The entire sky is divided into ——- constellations.

A

88

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6
Q

At the ——–, stars rise straight up and set straight down.

A

equator

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7
Q

Big Dipper is an example of a Pattern within the Constellation: ——–

A

ursa major

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8
Q

vertical

A

latitude

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9
Q

horizontal

A

longitude

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10
Q

The time it takes for the Moon to complete one full rotation on its axis = ——–

A

27.3 days

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11
Q

The dark areas on the Moon’s surface are called ———

A

maria

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12
Q

Our Moon is thought to have formed

A

when a mars sized bullet impacted earth

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13
Q

On December 21st, the Sun is ———

A

southern celestial equator

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14
Q

When exactly one half of the Moon is illuminated by the Sun, we say that the Moon is in the ——– phase.

A

quarter

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15
Q

The time taken for the Moon to complete one full cycle of lunar phases is ——–

A

29.5 days

16
Q

We can see both the near and far sides of the Moon from Earth!

A

false. rotation period = orbital period
synchronous rotation

17
Q

in 14,000 years what star will become the pole in the northern hemisphere?

A

vega

18
Q

A lunar eclipse is seen when

A

earth is in between the sun and moon

19
Q

how many planets can be seen with the unaided eye?

A

5

20
Q

Eratosthenes measured ——— by observing Sun rays at Alexandria and Syene in Egypt.

A

diameter of earth

21
Q

Aristotle and most of the ancient Greek scholars beleived in ———

A

an earth centric model

22
Q

——– is the apparent backward motion of planets against the background stars.

A

retrogade motion

23
Q

———- had to be introduced by Ptolemy in his model to explain the observed backward motion of planets.

A

epicycle

24
Q

———- was responsible in developing the new Sun-Centric Model.

A

copernicus

25
Q

Galileo’s observations regarding ———- showed that the Sun-Centric Model must be correct!

A

phases of venus

26
Q

It was the great European observer: ———, who had built sophisticated instruments to measure angles of celestial objects in the sky.

A

tycho brahe

27
Q

For every action there is an equal and opposite reaction. This is ———

A

newton’s third law of motion

28
Q

Maxwell had realized that light is a form of disturbance that propagates in space. It was called ———–

A

electromagnetic radiation

29
Q

The weight of an object depends on the local force of gravity. Given that Moon’s gravity is just 1/6th that of Earth’s, one’s weight would be ——- on the Moon.

A

lower

30
Q

According to Newton’s Second Law, in the presence of an external force, an object will ——–

A

accelerate

31
Q

Galileo’s observations regarding ———- provided the strongest evidence that the Sun-Centric Model must be correct!

A

phases of venus

32
Q

According to Newton’s Law of Gravity, the force of gravitational attraction between two bodies increases as their ———-

A

masses increase

33
Q

The speed required to escape from the gravitational influence of a body is termed the Escape Speed. What is the speed required to escape from Earth?

A

11 kms/second

34
Q

Light is a disturbance that can be characterized by the distance between successive crests of the disturbance. This is called the ———

A

wavelength

35
Q

Spring Tides are produced during ———

A

new and full moon

36
Q

Tides on Earth are produced by ——-

A

the moon and sun’s gravitational effects