Chapters 2 and 3 Flashcards

1
Q

From where on Earth could you observe all of the stars during the course of a year?

A

Equator line

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2
Q

What fraction of the sky can be seen from the North Pole?

A

Half of the sky

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3
Q

Explain, according to both geocentric and heliocentric cosmologies, why we see retrograde motion of the planets.

A

The geocentric model explains this with the epicycle
The heliocentric model explains this as the earth goes faster then around the sun then other planets
Both making the planets look like they are going opposite directions (retrograde motion).

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4
Q

What were four of Galileo’s discoveries that were important to astronomy?

A
  1. Venus phases
  2. 4 moons around Jupiter
  3. More stars then the human can see
  4. Craters and mountains on the moon
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5
Q

Ursa Minor contains the pole star, Polaris, and the asterism known as the Little Dipper. From most locations in the Northern Hemisphere, all of the stars in Ursa Minor are circumpolar. Does that mean these stars are also above the horizon during the day? Explain.

A

Yes, the stars are circumpolar (visible above the horizon at all times at a specified locality on the earth’s surface), but you can’t see them during the day due to sunlight/ moonlight.

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6
Q

How many degrees does the Sun move per day relative to the fixed stars?

A

The sun moves 1 degree a day

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7
Q

How many days does it take for the Sun to return to its original location relative to the fixed stars?

A

The sun takes 365 days

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8
Q

Is the ecliptic the same thing as the celestial equator? Explain.

A

Ecliptic: Annual path of the sun
Celestial equator: The 0 degree equator on earth lined outside
The earth is tilted 23.5 degrees, so they never align

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9
Q

What is an asterism? Can you name an example?

A

An asterism is a group of stars that are recognizable, an example are the big and little dipper

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10
Q

What two factors made it difficult, at first, for astronomers to choose between the Copernican heliocentric model and the Ptolemaic geocentric model?

A

One of the objections was if Earth were moving, we would all sense or feel this motion. Another objection was religious related, stating that God would make the us center of universe

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11
Q

What is a constellation as astronomers define it today? What does it mean when an astronomer says, “I saw a comet in Orion last night”?

A

A constellation is a well-defined area of the sky with borders, the astronomer is talking about a region in the sky with said constellation.

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12
Q

What were two arguments or lines of evidence in support of the geocentric model?

A

No parallax or wind, meaning earth is stationary and in the center.

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13
Q

Although the Copernican system was largely correct to place the Sun at the center of all planetary motion, the model still gave inaccurate predictions for planetary positions. Explain the flaw in the Copernican model that hindered its accuracy.

A

The model had the planetary orbits in perfect circles and the same speed for each planets orbit.

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14
Q

Why did Kepler need Tycho Brahe’s data to formulate his laws?

A

Tycho had more accurate measurements of the geocentric cycle.

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15
Q
  1. Which has more mass: an armful of feathers or an armful of lead?
  2. Which has more volume: a kilogram of feathers or a kilogram of lead?
  3. Which has higher density: a kilogram of feathers or a kilogram of lead?
A
  1. Lead
  2. Feathers
  3. Lead
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16
Q

Why do we say that Neptune was the first planet to be discovered through the use of mathematics?

A

Uranus’s orbit around the sun did not fit the equation, and it was predicted that there was another planet pulling on it

17
Q

According to Kepler’s second law, where in a planet’s orbit would it be moving fastest? Where would it be moving slowest?

A

It would be moving fastest at perhelion and slowest at aphelion

18
Q

Explain how a rocket can propel itself using Newton’s third law.

A

When a rocket engine burns fuel and expels hot exhaust gases backwards (the action), the force of those gases pushing against the rocket nozzle creates an equal and opposite force propelling the rocket forward (the reaction).

19
Q

A body moves in a perfectly circular path at constant speed. Are there forces acting in such a system? How do you know?

A

There has to be force present to create circular motion or else the object will go straight

20
Q

By what factor would a person’s weight be increased if Earth had 10 times its present mass, but the same volume?

A

10F, since force is directly proportional to mass, the person would weigh 10 times his or her present weight

21
Q

If 24 g of material fills a cube 2 cm on a side, what is the density of the material?

A

Use D= mass/volume, and cube volume formula: s^3,
24g/ 8cm^3 = 3g/cm^3

22
Q

What is the average distance from the Sun (in astronomical units) of an asteroid with an orbital period of 8 years?

A

a^3=p^2
a^3=8^2
a= 4AU