Chapter 2 Flashcards

1
Q

The word planet is derived from a Greek term meaning

A

Wanderer

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2
Q

The person who first showed that planetary orbits are ellipses was

A

Kepler

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3
Q

In an ellipse, the major axis is a distance measured

A

Along the longer diameter, passing through the foci of the ellipse

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4
Q

Where is a planet when it is moving mot rapidly in its orbit?

A

At perihelion

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5
Q

Mars moves in an elliptical orbit around he sun. The sun is located at

A

The focus of the ellipse that is closer to the point where Mars moves fastest

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6
Q

A major contribution of Johannes Kepler to the development of modern astronomy was

A

Proof that planetary obits are ellipses

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7
Q

Kepler’s 1st law states that a planet moves around the sun in a

A

Elliptical orbit, with the sun at one focus

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8
Q

A perfect circle is an ellipse wig an eccentricity of

A

Zero

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9
Q

Kepler’s 2nd law states hat a planet moves fastest when it

A

Is closets to the sun

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10
Q

Kepler’s 3rd law, the harmonic law, provides a relationship between a planet’s orbital

A

Period and the length of he semi major axis

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11
Q

1 AU is defined as

A

Mean distance between the earth and the sun

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12
Q

Why were Newton’s 3 laws so important to astronomy?

A

Newton’s laws showed that planets can move around the sub by hems elves forever, without coming to rest

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13
Q

According to newton’s 1st law

A

If no net force is acting on an object, hen both he object’s sped and direction of travel will be constant

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14
Q

Newton’s 2nd law states that

A

Force equals mass x acceleration

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15
Q

Acceding to Newton’s 3rd law, if a force is acting on an object, then

A

There must be some other force acting on a different object, with the same magnitude but in the opposite direction

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16
Q

If 2 massive bodies, initially held at rest in space, are released, then they will begin to

A

Move toward one another

17
Q

What is a hyperbola?

A

Indefinitely long curve that never closes on itself

18
Q

Which objects are often found to follow parabolic orbits?

A

Comets

19
Q

The force if gravity between 2 objects is proportional to the

A

Product of their masses

20
Q

In Newton’s law if universal gravitation, F = GMm/R^2, which defines the force between earth with mass M and an orbiting satellite if mass m at a distance R from Earth, G

A

Is a constant, throughout all measured space and time