Chapter 3 - Science Flashcards

Test Review for Chapter 3 (20 cards)

1
Q

Aphelion

A

The point in a planet’s orbit where it is farthest from the sun

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2
Q

Perihelion

A

The point in a planet’s orbit where it is closest to the sun

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3
Q

Apogee

A

The point in a moon’s orbit where it is furthest from the planet

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4
Q

Perigee

A

The point in a moon’s orbit where it is closest to the planet

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5
Q

Bound orbit

A

An orbit in which an object orbits another object repeatedly

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6
Q

Unbound orbit

A

An orbit in which an object passes by another object once and then never again

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7
Q

Eccentricity

A

How much an orbit deviates from a perfect circle

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8
Q

Escape velocity

A

The minimum speed needed to escape an object’s gravity from a certain point

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9
Q

Orbital period

A

How long an object takes to complete one orbit

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10
Q

Semimajor axis

A

The longer axis of an object’s orbit

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11
Q

Aristotle

A

Believed that the Earth was the center of the universe and everything else orbited it in perfect circles

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12
Q

Ptolemy

A

Developed the “circles on circles” model of the universe to explain apparent retrograde motion

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13
Q

Copernicus

A

Developed a heliocentric model of the universe where the Earth orbited the sun in perfect circles

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14
Q

Galileo

A

Supported the heliocentric model with observational evidence
Discovered several moons of Jupiter

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15
Q

Isaac Newton

A

Developed three laws of gravity which describe gravitational forces within the solar system with reasonable accuracy

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16
Q

Johannes Kepler

A

Used Brahe’s observations to develop three laws of planetary motion
Suggested that planets did not orbit in perfect circles

17
Q

Tycho Brahe

A

Made extremely detailed observations of the motion of stars, comets, and planets over many years

18
Q

What is Kepler’s First Law of Planetary Motion?

A

Planets orbit the sun in an elliptical orbit with the sun at one focus

19
Q

What is Kepler’s Second Law of Planetary Motion?

A

A planet sweeps out equal areas of its orbit in equal times

Application: planets orbit faster when farther from the sun and slower when closer to the sun

20
Q

What is Kepler’s Third Law of Planetary Motion?

A

A planet’s orbital period is proportional to the length of its semimajor axis

Orbital period squared = semimajor axis cubed