Keplers Laws Flashcards

1
Q

Kepler 1st law

A

An orbiting body travels in an elliptical path around a central, massive body, which is located at one of the ellipses foci

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2
Q

Two points inside an ellipse

A

Focal points

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3
Q

When the planet travels around the elliptical

A

The same time 1 month passes for each interval

Different distances are traveled because the closer to the body the object is the faster it goes

The area of the “triangles” is always the same

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4
Q

An ellipse

A

Is simply a flattened circle

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5
Q

The long axis of the ellipse contains the two foci is know as what ?

A

The major axis

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6
Q

Semi major axis

A

Half the length of the major axis containing the two foci

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7
Q

Eccentricity

A

Equal to the distance between the foci divided by the length of the major axis

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8
Q

A circle is an ellipse in which the two foci happen to coincide (occur at or during the same time). What is the eccentricity of a circle?

A

0

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9
Q

The semi major axis of a circle is what

A

It’s radius

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10
Q

Perihelion

A

The planets point of closest approach to the sun

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11
Q

Aphelion

A

A planets farthest distance in orbit from the sun

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12
Q

Kepler 2nd law

A

An imaginary line connecting the sun to any planet sweeps out equal areas of the ellipse in equal intervals of time

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13
Q

Sideral period

A

Time taken for a body to complete one full orbit around another

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14
Q

Keplers 3rd law

A

The square of a planets orbital period is proportional to the cube of its semimajor axis

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15
Q

Astronomical unit

A

The average distance of earth from the sun

149,603,500 km

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16
Q

One astronomical unit AU is ?

A

The semi major axis of earths orbit around the sun

17
Q

Keplers 3rd law formula

A

P^2 (in earths years) = a^3 + (in astronomical units)

18
Q

P^2 / a^3 should = 1

A

In all cases except Uranus and Neptune because of their gravitation attraction

19
Q

a

A

Orbital semimajor axis (AU)

20
Q

P

A

Orbital period (earth years)

21
Q

e

A

Orbital eccentricity