Test 2 Flashcards

1
Q

Mercury

A

Small
No volcanos
Lots of craters
Dead

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2
Q

Venus

A

Large
inactive volcanos
Has an atmosphere
Fewer craters
Alive(ish)

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3
Q

Earth

A

Largest rocky planet
Active geology
few craters
Alive

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4
Q

Mars

A

Small
inactive volcanos
lots of craters
Dead (ish)

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5
Q

Moon

A

Small
No volcanos
Lots of craters
Dead

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6
Q

Io

A

Small
tidal squeeze
volcanos
No craters
Alive

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7
Q

Europa

A

Small
tidal squeeze
some craters
Alive(ish)

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8
Q

Ganymede

A

Small
tidal squeeze
some craters
Alive (ish)

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9
Q

Callisto

A

small
less tidal squeeze
some craters
Dead (ish)

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10
Q

Titan

A

Small
Tidal squeeze
Atmosphere
Few Craters
Alive

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11
Q

Triton, Pluto

A

Small
Weird
Some avidence of cryovocanism
Alive(ish)

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12
Q

Keplers First Law

A

Law of Ellipses- Planets move around the sun in a circle positioned at one focus

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13
Q

Keplers Second law

A

Law of Equal Areas- Planets closer to the sun revolve around it at higher velocities than planets furthere from the sun.

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14
Q

Keplers Third Law

A

Planets further away from the sun take much longer to revolve around it than planets that are closer.

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15
Q

Eccentricity (Def, purpose, range)

A

Eccentricity is the measure of how close to a perfect circle an objects orbit is. It ranges from 1-0, with 0 being a perfect circle.

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16
Q

Finding the Semi-major axis

A

Longest Diameter of an Elipse diveded by 2

17
Q

Semi-Minor

A

Shortest diameter of an elipse

18
Q

Apogee

A

Furthest point in orbit from the Earth

19
Q

Aphelion

A

Furthest point in orbit from the Sun

20
Q

Apoapsis

A

As far away one object can be from another object

21
Q

Perigee

A

Closest point to Earth

22
Q

Perihelion

A

Closest point to the Sun

23
Q

Periapsis

A

As close one object can be in orbit to another.

24
Q

What did Copernicus insist on using in all his models

A

Perfect circles

25
What did Galileo notice about Venus
1.) Had phases 2.) Could appear larger or smaller on certain nights
26
What did Galileo notice about Jupiter
He saw that Jupiter had Moons orbiting around it which proved that not everything revolved around Earth.
27
What did Galileo notice about our moon specifically
He noticed that the moon was covered in craters and blemishes which proved that not all objects were "perfect"
28
Newton's first law
Inertia - object in motion stays in motion unless acted upon by an outside force.
29
Newton's second law
Law of acceleration- Force = mass x acceleration
30
Newton's third law
Law of motion- If one object exerts force on another object, that object will exert an equal and opposite force on the other object.
31
Newtons "fourth" Law
Law of Universal Gravitation
32
How did Brahe describe the solarsystems orbits
He combined Geocentric and Heliocentric thoughts and said that the sun revolves around the Earth while all other planets revolve around the Sun.
33
Arcminute
.016 Degrees
34
Spring Tides
Stronger Occur during Full and New moons Sun Earth Moon all in a line
35
Neap Tides
Weaker Occur during First and Third quarter moons Sun Earth Moon at a 90 degree angle
36
Orbital Period
Time it takes something to go around the Sun. Semi-major axis cubed = orbital period squared
37
Angular Momentum
Angular momentum is the rotational equivalent of linear momentum. It is conserved in a closed system, meaning an object's rotation speed changes if its shape or distance from the axis changes.
38