Topic 12 - Formation of planetary systems Flashcards

1
Q

What is gravitational attraction?

A

It produces regular motion, including the orbits of planets and moons.

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2
Q

What are some effects of tidal gravitational forces?

A

Ring systems, asteroid belts, internal heating.

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3
Q

What do we know about planetary ring systems?

A

The combined gravitational effects of Jupiter and its moons keeps the rings stable.

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4
Q

What do we know about the asteroid belts?

A

It has enough material to form small planets buts the tidal forces of Mars and Jupiter prevent anything larger than Ceres forming.

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5
Q

What is internal heating?

A
  • Tidal forces stretch and compress a planet
  • This creates tidal heating which creates synchronous rotation
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6
Q

What is special about Io?

A
  • It is volcanically active due to the forces from Jupiter
  • It’s average surface temperature is -130°C but it’s volcanoes reach 1650°C
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7
Q

What is chaotic motion?

A

Gravitational forces mean that interactions between more than two bodies can lead to unpredictable and chaotic behaviour.

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8
Q

What are resonances?

A

Planets and moons orbit with their orbit times in constant motion.

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9
Q

What do resonances do?

A

It makes planetary orbits more stable and reduces collisions.

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10
Q

Pluto and Neptune’s Resonance:

A

Pluto makes two orbits of the Sun for every three of Neptune ( makes it impossible for Pluto and Neptune to collide)

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11
Q

Jupiter’s Moons’ Resonance:

A

Io, Europa and Ganymede are in a 4:2:1 orbital resonance with each other

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12
Q

What are Lagrange Points?

A

Locations relative to two bodies where a smaller object can maintain a stable position.

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13
Q

List the Lagrange Points in order, clockwise and inwards.

A

L4, L2, L1, L5, L3

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14
Q

List evidence of collisions:

A
  • Uranus’ extreme orbital tilt
  • Impact craters on moons
  • Earth’s axial tilt (23.5°)
  • Venus’ retrograde spin
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15
Q

What does solar wind cause?

A
  • Planets to lose their atmosphere
  • Causes Aurorae
  • Causes ion tails on comets
  • Forms the heliosphere
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16
Q

What is the Roche Limit?

A
  • The minimum distance a large moon can approach a planet without being torn apart
  • 2.5 times the planet’s radius
17
Q

What has to occur for a planet or moon to have an atmosphere?

A
  • It has a high enough gravitational field
  • It isn’t too hot for gases to escape into space
  • It isn’t exposed to a strong solar wind
18
Q

List the methods for discovering exoplanets:

A
  • Transit Method
  • Astrometry Method
  • Radial Velocity Method
19
Q

What is the Transit Method?

A
  • When an exoplanet moves in front of its star, it blocks light
  • This tells us the planet’s size and distance from its star
20
Q

What is the Astrometry Method?

A

An exoplanet will cause its star to wobble. Powerful telescopes can detect this.

21
Q

What is the Radial Velocity Method?

A

An exoplanet will cause its star to wobble.
By observing the light, the shift in wavelength will tell us if the star is wobbling.

22
Q

What is the Goldilocks (Habitable) Zone?

A

Region where liquid water can be found on the planet’s surface.

23
Q

What does SETI stand for?

A

Search for Extra-Terrestrial Intelligence

24
Q

What is the Drake Equation?

A

N = R* x fp x ne x fl x fi x fc x L