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Lesson 8a Moons, Asteroids and Rings. Europa These interactions also keep Europa in a slight...

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Lesson 8a Moons, Asteroids and Rings
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Page 1: Lesson 8a Moons, Asteroids and Rings. Europa These interactions also keep Europa in a slight elliptical orbit as well. But since Europa is farther from.

Lesson 8a

Moons, Asteroids and Rings

Page 2: Lesson 8a Moons, Asteroids and Rings. Europa These interactions also keep Europa in a slight elliptical orbit as well. But since Europa is farther from.

Europa

• These interactions also keep Europa in a slight elliptical orbit as well.

• But since Europa is farther from Jupiter the effect is not as strong as on Io.

Page 3: Lesson 8a Moons, Asteroids and Rings. Europa These interactions also keep Europa in a slight elliptical orbit as well. But since Europa is farther from.

Europa’s interior

Page 4: Lesson 8a Moons, Asteroids and Rings. Europa These interactions also keep Europa in a slight elliptical orbit as well. But since Europa is farther from.
Page 5: Lesson 8a Moons, Asteroids and Rings. Europa These interactions also keep Europa in a slight elliptical orbit as well. But since Europa is farther from.

Possible volcanic vents on beneath Europa

Page 6: Lesson 8a Moons, Asteroids and Rings. Europa These interactions also keep Europa in a slight elliptical orbit as well. But since Europa is farther from.

Possible Life?

Page 7: Lesson 8a Moons, Asteroids and Rings. Europa These interactions also keep Europa in a slight elliptical orbit as well. But since Europa is farther from.

New theory on Europa ice flows

Page 8: Lesson 8a Moons, Asteroids and Rings. Europa These interactions also keep Europa in a slight elliptical orbit as well. But since Europa is farther from.
Page 10: Lesson 8a Moons, Asteroids and Rings. Europa These interactions also keep Europa in a slight elliptical orbit as well. But since Europa is farther from.

Orbits of all of Jupiter’s moons

Page 11: Lesson 8a Moons, Asteroids and Rings. Europa These interactions also keep Europa in a slight elliptical orbit as well. But since Europa is farther from.

What do you think about the origin of most of Jupiter’s moons?

Page 12: Lesson 8a Moons, Asteroids and Rings. Europa These interactions also keep Europa in a slight elliptical orbit as well. But since Europa is farther from.

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1 2 3 4

25% 25%25%25%1. Co-accretion origin2. Fission origin3. Capture origin4. Giant impact origin

Page 13: Lesson 8a Moons, Asteroids and Rings. Europa These interactions also keep Europa in a slight elliptical orbit as well. But since Europa is farther from.

What do you think about the origin of most of Jupiter’s moons?

Page 14: Lesson 8a Moons, Asteroids and Rings. Europa These interactions also keep Europa in a slight elliptical orbit as well. But since Europa is farther from.

Asteroid Belt

Page 15: Lesson 8a Moons, Asteroids and Rings. Europa These interactions also keep Europa in a slight elliptical orbit as well. But since Europa is farther from.
Page 16: Lesson 8a Moons, Asteroids and Rings. Europa These interactions also keep Europa in a slight elliptical orbit as well. But since Europa is farther from.
Page 17: Lesson 8a Moons, Asteroids and Rings. Europa These interactions also keep Europa in a slight elliptical orbit as well. But since Europa is farther from.

Lagrangian Points

Page 18: Lesson 8a Moons, Asteroids and Rings. Europa These interactions also keep Europa in a slight elliptical orbit as well. But since Europa is farther from.

Asteroids

Page 19: Lesson 8a Moons, Asteroids and Rings. Europa These interactions also keep Europa in a slight elliptical orbit as well. But since Europa is farther from.

Asteroids

Page 20: Lesson 8a Moons, Asteroids and Rings. Europa These interactions also keep Europa in a slight elliptical orbit as well. But since Europa is farther from.

Eros

Ida & Dactyl

Page 21: Lesson 8a Moons, Asteroids and Rings. Europa These interactions also keep Europa in a slight elliptical orbit as well. But since Europa is farther from.

Dawn mission to Vesta (current)

Page 22: Lesson 8a Moons, Asteroids and Rings. Europa These interactions also keep Europa in a slight elliptical orbit as well. But since Europa is farther from.
Page 23: Lesson 8a Moons, Asteroids and Rings. Europa These interactions also keep Europa in a slight elliptical orbit as well. But since Europa is farther from.
Page 24: Lesson 8a Moons, Asteroids and Rings. Europa These interactions also keep Europa in a slight elliptical orbit as well. But since Europa is farther from.

Phobos – Martian Moon

Page 25: Lesson 8a Moons, Asteroids and Rings. Europa These interactions also keep Europa in a slight elliptical orbit as well. But since Europa is farther from.
Page 26: Lesson 8a Moons, Asteroids and Rings. Europa These interactions also keep Europa in a slight elliptical orbit as well. But since Europa is farther from.

Deimos – Martian moon

Page 27: Lesson 8a Moons, Asteroids and Rings. Europa These interactions also keep Europa in a slight elliptical orbit as well. But since Europa is farther from.

• What is the likely origin of the moons of Mars?

Page 28: Lesson 8a Moons, Asteroids and Rings. Europa These interactions also keep Europa in a slight elliptical orbit as well. But since Europa is farther from.

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1 2 3 4

25% 25%25%25%1. Fission2. Co-accretion3. Capture4. Giant impact

Page 29: Lesson 8a Moons, Asteroids and Rings. Europa These interactions also keep Europa in a slight elliptical orbit as well. But since Europa is farther from.

Russian probe Phobos-Grunt.

• Probe stuck in Earth’s orbit.• Would have landed on Phobos and returned

to Earth, soil and rock samples.

• If Phobos is chemically similar to Mars, then it could be the Phobos and Demos originated as shot out debris from a Martian impact.

Page 30: Lesson 8a Moons, Asteroids and Rings. Europa These interactions also keep Europa in a slight elliptical orbit as well. But since Europa is farther from.

• Phobos orbits Mars every 11 hours.• Demos orbits Mars every 30 hours.• Mars rotates on its axis every ~ 25 hours.

• In the next 50 million years, Phobos will crash into Mars.

Page 31: Lesson 8a Moons, Asteroids and Rings. Europa These interactions also keep Europa in a slight elliptical orbit as well. But since Europa is farther from.

Earth and the Moon

Page 32: Lesson 8a Moons, Asteroids and Rings. Europa These interactions also keep Europa in a slight elliptical orbit as well. But since Europa is farther from.

• Why will Phobos crash into Mars?

Page 33: Lesson 8a Moons, Asteroids and Rings. Europa These interactions also keep Europa in a slight elliptical orbit as well. But since Europa is farther from.

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1 2 3

33% 33%33%1. Phobos is too close and Mars

gravity will pull it in.2. Phobos is orbiting faster than Mars

spins. Mars is slowing it up.3. Demos is pulling on Phobos

causing it to fall into Mars

Page 34: Lesson 8a Moons, Asteroids and Rings. Europa These interactions also keep Europa in a slight elliptical orbit as well. But since Europa is farther from.

Effect of sub-synchronous orbit.

Phobos is speedingUp Mars rotation, and Mars is slowing up Phobos’sOrbital speed.

Page 35: Lesson 8a Moons, Asteroids and Rings. Europa These interactions also keep Europa in a slight elliptical orbit as well. But since Europa is farther from.
Page 36: Lesson 8a Moons, Asteroids and Rings. Europa These interactions also keep Europa in a slight elliptical orbit as well. But since Europa is farther from.
Page 37: Lesson 8a Moons, Asteroids and Rings. Europa These interactions also keep Europa in a slight elliptical orbit as well. But since Europa is farther from.

• What does this 3:1 represent?

Page 38: Lesson 8a Moons, Asteroids and Rings. Europa These interactions also keep Europa in a slight elliptical orbit as well. But since Europa is farther from.

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1 2 3 4

25% 25%25%25%1. Jupiter is 3 times farther from the Sun than the gap is.

2. Jupiter completes 3 orbits for every 1 gap orbit.3. The gap is 3 times closer to the Sun than Jupiter4. The gap completes 3 orbits for every 1 of

Jupiter’s orbits.

Page 39: Lesson 8a Moons, Asteroids and Rings. Europa These interactions also keep Europa in a slight elliptical orbit as well. But since Europa is farther from.

Keplers 3rd law relates period to semi-major axis

• Kirkwood gap with resonance 3:1.• Semi-major axis is a = 2.5 AU.

P2 = a3 P = (2.53)0.5 = 3.95 yearsJupiter has a = 5.2 AU. PJ = (5.23)0.5 = 11.85 years.

11.85/3.95 = 3 This is the 3:1 resonance

Page 40: Lesson 8a Moons, Asteroids and Rings. Europa These interactions also keep Europa in a slight elliptical orbit as well. But since Europa is farther from.
Page 41: Lesson 8a Moons, Asteroids and Rings. Europa These interactions also keep Europa in a slight elliptical orbit as well. But since Europa is farther from.
Page 42: Lesson 8a Moons, Asteroids and Rings. Europa These interactions also keep Europa in a slight elliptical orbit as well. But since Europa is farther from.

Eris

Page 43: Lesson 8a Moons, Asteroids and Rings. Europa These interactions also keep Europa in a slight elliptical orbit as well. But since Europa is farther from.

Kuiper belt and scattered disk

Page 44: Lesson 8a Moons, Asteroids and Rings. Europa These interactions also keep Europa in a slight elliptical orbit as well. But since Europa is farther from.
Page 45: Lesson 8a Moons, Asteroids and Rings. Europa These interactions also keep Europa in a slight elliptical orbit as well. But since Europa is farther from.

The Planets• Currently there is little evidence that the

planets in the Solar System are in any type of resonance orbit.

• Example:• Jupiter orbital period = 11.86 years• Saturn orbital period = 29.46 years 29.46/11.86 = 2.48 Close to a 2:5 resonance• But this wasn’t always the case.

Page 46: Lesson 8a Moons, Asteroids and Rings. Europa These interactions also keep Europa in a slight elliptical orbit as well. But since Europa is farther from.

• It has been shown with theoretical modeling that Saturn likely formed much closer to Jupiter.

• Also Uranus and Neptune were within 15 AU of the Sun originally. Now they are at 19 AU and 30 AU.

• Some models suggest that Neptune actually formed closer to the Sun than Uranus.

• When Jupiter and Saturn formed they were very close to 1:2 resonance orbit

Page 47: Lesson 8a Moons, Asteroids and Rings. Europa These interactions also keep Europa in a slight elliptical orbit as well. But since Europa is farther from.

The giant planets and Kuiper belt objects.

Page 48: Lesson 8a Moons, Asteroids and Rings. Europa These interactions also keep Europa in a slight elliptical orbit as well. But since Europa is farther from.

• Jupiter and Saturn exchanged angular momentum and finally Saturn reached a resonance 1:2 orbit with Jupiter.

• When this happened in a very short period of time the combined effects of the two enormous planets was to move Uranus and Neptune outward.

• Their motion also effect Saturn, like-wise moved outward.

Page 49: Lesson 8a Moons, Asteroids and Rings. Europa These interactions also keep Europa in a slight elliptical orbit as well. But since Europa is farther from.

A model of planetary migration

Page 50: Lesson 8a Moons, Asteroids and Rings. Europa These interactions also keep Europa in a slight elliptical orbit as well. But since Europa is farther from.
Page 51: Lesson 8a Moons, Asteroids and Rings. Europa These interactions also keep Europa in a slight elliptical orbit as well. But since Europa is farther from.

Other models of this migration

Page 52: Lesson 8a Moons, Asteroids and Rings. Europa These interactions also keep Europa in a slight elliptical orbit as well. But since Europa is farther from.

The effect of this migration

• Jupiter moved inward in its orbit. It is thought that this is what allowed it to capture some of its moons and as it moved into the asteroid belt, it picked up the Trojan asteroids in its lagrange points.

• Neptune moved rapidly outward. Its elliptical orbit settled down to circular by exchanging angular momentum with the Kuiper objects.

Page 53: Lesson 8a Moons, Asteroids and Rings. Europa These interactions also keep Europa in a slight elliptical orbit as well. But since Europa is farther from.

New evidence published this year

• Gravity models using just the four gas giant planets is not able to produce the orbits we see today.

• Early on in the solar system it is thought that this extra planet was sped up by interactions and flung out of the solar system.

Page 54: Lesson 8a Moons, Asteroids and Rings. Europa These interactions also keep Europa in a slight elliptical orbit as well. But since Europa is farther from.

• Many of the Kuiper objects were moved outward onto highly eccentric orbits. Some inhabited a large region around the Solar System called the Oort cloud. These are seen today as comets when they near the Sun.

• Others were sent down to the center of the solar system where they collided with the Sun and the terrestrial planets.

• This time is called the “Late Heavy Bombardment” around 4 billion years ago.

Page 55: Lesson 8a Moons, Asteroids and Rings. Europa These interactions also keep Europa in a slight elliptical orbit as well. But since Europa is farther from.

• It is thought that the large impacts that made the Lunar Maria came from this event.

• Also Hellas crater on Mars.• Also the axis tilts of Saturn, Uranus and

Neptune probably occurred because of this migration.

Page 56: Lesson 8a Moons, Asteroids and Rings. Europa These interactions also keep Europa in a slight elliptical orbit as well. But since Europa is farther from.
Page 57: Lesson 8a Moons, Asteroids and Rings. Europa These interactions also keep Europa in a slight elliptical orbit as well. But since Europa is farther from.

• It is thought that the large impacts that made the Lunar Maria came from this event.

• Also Hellas crater on Mars.• Also the axis tilts of Saturn, Uranus and

Neptune probably occurred because of this migration

• After the Jupiter-Saturn 1:2 resonance event, the Solar System settled into the configuration seen today.

Page 58: Lesson 8a Moons, Asteroids and Rings. Europa These interactions also keep Europa in a slight elliptical orbit as well. But since Europa is farther from.

New evidence published in 2011• Gravity models using just the four gas giant

planets are not able to produce the orbits we see today.

• By adding an additional Neptune-size planet the orbits of the current gas-giants are correct.

• Early on in the solar system it is thought that this extra planet was sped up by interactions and flung out of the solar system.


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