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The Moon

The Moon. What We See Where We’ve Been The Big Features Oceanus (ocean) Maria (Mare) (sea) Craters Highlands – bright, cratered regions Lowlands/Maria

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Page 1: The Moon. What We See Where We’ve Been The Big Features Oceanus (ocean) Maria (Mare) (sea) Craters Highlands – bright, cratered regions Lowlands/Maria

The Moon

Page 2: The Moon. What We See Where We’ve Been The Big Features Oceanus (ocean) Maria (Mare) (sea) Craters Highlands – bright, cratered regions Lowlands/Maria

What We See

Page 3: The Moon. What We See Where We’ve Been The Big Features Oceanus (ocean) Maria (Mare) (sea) Craters Highlands – bright, cratered regions Lowlands/Maria

Where We’ve Been

Page 4: The Moon. What We See Where We’ve Been The Big Features Oceanus (ocean) Maria (Mare) (sea) Craters Highlands – bright, cratered regions Lowlands/Maria

The Big Features

Oceanus (ocean)Maria (Mare) (sea)Craters

Highlands – bright, cratered regionsLowlands/Maria – dark, flat regions

Page 5: The Moon. What We See Where We’ve Been The Big Features Oceanus (ocean) Maria (Mare) (sea) Craters Highlands – bright, cratered regions Lowlands/Maria

Other Features

Mountains

Valleys

Page 6: The Moon. What We See Where We’ve Been The Big Features Oceanus (ocean) Maria (Mare) (sea) Craters Highlands – bright, cratered regions Lowlands/Maria
Page 7: The Moon. What We See Where We’ve Been The Big Features Oceanus (ocean) Maria (Mare) (sea) Craters Highlands – bright, cratered regions Lowlands/Maria

Librations

The result of (a) wobbling of the Moon’s axis toward/away from earth(b) Relative motion of the observer as Earth rotates(c) Non-circularity of moon’s orbit (change in size)

Page 8: The Moon. What We See Where We’ve Been The Big Features Oceanus (ocean) Maria (Mare) (sea) Craters Highlands – bright, cratered regions Lowlands/Maria

What’s it made of?

I…am…IRON MOON

Ti abundance(blue = lots, orange/purple = less)

But…no dipolar magnetic field. The moon’s weak B field comes from magnetic minerals.

Page 9: The Moon. What We See Where We’ve Been The Big Features Oceanus (ocean) Maria (Mare) (sea) Craters Highlands – bright, cratered regions Lowlands/Maria

The Real Dark Side of the Moon

Note which side the maria are on.Why only that side?

•Anorthosite: igneous rock rich in Ti, Fe•Basalt: fine-grained igneous rock caused by cooling magma

Page 10: The Moon. What We See Where We’ve Been The Big Features Oceanus (ocean) Maria (Mare) (sea) Craters Highlands – bright, cratered regions Lowlands/Maria

Mascons

Page 11: The Moon. What We See Where We’ve Been The Big Features Oceanus (ocean) Maria (Mare) (sea) Craters Highlands – bright, cratered regions Lowlands/Maria

Water?

Chandrayaan-1(water in blue)

Lunar Prospector measures neutrons from H

1996: Clementine indicates ice in deep craters1998: Lunar Prospector indicates ice1998: LP crashed into surface; no water seen2009: Moon Mineral Mapper aboard Chandrayaan-1 detects water

Page 12: The Moon. What We See Where We’ve Been The Big Features Oceanus (ocean) Maria (Mare) (sea) Craters Highlands – bright, cratered regions Lowlands/Maria

LCROSS• Launched with LRO in 2008• Atlas-Centaur rocket impactor

targeted Cabeus crater• Impactor (2305

kg/10,000mph) produced ejecta plume

• LCROSS probe flew through the plume and crashed, relaying data

• Data indicate 5% of plume mass was water

Page 13: The Moon. What We See Where We’ve Been The Big Features Oceanus (ocean) Maria (Mare) (sea) Craters Highlands – bright, cratered regions Lowlands/Maria

Where did the moon come from?

• 4 theories– Fission (moon broke off from earth)– Sisterhood/Co-accretion (formed at the

same time)– Capture (moon formed somewhere else but

drifted by and ended up in the Earth’s gravitational field)

– Giant Impactor (something hit the earth and the resulting material formed the moon)

Page 14: The Moon. What We See Where We’ve Been The Big Features Oceanus (ocean) Maria (Mare) (sea) Craters Highlands – bright, cratered regions Lowlands/Maria

Which one is right?

1. Fissiona. Composition of E and M are similar, but not that

similar.

b. Not enough mass in the Pacific Basin to account for the moon.

2. Sisterhood/Co-accretiona. See #1 about composition.

b. E and M should be the same age; M is younger.

Page 15: The Moon. What We See Where We’ve Been The Big Features Oceanus (ocean) Maria (Mare) (sea) Craters Highlands – bright, cratered regions Lowlands/Maria

Which one is right?3. Capture

a. E and M are too similar for the moon to have formed elsewhere

b. Angular momentum of the E/M system isn’t right for the moon having flown in and stopped

4. Giant Impactora. Given a Mars-sized impactor,

mass is rightb. Volatile metals and lack of water

on the moon indicate high temperatures in the past.

c. Simulations show it’s viable (angular momentum OK)

d. Lower density of moon, lack of iron are consistent with violent impact

Page 16: The Moon. What We See Where We’ve Been The Big Features Oceanus (ocean) Maria (Mare) (sea) Craters Highlands – bright, cratered regions Lowlands/Maria

Whack-a-Moon

t=0

t=24h

•Eventually, the cloud becomes a disk and then a moon.•The impactor core becomes the moon’s core•Intense heat is consistent with lack of volatiles and lack of similarity to the earth.