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The Moon Our nearest neighbor

The Moon - physics.udel.edujlp/classweb2/directory/powerpoint/moon.pdf · region (700 km deep) –tides 2) Vibrations from impacts 3) Thermal quakes from expansion of crust 4) Shallow

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Page 1: The Moon - physics.udel.edujlp/classweb2/directory/powerpoint/moon.pdf · region (700 km deep) –tides 2) Vibrations from impacts 3) Thermal quakes from expansion of crust 4) Shallow

The Moon

Our nearest neighbor

Page 2: The Moon - physics.udel.edujlp/classweb2/directory/powerpoint/moon.pdf · region (700 km deep) –tides 2) Vibrations from impacts 3) Thermal quakes from expansion of crust 4) Shallow
Page 3: The Moon - physics.udel.edujlp/classweb2/directory/powerpoint/moon.pdf · region (700 km deep) –tides 2) Vibrations from impacts 3) Thermal quakes from expansion of crust 4) Shallow

Info about the Moon◼ Diameter: 3,476 km (0.27 earth) (5th largest, 2nd in density)

◼ Distance from Earth: 384,000 km (239,000 miles)

◼ Surface gravity: 0.16

◼ Roughly same surface area as Africa

◼ Orbital period: 27.3 days

◼ Day: 27.3 days (tidally locked)

◼ No atmosphere◼ Daytime Temp = 224F, night= -244F

◼ Surface features: ◼ Heavily cratered, old uplands

◼ Maria, or lava flows, 16% surface

◼ Water on the Moon?

◼ Crust is 60-70 km (3x earth’s)

◼ Mantle

◼ Core is probably iron, > 450km in diameter (25% lunar diameter)

Page 4: The Moon - physics.udel.edujlp/classweb2/directory/powerpoint/moon.pdf · region (700 km deep) –tides 2) Vibrations from impacts 3) Thermal quakes from expansion of crust 4) Shallow

Lunar Interior

Page 5: The Moon - physics.udel.edujlp/classweb2/directory/powerpoint/moon.pdf · region (700 km deep) –tides 2) Vibrations from impacts 3) Thermal quakes from expansion of crust 4) Shallow

Moonquakes

1) Deep earthquakes from mantle

region (700 km deep) – tides

2) Vibrations from impacts

3) Thermal quakes from expansion

of crust

4) Shallow quakes 20-30 km deep,

can last for 10 minutes, mag 5.5

Page 6: The Moon - physics.udel.edujlp/classweb2/directory/powerpoint/moon.pdf · region (700 km deep) –tides 2) Vibrations from impacts 3) Thermal quakes from expansion of crust 4) Shallow

Near and Far Sides of the Moon

Page 7: The Moon - physics.udel.edujlp/classweb2/directory/powerpoint/moon.pdf · region (700 km deep) –tides 2) Vibrations from impacts 3) Thermal quakes from expansion of crust 4) Shallow
Page 8: The Moon - physics.udel.edujlp/classweb2/directory/powerpoint/moon.pdf · region (700 km deep) –tides 2) Vibrations from impacts 3) Thermal quakes from expansion of crust 4) Shallow

North and South Poles

Page 9: The Moon - physics.udel.edujlp/classweb2/directory/powerpoint/moon.pdf · region (700 km deep) –tides 2) Vibrations from impacts 3) Thermal quakes from expansion of crust 4) Shallow

Phases of the Moon

Page 10: The Moon - physics.udel.edujlp/classweb2/directory/powerpoint/moon.pdf · region (700 km deep) –tides 2) Vibrations from impacts 3) Thermal quakes from expansion of crust 4) Shallow

Map of Sunlight on the North Pole

Page 11: The Moon - physics.udel.edujlp/classweb2/directory/powerpoint/moon.pdf · region (700 km deep) –tides 2) Vibrations from impacts 3) Thermal quakes from expansion of crust 4) Shallow

The Surface of the Moon

Maria (seas) – dark areas

– solidified pools of ancient

lava reflect less light

Terrae (highlands) – light

areas – very ancient surface

of moon

Impact craters – “spots”

Page 12: The Moon - physics.udel.edujlp/classweb2/directory/powerpoint/moon.pdf · region (700 km deep) –tides 2) Vibrations from impacts 3) Thermal quakes from expansion of crust 4) Shallow
Page 13: The Moon - physics.udel.edujlp/classweb2/directory/powerpoint/moon.pdf · region (700 km deep) –tides 2) Vibrations from impacts 3) Thermal quakes from expansion of crust 4) Shallow

Maria

1) Solidified pools of basaltic lava – lava

flowed into old impact basins

1) Thin crust allowed lava flows

2) High iron content

3) Evidence for old shield volcanoes

4) Found mostly on near side – 31% of

surface on near side

5) Most 3-3.5 billion years old, a few as

young as 1.2 billion years

Page 14: The Moon - physics.udel.edujlp/classweb2/directory/powerpoint/moon.pdf · region (700 km deep) –tides 2) Vibrations from impacts 3) Thermal quakes from expansion of crust 4) Shallow

Volcanoes on the Moon

Page 15: The Moon - physics.udel.edujlp/classweb2/directory/powerpoint/moon.pdf · region (700 km deep) –tides 2) Vibrations from impacts 3) Thermal quakes from expansion of crust 4) Shallow

Volcanoes on Earth, Io, Moon

Page 16: The Moon - physics.udel.edujlp/classweb2/directory/powerpoint/moon.pdf · region (700 km deep) –tides 2) Vibrations from impacts 3) Thermal quakes from expansion of crust 4) Shallow
Page 17: The Moon - physics.udel.edujlp/classweb2/directory/powerpoint/moon.pdf · region (700 km deep) –tides 2) Vibrations from impacts 3) Thermal quakes from expansion of crust 4) Shallow

Lunar Surface

Page 18: The Moon - physics.udel.edujlp/classweb2/directory/powerpoint/moon.pdf · region (700 km deep) –tides 2) Vibrations from impacts 3) Thermal quakes from expansion of crust 4) Shallow

Lunar Highlands

• Heavily Cratered

• Ancient – as old as 4 billion

years

• Shows dominance of

impacts in early history of

solar system – 300k craters

larger than 1 km

• Evidence that formed from

magma ocean

• “mountains” do not have

same origin as earth

Page 19: The Moon - physics.udel.edujlp/classweb2/directory/powerpoint/moon.pdf · region (700 km deep) –tides 2) Vibrations from impacts 3) Thermal quakes from expansion of crust 4) Shallow
Page 20: The Moon - physics.udel.edujlp/classweb2/directory/powerpoint/moon.pdf · region (700 km deep) –tides 2) Vibrations from impacts 3) Thermal quakes from expansion of crust 4) Shallow

Impact Craters

◼ ~0.5 million craters

◼ Can be used to

estimate age

Page 21: The Moon - physics.udel.edujlp/classweb2/directory/powerpoint/moon.pdf · region (700 km deep) –tides 2) Vibrations from impacts 3) Thermal quakes from expansion of crust 4) Shallow

Crater Formation

Page 22: The Moon - physics.udel.edujlp/classweb2/directory/powerpoint/moon.pdf · region (700 km deep) –tides 2) Vibrations from impacts 3) Thermal quakes from expansion of crust 4) Shallow

Crater Formation 2

Page 23: The Moon - physics.udel.edujlp/classweb2/directory/powerpoint/moon.pdf · region (700 km deep) –tides 2) Vibrations from impacts 3) Thermal quakes from expansion of crust 4) Shallow

Copernicus Crater

Age: 800 million

years (Apollo 12)

Size: 93 km

Page 24: The Moon - physics.udel.edujlp/classweb2/directory/powerpoint/moon.pdf · region (700 km deep) –tides 2) Vibrations from impacts 3) Thermal quakes from expansion of crust 4) Shallow

Fresh Crater Showing Ejecta

Page 25: The Moon - physics.udel.edujlp/classweb2/directory/powerpoint/moon.pdf · region (700 km deep) –tides 2) Vibrations from impacts 3) Thermal quakes from expansion of crust 4) Shallow
Page 26: The Moon - physics.udel.edujlp/classweb2/directory/powerpoint/moon.pdf · region (700 km deep) –tides 2) Vibrations from impacts 3) Thermal quakes from expansion of crust 4) Shallow

Copernicus

Page 27: The Moon - physics.udel.edujlp/classweb2/directory/powerpoint/moon.pdf · region (700 km deep) –tides 2) Vibrations from impacts 3) Thermal quakes from expansion of crust 4) Shallow

Tycho Crater

• 110 Million years

• 85 km

• Bright ejecta make

it a prominent

feature

Page 28: The Moon - physics.udel.edujlp/classweb2/directory/powerpoint/moon.pdf · region (700 km deep) –tides 2) Vibrations from impacts 3) Thermal quakes from expansion of crust 4) Shallow
Page 29: The Moon - physics.udel.edujlp/classweb2/directory/powerpoint/moon.pdf · region (700 km deep) –tides 2) Vibrations from impacts 3) Thermal quakes from expansion of crust 4) Shallow

Piece of Ejecta from Tycho

Page 30: The Moon - physics.udel.edujlp/classweb2/directory/powerpoint/moon.pdf · region (700 km deep) –tides 2) Vibrations from impacts 3) Thermal quakes from expansion of crust 4) Shallow

Other Lunar Features

Graben: trench that forms due to expansion of lunar surface

Evidence that

the moon is still

contracting

Page 31: The Moon - physics.udel.edujlp/classweb2/directory/powerpoint/moon.pdf · region (700 km deep) –tides 2) Vibrations from impacts 3) Thermal quakes from expansion of crust 4) Shallow

Topographical Map of Graben

Page 32: The Moon - physics.udel.edujlp/classweb2/directory/powerpoint/moon.pdf · region (700 km deep) –tides 2) Vibrations from impacts 3) Thermal quakes from expansion of crust 4) Shallow

Lobate Scarps – More evidence of contraction

• Known as a thrust fault –

where crust of the moon is

pushing together.

• Steep face on one side, gentle

slope on the other

Page 33: The Moon - physics.udel.edujlp/classweb2/directory/powerpoint/moon.pdf · region (700 km deep) –tides 2) Vibrations from impacts 3) Thermal quakes from expansion of crust 4) Shallow
Page 34: The Moon - physics.udel.edujlp/classweb2/directory/powerpoint/moon.pdf · region (700 km deep) –tides 2) Vibrations from impacts 3) Thermal quakes from expansion of crust 4) Shallow
Page 35: The Moon - physics.udel.edujlp/classweb2/directory/powerpoint/moon.pdf · region (700 km deep) –tides 2) Vibrations from impacts 3) Thermal quakes from expansion of crust 4) Shallow

Rilles – Canyons/Trenches on the Moon

Page 36: The Moon - physics.udel.edujlp/classweb2/directory/powerpoint/moon.pdf · region (700 km deep) –tides 2) Vibrations from impacts 3) Thermal quakes from expansion of crust 4) Shallow

Rille – from a

collapsed lava

tube?

Page 37: The Moon - physics.udel.edujlp/classweb2/directory/powerpoint/moon.pdf · region (700 km deep) –tides 2) Vibrations from impacts 3) Thermal quakes from expansion of crust 4) Shallow
Page 38: The Moon - physics.udel.edujlp/classweb2/directory/powerpoint/moon.pdf · region (700 km deep) –tides 2) Vibrations from impacts 3) Thermal quakes from expansion of crust 4) Shallow

Longest Rille on the Moon

160 km x 10 km

Page 39: The Moon - physics.udel.edujlp/classweb2/directory/powerpoint/moon.pdf · region (700 km deep) –tides 2) Vibrations from impacts 3) Thermal quakes from expansion of crust 4) Shallow

Wrinkle Ridges

160 km x 10 km

• Formed when lava

cools and

contracts

Page 40: The Moon - physics.udel.edujlp/classweb2/directory/powerpoint/moon.pdf · region (700 km deep) –tides 2) Vibrations from impacts 3) Thermal quakes from expansion of crust 4) Shallow

Wrinkle Ridges in the Sea of Tranquillity.

Page 41: The Moon - physics.udel.edujlp/classweb2/directory/powerpoint/moon.pdf · region (700 km deep) –tides 2) Vibrations from impacts 3) Thermal quakes from expansion of crust 4) Shallow
Page 42: The Moon - physics.udel.edujlp/classweb2/directory/powerpoint/moon.pdf · region (700 km deep) –tides 2) Vibrations from impacts 3) Thermal quakes from expansion of crust 4) Shallow
Page 43: The Moon - physics.udel.edujlp/classweb2/directory/powerpoint/moon.pdf · region (700 km deep) –tides 2) Vibrations from impacts 3) Thermal quakes from expansion of crust 4) Shallow

Lunar Soil (regolith)

Page 44: The Moon - physics.udel.edujlp/classweb2/directory/powerpoint/moon.pdf · region (700 km deep) –tides 2) Vibrations from impacts 3) Thermal quakes from expansion of crust 4) Shallow

Regolith

• Mechanical disintegration of

basalt and other rocks on the

moon due to meteor impacts

and bombardment by solar

and cosmic high energy

particles.

• No organic components.

• Rock fragments, glass,

volcanic and impact

spherules

Page 45: The Moon - physics.udel.edujlp/classweb2/directory/powerpoint/moon.pdf · region (700 km deep) –tides 2) Vibrations from impacts 3) Thermal quakes from expansion of crust 4) Shallow
Page 46: The Moon - physics.udel.edujlp/classweb2/directory/powerpoint/moon.pdf · region (700 km deep) –tides 2) Vibrations from impacts 3) Thermal quakes from expansion of crust 4) Shallow

Water

Page 47: The Moon - physics.udel.edujlp/classweb2/directory/powerpoint/moon.pdf · region (700 km deep) –tides 2) Vibrations from impacts 3) Thermal quakes from expansion of crust 4) Shallow

Apollo 11 Landing Site

Page 48: The Moon - physics.udel.edujlp/classweb2/directory/powerpoint/moon.pdf · region (700 km deep) –tides 2) Vibrations from impacts 3) Thermal quakes from expansion of crust 4) Shallow
Page 49: The Moon - physics.udel.edujlp/classweb2/directory/powerpoint/moon.pdf · region (700 km deep) –tides 2) Vibrations from impacts 3) Thermal quakes from expansion of crust 4) Shallow

Views from the lunar surface

Page 50: The Moon - physics.udel.edujlp/classweb2/directory/powerpoint/moon.pdf · region (700 km deep) –tides 2) Vibrations from impacts 3) Thermal quakes from expansion of crust 4) Shallow

Apollo 12

Page 51: The Moon - physics.udel.edujlp/classweb2/directory/powerpoint/moon.pdf · region (700 km deep) –tides 2) Vibrations from impacts 3) Thermal quakes from expansion of crust 4) Shallow

Apollo 13 Views of Far Side of the Moon

Page 52: The Moon - physics.udel.edujlp/classweb2/directory/powerpoint/moon.pdf · region (700 km deep) –tides 2) Vibrations from impacts 3) Thermal quakes from expansion of crust 4) Shallow

Apollo 14

Page 53: The Moon - physics.udel.edujlp/classweb2/directory/powerpoint/moon.pdf · region (700 km deep) –tides 2) Vibrations from impacts 3) Thermal quakes from expansion of crust 4) Shallow

Apollo 17

Page 54: The Moon - physics.udel.edujlp/classweb2/directory/powerpoint/moon.pdf · region (700 km deep) –tides 2) Vibrations from impacts 3) Thermal quakes from expansion of crust 4) Shallow

Orbit of the Moon

Plane of Earth’s equator: Celestial equator – tilted 23.5 deg wrt Solar system

Tilt of moon’s equator wrt its orbit – 6.68 deg

Tilt of moon’s axis wrt solar system = 1.53 deg

Axis of moon – tilted 1.53 deg wrt moon’s orbit

Page 55: The Moon - physics.udel.edujlp/classweb2/directory/powerpoint/moon.pdf · region (700 km deep) –tides 2) Vibrations from impacts 3) Thermal quakes from expansion of crust 4) Shallow

Orbit of the Moon

Barycenter = underneath the surface of the earth

Barycenter = ∑(rimi)/∑(mi)

Page 56: The Moon - physics.udel.edujlp/classweb2/directory/powerpoint/moon.pdf · region (700 km deep) –tides 2) Vibrations from impacts 3) Thermal quakes from expansion of crust 4) Shallow

Lunar Libration

Page 57: The Moon - physics.udel.edujlp/classweb2/directory/powerpoint/moon.pdf · region (700 km deep) –tides 2) Vibrations from impacts 3) Thermal quakes from expansion of crust 4) Shallow

Evolution of Moon’s orbit◼ Tides

◼ Neither the moon or the earth is perfectly symmetric

◼ When formed, Earth/moon much closer together and rotated much faster◼ Moon 12,000-29,000 miles away

◼ Orbital period ~4hrs

◼ Earth’s day a few hours less (dinosaur day about 2 hrs shorter)

◼ Tides are transferring momentum from Earth to the moon

◼ Means – moon is moving further away from Earth (1.5 in/yr)

◼ Earth’s rotation period slowing about 0.002 s/century

◼ Final solution = ◼ Orbital period and Earth’s day ~ 47 days.

◼ Moon’s distance 348,000 miles instead of 239,000

◼ 10s of billions of years

Page 58: The Moon - physics.udel.edujlp/classweb2/directory/powerpoint/moon.pdf · region (700 km deep) –tides 2) Vibrations from impacts 3) Thermal quakes from expansion of crust 4) Shallow

Formation

◼ Fission Hypothesis

◼ Capture

◼ Co-Formation

◼ Impact

Page 59: The Moon - physics.udel.edujlp/classweb2/directory/powerpoint/moon.pdf · region (700 km deep) –tides 2) Vibrations from impacts 3) Thermal quakes from expansion of crust 4) Shallow

Collision