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Page 1: Venus and Mercury

Venus and Mercury

Page 2: Venus and Mercury

The Inner Planets

Page 3: Venus and Mercury

Venus• Only a bit smaller than Earth

• Nearest planet (26 million miles)

• Shows phases as it orbits the Sun

• Most circular orbit

• Atmosphere mostly Carbon Dioxide– 90 times as dense as Earth– Runaway Greenhouse Effect– Surface Temperature 450 C (850 F)

Page 4: Venus and Mercury

Venus’ Odd Rotation• Venus Rotates in 243 days relative to the stars• Longer than its year (225 days)• Solar Day = 117 days• You can jog as fast as Venus rotates• Opposite to all other planets’ rotation

(retrograde)• Why?

– Mega-Impact?– Tidal Effects?– Possible tidal lock on Earth?

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Venus from Pioneer Venus Orbiter

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Polar View of Venus

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Topography of Venus

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Earth Elevations

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Radar Map of Venus

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Radar Map of Venus

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Surface of Venus

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Venus has

Craters

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Venus is Volcanic

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“Pancake” Volcanoes

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Coronas

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How Coronas Form?

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Venus Differs from Earth in One Important Way:

• Venus has no Plate Tectonics

• Earth’s internal heat causes hot material to rise within Earth and plates to move

• Venus’ crust is too rigid

• Heat builds up and escapes in planet-wide volcanic activity

• Last event about 600 million years ago

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Why Venus Has No Plate Tectonics

• It’s Hot! We’d expect hot rocks to be less rigid, not more!

• But it’s also dry! Dry rocks are ten times stronger at high temperatures than wet rocks.

• Earth is wet. That affects not just the outside, but the inside as well.

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Did Venus Once Have Oceans?

• Resurfacing means no visible trace of early history

• Deuterium: Ghost of a Vanished Ocean?– Deuterium is hydrogen with one neutron– Twice as heavy as normal hydrogen– Less likely to escape– D/H on Venus 100x that of Earth

• Photodissociation + Stripping– Venus lacks magnetic field

Page 21: Venus and Mercury

Venus and the Da Vinci Code• 13 Venus years = 13 x 224.7 = 2921.1 days

• 8 Earth Years = 8 x 365.25 = 2922 days

• 5 Synodic periods of Earth and Venus = 5 x 583.9 = 2919.5 days

• 1/5 of a circle = 72 degrees

• In 583.9 days, Earth moves 360 + 215.5 degrees (almost 360 + 3 x 72)

• In 583.9 days, Venus moves 720 + 215.5 degrees

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Venus and Earth

• 13 Venus years = 13 x 224.7 = 2921.1 days

• 8 Earth Years = 8 x 365.25 = 2922 days

• 5 Synodic periods of Earth and Venus = 5 x 583.9 = 2919.5 days

• 12 Venus rotations = 2916 days

• Venus shows nearly the same face to Earth every 584 days.

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Venus and Earth

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Mercury• Closest planet to Sun

• Very elliptical orbit (e = .205)

• Only 3000 miles (5000 km) in diameter

• Rotation locked to Sun: 3 rotations in 2 orbits (58 days)

• Moon-like on the outside (craters)

• Earth-like on the inside (dense core, magnetic field)

Page 25: Venus and Mercury

Mercury’s Rotation

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Mercury’s Interior

• Density = 5.43 (Earth = 5.5)

• Much smaller than Earth, less pressure inside

• Core about 2/3 of Mercury’s diameter (Earth = ½)

• Mega-Impact may have blown away silicate outer part

Page 27: Venus and Mercury

Mercury from Mariner

10, 1973

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Mercury has Craters

• Not as dense as on Moon

• Most of Mercury covered with lava plains (intercrater plains)

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Mercury has a huge

impact basin, the

Caloris Basin

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Because of Mercury’s locked rotation, it has two

“hot poles”

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And Mercury has the last thing you’d expect to find: ice caps

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Mercury’s ice seems to be hiding in polar craters

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We’re B-a-a-ck

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Page 35: Venus and Mercury

“Spider” Crater

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Caloris Basin

Page 37: Venus and Mercury

Volcano on Mercury


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