venus and mercury

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Venus and Mercury

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Venus and Mercury. The Inner Planets. 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). - PowerPoint PPT Presentation

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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?

Page 5: Venus and Mercury

Venus from Pioneer Venus Orbiter

Page 6: Venus and Mercury

Polar View of Venus

Page 7: Venus and Mercury

Topography of Venus

Page 8: Venus and Mercury

Earth Elevations

Page 9: Venus and Mercury

Radar Map of Venus

Page 10: Venus and Mercury

Radar Map of Venus

Page 11: Venus and Mercury

Surface of Venus

Page 12: Venus and Mercury

Venus has

Craters

Page 13: Venus and Mercury

Venus is Volcanic

Page 14: Venus and Mercury

“Pancake” Volcanoes

Page 16: Venus and Mercury

Coronas

Page 17: Venus and Mercury

How Coronas Form?

Page 18: Venus and Mercury

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

Page 19: Venus and Mercury

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.

Page 20: Venus and Mercury

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

Page 22: Venus and Mercury

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.

Page 23: Venus and Mercury

Venus and Earth

Page 24: Venus and Mercury

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

Page 26: Venus and Mercury

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

Page 28: Venus and Mercury

Mercury has Craters

• Not as dense as on Moon

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

Page 29: Venus and Mercury

Mercury has a huge

impact basin, the

Caloris Basin

Page 30: Venus and Mercury

Because of Mercury’s locked rotation, it has two

“hot poles”

Page 31: Venus and Mercury

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

Page 32: Venus and Mercury

Mercury’s ice seems to be hiding in polar craters

Page 33: Venus and Mercury

We’re B-a-a-ck

Page 34: Venus and Mercury
Page 35: Venus and Mercury

“Spider” Crater

Page 36: Venus and Mercury

Caloris Basin

Page 37: Venus and Mercury

Volcano on Mercury