Terrestrial Planets: Mercury, Venus, Earth, Mars

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14 Terms

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Mercury

  • Closest to Sun (0.38 AU), orbits in 88 days

  • No moons!

  • Moon-like, no atmosphere

  • lots of craters from impacts

  • Slow rotation - 59 days

  • no delay temp change, equator temperature day/night

  • Absurdly large metal core

  • 80% planet radius!

  • low mass, surface gravity 38% earth’s

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Venus

  • Closer to Sun (0.72 AU), 224 day orbits

  • Rotates slower than Mercury (243 days) and slower than orbits, also opposite direction

  • No moons!

  • Sometimes called “Earth’s sister”

  • similar size, density, gravity, has atmosphere, clouds

  • hottest surface, very strong greenhouse effect

  • thick atmosphere carbon dioxide, like being 1km (3000ft) under the ocean

  • Very young surface: 300-500 million years

  • Probably active volcanoes still!

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Earth

  • Largest terrestrial planet

  • Wet! 70% surface covered in water

  • only planet with surface liquid, active chemistry, life

  • Most geologically active planet

  • surface <1 billion years old, constantly renewed

  • plate tectonics, volcanism, erosion, weathering

  • large elevation map, age of continental plates and age of ocean plates

  • record of ancient impacts almost entirely erased, heat map of every meteorite strike ever

  • Thick atmosphere, nitrogen and some oxygen

  • protects surface from high energy light

  • Strong global magnetic field

- protects atmosphere, sometimes changes polarity

  • Absurdly large natural satellite, our moon

  • ¼ size of earth, ½ size of mars

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Mars

  • Farthest terrestrial from Sun (1.5 AU)

  • Two tiny asteroids moons

  • Small with surface gravity 38% Earth’s, but record for largest volcano and canyon

  • Geologically inactive, but similar to Earth

- similar day, axial tilt and seasons

- ice caps, clouds, dust storms, dust devils

  • Thin atmosphere, carbon dioxide

  • Wet past!

- active volcanoes in the past!

- water hiding beneath the surface, under ice caps of dry ice

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Terrestrials cool from 

Formation

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Terrestrials heat from

radioactive decay

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Earth and Venus

Lots of internal energy

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Mars and Mercury 

cooled off

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Magnetic fields

  • Earth’s is strong (liquid core + rotation)

  • Mars doesn’t have one (not enough core liquid)

  • Mercury’s very weak (partially melted by heat crystallization, Earth’s solid core already crystallized)

  • Venus doesn’t have one (slow rotator)

  • Atmosphere bound by gravity, replenished by volcanoes, but magnetic field helps protect

  • particles from solar wind of sun, also explosions on surface of Sun (CME’s)

  • high-speed charged particles from supernova in galaxy

  • magnetic field funnels particles to poles, where slam into atmosphere, excite gas, cause aurora

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Atmospheres

  • Composition

  • Venus and Mars: carbon dioxide

- gasses from volcanoes

  • Earth: 70% nitrogen, 28% oxygen

- changed over time

- carbon dioxide locked up (plate tectonics) nitrogen built up

- algae “polluted” with oxygen, almost caused own extinction

  • Different thickness due to gravity, surface temp, volcanic activity

- Earth: 14.6 pounds per square inch

- Venus: 92xEarth’s

- didn’t lock any up in rocks, has gravity to hold onto it all

- Mars: 1/1000 x Earth’s

- too low gravity, losing atmo

- Mercury: none

- too low gravity, surface too hot!

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Greenhouse effect

  • Good: Earth is warmer by 30k (50 degrees F) than expected temp

  • Bad: Venus is blistering 737K (867 degrees F), hotter than Mercury

  • Surface temp is balance incoming and outgoing energy

- incoming sunlight adds energy, heats surface (also heat from still cooling)

- planet loses energy by emitting infrared (nothing to do with volcanoes!)

  • Greenhouse gases (ggs) delay escape of infrared light, insulation blanket holds onto thermal energy longer

- Earth natural balance of carbon dioxide, methane, water in atmosphere

- released from volcanoes, decay of dead things

- trapped in oceans, rock, living plants, frozen tundra

  • Change ggs, change balance

- Venus closer to Sun, oceans evaporated, active volcanoes = thick ggs

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Seasons

  • Change in sunlight from tilted rotation axis

- summer warmer, winter cooler regardless of atmosphere composition or surface feature

  • Mercury: axis perpendicular = no seasons

  • Venus: axis perpendicular = no seasons

- also, very little sunlight reaches surface

  • Earth (23.5 degrees) and Mars (25 degrees) tilted = seasons

- Mars winter: 25% atmosphere condenses onto polar ice cap, air pressure plummets

- Mars spring/summer: dust storms, can grow to cover entire planet

  • Mars orbit more eccentric, unequal length seasons compared to Earth

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Impacts

  • Some refresh surface, hide impacts

- Venus paved over by volcanoes

- Earth’s renewed by active geology

  • Early solar system full of debris, cleared out when hit objects

  • Fewer impacts now, but still happen

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Liquid water

  • Water delivered to every planet by comet, asteroid impacts

  • Earth is liquid water king!

  • Mercury too close to sun, too small

- ice hiding in deep polar craters, permanent shadow keeps it very, very cold

  • Venus too hot, lost its water

- didn’t lock up carbon dioxide, runaway Green house effect

- if ocean, eventually water evaporated into atmosphere

- broken down by sunlight (into hydrogen, oxygen), leaked into space

- maybe viable for few billion years

  • Mars too cold now, but water in the past

- when volcanoes still active, Mars had thicker warmer atmosphere

- planet cooled, volcanoes and magnetic field died

- solar wind stripped atmosphere, water evaporated, leaked into space

- planet died after 1 billion years, became cold dry dessert