11-2 Inner Planets.

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Presentation transcript:

11-2 Inner Planets

Terrestrial Planets Solid and rocky Metallic cores Planets closest to the Sun Impact craters

Mars 4th planet from the sun Probes sent to explore planet Polar ice caps Signs that once had liquid water

Year = 687 days Day = 24 hours 37 mins Volcanic activity Valleys eroded by water 2 Moons

Mars Red Planet – looks red due to iron oxide on surface

The Face on Mars

The Face on Mars Martian sculpture? New images show eroded raised surface

Volcanoes 100 larger than Earth’s Olympus Mons – 3 times larger than Everest No tectonic plates

Still active volcanoes? Marsquakes – Viking craft landed to detect

Water? Pressure and temperature too low for liquid water Icecaps and subsurface Rovers – Spirit and Opportunity Evidence for past liquid water

Earth 3rd planet from sun Water exists as a liquid, solid, and gas Atmosphere keeps UV rays out Only planet with life

Venus 2nd planet Greenhouse effect - Thick clouds trap heat Hotter than Mercury Rains sulfuric acid

Twinsies!

Year = 225 days Day = 244 days A day is longer than a year. 90 times the pressure of Earth 96% CO2 atmosphere Rotates east to west No Moons

Probes 1970’s – Soviet Union 1990’s – US Basalt and Granite Orbit for 4 years Radio waves of surface Crashed to collect atmospheric data

Magellan Mountains, volcanoes, lava plains, sand dunes Young craters Massive volcanic resurfacing

Mercury Closest to the sun Smooth plains and high cliffs Lots of craters on surface

Large cliffs – wrinkles when molten Year = 88days Day = 59 days No moons Large cliffs – wrinkles when molten 427 C -173 C Little to no atmosphere No wind