Terrestrial

Announcements: 

Announcements Homework 6 due Monday First project due in one week! Last chance to check solutions to first test (near south door of SL building)

The Terrestrial Planets: 

The Terrestrial Planets 6 October 2006

Today:: 

Today: Tour of the inner solar system: Mercury, Venus, Earth, Earth’s moon, and Mars Sizes, masses, geology, atmospheres, temperatures, life

The planets, to scale: 

The planets, to scale

The Inner Solar System: 

The Inner Solar System Mercury Venus Earth Mars Sun On this scale: 1 A.U. = 120 pixels Diam. of Sun = 1 pixel Diam. of moon’s orbit = 1/2 pixel Diam. of earth = 1/100 pixel

Mercury: 

Mercury About 1/3 earth’s diameter 1/20 earth’s mass Visited by robotic spacecraft Mariner 10 (3 flybys), 1974 Another probe, Messenger, is on its way (launched 2004, will fly by in 2008, orbit in 2011) Cratered surface, like our moon Negligible atmosphere 700 K on sunny side

Venus: 

Venus 95% earth’s diameter 81% earth’s mass Covered by opaque clouds, dense atmosphere Radar maps show rolling hills, volcanoes 750 K average surface temperature(!) Visited by several robotic spacecraft: successful Soviet landings 1975-82; US orbiting probe mapped surface with radar in early 1990’s.

Venus: 

Venus

Venus’s Atmosphere: 

Venus’s Atmosphere 90 times the pressure of earth’s! 96% carbon dioxide; rest is mostly nitrogen Clouds are sulfuric acid (yum!) Carbon dioxide traps the sun’s heat: “greenhouse effect”

Earth: 

Earth My favorite planet Largest known rock Very geologically active Atmosphere of nitrogen and oxygen 3/4 covered with water Nice, comfortable surface temperature Only known home of life

Earth’s Moon: 

Earth’s Moon 1/4 earth’s diameter 1/80 earth’s mass Covered with craters, ancient lava flows Geologically inactive No atmosphere Essentially no water Hot days, cold nights Only other world humans have visited (1969-72)

Apollo Moon Landings: 

Apollo Moon Landings

Mars: 

Mars 1/2 earth’s diameter 1/10 earth’s mass Volcanoes, canyons, ice caps Very thin atmosphere of carbon dioxide No liquid water on surface Mostly frigid (200 K), but occasionally warm (290 K) Two tiny moons (20 km diameter)

Mars topography and geology: 

Mars topography and geology Some craters Huge volcanoes, apparently extinct Canyons, channels (from past water?)

Mars landings: 

Mars landings 2 Viking landers, 1976 Pathfinder/Sojourner, 1997 Spirit & Opportunity, 2004 (and still working!)

Life on Mars?Allen Hills Meteorite, found in Antarctica 1984Big news story 1996: 

Life on Mars? Allen Hills Meteorite, found in Antarctica 1984 Big news story 1996 Definitely from Mars: trapped gases match Mars atmosphere. Ejected by meteor impact 15 million years ago, landed in Antarctica 13,000 years ago. Contains carbon globules, magnetite, bacteria-like structures. Signs of life on Mars? Most scientists doubt it. But: Mars was definitely warmer and wetter in the past…

Mars mythology: 

Mars mythology

Mars misconceptions: 

Mars misconceptions "Mars is essentially in the same orbit... Mars is somewhat the same distance from the Sun, which is very important. We have seen pictures where there are canals, we believe, and water. If there is water, that means there is oxygen. If oxygen, that means we can breathe." -- Vice President Dan Quayle, 8/11/89

Mars mania: 

Mars mania “There are some nuts (and I mean that in the nicest possible way!) who REALLY, REALLY, REALLY want to go to Mars. I mean REALLY. You can find out about them at, for example, The Mars Society . They even have a station in the Utah desert! Crazy nuts. I love them. We'd never get anything done if it wasn't for nutty nuts!” -- Dr. Stacy Palen

The Terrestrial Planets: 

The Terrestrial Planets