9terrestrial3s
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Transcript 9terrestrial3s
The Terrestrial Planets
Astronomy 311
Professor Lee Carkner
Lecture 9
Early Missions to the Inner Planets
1962 -- Mariner 2
Venus Fly-by
1964 -- Mariner 4
Mars Fly-by
1970 Venera 7
Venus lander
1973 Mariner 10
Venus/Mercury Fly-by
1975 Viking 1 and 2
Mars lander
Planetary Probes
Large number of missions from 1960-1978
Almost all planetary missions from the US
or the USSR
Future missions may be more multinational
US and Soviet Planetary
Missions
Very large number of Soviet missions, most were
failures
Venus:
Most notable success was the Venus Venera landers
Mars:
Smaller number of US missions, but higher
success rate
Mercury:
Venus:
Mars:
Sources of Information for the
Inner Planets
Mercury:
Mariner 10 --
Venus:
Soviet Venera landers -Magellan --
Mars:
Viking, Pathfinder, Spirit, Opportunity -Viking, Global Surveyor, Odyssey --
Inner Planet Facts
Mercury
Diameter: 0.38
Mass: 0.06
Venus
Diameter: 0.95
Mass: 0.82
Earth
Diameter: 1
Mass: 1
Mars
Diameter: 0.53
Mass: 0.11
Determining Planetary
Properties
Mass
Distance
Diameter
Determining Planetary
Properties (cont.)
Average Density
Atmospheric composition
The Planets That Weren’t
There should have been 2 other inner
planets
The Moon Impactor
The Asteroid Belt
The Moon and the Earth
The Moon
The Moon
First visited in 1959 by Luna 1 (USSR)
Moon facts
Diameter: 0.27
Mass: 0.01
Orbital Radius (from Earth): 0.003
Moons of the Inner Planets
Venus and Mercury have no moons
Earth has one large moon
Mars has two moons, Phobos and Deimos
Inner planets may be too small to capture
moons easily
Asteroids
Millions of small bodies orbit the Sun,
most between Mars and Jupiter (the
asteroid belt)
Meteors
Spacecraft
Asteroid Facts
Asteroids
Diameter: <0.14
Mass: <0.02
Orbital Radius: 2.8
Most have orbits within the asteroid
belt (~2-3.5 AU)
The Asteroid Gaspra
Sizes of the Inner Planets
Sizes relative to Earth
Earth:
Venus:
Mars:
Mercury:
Moon:
Asteroid:
All are small compared to the gas giants
(Neptune is ~4 times the diameter of the
Earth and ~64 times the volume)
Composition
All of the inner planets have about the same
density (~5000 kg/m3)
What makes up the difference?
“Rocky” planets could also be called the “metal”
planets
Composition (cont.)
Earthquake studies indicate that the
Earth has a iron core
We believe that the other inner planets
have a similar structure
Interior Structure
Atmospheres
Asteroids, Moon, Mercury -- no atmosphere
Mars
Composition = 95 % CO2, 3 % N (also water
vapor, oxygen)
Venus:
Composition = 96 % CO2, 4 % N (also sulfur
compounds such as sulfuric acid, H2SO4)
Atmospheres (cont.)
Earth:
Composition = 77 % N, 21 % O2 (also
water vapor, CO2, trace elements)
Why are the atmospheres of Venus,
Mars and the Earth so different?
The Carbonate-Silicate Cycle
Atmosphere
Water
+
CO2
(rain)
CO2
Volcano
CO2
+ silicate
(subvective
melting)
Ocean
Carbonate + silicate
(Sea floor rock)
Carbonate
+ water
(stream)
CO2 and Greenhouse Effect
Water washes CO2 out of atmosphere
where it is eventually deposited as rock
CO2 is a greenhouse gas
Carbonate-Silicate Feedback
Hot
cools off
Cool
heats up
CO2 and the Inner Planets
Venus:
nearer the Sun so it is hotter
no way to get CO2 out of atmosphere
Mars:
no way to get CO2 out of rocks
Earth:
Carbonate-silicate cycle
Summary
Inner or Terrestrial region
4 planets (Mercury, Venus, Earth, Mars)
1 large moon (The Moon)
thousands of asteroids
Information from 30 years of space
missions
Size
Earth and Venus about the same
Mars, Mercury, the Moon, 1/2 -1/4 size of
the Earth
Asteroids few km
Summary (cont.)
Composition
silicate rock crust
iron-silicate mantle
iron core
each planet has different proportions of each
Atmosphere
Mercury, Moon, asteroids -- none
Venus -- no water means CO2 is in atmosphere
Mars -- no plate tectonics means CO2 is in
rocks
Earth -- carbonate-silicate cycle balances
greenhouse effect