ASTR Spring 2008 Joel E. Tohline, Alumni Professor 247 Nicholson Hall [Slides from Lecture30]
Chapter 11: Terrestrial Planets Mercury –Heavily cratered (like the Earth’s moon) –Some evidence of lava flows and shrinkage of the planet’s crust –Generally considered a “dead” planet Venus Mars
Chapter 11: Terrestrial Planets Mercury –Heavily cratered (like the Earth’s moon) –Some evidence of lava flows and shrinkage of the planet’s crust –Generally considered a “dead” planet Venus Mars
Chapter 11: Terrestrial Planets Mercury –Heavily cratered (like the Earth’s moon) –Some evidence of lava flows and shrinkage of the planet’s crust –Generally considered a “dead” planet Venus Mars
Chapter 11: Terrestrial Planets Mercury –Heavily cratered (like the Earth’s moon) –Some evidence of lava flows and shrinkage of the planet’s crust –Generally considered a “dead” planet Venus Mars
Chapter 11: Terrestrial Planets Venus –Rotating very slowly…and backwards! –Atmosphere: Dense, hot, and corrosive! –Properties of atmosphere due to runaway “greenhouse” effect Venus Mars
Venus: Image of the surface of Venus obtained by radar imaging.
Venus: topographic map
Chapter 11: Terrestrial Planets Venus –Rotating very slowly…and backwards! –Atmosphere: Dense, hot, and corrosive! –Properties of atmosphere due to runaway “greenhouse” effect Venus Mars
Chapter 11: Terrestrial Planets Venus –Rotating very slowly…and backwards! –Atmosphere: Dense, hot, and corrosive! –Properties of atmosphere due to runaway “greenhouse” effect Venus Mars
Atmospheres of Earth & Venus
Venus: Ultraviolet image of Venus highlighting the Cloud layer structure.
Chapter 11: Terrestrial Planets Venus –Rotating very slowly…and backwards! –Atmosphere: Dense, hot, and corrosive! –Properties of atmosphere due to runaway “greenhouse” effect Venus Mars
Chapter 11: Terrestrial Planets Mars –Surface imaged by spacecraft extremely well –Surface explored by spacecraft that have successfully soft-landed on surface Viking Lander (VL1 & VL2) Mars Pathfinder (MP) Exploration Rovers (Opportunity & Spirit) –Evidence for (subsurface) water
Chapter 11: Terrestrial Planets Mars –Surface imaged by spacecraft extremely well –Surface explored by spacecraft that have successfully soft-landed on surface Viking Lander (VL1 & VL2) Mars Pathfinder (MP) Exploration Rovers (Opportunity & Spirit) –Evidence for (subsurface) water
Mars: topographic map
Chapter 11: Terrestrial Planets Mars –Surface imaged by spacecraft extremely well –Surface explored by spacecraft that have successfully soft-landed on surface Viking Lander (VL1 & VL2) Mars Pathfinder (MP) Exploration Rovers (Opportunity & Spirit) –Evidence for (subsurface) water
Chapter 11: Terrestrial Planets Mars –Surface imaged by spacecraft extremely well –Surface explored by spacecraft that have successfully soft-landed on surface Viking Lander (VL1 & VL2) Mars Pathfinder (MP) Exploration Rovers (Opportunity & Spirit) –Evidence for (subsurface) water
Mars: topographic map
Chapter 11: Terrestrial Planets Mars –Surface imaged by spacecraft extremely well –Surface explored by spacecraft that have successfully soft-landed on surface Viking Lander (VL1 & VL2) Mars Pathfinder (MP) Exploration Rovers (Opportunity & Spirit) –Evidence for (subsurface) water
Mars: topographic map
Chapter 11: Terrestrial Planets Mars –Surface imaged by spacecraft extremely well –Surface explored by spacecraft that have successfully soft-landed on surface Viking Lander (VL1 & VL2) Mars Pathfinder (MP) Exploration Rovers (Opportunity & Spirit) –Evidence for (subsurface) water
Mars: topographic map
Rover ‘Opportunity’: Landing Site
Rover ‘Opportunity’: Four+ years of travel
Rover ‘Opportunity’: View from edge of Victoria Crater
Chapter 11: Terrestrial Planets Mars –Surface imaged by spacecraft extremely well –Surface explored by spacecraft that have successfully soft-landed on surface Viking Lander (VL1 & VL2) Mars Pathfinder (MP) Exploration Rovers (Opportunity & Spirit) –Evidence for (subsurface) water