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Premium member Presentation Transcript The Red Planet: The Red PlanetRobotic Missions to Mars: Robotic Missions to MarsViking Lander: Viking LanderMartian landscape with frost: Martian landscape with frost“Face” on Mars ?: “Face” on Mars ?Mars – Vital Statistics: Mars – Vital Statistics Mass ~ 1/10 Earth’s Diameter = 4200 mi, ½ Earth’s Density = 3.9 x water Year = 1.9 Earth years Day = 24 hr 37 min Distance to Sun = 1.5 AU (227 million Kms) Surface gravity (g) = 0.38 Earth’s Tilt of rotation axis = 25 degrees (seasons!) Surface T: Max 70 F, but usually -100 to -220 F Large variations in T (thin atmosphere)Martian Gravity : Martian Gravity Although Mars almost certainly had a primordial atmosphere similar to Earth’s, most of it was lost primarily because of low gravity Gravitational acceleration g(Mars) = 0.38 g(E) M (Mars) ~ 1/10 M(E); R(Mars) ~ ½ R(E) g(Mars) = G M(Mars) / R(Mars)^2 g(Mars) / g(E) = (1/10) / (1/4) = 0.4 Objects on Mars fall 2 ½ times slower Mother of all canyons: Valles Marineris: Mother of all canyons: Valles Marineris 5000 Kms (coast-to-coast if in US)Polar “dry ice” caps (CO2): Polar “dry ice” caps (CO2) Polar icecaps are dry ice on top and water ice underneathPolar cap with dust lanes: Polar cap with dust lanesEvidence of ancient water flows on Mars : Evidence of ancient water flows on Mars “Canal” type features (dried up riverbeds); Martian climate was warm and wet in the past. Why did it change to the barren environment today ? The atmosphere evaporated ! Anti-greenhouse Effect !! Opposite of Venus !!!More evidence of water: More evidence of waterAncient volcanic flows: Ancient volcanic flows Recent volcanic activity (~ 100 million yrs) with huge runny lava flows (why?) Low gravity !Mother of all volcanoes: Olympus Mons: Mother of all volcanoes: Olympus Mons 24 Kms high (3 times Mt. Everest), 600 Kms across (as big as Missouri)Volcanic Plains – Giagantic Shield Volcanoes: Volcanic Plains – Giagantic Shield Volcanoes Summits capped with “Calderas” – flat, broad, collapsed craters“Mud-splash” crater: “Mud-splash” craterTopography: Warmer, Volcanic Northern Hemisphere and colder, cratered Southern Hemisphere: Topography: Warmer, Volcanic Northern Hemisphere and colder, cratered Southern HemisphereSome Basic Features of Mars: Some Basic Features of Mars First superior planet, best seen at opposition Most like Earth (season like on Earth, but twice as long) Eccentricity = 0.09, 3 times that of Earth’s orbit; Mars is 20% closer to the Sun at perihelion; receives 44% more sunlight Perihelion occurs during southern summers, which are shorter but hotter than northern summers, but southern winters are much longer; large variations in southern polar ice caps (may extend halfway to equator) North is warmer than the south !Recycling heavy compounds H2O and CO2 and the Greenhouse Effect: Recycling heavy compounds H2O and CO2 and the Greenhouse Effect H2O,N2 remain in the atmosphere; CO2 is recycled on earth via photosynthesis H2O breaks up from UV; H2,N2,O2 escape; CO2 freezes on Mars as permafrost, or on polar icecaps Martian atmosphere (0.007 bars) is 95% CO2 EARTH MARSOppositions of Mars (Best Viewing): Oppositions of Mars (Best Viewing) The best time to view a superior planet is at Opposition, whereas the best time to view an inferior planet is at maximum elongationOpposition and Retrograde motion: Opposition and Retrograde motionSteps to a Martian Dust Storm:: Steps to a Martian Dust Storm: Convection between night and day sides produces 50-200 MPH winds Dust blown into upper atmosphere (no rain to clear!) Sunlight blocked by dust upper air gets warmer, surface cooler “anti-greenhouse effect” Temperature difference makes convection worse, so more dust blown into atmosphere Nuclear Winter (nuclear war!) Extinction of Dinosaurs (asteroid impact!)Life on Mars: Life on Mars Viking Landers, Pathfinder, Rover and Spirit robotic missions TV Nothing big seen moving around (at least so far) No organic compounds (C,H,O molecules) found No micro-organisms found Biological tests by robotic experiments are sensitive enough to have detected life in AntarcticaTerra-forming: Terra-forming Altering a planet’s environment to create a climate simulating Earth’s Prescription for Mars: Melt polar CO2 to start greenhouse effect Raises the temperature so rest of ice melts Plant algae, etc. for photo-synthesis: CO2 O2 (Voila !) How does one start step 1? Small Moons of Mars: Small Moons of Mars Moons of Mars are about the size of Columbus I-270 beltway You do not have the permission to view this presentation. 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A161 13 Marietta1 Download Post to : URL : Related Presentations : Share Add to Flag Embed Email Send to Blogs and Networks Add to Channel Uploaded from authorPOINTLite Insert YouTube videos in PowerPont slides with aS Desktop Copy embed code: (To copy code, click on the text box) Embed: URL: Thumbnail: WordPress Embed Customize Embed The presentation is successfully added In Your Favorites. Views: 42 Category: Education License: All Rights Reserved Like it (0) Dislike it (0) Added: January 24, 2008 This Presentation is Public Favorites: 0 Presentation Description No description available. Comments Posting comment... Premium member Presentation Transcript The Red Planet: The Red PlanetRobotic Missions to Mars: Robotic Missions to MarsViking Lander: Viking LanderMartian landscape with frost: Martian landscape with frost“Face” on Mars ?: “Face” on Mars ?Mars – Vital Statistics: Mars – Vital Statistics Mass ~ 1/10 Earth’s Diameter = 4200 mi, ½ Earth’s Density = 3.9 x water Year = 1.9 Earth years Day = 24 hr 37 min Distance to Sun = 1.5 AU (227 million Kms) Surface gravity (g) = 0.38 Earth’s Tilt of rotation axis = 25 degrees (seasons!) Surface T: Max 70 F, but usually -100 to -220 F Large variations in T (thin atmosphere)Martian Gravity : Martian Gravity Although Mars almost certainly had a primordial atmosphere similar to Earth’s, most of it was lost primarily because of low gravity Gravitational acceleration g(Mars) = 0.38 g(E) M (Mars) ~ 1/10 M(E); R(Mars) ~ ½ R(E) g(Mars) = G M(Mars) / R(Mars)^2 g(Mars) / g(E) = (1/10) / (1/4) = 0.4 Objects on Mars fall 2 ½ times slower Mother of all canyons: Valles Marineris: Mother of all canyons: Valles Marineris 5000 Kms (coast-to-coast if in US)Polar “dry ice” caps (CO2): Polar “dry ice” caps (CO2) Polar icecaps are dry ice on top and water ice underneathPolar cap with dust lanes: Polar cap with dust lanesEvidence of ancient water flows on Mars : Evidence of ancient water flows on Mars “Canal” type features (dried up riverbeds); Martian climate was warm and wet in the past. Why did it change to the barren environment today ? The atmosphere evaporated ! Anti-greenhouse Effect !! Opposite of Venus !!!More evidence of water: More evidence of waterAncient volcanic flows: Ancient volcanic flows Recent volcanic activity (~ 100 million yrs) with huge runny lava flows (why?) Low gravity !Mother of all volcanoes: Olympus Mons: Mother of all volcanoes: Olympus Mons 24 Kms high (3 times Mt. Everest), 600 Kms across (as big as Missouri)Volcanic Plains – Giagantic Shield Volcanoes: Volcanic Plains – Giagantic Shield Volcanoes Summits capped with “Calderas” – flat, broad, collapsed craters“Mud-splash” crater: “Mud-splash” craterTopography: Warmer, Volcanic Northern Hemisphere and colder, cratered Southern Hemisphere: Topography: Warmer, Volcanic Northern Hemisphere and colder, cratered Southern HemisphereSome Basic Features of Mars: Some Basic Features of Mars First superior planet, best seen at opposition Most like Earth (season like on Earth, but twice as long) Eccentricity = 0.09, 3 times that of Earth’s orbit; Mars is 20% closer to the Sun at perihelion; receives 44% more sunlight Perihelion occurs during southern summers, which are shorter but hotter than northern summers, but southern winters are much longer; large variations in southern polar ice caps (may extend halfway to equator) North is warmer than the south !Recycling heavy compounds H2O and CO2 and the Greenhouse Effect: Recycling heavy compounds H2O and CO2 and the Greenhouse Effect H2O,N2 remain in the atmosphere; CO2 is recycled on earth via photosynthesis H2O breaks up from UV; H2,N2,O2 escape; CO2 freezes on Mars as permafrost, or on polar icecaps Martian atmosphere (0.007 bars) is 95% CO2 EARTH MARSOppositions of Mars (Best Viewing): Oppositions of Mars (Best Viewing) The best time to view a superior planet is at Opposition, whereas the best time to view an inferior planet is at maximum elongationOpposition and Retrograde motion: Opposition and Retrograde motionSteps to a Martian Dust Storm:: Steps to a Martian Dust Storm: Convection between night and day sides produces 50-200 MPH winds Dust blown into upper atmosphere (no rain to clear!) Sunlight blocked by dust upper air gets warmer, surface cooler “anti-greenhouse effect” Temperature difference makes convection worse, so more dust blown into atmosphere Nuclear Winter (nuclear war!) Extinction of Dinosaurs (asteroid impact!)Life on Mars: Life on Mars Viking Landers, Pathfinder, Rover and Spirit robotic missions TV Nothing big seen moving around (at least so far) No organic compounds (C,H,O molecules) found No micro-organisms found Biological tests by robotic experiments are sensitive enough to have detected life in AntarcticaTerra-forming: Terra-forming Altering a planet’s environment to create a climate simulating Earth’s Prescription for Mars: Melt polar CO2 to start greenhouse effect Raises the temperature so rest of ice melts Plant algae, etc. for photo-synthesis: CO2 O2 (Voila !) How does one start step 1? Small Moons of Mars: Small Moons of Mars Moons of Mars are about the size of Columbus I-270 beltway