GEOL3045: Planetary Geology Lysa Chizmadia Venus From Mariner to Venera to Venus Express Introduction Second planet from the Sun Distance = 1.1 x 108 km 0.72 AU Diameter = 1.2 x 104 km Mass = 4.9 x 1023 kg Very circular orbit Eccentricity < 1% Aphelion: 1.09 x 108 km Perihelion: 1.07 x 108 km Retrograde rotation From east to west Venusian day = 243 days Venusian year = 225 days Image from: http://www.nineplanets.org/venus.html Shows phases Supported Copernicus’ heliocentric theory Mean surfaces temperature = 462C ~isothermal Hotter than Mercury Earth’s Twin Planet Similar sizes: 1.2 x 104 km (95% of ) = 1.3 x 104 km Similar masses: Relative sizes of the terrestrial planets 4.9 x 1023 kg (80% of ) = 6.0 X 1024 kg Similar densities 5.25 g/cm3 vs. 5.52 g/cm3 vs. Similar bulk compositions Young surfaces Recent geologic activity Including volcanism & weathering Rare impact crater on Venus Images from: http://en.wikipedia.org/wiki/Venus Venusian Geography Highlands (~ continents) Ishtar Terra ~ size of Australia Northern hemisphere Interior high plateau: Lakshmi Planum Surrounding by highest mountains Maxwell Montes Map of Venus, higher elevations in reds & yellows Image from: http://en.wikipedia.org/wiki/Venus Highest mts have high albedo substance Speculation: Te & PbS Aphrodite Terra ~ size of S. America Equator Broad depressions (~ ocean basins) Atalanta Planitia Guinevere Planitia Lavinia Planitia Magellan radar map (false color) Image from: http://www.nineplanets.org/venus.html Venusian Atmosphere Densest of all terrestrial planets 96.5% CO2 & 3.4% N2 90-92 times thicker than Greenhouse effect Responsible for high Ts Receives 25% of sunlight as Mercury Venus in visible light Clouds of CO2 & H2SO4 Atm contains 0.015% SO2 Has intermittent lightning Indicates weathering Venus Express 2005-2009 Studying atmosphere Venus in UV light Images from: http://en.wikipedia.org/wiki/Venus Venusian Volcanism Magellan’s radar showed much of Venus is covered in lava flows Several shield volcanoes Sif Mons E.g. Sif Mons & Sapas Mons >152 volcanic domes Flat-top domes called pancake domes Consistent w/ viscous lavas Radial lava flows Sapas Mons High silica lavas? Pancake volcanoes in Alpha Regio region Images from: http://www.geology.sdsu.edu/how_volcanoes_work/venus.html Coronae & Arachnoids Coronae Circular raised structures surrounded by ridges & grooves & radial lines Seem to be collapsed domes over large magma chambers Pandora Coronae Image from: http://www.nineplanets.org/venus.html E.g. Crater Lake Arachnoids Ovoid features w/ concentric rings & complex fracture networks Similar but smaller than coronae Possibly precursor to coronae Ba’het Coronae Arachnoids Images from: http://www.geology.sdsu.edu/how_volcanoes_work/venus.html Prominent U.S. Satellites Mariner 2: First satellite to visit Venus Flyby in December 1962 Discovered Venus is very hot (~800C) w/ dense CO2-rich atmosphere Pioneer Venus in 1978 Orbiter & 4 atmospheric probes Made 1st high quality map of Venus Magellan in 1989 Mapped 98% of surface Gravity field map for 95% of surface Venera 7, 9 & 10 Venera 7 in 1970 1st probe to return surface data from another planet Venera 9 & 10 in 1975 1st spaceship to land on another planet Clouds 30-40 km thick Pressure 90 atm Temperature 485C Windspeed 3.5 m/s Venusian surface from Venera 9 Image from: http://www.nineplanets.org/venus.html Venusian surface from Venera 9 & 10 Image from: http://en.wikipedia.org/wiki/Venera_10 Also Venera 11-16 Detected possible seismic activity Observed strong lightning Discovered pancake volcanoes, coronae & arachnoids Venusian surface from Venera 13 Image from: http://www.solarviews.com/eng/venus.htm Summary Earth’s twin in size & bulk composition Also, young surfaces Geologic activity & weathering Densest atmosphere for terrestrial planets ~90 times higher than Earth Greenhouse effect keeps T high & constant Lightning & “snow” indicate weather Prominent features include Volcanoes (shield & pancake) Coronae (magma rising) Arachnoids (collapsed volcanoes)