PPT-Mars
Author : mitsue-stanley | Published Date : 2017-04-06
and Curiosity Rover Metka Batič Mars Red planet iron oxide Thin atmosphere Large temperature changes No magnet field radiation 2 Moons Phobos Deimos
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Mars: Transcript
and Curiosity Rover Metka Batič Mars Red planet iron oxide Thin atmosphere Large temperature changes No magnet field radiation 2 Moons Phobos Deimos. Mars is the only planet in our solar system to have frozen carbon dioxide snow it happens all year round. . in the north end.. . pictures from the mars curiosity shows landscapes made by bodies of water, rain and ancient rivers with the force of 10,000 Mississippi rivers.. Keith Piersol. Geochemistry. Article. Article is “Making a splash on MARS” by Charles W. Petit.. Published July 2005 in National Geographic, volume 208.. Goes over the discoveries of the Spirit and Opportunity landers.. By: Kaleb Robertson. 8. . successfully landed . M. ars Rovers/Landers. May 1971:. . Mars . 3 successfully lands on mars but has a malfunction and loses connection seconds later.. Aug.–Sept. 1975: . Flight into Valles Marineris. Geological Processes. Chaotic Terrain. Forms when subsurface water or ice causes a loss of support and the ground collapses.. Graben. A depressed block of land bordered by parallel faults (graben is German for ditch).. Content. The Observation. Silver Market Long Term Cycles Since 1990. Mars Direct Stations and Silver Long Term Cycle Peaks /Troughs Since 1990. Conclusion and Forecast. Nice picture Ken!. Mars: The Planet of Fire (. Ester Aranzana. 13 de . Enero. de 2012. Introduction. Rock core (Fe-. FeS. ). No internal magnetic field, no dynamo action but. . it has one in the past. mini-magnetospheres of crustal origin . Observations. 10.1 Orbital Properties. 10.2 Physical Properties. 10.3 Long-Distance Observations of Mars. 10.4 The Martian Surface. 10.5 Water on Mars. Life on Mars?. 10.6 The Martian Atmosphere. 10.7 Martian Internal Structure. By. . Ej. Do you know Mars can. . spin.. Mars is -81 degrees F.. Mars is a . planit. far away from the sun. Mars has. Hard rocks.. Mars has heavy dust . stoms. . Mars has los of. Valcanose. .. With its next . lander. , NASA plans to discover what turned Mars from a warm, wet place to the cold, arid planet we see today.. Long ago, the Red Planet was very different from the frozen, barren desert we have seen on our TV screens courtesy of Pathfinder. . Advisory Group. Matt Wallace . Mars 2020 Deputy Project Manager. February 22, 2017. © 2016 California Institute of Technology. Government sponsorship acknowledged.. Project Overview. Salient Features. Science Team View at Workshop #3. February 8, 2017. Mars 2020. Landing Site Working Group. (LSWG). The Mars 2020 Landing Site Working Group (LSWG) was chartered to evaluate the eight sites selected as a result of the second site selection workshop in August, 2015 with respect to the scientific objectives of the mission.. Launch in July-August 2020 from Cape Canaveral Air Force Station, FloridaLaunching on a ULA Atlas 541 procured under NASAs Launch Services Programlled Jezero Craterexploring the landing sit cool surface features. Lets look at some!. (all images credit: Mike . Sussman. ). The famous “Face on Mars”. Now don’t get all excited…. How Come We Missed These?. Look harder!. The Panda!. George Washington Screaming!. Mars is the forth planet from the . sun. Mars has two moons in orbit. The names of the moons are called Phobos and Deimos. Mars is currently 218.27 million KMs from the sun. Mars’ diameter is 6,779kms.
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