PPT-Martian Meteorites

Author : liane-varnes | Published Date : 2017-05-16

Leah Salditch February 27 2017 Mars Final Project 3 main types of meteorites Iron StonyIron Pallasite Mesosiderite Stony Chondrites Achondrites Pallasite Achondrites

Presentation Embed Code

Download Presentation

Download Presentation The PPT/PDF document "Martian Meteorites" is the property of its rightful owner. Permission is granted to download and print the materials on this website for personal, non-commercial use only, and to display it on your personal computer provided you do not modify the materials and that you retain all copyright notices contained in the materials. By downloading content from our website, you accept the terms of this agreement.

Martian Meteorites: Transcript


Leah Salditch February 27 2017 Mars Final Project 3 main types of meteorites Iron StonyIron Pallasite Mesosiderite Stony Chondrites Achondrites Pallasite Achondrites Basaltic Common comprise 5 of all meteorite findings . Martian Terraforming 2For the past several decades, scientists have worked to develop a plan for terraforming (i.e. making more like Earth) other planetary bodies within our solar system. Mar Unit 4. Appearances of comet Kohoutek (1973), Halley (1986), and Hale-Bopp (1997) caused great concern among superstitious.. Comet Hyakutake in 1996. Throughout history, comets have been considered as portents of doom, even very recently: . About Ray Bradbury. Born in 1920 and died in 2012. Lived the early years of his life in Waukegan, Illinois. This had a large influence on his settings in later works, many of which have a small town setting in them.. Meteorites hit the atmosphere with speeds from 12 to 72 km/. s. .. Earth’s orbital speed is 30 km/. s. and the escape speed from the solar system at the Earth is 42 km/. s. Q: draw a diagram and use it to show why the maximum speed is 72 km/. Compiled by David Beaty, Lars Borg, David Draper, Walter Kiefer, Jim Papike, Kevin Righter, Chip Shearer, Sue Smrekar, Jeff Taylor . Correspondence author: Dave Beaty . (JPL/Caltech), . David.W.Beaty@jpl.nasa.gov. Preliminary Summary of Strategic Knowledge Gaps . P-SAG (jointly sponsored by MEPAG and SBAG). May 1, 2012. Strategic Knowledge Gaps. 2. The Gap in Knowledge Needed to Achieve a Specific Goal . Knowledge we have. Compiled by David Beaty, Lars Borg, David Draper, Walter Kiefer, Jim Papike, Kevin Righter, Chip Shearer, Sue Smrekar, Jeff Taylor . Correspondence author: Dave Beaty . (JPL/Caltech), . David.W.Beaty@jpl.nasa.gov. Introduction to methods. Identification and classification. EL YAZIDI . Mayssa. . Le 31/03/2016 – . Kélibia. . Plan . Introduction. Terminology. Origin. Identification . criteria. Classification. Solanum lycopersicum. Seed Germination in Microgravity. . Sabrina Benitez (Co-Principal Investigator). Juan Pablo Flanagan (Co-Principal Investigator). Sofia Escobar (Co-Principal Investigator). Laura Nikstad (Teacher Facilitator) . Martian geology: a rapid summary. Mars is geologically distinctive at the large scale. The southern hemisphere is made of ancient cratered terrain and the northern hemisphere flat, more recent (less impacted) terrain that is at lower elevation. This distinctive geology is called the . Jacob Bleacher. Goddard Space Flight Center. 3. rd. Affordable Mars Workshop. Dec. 2, 2015. Geologic field work can be loosely defined as the body of work necessary to:. Determine the spatial distribution, age and attitude of the rock types within an area. Apostolos Christou. Armagh Observatory and Planetarium. Northern Ireland, UK. DPS . 49 ● . Provo, Utah. ● . Oct 18, 2017. Email: . aac@arm.ac.uk. ● . Population control of Martian Trojans. Small Solar System Bodies. Did you find a meteorite?. Credit: Public domain. Did you find a curious looking rock? With the help of these instructions you can investigate . if it could be a meteorite.. View of gullies along the rim and relative sea level lower on the wall of . Krupac. crater on Mars. Credit: NASA/JPL/. UArizona. .. What is the science question?. . Different theories have been proposed for landslides and seasonal flows of material on the Martian surface, but none completely explain these intriguing features. Chloride (Cl) salts and melting ice have been considered previously, but those scenarios were not fully consistent with Martian environments..

Download Document

Here is the link to download the presentation.
"Martian Meteorites"The content belongs to its owner. You may download and print it for personal use, without modification, and keep all copyright notices. By downloading, you agree to these terms.

Related Documents