PDF-All about craters

EXPLORING OUR PASTSECURING OUR FUTURE All About Craters For Team Members The goal of this acx00740069vity is to provide team members with a 2045 minute acx00740069vity to do in a formal schoo. Background also see Teachers Guide Pages 1 2 photo on 8 12 and photo on 13 The circular features so obvious on the Moons surface are impact craters formed when impactors smashed into the surface The explosion and excavation of materials at the impac Nadine G. Barlow. Dept. Physics and Astronomy. Northern Arizona University. Flagstaff, AZ 86011-6010. Nadine.Barlow@nau.edu. Office: 928-523-5452 Cell: 928-600-9253. Co-authors: Joseph M. Boyce (U. HI) and Lionel Wilson (Lancaster U.). Francis Nimmo. Last Week - Volcanism. How and why are melts generated?. Increase in mantle potential temperature; or. Reduction in solidus temperature (e.g. water); or. Thinning of the lithosphere. How do melts ascend towards the surface?. Characterizing LROC NAC Images. Created by: . Belfry High School. Participants. Taylor Runyon. Mickayla Walters. Sarah Compton. Staci Coleman. Brianna Sullivan. Our Purpose. Our purpose of doing this project is to understand morphology and the composition of the Tycho . March 11, 2014. Earth 438. Rampart Craters: A Case for Water on Mars. Outline. What. What is a Rampart Crater?. Cratering Mechanics and . Types. Why. Rampart Crater Formation Theory. Where. Rampart Craters on Mars. Geoffrey George, Charles Gutierrez Miguel . Nze. , Matt Malacara, Brandon Rangel, Juan . Urquidi. , Alex Valdez. Robert E. Lee High School/S.T.E.M. RAM Academy. San Antonio, Texas. Project Selection. Test . 2. : Passage 1. Passage 1. Unmanned spacecraft taking images of Jupiter's moon Europa have found its surface to be very smooth with few meteorite craters. Europa's surface ice shows evidence of being continually . Houle. 11:00 E. 10:00 C. Red. RB. Bank. High. School. Lunar-tics!. Scientific Research. Southeastern Imbrium Crater Age Dating and Ejecting Data. March 30, 2011. . Objectives Covered. What we covered for Phase II. Marta Lúthien Gutiérrez Albarrán, 2014. Venus:. Topography. Radar mapping (. Magellan. ). . Venus’s atmosphere in UV (. Pioneer-12. ) and radar mapping (. Magellan. ). Venus:. Surface features. Lunar Concentric Craters?. Doughnut-shaped concentric . ridges inside small lunar craters . (<15 km diameters) may . have formed when intrusion of magma caused uplift of the crater floor.. 11.5-km-diameter unnamed concentric crater. Prentice Hall Earth Science. 22.3 Objectives. Describe . how the physical features of the lunar surface were created. Explain . the history of the moon . 22.3 Vocabulary. crater. ray. mare. rille. lunar regolith. Prentice Hall Earth Science. 22.3 Objectives. Describe . how the physical features of the lunar surface were created. Explain . the history of the moon . 22.3 Vocabulary. crater. ray. mare. rille. lunar regolith. Formation of the Moon Before visit to the Observatory Overview Introduction to the Formation of the Moon Video about the Evolution of the Moon Classroom demonstrations on distances to the Moon Classroom activity – Craters on the Moon What Are The Type s of Volcanoes ? kinds of volcanoes to see. Laidlaw Volcano and Pillar Butte are Shield Volcanoes that form when liquid rock oozes and flows out of a central vent. Pilot Butte