PDF-affected; shallow “moon craters” are present

Author : tawny-fly | Published Date : 2017-01-25

Level 0 NO EROSION Level 1 MILD Level 2 MODERATE Deep 147moon craters148 or depressions are present and may coalesce Level 3 SEVERE Teeth are slick with little or

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affected; shallow “moon craters” are present: Transcript

Level 0 NO EROSION Level 1 MILD Level 2 MODERATE Deep 147moon craters148 or depressions are present and may coalesce Level 3 SEVERE Teeth are slick with little or no anatomy present possible pu. 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 CTROD 3/4”-205/8”-243/4”-205/8”-24 UREM37BYMASSIVE CTROD CTROD 3/4”-205/8”-243/4”-205/8”-24 UREM37BYMASSIVE CTROD CTROD 3/4”-205/8”-24 UREM37BYMASSIVE Thetaxpepaermusthaveonesignstatingrelevant andmaintainrecodspovingthose aereal.Anyadvertisedtermssuchas“expert,”“maste,”“consultant,”or“specialist”mustbe hee.Fe http://www.collaborativelearning.org/tiddler.pdf “TIDDLER’S LATE”“TIDDLER’S LATE”“TIDDLER’S LATE”“TIDDLER’S LATE”“TIDDLER’S LATE&# 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 . 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. 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. 4’10” 4’11” 5’0” 5’1” 5’2” 5’3” 5’4” 5’5” 5’6” 5’7” 5’8” 5’9” 5’10” 5& “1” then “#”, “2” then “#”,“5” then “#”,“6” then “#”,“3” then “#”. STEVEN JAY STEELE . . SIZE. . MOON. THE SIZE OF THE MOON . IS . 3,474 KM. . . EARTH. THE EARTH IS 12,742 KILOMETERS WIDE. LANDFORMS/CRATERS. . Convection during . the . MJO . over Manus. David . Zermeno. and . Chidong. Zhang. RSMAS University of Miami. collaborations from. Pavlos. . Kollias. and Heike . Kalesse. University of McGill. Contact: . 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. M. Bruzzi. 1. , R. Mori. 1. , M. Scaringella. 1. , Z. Li. 2. 1. INFN and University of Florence, Florence (Italy). 2. BNL, Upton New York (US). M. . Bruzzi. , R. Mori, M. . Scaringella. , Z. Li . Shallow levels analysis in n-type MCZ Si detectors after mixed irradiation, .

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