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Aitken (crater)
Aitken Basin
Small, Young Volcanic Deposits Around the Lunar Farside Craters Rosseland, Bolyai, and Roche
March 21–25, 2016
DMAAC – February 1973
Science Rationale for South Pole-Aitken Basin Locations for Sample Return
Part B Aitken Crater and Its Environs Crater
Mare Volcanism on the Farside and in the Orientale Region of the Moon
South Pole-Aitken Basin
Apollo 17 Lunar Sounder Data Provide Insight Into Aitken Crater’S Subsurface Structure
Abstract #2065: 34Th Lunar and Planetary Science Conference, March 2003, Houston TX
SIDE of the MOON. J. J. Gillis1, B. L. Jolliff1, and P. G. Lucey2
Near Taruntius Crater Appears to Be Relatively Young (~1 Ga) [14]. of >80
Topographic Characterization of Lunar Complex Craters Jessica Kalynn,1 Catherine L
Characterization of Previously Unidentified Lunar Pyroclastic Deposits Using Lunar Reconnaissance Orbiter Camera Data J
2015 Spring Commencement Metropolitan State University of Denver
POSTER SESSION: the CRATERING PROCESS: MECHANICS and SCALING 6:00 P.M
Fall 2020 Media Guide Supplement
Bulk Mineralogy of Lunar Crater Central Peaks Via Thermal Infrared Spectra from the Diviner Lunar Radiometer - a Study of the Moon’S Crustal Composition at Depth
Top View
Elliptical Structure of the Lunar South Pole-Aitken Basin
An Indigenous Origin for the South Pole Aitken Basin Thorium Anomaly Ian Garrick-Bethell and Maria T
Characterizing the Depths and Central Peaks of Lunar Complex Craters with Lola Topography
Image Map of the Moon
RPD SI Updated Pre-Subm Version PL
Thedatabook.Pdf
National Aeronautics and Space Administration) 111 P HC AO,6/MF A01 Unclas CSCL 03B G3/91 49797
Morphological Analysis of the Cratering of the South Pole–Aitken
HARVARD COLLEGE OBSERVATORY Cambridge, Massachusetts 02138
Advances in Space Research 42 (2008) 248–258
Vladislav Shevchenko · Zhanna Rodionova Gregory Michael
Geological Characteristics of Von Kármán Crater, Northwestern South Pole-Aitken Basin: Chang’E-4 Landing Site Region
Mare Ingenii Van De Graaff a B C
Longitude (0 E) Figure 6: the Red Dots Represent the Craters Examined in the Near Side Highland Region
Prepared on Behalf of the National Aeronautics and Space Administration GEOMETRIC INTERPRETATION of LUNAR CRATERS G23QIJQ8
Protobasins Are Not Part of the Normal Sequence, Target Is Important, and Other Musings on the Central-Peak to Peak-Ring Transition Based on Mercury’S Impact Craters
1. Introduction
Apollo 17 Lunar Sounder Data Provide Insight Into Aitken Crater’S Subsurface Structure
Highlights in Space 2008
Compositional Variations of the Lunar Crust: Results from Radiative Transfer Modeling of Central Peak Spectra J