Images Featured Sites Quickmap Videos Gigapan Exhibits Exciting New Images from The LROC Team. Total posts from Topography 145 Search Tycho: A Model Central Peak Color-shaded relief map showing elevations for the central peak of Tycho crater. Black areas indicate shadows in the stereo images, where no topography could be extracted [NASA/GSFC/Arizona State University]. Published on 29 Mar 2023 Malapert Massif Malapert massif (informal name) is thought to be a remnant of the South Pole - Aitken basin rim, which formed more than 4 billion years ago. More recently, this magnificent peak (lower left) was selected as an Artemis 3 candidate landing region. Image is 25 kilometers wide in the center, Narrow Angle Camera M1432398306LR (NASA/GSFC/Arizona State University). Published on 13 Mar 2023 Three Impact Events Spectacular 4500-meter diameter crater (10.67°S, 225.82°E) formed at the intersection of the rims of Lowell W crater (18-kilometer diameter) and the Orientale basin (750-kilometer diameter). Impact melt and debris spilled from the low point of this not-named crater, 1800-meters downslope from the crater rim high point. East-to-west view, spacecraft altitude 76 kilometers, M1231377442LR [NASA/GSFC/Arizona State University]. Published on 20 Feb 2023 Thousands of Thrust Faults! Prominent lobate thrust fault scarp in the Mandel’shtam cluster, one of the thousands discovered in Lunar Reconnaissance Orbiter Camera (LROC) images. The fault scarp or cliff is like a stair-step in the lunar landscape formed when the near-surface crust is pushed together, breaks, and is thrust upward along a fault; note the two craters overridden by the fault. Image width 1430 meters, north is towards the top, NAC M103460280LR [NASA/GSFC/Arizona State University]. Published on 14 Feb 2023 Ancient Impact Melt Lobate margin of ancient impact melt flow within a nameless farside crater, 45.84° S, 227.32° E, NAC M1117380495LR [NASA/GSFC/Arizona State University]. Published on 28 Dec 2022 Dramatic Contrast The dark rim of Aristarchus crater (23.7°N, 312.5°E) dramatically highlights its bright interior and central peak. There are more than 2700 meters of relief from the rim to the crater floor, and the central peak is 3,000 meters wide (left-to-right) and 400 meters tall. Image acquired from an altitude of 96 kilometers looking east-to-west, 12 kilometers wide in the center, NAC M1259171271LR [NASA/GSFC/Arizona State University]. Published on 01 Dec 2022 Lunar Terminator Western portion of Mare Moscoviense seen under extreme lighting, east-to-west view snapped 25 August 2019. The illuminated rim in the background is an unnamed crater 21 kilometers in diameter (24.2°N, 146.3°E); spacecraft altitude was 94 kilometers, image M1321388053LR [NASA/GSFC/Arizona State University]. Published on 15 Apr 2022 NAC Anaglyph: Alphonsus Vent A dike (subsurface magma body) was likely intruded under the floor of Alphonsus crater creating an array of fractures seen here. Image is 5700 meters wide, north is towards the top [NASA/GSFC/Arizona State University]. Published on 19 Feb 2022 A “Secondary” View of Copernicus NAC DTM showing a chain of Copernicus secondaries (15.5°N, 343.4°E). North is pointing right [NASA/GSFC/Arizona State University]. Published on 04 Feb 2022 Mass Wasting: Klute Crater Mass wasting in Klute Crater (36.79° S, 217.7°E) NAC controlled mosaic containing images, M1155169631LR, M1155162511LR, M1155155392LR [NASA/GSFC/Arizona State University]. Published on 26 Apr 2021 Prev 1 2 3 4 5 … 15 Next ← Previous Next → Displaying Post 1 - 10 of 145 in total
