Images Featured Sites Quickmap Videos Gigapan Exhibits Exciting New Images from The LROC Team. Total posts from Basins 49 Search Looking Over the Orientale Basin Indian Ocean as seen from lunar orbit (2015-12-10 06:00:29.202 UTC). NAC high-resolution monochrome image merged with WAC lower-resolution color observations. North is to the left, Antarctica to the right, Australia at the top, and Africa at the bottom (E1204366496L, M1204365627C [NASA/GSFC/Arizona State University]). Published on 07 Apr 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 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 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 The Highs and Lows of Ryder Crater Ryder Crater (13 x 17 km across) controlled Feature Mosaic; located at 43.8° S, 143.2° E, north is up, LROC NAC images M1172098182, M1172105288, and M1172112395 [NASA/GSFC/Arizona State University]. Published on 19 Oct 2020 Apennine Bench Formation: A Window into Ancient Volcanism LROC Wide Angle Camera (WAC) 100 m/px mosaic with 6 colorized Digital Terrain Models (DTMs) of the Apennine Bench Formation (centered near 26° N, 356° E - here in Quickmap), an enigmatic light plains unit located on the central lunar nearside, west of the Apennine Mountains and the Apollo 15 landing site at Hadley Rille [NASA/GSFC/Arizona State University]. Published on 29 Jun 2020 Rilles and Rilles: Sinuous, Straight, and Arcuate Rilles are all over the Moon! Controlled feature mosaics help us see these features with great detail. Pictured: Rimae Sulpicious Gallus (20°N Lat, 10°E Lon), Rima Sharp (46°N Lat, 309°E Lon), Rima Cauchy (10°N Lat, 38°E Lon) [NASA/GSFC/Arizona State University]. Published on 30 Apr 2020 Feature Mosaics: Behind the Seams A seamless mosaic of a portion of Karpinsky crater (91 km diameter, 72.61° N, 166.80°E) seamless mosaic. Scene is 55 km across, NAC images M1309496597L/R, M1309503618L/R, M1309510644L/R, M1309517669L/R, and M1309524696L/R [NASA/GSFC/Arizona State University]. Published on 16 Mar 2020 Plumbing the Depths by Scaling the Heights The central mountainous peaks of Maunder crater are thought to be made of rock that was melted by the impact event that resulted in the Orientale basin. This impact melt rock deposit was then lifted up from below the surface during the Maunder impact event. Material that was melted by the younger Maunder impact event ponded and solidified at the base of this mountain (bottom of the scene). Scene is 2.75 km across and centered at 14.62° S, 266.21° E; NAC image M1200748730LE [NASA/GSFC/Arizona State University]. Published on 19 Feb 2020 Prev 1 2 3 4 5 Next ← Previous Next → Displaying Post 1 - 10 of 49 in total
