Images Featured Sites Quickmap Videos Gigapan Exhibits Exciting New Images from The LROC Team. Total posts from Basins 46 Search 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 On and Around Mons Piton Mons Piton rises 2300 meters above the dark volcanic rocks of Mare Imbrium. The image covers an area 15.5 kilometers wide, north is up, and the Sun shines from the east (right). LROC NAC image pair M190609650LR [NASA/GSFC/Arizona State University]. Published on 09 May 2019 The West Side of Plato Crater Western Plato crater (at right) and the geologically complex region west of its rim — part of a controlled and corrected mosaic made up of Lunar Reconnaissance Orbiter Camera (LROC) Narrow Angle Camera (NAC) images. The late afternoon Sun (incidence angle 77°) casts long shadows, accentuating surface relief. image width is 57 kilometers across the center. NAC image pairs M1188416966LR, M1188423994LR, M1188431022LR, M1188438051LR, and M1188445079LR [NASA/GSFC/Arizona State University]. Published on 18 Jan 2019 Von Kármán Crater: Awaiting A Visitor Von Kármán crater (186 kilometer diameter), a treasure house of geologic landforms! LROC Wide Angle Camera mosaic, five degree latitude and longitude grid [NASA/GSFC/Arizona State University]. Published on 02 Jan 2019 Prev 1 2 3 4 5 Next ← Previous Next → Displaying Post 1 - 10 of 46 in total
