Where is mare imbrium

This is characterised by peaks of around 2, meters, craters Tobias Mayer 35 km and Gay-Lussac 24 km , and in the north, the promontory Cape Banat. Smaller mountain chains are also found within the basin, for instance the northern Montes Recti 2, m high , Teneriffe 1, , and eastern Spitzbergen 1, Mons Pico and Mons Piton , both around 2, meter high, are two isolated mountain peaks that stand out in the northeast.

Major Craters Along with Sinus Iridum , the region under study features many other well-known large craters. Eratosthenes 60 km is located just south of the Montes Apenninus near Sinus Aestuum and it is characterised by an elevated crater rim 3, m.

Aristillus and Autolycus are two major craters found in the west of the basin, the former characterised by a system of valleys radiating towards Mare Imbrium and Palus Nebularum. Other major craters within the mare are Cassini 29 km — 2, m , Timocharis 40 — 2, , Lambert 29 — 2, , Euler 28 —2, , Delisle 26 — 2, , Diophantus 21 — 2, , Le Verrier 18 — 2, Schroter's observation of a peculiar phenomenon at Mare Imbrium Source: W.

Corliss, Mysterious Universe; a handbook of astronomical anomalies , pages Bispham, K. These are in connection with Moore's remarks on the rarity of flashes on the moon. Of the multitude of changes reported in Schroter's book, this is surely one of the strangest.

Whitaker's book. The Sixteen-West ray a nickname by Danny Caes for the easternmost one of the two pronounced ejecta-rays from Copernicus running at approximately 16 degrees West across the southern part of Mare Imbrium. The Nineteen-West ray a nickname by Danny Caes for the westernmost one of the two pronounced ejecta-rays from Copernicus running at approximately 19 degrees West across the southern part of Mare Imbrium. Bibliography Schultz, P. Like most of the other maria on the Moon, Mare Imbrium was named by Giovanni Riccioli, whose nomenclature system has become standardized.

The earliest known name for the mare may be "The Shrine of Hecate"; Plutarch records that the Ancient Greeks gave this name to the largest of the "hollows and deeps" on the Moon, believing it to be the place where the souls of the deceased were tormented. Ewen A. Whitaker argues that this likely refers to Mare Imbrium, "the largest regular-shaped dark area unbroken by bright patches" that can be seen with the naked eye.

Mare Imbrium is visible to the naked eye from Earth. In the traditional 'Man in the Moon' image seen on the Moon in Western folklore, Mare Imbrium forms the man's right eye. On 17 November at Universal Time, the Soviet spacecraft Luna 17 made a soft landing in the mare, at latitude Luna 17 carried Lunokhod 1, the first rover to be deployed on the Moon. Lunokhod 1, a remote-controlled rover, was successfully deployed and undertook a mission lasting several months.

In , the crewed Apollo 15 mission landed in the southeastern region of Mare Imbrium, between Hadley Rille and the Apennine Mountains. Command Module Pilot Alfred Worden remained in orbit and acquired hundreds of high-resolution photographs of Mare Imbrium and other regions of the moon as well as other types of scientific data.

The crew on the surface explored the area using the first lunar rover and returned to Earth with of lunar surface material. On 17 March , an object hit the lunar surface in Mare Imbrium and exploded in a flash of apparent magnitude 4.

The crater could be as wide as 20 meters. This was the brightest impact recorded since NASA's lunar impact team began monitoring in Chang'e 3 landed on 14 December on Mare Imbrium, about 40 km south of the 6 km diameter Laplace F crater, at The lander deployed the Yutu rover 7 hours and 24 minutes later. Lunar Orbiter image IV- M. This oblique view of Orientale emphasizes the distribution of ejecta material on the southeast side of the basin. Portions of all three major basin rings are visible.

Basin ejecta begins just outside the Cordillera Mountains and extends up to kilometers beyond the base of the mountains. This ejecta has a rough, hummocky texture and contains linear patterns that point back at the center of Orientale. Lunar Orbiter image IVM.

This image illustrates details of the Outer Rook left and Cordillera Mountains right. The shadows on the western sides of both mountain ranges emphasize the large topographic relief of these mountains. Most of the region between the two basin rims is relatively rough, with only a few smooth regions.

These smooth regions are thought to be material that was melted by the energy of the impact and emplaced as sheets on top of the other impact ejecta. Lunar Orbiter image IVH2. This image shows the southern portion of Mare Orientale.

The central portion of Mare Orientale top of picture is covered by a thin layer of mare basalt. This layer is probably less than 1 kilometer deep, much less than in other nearside mare basins. Lunar Orbiter image IVH1. This image provides an overview of Mare Humorum and the surrounding region. Unlike the Orientale Basin, the Humorum Basin is filled with a thick layer of mare basalt. In the center of the basin, the basalt is believed to exceed 3 kilometers in thickness. On the north edge of Mare Humorum is the large crater Gassendi, which was considered as a possible landing site for Apollo When a load of basalt several kilometers thick is emplaced on the Moon's surface, it causes the underlying material to sag under the extra weight.

The resulting motion can cause the surface to buckle, producing a series of ridges on the mare surface. This image of the southeastern portion of Mare Humorum shows several such ridges in the upper left corner. These structures are frequently termed wrinkle ridges and are common in many mare regions, including Mare Serenitatis and Mare Imbrium.

Geologically, this type of ground motion occurs on a thrust fault. While the basalt load causes the central portion of the mare basin to subside, more distant regions may actually be flexed upward by the resulting ground motion.

This stretches the crust and may produce graben, which are narrow valleys surrounded on both sides by faults. This image lies to the east of the previous image, at a greater distance from the center of the Humorum Basin. Several examples of graben are clearly seen on the left side of the image.