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List Of Valleys On The Moon
There are several large valleys that have been given names on the surface of the Moon. These are listed below. Most of these valleys are named after a nearby crater; see the list of craters on the Moon for more information. See also * List of craters on the Moon * List of features on the Moon * List of maria on the Moon * List of mountains on the Moon External links Digital Lunar Orbiter Photographic Atlas of the Moon {{DEFAULTSORT:Valleys on the moon Moon The Moon is Earth's only natural satellite. It is the fifth largest satellite in the Solar System and the largest and most massive relative to its parent planet, with a diameter about one-quarter that of Earth (comparable to the width of ... Moon-related lists ... [...More Info...] [...Related Items...] OR: [Wikipedia] [Google] [Baidu] |
Valley
A valley is an elongated low area often running between hills or mountains, which will typically contain a river or stream running from one end to the other. Most valleys are formed by erosion of the land surface by rivers or streams over a very long period. Some valleys are formed through erosion by glacial ice. These glaciers may remain present in valleys in high mountains or polar areas. At lower latitudes and altitudes, these glacially formed valleys may have been created or enlarged during ice ages but now are ice-free and occupied by streams or rivers. In desert areas, valleys may be entirely dry or carry a watercourse only rarely. In areas of limestone bedrock, dry valleys may also result from drainage now taking place underground rather than at the surface. Rift valleys arise principally from earth movements, rather than erosion. Many different types of valleys are described by geographers, using terms that may be global in use or else applied only locally ... [...More Info...] [...Related Items...] OR: [Wikipedia] [Google] [Baidu] |
Martianus Capella
Martianus Minneus Felix Capella (fl. c. 410–420) was a jurist, polymath and Latin prose writer of late antiquity, one of the earliest developers of the system of the seven liberal arts that structured early medieval education. He was a native of Madaura. His single encyclopedic work, '' De nuptiis Philologiae et Mercurii'' ("On the Marriage of Philology and Mercury"), also called ''De septem disciplinis'' ("On the seven disciplines"), is an elaborate didactic allegory written in a mixture of prose and elaborately allusive verse. Martianus often presents philosophical views based on Neoplatonism, the Platonic school of philosophy pioneered by Plotinus and his followers. Like his near-contemporary Macrobius, who also produced a major work on classical Roman religion, Martianus never directly identifies his own religious affiliation. Much of his work occurs in the form of dialogue, and the views of the interlocutors may not represent the author's own. Life According to ... [...More Info...] [...Related Items...] OR: [Wikipedia] [Google] [Baidu] |
Rheita (crater)
Rheita is a lunar impact crater located in the southwestern sector of the Moon. It was named after Czech astronomer and optician Anton Maria Schyrleus of Rheita. It lies to the northeast of the crater Metius, and northwest of Young. The southwestern rim overlies the edge of Vallis Rheita, a long lunar valley stretching for over 200 kilometers on a line running northeast to southwest. At its widest the valley is 25 kilometers wide and a kilometer deep. The rim of Rheita remains well-defined with a sharp lip and a terrace Terrace may refer to: Landforms and construction * Fluvial terrace, a natural, flat surface that borders and lies above the floodplain of a stream or river * Terrace, a street suffix * Terrace, the portion of a lot between the public sidewalk an ...d inner wall. The rim overlaps a slightly smaller crater to the east, and has a pair of small impact craters in the northern wall. The crater floor is flat and it has a central peak. Satellite craters By convention ... [...More Info...] [...Related Items...] OR: [Wikipedia] [Google] [Baidu] |
Anton Maria Schyrleus Of Rheita
Anton (or Antonius) Maria Schyrleus (also Schyrl, Schyrle) of Rheita (1604–1660) ( Antonín Maria Šírek z Reity) was an astronomer and optician. He developed several inverting and erecting eyepieces, and was the maker of Kepler's telescope. "Things appear more alive with the binocular telescope," he wrote, "doubly as exact so to speak, as well as large and bright. His binocular telescope is the precursor to our binoculars. Biography Two different stories exist about Rheita's early life. The most popular account holds that he is of Czech origin, born in 1597. According to this story he was a priest and a member of the order of Capuchin friars at Rheita, Bohemia, hence his name. At the outbreak of the Thirty Years' War in 1618, he left the order and established himself in Belgium. The other, more probable account, starts in 1604, when Schyrleus is born in Reutte, Austria. After joining the Augustine order in 1622, he is sent to the university at Ingolstadt, where he probabl ... [...More Info...] [...Related Items...] OR: [Wikipedia] [Google] [Baidu] |
Vallis Rheita
Vallis Rheita is a linear valley on the near side of the Moon. It is located in the southeastern quadrant, and is oriented radially to Mare Nectaris. This valley appears to share a common origin with the Vallis Snellius to the northeast, as both are oriented radially with Mare Nectaris. The center of the valley lies at selenographic coordinates , and it has a length of 445 km. At its maximum extent this valley has a width of about 30 km, but it narrows to 10 km at the southeastern extreme. It is the second longest such valley on the near side of the Moon, being exceeded only by Vallis Snellius. Vallis Rheita has been eroded by a series of impacts, and several notable craters lie along the length of this valley. Near the northwestern end is the crater Rheita, for which this formation was named. Further to the southeast is the crater Young, nearly centered across the valley. Next to Young is Young D, also lying across the valley but less distorted by the rift. Further southeast ... [...More Info...] [...Related Items...] OR: [Wikipedia] [Google] [Baidu] |
Planck (crater)
Planck is a large lunar impact crater, approximately 319 kilometers in diameter, that is located in the southern hemisphere of the Moon, on the far side as seen from the Earth. It lies to the west of the walled plain Poincaré, another enormous formation only slightly larger than Planck. Lying across the southeast rim of Planck is the crater Prandtl, to the northeast is Hildegard, and to the west is Fechner. Planck is located within the South Pole–Aitken basin. Formation According to a 2012 study, Planck formed roughly 4.09 Ga (billion years) ago, partially resurfacing the area of the South Pole-Aitken basin that it impacted. Description Like many lunar formations of this size, the outer rim has been damaged and eroded by lesser impacts, leaving a rugged ring of peaks and ridges that is notched and incised by small craters. The western rim of this walled plain is neatly overlain by a long lunar valley designated the Vallis Planck. Despite its name, however, this valley ... [...More Info...] [...Related Items...] OR: [Wikipedia] [Google] [Baidu] |
Max Planck
Max Karl Ernst Ludwig Planck (, ; 23 April 1858 – 4 October 1947) was a German theoretical physicist whose discovery of energy quanta won him the Nobel Prize in Physics in 1918. Planck made many substantial contributions to theoretical physics, but his fame as a physicist rests primarily on his role as the originator of quantum theory, which revolutionized human understanding of atomic and subatomic processes. In 1948, the German scientific institution Kaiser Wilhelm Society (of which Planck was twice president) was renamed Max Planck Society (MPG). The MPG now includes 83 institutions representing a wide range of scientific directions. Life and career Planck came from a traditional, intellectual family. His paternal great-grandfather and grandfather were both theology professors in Göttingen; his father was a law professor at the University of Kiel and Munich. One of his uncles was also a judge. Planck was born in 1858 in Kiel, Holstein, to Johann Julius Wilhelm Pl ... [...More Info...] [...Related Items...] OR: [Wikipedia] [Google] [Baidu] |
Vallis Planck
Vallis Planck is a long, linear valley located on the far side of the Moon. It is oriented radially to the huge Schrödinger basin, and was most likely formed by that impact. The selenographic coordinates of this feature are , and it has a length of 451 km. This cleft in the surface crosses the western part of the huge walled plain Planck, and it was named after that feature (which has an eponym of Max Planck Max Karl Ernst Ludwig Planck (, ; 23 April 1858 – 4 October 1947) was a German theoretical physicist whose discovery of energy quanta won him the Nobel Prize in Physics in 1918. Planck made many substantial contributions to theoretical p ...). The southern edge closest to Schrödinger begins near the northeastern outer rampart of the crater Grotrian. It then continues to the north-northwest, where it suffers a disruption where it crosses the crater Fechner. The remainder of the feature continues to the northwestern outer rim of the walled plain Planck, unti ... [...More Info...] [...Related Items...] OR: [Wikipedia] [Google] [Baidu] |
Palitzsch (crater)
Palitzsch is a lunar impact crater that is located in the southeast part of the Moon, near the southeast rim of the crater Petavius. Just to the southwest of Palitzsch is Hase, while to the east-southeast is Legendre. The northeast rim of Palitzsch forms the southern end of Vallis Palitzsch, a lunar valley that follows the eastern rim of Petavius for a distance of about 110 kilometers. The crater rim is relatively low and inconspicuous, while the floor forms a depression in the surface that follows the contours of the neighboring valley. Satellite craters By convention these features are identified on lunar maps by placing the letter on the side of the crater midpoint that is closest to Palitzsch. Due to its rays, Palitzsch B is mapped as part of the Copernican System.The geologic history of the Moon, 1987, Wilhelms, Don E.; with sections by McCauley, John F.; Trask, Newell J. USGS The United States Geological Survey (USGS), formerly simply known as the Geological S ... [...More Info...] [...Related Items...] OR: [Wikipedia] [Google] [Baidu] |
Johann Palitzsch
Johann Georg Palitzsch (11 June 1723 – 21 February 1788) was a German astronomer who became famous for recovering Comet 1P/Halley (better known as Halley's Comet) on Christmas Day, 1758.Hoffmann, Christian Gotthold (1759 January 20) "Nachricht von dem Kometen, welcher seit dem 25. December gesehen wird" (News of the comet, which has been seen since the 25th of December), ''Dreßdnischen Gelehrten Anzeigen'', 2nd issue. The periodic nature of this comet had been deduced by its namesake Edmond Halley in 1705, but Halley had died before seeing if his prediction would come true. Raised to become a successful farmer under a strict stepfather, Palitzsch secretly studied as much astronomy as he could from the books he could afford. He learned contemporary astronomy from the book “Vorhof der Sternwissenschaft” (“The Forecourt of Astronomy”) by Christian Pescheck. He learned Latin and, at age 21, inherited the farm, which allowed him to construct his own botanical garde ... [...More Info...] [...Related Items...] OR: [Wikipedia] [Google] [Baidu] |
Vallis Palitzsch
The Vallis Palitzsch is a geological structure of the surface of the Moon. The name of the valley was given in 1964 by the International Astronomical Union and comes from the adjacent crater, which in turn was named after the German astronomer Johann Georg Palitzsch (1723–1788). References Valleys on the Moon {{Valleys on the Moon ... [...More Info...] [...Related Items...] OR: [Wikipedia] [Google] [Baidu] |
Inghirami (crater)
Inghirami is a lunar impact crater that is located toward the southwestern limb of the Moon. It lies to the southwest of the large walled plain Schickard. Northwest of Inghirami is the wide Vallis Inghirami, a wide, straight valley that is radial to the Mare Orientale impact basin. The valley has a length of about 140 kilometers and ends at the northern edge of the crater. Inghirami is located near the southeastern edge of the immense skirt of ejecta that surrounds the Mare Orientale. This material has formed linear ridges and valleys that continue across most of the crater rim and interior from the northwestern face. Much of the outer rim has been modified by this impact material, and the most intact part of the rim lies along the southeast edge. The partly buried rim of this crater is roughly circular and somewhat irregular. There are some shelves and terraces along the sides, but these features are moderately eroded. A few small craters lie along or near the rim. The most not ... [...More Info...] [...Related Items...] OR: [Wikipedia] [Google] [Baidu] |
