oceanus procellarum location

Wikipedia. Today's Featured Image is a great example of typical young and old craters. The Procellarum region is a broad region of low topography covered in dark mare basalt. The gravity gradients reveal a giant rectangular pattern of structures surrounding the region. Differing ages may indicate that mare volcanism occurred over a long period of time (>1.5 Ga). After a few tens of millions of years it collided with the Moon and due to a small collisional velocity simply piled up on one side of the Moon forming what is now known as far side highlands. The Chang’e-5 mission is expected to realize four “firsts” in China’s space history: Found insideThe large dark area in this picture is Oceanus Procellarum. ... the formation of two plateaus, which help in determining the basin sizes and locations. Found inside“And that's Oceanus Procellarum, the amusement park we went to last week! ... and Oceanus Procellarum was standing on the shore that was located on the side ... The discovery provides the first compositional evidence that the Procellarum basin was the relic of a gigantic impact, which could be confirmed by future lunar sample return missions, such as Moonrise, a proposed NASA mission that would send an unmanned probe to collect lunar dirt and return it to Earth. The area is geologically complex and known for its volcanic activity. "Using the gradients in the gravity data to reveal the rectangular pattern of anomalies, we can now clearly and completely see structures that were only hinted at by surface observations.". They may be different for your location. 1). Earth's moon as observed in visible light (left), topography (center, where red is high and blue is low), and the GRAIL gravity gradients (right). Found inside – Page 506291-429 Oceanus Procellarum , Apollo 12 , scientific results : Simmons , Gene . 291-431 Physical mapping , photometric parameters : Shevchenko , V. V. ... Around its edges are small maria 'bays'. Oceanus Procellarum and the western maria . • Oceanus Procellarum has diverse range of mare compositions and ages • Implications for remotely-sensed ages of Mars and all other terrestrial planets • Systematic analyses of Procellarum region will clarify geologic relationships, stratigraphy, ISRU potential youngest mare volcano Aristarchus plateau Image 75 km wide A few years ago the world was suddenly astounded by hearing of an experiment of a most novel and daring nature, altogether unprecedented in the annals of science. Low-relief mare features such as ridges and arches are best studied by using stereoscopic photographs taken at low Sun angles. Country of origin: Ecuador Location: Quito, Pichincha Status: Active Formed in: 2004 Genre: Black Metal/Ambient Lyrical themes: N/A Current label: Unsigned/independent Years active: 2004-present Discography; Members; Surveyor 1 was the first lunar soft-lander in the uncrewed Surveyor program of the National Aeronautics and Space Administration (NASA, United States).This lunar soft-lander gathered data about the lunar surface that would be needed for the crewed Apollo Moon landings that began in 1969. Found inside – Page 32These authors suggested that the source region of the Oceanus Procellarum basalts that flooded Mare Humorum can be located in the Sharp Formation near the ... Apollo 12 Landing Site. Found inside – Page 88Landing date : June 2 , 1966 Location : Near the center of Oceanus Procellarum ( Ocean of Storms ) Details : The first successful soft - landing by a US ... NASA/Colorado School of Mines/MIT/JPL/GSFC, NASA news releases and other information are available automatically by sending an e-mail message with the subject line, To unsubscribe from the list, send an e-mail message with the subject line. Found inside – Page 305Location Feature Cavalerius w F Х ( B - 4 ) ( A - 4 ) Galilaei M ( KRAFFT ) ... B - 1 ) Procellarum ( Oceanus ) E Feature Location Lichtenberg AA ( B - 1 ) ... The Oceanus Procellarum Group The Oceanus Procellarum Group covers approximately 1.7 x 106 km 2, which represents 4.5% of the total surface area of the moon. Table 1. The lava-flooded rift valleys are unlike anything found anywhere else on the moon and may at one time have resembled rift zones on Earth, Mars and Venus. To unsubscribe from the list, send an e-mail message with the subject line unsubscribe to hqnews-request@newsletters.nasa.gov. After several decades spent in astronomical semi-obscurity, the Moon has of late suddenly emerged as an object of considerable interest to students of astronomy as well as of other branches of natural science and technology; and the reasons ... Found inside – Page 486A portion of Oceanus Procellarium near the crater Reiner Gamma is shown in Figure ... appearing crater seen in Figure 24 is located in Oceanus Procellarum. Located in Oceanus Procellarum between the Marius Hills and Kepler crater, it is about 165 km long and trends in a NNW-SSE direction. The twin spacecraft flew in a nearly circular orbit until the end of the mission on Dec. 17, 2012, when the probes intentionally were sent into the moon’s surface. On its north-west edge lies the 32 km wide Aristarchus ray crater, the brightest feature on the Near side of the Moon. lunar orbiter iv—lunar disc with gassendi crater, mare humorum, & oceanus procellarum Together 4 gelatin silver prints from frame 4143, 17 x 21 inches each, including high res images 143 H1, H2, & H3 which tile together to form a 17 x 63 inch panorama, and medium res image 143 M. [9], The robotic lunar probes Luna 9, Luna 13, Surveyor 1 and Surveyor 3 landed in Oceanus Procellarum. THE APOLLO LANDING SITES; Mission Site Location Latitude Longitude Date of Landing; 11: Mare Tranquillitatis: 0°41'15" N: 23°26' E: July 20, 1969: 12: Oceanus Procellarum Found inside(2003) located in Mare Cognitum and further five areas P5, P41, P49, P50, and P51 defined by Hiesinger et al. (2003) located in Oceanus Procellarum. Oceanus is huge, by lunar standards, 434 by 303 miles with indistinct walls. Mare surface age varies by location; FeO/TiO2 is uniform. Oceanus Procellarum /oʊˈsiːənəs prɒsɛˈlɛərəm/ (Latin Ōceanus procellārum, the "Ocean of Storms") is a vast lunar mare on the western edge of the near side of the Moon. Oceanus Procellarum Edit Edit source History Talk (0) Oceanus Procellarum Oceanus Procellarum Location Statistics. These showcase the Oceanus Procellarum (“Ocean of Storms”), a large lunar mare located at the western edge of the near side of the Moon. However, mission scientists studying GRAIL data believe they have found evidence the craggy outline of this rectangular region -- roughly 1,600 miles (2,600 kilometers) across -- is actually the result of the formation of ancient rift valleys. This area was believed to … The Beacon of Oceanus Procellarum. "Our gravity data are opening up a new chapter of lunar history, during which the moon was a more dynamic place than suggested by the cratered landscape that is visible to the naked eye," said Andrews-Hanna. Known as Site 5, this was the second backup landing site for Apollo 11. Additional evidence of thickened basalt lens is provided by presence of a positive gravity anomaly in this region. NASA picks a dozen science and tech projects to bring to the surface of the Moon. To the northeast, Oceanus Procellarum is separated from Mare Imbrium by the Carpathian Mountains. . The findings are published online in the journal Nature. The Rümker region is located in northern Oceanus Procellarum, away from previous sampling sites. We're proud to offer impressive parcels in the southern section of Storms, within view of Craters Billy and Hansteen and only a short jaunt from Crater Flamsteed, historic landing site of Surveyor 1. The Chang’e-5 orbiter was instrumental in the successful collection of lunar material from Oceanus Procellarum late last year. At more than 3,000km wide, the Ocean of Storms (Oceanus Procellarum) is thought to be an impact basin. The lander is … Found inside – Page 400These are located in four mare regions ; Oceanus Procellarum , Northern Imbrium , Mare Serenitatis , and Mare Tranquilitatis . Each of these tubes has met ... 14390 Air and Space Museum Parkway Another theory arising from recent data analysis suggests this region formed as a result of churning deep in the interior of the moon that led to a high concentration of heat-producing radioactive elements in the crust and mantle of this region. Early theories suggested the craggy outline of a region of the moon’s surface known as Oceanus Procellarum, or the Ocean of Storms, was caused by an asteroid impact. The Chang’e 5 lander set down in the moon’s Oceanus Procellarum, or Ocean of Storms, region in the northern hemisphere of the near side of the moon, east of a … Apollo 12 Traverses. The interior conditions of a lava tube are equally important to scientists and lunar base Gravity Gradients Frame Oceanus Procellarum. the location of vents. The complex Chang'e-5 mission landing target is in the Oceanus Procellarum (Ocean of Storms). Apollo 12. Dwayne Brown Lunar seas are actually huge craters with an age over 3 billion years. location of a thickened lens of basalt approximately 600 km in diameter. Oceanus Procellarum - the lunar Ocean of Storms - is a vast volcanic plain, thought to have been created in an ancient asteroid impact. among those The gross topography in southern Mare Imbrium and northern Oceanus Procellarum correlates with the buried structure and deposits of the Imbrium Basin and its rim, and many of the mare slopes may be depositional and reflect the pre-existing major features of the basin. Both patterns appear to be related to volcanic and tectonic processes operating on their respective worlds. Ossolinski (Van Langren's disallowed name for the bright spot Sirsalis A). Named after. 703-572-4118 Found inside – Page 91... from both the physical and chemical point of view as from a single lunar location, namely the Oceanus Procellarum landing site of the Apollo 12 mission, ... NASA Mission Points to Origin of “Ocean of Storms” on Earth’s Moon. Table 1. Location of the Rümker region and previous landing sites. Box indicates Chang'e 5 lander on the basaltic plains of Oceanus Procellarum ("Ocean of Storms") on 02 December 2020 09:54 EST (14:53:55 UTC). Figure 1. Identified location for the collection of samples: The Chinese probe will collect 2 kg of surface material from a previously unexplored area known as Oceanus Procellarum — or “Ocean of Storms” — which consist of a vast lava plain. Luna 13 landed southeast of Seleucus crater, later in 1966. young basalts of Mare Smythii [e.g., Schultz and Spudis, 1983], we conclude that Oceanus Procellarum not only exhibits the widest range of ages of all investigated basins but probably also is the location of some of the youngest basalts on the lunar surface. Absolute model ages and geochemical averages determined for portions of NE Oceanus Procellarum. With the Artemis mission scheduled to put boots on lunar regolith as … The rifts are buried beneath dark volcanic plains on the nearside of the moon and have been detected only in the gravity data provided by GRAIL. For comparison, the Deccan basalts of northern In- dia have a surface area of 0.26 x 106 km 2 [Macdonald, 1972]. INDEX By J. NASA astronauts Pete Conrad and Alan Bean landed in Oceanus Procellarum, the "Ocean of Storms," on 19 November 1969 while Richard Gordon remained in lunar orbit inside the Apollo command and service module. Independence Ave at 6th St, SWWashington, DC 20560 A favourable reception of the first edition of this book - due no doubt to the nature of its subject - which went out of print in 2 years, gave its author a welcome oppor tunity to update at present its contents. Apollo 12 — Oceanus Procellarum Lunar Landing Time 01:54:35 a.m. EST, November 19, 1969 Landing Site Coordinates 3.01239° S latitude, 23.42157° W longitude . The sample-return mission made a successful soft landing in the Oceanus Procellarum ("Ocean of Storms") region on Tuesday (Dec. 1) and almost immediately began its … Oceanus Procellarum, “Ocean of Storms” Oceanus Procellarum Center: 56.677˚ W, 20.671˚ N Range: 81.084˚ - 26.850˚ W, 16.266˚ S - 57.433˚ N Mare 1611 x 353 mi Ocean of Storms Crater Lohrmann D cut through by one of the rilles of Rimae Hevelius (arrow points to another part of Rimae Hevelius) Location: On the western side of the Moon (from the northern hemisphere this would be on the left) Size: 2,500 km Features: Largest of lunar mare. One of the most likely is that Procellarum was a result of an ancient giant impact on the near side of the Moon. Chang'e 5 (Chinese: 嫦娥五号; pinyin: Cháng'é wǔhào) is the fifth lunar exploration mission of the Chinese Lunar Exploration Program, and China's first lunar sample-return mission. The first of Oceanus Procellarum’s craters to see sunlight is Copernicus, famous for its dazzling rays that burst into view against the darker surroundings. Post-depositional, local distortion of the mare surface, however, is present and in many places associated with mare ridges. For a time it was also the backup landing site for Apollo 12. Surveyor 1 Lands on the Moon. [6] The GRAIL mission, which mapped the gravity gradients of the Moon, found square formations resembling rift valleys surrounding the region beneath the lava plains, suggesting the basin was formed by heating and cooling of the lunar surface by internal processes rather than by an impact, which would have left a round crater. Basalts in Oceanus Procellarum have been estimated to be as young as one billion years old. Unlike the other lunar maria, however, Oceanus Procellarum may or may not be contained within a single, well-defined impact basin. Location: Zsámbék, Hungary Technique: white paper, black pencil. Model ages of unit P58 in Figure 1a Study Ageb Count Locationc Boyce[17] 3.2 East Hiesinger, et al. NASA later named the impact site in honor of late astronaut Sally K. Ride, who was America's first woman in space and a member of the GRAIL mission team. National   Air   and   Space   Museum Apollo 15 Aristarchus Crater.jpg 3,274 × 3,550; 2.05 MB. Northeastern Oceanus Procellarum (NE-OP). It is the only one of the lunar maria to be called an "Oceanus" (ocean), due to its size: Oceanus Procellarum is the largest of the maria ("seas"), stretching more than 2,500 km (1,600 mi) across its north–south axis and covering roughly 4,000,000 km2 (1,500,000 sq mi), accounting for 10.5% of the total lunar surface area.[2]. Found inside – Page 256... being the enormous " mare " ' which occupied the place of the present - day ... which Mare Nectaris and Oceanus Procellarum were subsequently to replace ... Oceanus Procellarum A specific example, albeit only one of many, of an interesting target for exploration away from the polesis provided by therelatively young basaltic lava flows in northern Oceanus Procellarum (Fig. Apollo 12 Traverses. Map showing location of the crater Lichtenberg The images show crater Lichtenberg in the Oceanus Procellarum region on the Moon, centred on an area located at 66.8° West, 32.6° North. The following 60 files are in this category, out of 60 total. Prinz, which is a lava-filled impact crater, is located in the Oceanus Procellarum on the Western edge of the near side of the moon.Extending from the right we can see the Rimae Prinz, a series of sinous rilles extending away from the crater for up to 80 km. Aristarchus and Herodotus craters Apollo 15.jpg 750 × 675; 120 KB. Cardanus is a lunar impact crater that is located in the western part of the Moon, in the western part of the Oceanus Procellarum.Due to its location the crater appears very oval because of foreshortening, and it is viewed almost from the side. Oceanus Procellarum (Ocean of Storms) Found inside – Page 238Mission J - 1 ( Apollo 16 ) Landing Site : Descartes - Location : 15 ° 34 ' E ... a region of domes and cones located near the centre of Oceanus Procellarum ... This official NASA history traces behind-the-scenes conflicts and cooperation between scientists and engineers. Scientists studied the gradients in gravity data from GRAIL, which revealed a rectangular shape in resulting gravitational anomalies. Oceanus Procellarum (Latin Ōceanus procellārum, the "Ocean of Storms") is a vast lunar mare on the western edge of the near side of the Moon. Today's Featured Image is a great example of typical young and old craters. Apollo 12 — Oceanus Procellarum Lunar Landing Time 01:54:35 a.m. EST, November 19, 1969 Landing Site Coordinates 3.01239° S latitude, 23.42157° W longitude . 3.01239° S latitude, 23.42157° W. longitude, Apollo 12 Landing Site. Diagram based on Apollo 11, 12, and 14 traverse map prepared by the U.S. Geological Survey and published by the Defense Mapping Agency for NASA. Launched as GRAIL A and GRAIL B in September 2011, the probes, renamed Ebb and Flow, operated in a nearly circular orbit near the poles of the moon at an altitude of about 34 miles (55 kilometers) until their mission ended in December 2012. 303-273-3088kmorton@mines.edu. The map will provide a better understanding of how Earth and other rocky planets in the solar system formed and evolved. Northern Oceanus Procellarum was selected as the CE-5 landing site because it contains some of the young-est mare basalts (Liu et al., 2021). Proceedings of Symposium No. 47 organized by the IAU held in Newcastle upon Tyne, England, March 22-26, 1971 The exact location of that little swirl is: 1° South/ 61° West. Fresh and degraded craters in Oceanus Procellarum, near the crater Flamsteed P. Illumination is from left side of the image, incidence angle is 78°, width is 1400 m [NASA/GSFC/Arizona State University]. It is not to be confused with, Most of the dark region is Oceanus Procellarum and smaller mare, such as, Moon – Oceanus Procellarum ("Ocean of Storms"), DK Space Encyclopedia: The Near Side of the Moon, Learn how and when to remove this template message, one of the three largest craters in the Solar System, "Moon's Mysterious 'Ocean of Storms' Explained", "NASA Mission Points to Origin of "Ocean of Storms" on Earth's Moon", "China's Chang'e 5 moon landing site finally has a name", "China's Chang'e-5 mission returns to Earth with moon samples", "Pinpoint Landing on the Ocean of Storms | Lunar Reconnaissance Orbiter Camera", https://en.wikipedia.org/w/index.php?title=Oceanus_Procellarum&oldid=1046003007, Articles needing additional references from December 2009, All articles needing additional references, Pages using multiple image with manual scaled images, Creative Commons Attribution-ShareAlike License, This page was last edited on 23 September 2021, at 13:23. Located on astronomical body. NASA news releases and other information are available automatically by sending an e-mail message with the subject line subscribe to hqnews-request@newsletters.nasa.gov. The area is southwest of Copernicus crater, the large, light grey crater within the largest dark region on the left-hand side of the Moon. have been obliterated by later impacts and volcanism. This book is part of the TREDITION CLASSICS series. The creators of this series are united by passion for literature and driven by the intention of making all public domain books available in printed format again - worldwide. The GRAIL mission was managed by NASA’s Jet Propulsion Laboratory (JPL) in Pasadena, California, for NASA's Science Mission Directorate in Washington. Lunar Mare Basalt Age and Composition in Northeastern Oceanus Procellarum. "The nearside of the moon has been studied for centuries, and yet continues to offer up surprises for scientists with the right tools," said Maria Zuber, principal investigator of NASA's GRAIL mission, from the Massachusetts Institute of Technology, Cambridge. Its name comes from a myth that … Oceanus Procellarum is a vast lunar mare on the western edge of the near side of the Moon. [12] Their landing site has become known as Statio Cognitum (Latin, "to be known from experience"). oceanus. This area consists of a patchwork of discrete lava flows with estimated individual ages ranging from about 3.5 to 1.2 Gyr. DIVInformative, profusely illustrated guide to locating and identifying craters, rills, seas, mountains, other lunar features. Newly revised and updated with special section of new photos. Over 100 photos and diagrams. /div North is toward the top. On the northern edge of Oceanus Procellarum lies Sinus Roris. Topography of Earth's moon generated from data collected by the Lunar Orbiter Laser Altimeter, aboard NASA's Lunar Reconnaissance Orbiter, with the gravity anomalies bordering the Procellarum region superimposed in blue. Model ages & composition for sites in P58 # a Lat/Lon (Center) 2 N Area b (sq km ) Age (Ga) FeO (wt%) TiO 2 (wt%) Apollo 12 was the second mission to land humans on the Moon. Basalts in Oceanus Procellarum have been estimated to be as young as one billion years old. The mission zeroed in on landing in the Oceanus Procellarum, or Ocean of Storms, near a location called the Mons Rumker. The same bedrock would also be an ideal location to conduct seismic investigations. * Times are for the Traverse City/Interlochen area of Michigan. storm. He helps capture the Red Hawk and then helps to free him. Fresh and degraded craters in Oceanus Procellarum, near the crater Flamsteed P. Illumination is from left side of the image, incidence angle is 78°, width is 1400 m [NASA/GSFC/Arizona State University]. The mission launched in late November and saw a … Cardanus is distinctive for the chain of craters, designated Catena Krafft, that connect its northern rim with the crater Krafft to the north. GRN: N13W39. Approximately 250 seconds after landing in the Oceanus Procellarum, four petals that covered the top half of the spacecraft opened outward for increased stability. The Rümker region is located in northern Oceanus Procellarum, away from previous sampling sites. It is close to … The latter postulates that in addition to the present Moon, another smaller (about 1,200 km in diameter) moon was formed from debris of the giant impact. The surface of the moon’s nearside is dominated by a unique area called the Procellarum region, characterized by low elevations, unique composition, and numerous ancient volcanic plains. Oceanus Procellarum (Ocean of Storms),close to crater Copernicus Between full and last quarter One of the moon's most impressive craters … The 42 km diameter crater and its ejecta are especially interesting because of its location on the uplifted southeastern corner of the Aristarchus plateau. This is one of the … [5], There are several hypotheses about the origin of Oceanus Procellarum and a related asymmetry between the near and far sides of the Moon. The distance between the twin probes changed slightly as they flew over areas of greater and lesser gravity caused by visible features, such as mountains and craters, and by masses hidden beneath the lunar surface. Chantilly, VA 20151 Apollo 12. Oceanus Procellarum. NASA Lunar Orbiter photograph III-154-H2. This area consists of a patchwork of discrete lava flows with estimated individual ages ranging from about 3.5 to 1.2 Gyr. Headquarters, Washington [2], The impact likely happened very early in the Moon's history: at the time when magma ocean still existed or just ceased to exist. B. Reid and U. Mare Imbtium, Mare Humorum, and Mare Vaporum, and Sinus Medii are . The largest young crater (lower right corner) is about 100 meters wide. The Rümker region, located in the northern Oceanus Procellarum, is the candidate landing region for China's Chang'E-5 lunar sample-return mission. Oceanus Procellarum (Ocean of Storms) 3.01239° S latitude, 23.42157° W. longitude. remote sensing Article Thermophysical Features of the Rümker Region in Northern Oceanus Procellarum: Insights from CE-2 CELMS Data Zhiguo Meng 1,2,3,* , Jietao Lei 1, Yuqi Qian 4,5, Long Xiao 4, James W. Head 5, Shengbo Chen 1, Weiming Cheng 2, Jiancheng Shi 6, Jinsong Ping 7 and Zhizhong Kang 8,9 1 College of Geoexploration Science and Technology, Jilin University, Changchun … Apollo 14 — Fra Mauro Lunar Landing Time 4:18 a.m. EST, February 5, 1971 Landing Site Coordinates 3.64530° S latitude, 17.47136° W longitude Oceanus Procellarum (Van Langren's Oceanus Philippicus) (the southwestern part of it, occupying the upper-right section of Chart 39). Around its edges lie many minor bays and seas, including Sinus Roris to the north, and Mare Nubium and Mare Humorum to the south. As … the Beacon of Oceanus Procellarum location Statistics credit: Barker, et al., Surveyor! Aristarchus Crater.jpg 1,855 × 1,089 ; 1 MB the near side of 's... × 675 ; 120 KB Study Ageb Count Locationc Boyce [ 17 ] 3.2 Hiesinger! Observer, this is a vast lunar mare on the western edge of the TREDITION CLASSICS series Ábrahám the! 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Orbiter was instrumental in the center and upper left of this image comes a. ; 1 MB Procellarum have been estimated to be as young as one billion years reviews results... Miles with indistinct walls the gradients in gravity data from grail, which revealed a shape. Are actually huge craters with an age over 3 billion years old area. Has become known as site 5, this is the large mare in the Oceanus Procellarum Statistics! Camera merged hillshade map ( simple cylindrical projection ) East Hiesinger, et al illustrated guide to locating and craters! Positive gravity anomaly in this picture is Oceanus Procellarum ) is about 100 meters wide southern Oceanus Procellarum Statistics... The second mission to land humans on the Moon Apollo 16 metric Camera photography of the.. Other rocky planets in the Apollo 14 and 12 soils and the future Study Ageb Count Locationc Boyce [ ]... Latin, `` to be known from experience '' ) Serenity ; Temporal ;. Known from experience '' ) mission to land humans on the far side `` to be an impact basin the! ] Okonnor -- American warrior of pure blooded descent, who as billion...: Zsámbék, Hungary Technique: white paper, black pencil 1 ( success ): near..., by lunar standards, 434 by 303 miles with indistinct walls formed be... Imbtium, mare Humorum, and Sinus Medii are 1.5 Ga ) Moon on the southeastern. Metric Camera photography of the Moon but underestimated Crota and his spawn guide to locating and craters... `` to be as young as one of Raban, the new research suggests processes beneath the.... Portions of NE Oceanus Procellarum ( fig 61° west generated the highest resolution gravity field map of any body... To locating and identifying craters, rills, seas, Mountains, lunar. Moon in the Oceanus Procellarum, Ocean of Storms ) 3.01239° s,. Inside – Page 2515–7: Excellent ): Crashed near Copernicus crater ( lower right corner ) is thought be! Marshall Space Flight center in Huntsville, Alabama thickened basalt lens is provided by presence of a patchwork of lava! Unsubscribe to hqnews-request @ newsletters.nasa.gov consist of wide-spread mare basalt, who as one billion years the successful of... Heating during the Moon on its north-west edge lies the 32 km wide Aristarchus ray crater the. Tube are equally important to scientists and engineers located on the far side Aristarchus Crater.jpg 3,274 × ;... Be known from experience '' ) collection of lunar material from Oceanus Procellarum wide-spread mare.. Mons Rumker Consensus believed they were strong enough to contain a small human base and engineers ( ). 1,855 × 1,089 ; 1 MB 3 landed in Oceanus Procellarum: Procellarum... Portions of NE Oceanus Procellarum late last year Aristarchus and Herodotus craters Apollo 15.jpg 750 × ;! W. longitude giant impact on the Moon formed and evolved within the larger Flamsteed ). Age over 3 billion years old especially interesting because of its location on far.
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