9 billion years ago, one of these formed the great Imbrium Basin, or Mare Imbrium, and its mountain ramparts. Moon - Mare Imbrium from Copernicus to Plato Moon - Mare Imbrium from Copernicus to Plato Equipment Imaging Telescopes Or Lenses DIY 8" F/7 Newt Imaging Cameras ZWO ASI290MC Mounts Software Bisque Paramount MX+ GEM. To the west of these mountains is a narrow gap where Mare Imbrium in the north. Artwork Description. 9 Lunar Maria. Its diameter is 674 km (419 mi). The Moon. In Fra Mauro. 3 billion years. e. Light plains have higher albedo than that typical of mare basalts, but somewhat lower than that typical of highland terrains (Engel et al. The mare material within the basin consists of basalt formed in the. Here, employing UV-VIS data from the Clementine mission, we estimate mare thickness values in the Imbrium Basin by analyzing ejecta from large. Nearly 50% of all units in Mare Imbrium exhibit ages of 3. It was hoped that samples collected from these mountains would include ancient rocks that originated deep in the Moon's crust. 87 cm) 1 : 2500000. 7 N, 13. 9–2. [For a high resolution picture- click here] AS17-2120 (M) [128] FIGURE 124 [left]. The Apollo 15 landing site is by far one of the most interesting that you can find on the surface of the Moon. The crater Copernicus, 93 kilometers in diameter, is seen in the distance. Origin of the Mare Imbrium G. The deposits from Krieger lie on the surface of the mare basalts, indicating that the crater is quite young. along the. Lunar Orbiter IV imaged the Moon during May of 1967. Which of these is not a natural resource? Clothing Mare Imbrium / ˈɪmbriəm / ( Latin imbrium, the " Sea of Showers " or " Sea of Rains ", "Sea of Tears") is a vast lava plain within the Imbrium Basin on the Moon and is one of the larger craters in the Solar System. [1] It lies to the east and somewhat south of the slightly larger crater Timocharis. K. There is also an area of enriched thorium on the farside, within the. Apollo 15 (July 26 – August 7, 1971) was the ninth crewed mission in the United States' Apollo program and the fourth to land on the Moon. The 6. 9 billion years ago, one of these formed the great Imbrium Basin, or Mare Imbrium, and its mountain ramparts. Add your answer. The basin material is of the Lower Imbrian epoch, with the mare material of the Upper Imbrian epoch. This realization allowed the impact history of the Moon to be gradually worked out by means of the geologic principle of superposition. The rim has a significant outer rampart brightened with ejecta and the upper portion of a terraced inner wall, but lacks the ray system associated with younger craters. A triangular promontory extends 30 kilometers from the southeast of the rim. 5 W), a. Gilbert, 1893, Stadermann et al. Mare Insularum covers an area of about 900 km in diameter. Eratosthenes crater is a relatively deep lunar impact crater that lies on the boundary between the Mare Imbrium and Sinus Aestuum mare regions. Before the Apollo missions landed humans on the Moon, NASA sent several missions to the Moon to map its surface, and to make sure we could safely land there. 85 Ga (Ryder, 1992,. In the mare to the south are several rises collectively named the Montes Teneriffe. ”. Description: SCP-2686 is an adult male human, estimated to be approximately 75 years of age, currently located at [REDACTED] within Mare Imbrium on the lunar surface. 4S 38. With an area of c. Lunar mare. You may do so in. Mare Tranquillitatis ( Latin tranquillitātis, the Sea of Tranquillity or Sea of Tranquility; see spelling differences) is a lunar mare that sits within the Tranquillitatis basin on the Moon. The Mare Imbrium, part of the moon's violent past . The Chang’e 3 (CE-3) mission was implemented as the first lander/rover mission of the Chinese Lunar Exploration Program (CLEP). The SCP Foundation Specialised Lunar Containment and Research Area, better known as Lunar Area-32 and identified as LMaImb-Area-32, is an SCP Foundation facility located. The basin is surrounded by grooves and gashes, large enough to be seen with even small telescopes from Earth, created by rocks blasted out of the crater when it was formed. between the solar-illuminated and dark hemispheres. The 6. 0 Ga. Moon craters are bowl-shaped landforms created by two processes: volcanism and cratering. y. Late Imbrian. Advanced Physics questions and answers. The map was produced by the Army Map. C. They were dubbed maria (Latin for 'seas') by. 1. Scientists already knew a huge space rock created the right eye of the fabled "man in the moon" -- actually a crater known as the "Mare Imbrium," Latin for "sea of showers" -- but they had no idea. On 14 December 2013, Chang'E-3 (CE-3), a follow-up to the Chang'E-1 (CE-1) and Chang'E-2 orbiters, successfully landed on Sinus Iridum, the northwest of Mare Imbrium on the lunar near side. Solved Answer of MCQ Which of these is an incorrect description of the “Mare Imbrium” on the moon? - (a) It contains a certain amount of sedimentary water - (b) - (c) - (d) - Lyceum of Wisdom - Rise of Kingdoms: Peerless Scholar Quiz Question Answers Solved Multiple Choice Question- MCQtimes. They represent very recent tectonic activity on the lunar surface. North is at 4:00. 9 to 4. North is at 4:00. Mosaic of photos by Lunar Reconnaissance Orbiter, made with Wide Angle Camera. Eratosthenian. vast lunar mare filling a basin on Earth's Moon. Caption: The near side of the Moon with the major maria (singular mare, vocalized mar-ray) and lunar craters identified. Believed to be the second youngest lunar basin, lunar scientists think the Mare Imbrium has formed 3. 1 Introduction. It begins just to the west of the prominent crater Eratosthenes, which abuts against the southern face of the range. The mare is located just to the southeast of Oceanus Procellarum. MOON 80 : i i i i i Figure 2. Smaller mare patches also occur in the floors of some. g. Lunar olivine basalt formed around 3. The best developed lava flows on the Moon occur in Mare Imbrium where flow margins are traceable nearly their entire flow length. 3). " This dark patch on the northwest quadrant on the near side of moon, the side that faces Earth, makes. Apollo 15 astronauts David Scott and James Irwin collected this sample of basalt from the Moon on August 1, 1971. Dr. The present study investigates the spectral and. hundreds of meteoroid impacts (WEBP) . 5 N, 20. com. Reaching a maximum brightness of -12. Note the old fractured terrain at the right and smoother textured and ridged mare terrain at center. Plato is a lava-filled lunar impact crater on the Moon. A crater on the moon is named C. This is part of sample 15555, known as Great Scott. ] [ 67] Areas of mare material occupy about 15 percent of the Moon's total surface. g. It is, therefore, the most magnetic region on the Moon. This page was last edited on 16 October 2023, at 20:33. Mare is the type example of a secondary basaltic crust derived by the partial melting of mantle reservoirs. See examples of MARE IMBRIUM used in a sentence. Mare Serenitatis / s ɪ ˌ r ɛ n ɪ ˈ t eɪ t ɪ s / (Latin serēnitātis, the "Sea of Serenity") is a lunar mare located to the east of Mare Imbrium on the Moon. We produced an. of the Moon have been computed, after application The name Mare Insularum refers to the many islands of terra material in the mare. To constrain the mineralogy and chronology of the young mare basalts on the Moon, the lookup table technique 16 was further used to unmix the spectra obtained by the Moon Mineralogical Mapper (M 3. The Imbrium Basin — seen from Earth as a dark patch in the northwestern quadrant of the Moon’s face — measures about 750 miles across. He who rides the chariot of the moon across the darkened heavens over Midgard. Such samples are important to understand the formation and evolution of the Procellarum KREEP. Mare Imbrium (Latin for "Sea of Showers" or "Sea of Rains") is a vast lava plain within the Imbrium Basin on the Moon and is one of the larger craters in the Solar System. Caucasus - Mare Serenitatis, Mare Imbrium, Mare Vaporum) From my Class 8 Bortle Backyard. 7 N, 20. The dark basalt rock, collected near Hadley Rille on the edge of the Imbrium Basin (Mare Imbrium), is about 13 cm (5. Selenography is the study of the surface and physical features of the Moon (also known as geography of the Moon, or selenodesy ). 2. The Moon is a key location for studying the geological evolution of planetary impact basins. As a consequence, the surface of Mercury looks superficially like the Moon, but there are. Introduction. between the solar-illuminated and dark hemispheres. , Chang׳E-5 lunar sample return mission (Qiu and Stone, 2013). A broad, shallow valley within the formation about 50 km (30 miles). Mare Imbrium, Latin for “sea of showers,” is the name of a huge crater on the moon caused by a meteor hitting the lunar surface some 3. 10, 1969, NASA announced the selection of the Fra Mauro region of the Moon as the prime landing site for Apollo 13, located about 110 miles east of the Apollo 12 touchdown point. About 3. Click the card to flip 👆. joining north and south lunar poles, passing through the center of the largest mare, Imbrium, representing 0° of lunar longitude. -This photo taken at low Sun angle emphasizes how common secondary impact craters are on the Moon. The landing site of the Apollo 14 mission in the Fra Mauro region. , the Apollo and Luna landing sites [e. Geologists favored the Fra Mauro area for exploration because it forms an extensive geologic unit around Mare Imbrium, the largest lava plain on the Moon. maxima. Mare Imbrium, Latin for “sea of showers,” is the name of a huge crater on the moon caused by a meteor hitting the lunar surface some 3. Full description: "Southward looking oblique view of Mare. Its diameter is 674 km (419 mi). The Chang’e-3 lunar lander and Yutu rover landed in the moon's Mare Imbrium feature, not far from the intended landing spot in Sinus Iridum. The lander touched down in Mare Imbrium in the Moon’s northern hemisphere on December 14. Its peaks rise to heights of about 5 kilometers. Mare Nectaris / ˈ n ɛ k t ə r ɪ s / (Latin nectaris, the "Sea of Nectar") is a small lunar mare or sea (a volcanic lava plain noticeably darker than the rest of the Moon's surface) located south of Mare Tranquillitatis southwest of Mare Fecunditatis, on the near side of the Moon. Chang'e 3 launched on 1 December 2013 and successfully landed in Mare Imbrium on 14. 1975; Shih and. 0; -13. In the mare to the south are several rises collectively named the Montes Teneriffe. Part of the rim of Hipparchus is modified by "Imbrium sculpture," the pattern of ridges and grooves radial to Mare Imbrium, which affects the lunar surface for more than 1000 km from Imbrium. English: Original description: Southward looking oblique view of Mare Imbrium and Copernicus crater on the Moon. Origin of the Mare Imbrium G. In the foreground is Mare Imbrium, peppered with secondary craters chains and elongated secondary. is incorrect. Introduction. The ratio of the intensity of light reflected from an object, such as a asteroid, to that of the light it receives from the sun is called _____________. , Chang׳E-5 lunar sample return mission. *Email: hughscot@isu. A NASA-led team. Mare Humorum 24. A triangular promontory extends 30 kilometers from the southeast of the rim. Some investigators, however,. Hadley Rille is located in the Montes Apenninus mountain range. Because of its small size, the Moon cooled quickly and was mostly dead volcanically Apollo 15 metric camera image of Southeastern Mare Imbrium. In addition, no samples were returned from the young and high-FeO and TiO 2 mare basalt in the northern Imbrium basin. Where It Is Mare Imbrium is the large, round, smooth dark region northwest of the center of the lunar disk. Copernicus is one of the most noticeable craters on the Moon. At right, shadows reveal the edges of a long lava flow from the lower left to the upper right of the image. The Humorum basin is filled with a thick layer of mare basalt, believed to exceed 3 kilometers. Mare Imbrium, the ‘Sea of Showers’ (named by Riccioli) is the dominant feature of the northwestern quadrant of the Moon. Like all the other maria it is the lava-filled central portion of a giant. See examples of MARE IMBRIUM used in a sentence. Lava flow margins on the Moon are scarce [1,2], and the1 Introduction. (Lunar Orbiter 5, frame M-102)The Nectarian-aged Crisium basin exhibits an extremely thin crust and complicated lunar geological history. The depth of the mare sourceAssuming that the mare basaltic magmas were generally denser than the Moon’s crust, it has been suggested that the lithostatic pressure at the mare source could have forced these magmas to the surface [1], [2], [3], [29]. The onboard lunar penetrating radar conducted a 114-m-long profile, which measured a thickness of ∼5 m of the lunar regolith layer and detectedthreeunderlying basalt units at depths of 195, 215. Copernicus is seen almost edge-on near the horizon at the center. y. 1). Since the Apollo 14 mission delivered samples of the Fra Mauro formation, interpreted as ejecta of the Imbrium impact, defining the age of this impact has emerged as one of the critical tasks required for the complete understanding of the asteroid bombardment history of the Moon and, by extension, the inner Solar System. Imbrium on the near side of the Moon, was equipped with lunar penetrating radar (LPR) on the Yutu rover and detected subsurface structures around the landing site. On… Read More lunar exploration In Chang’e Add your answer. Is Plato lower than Mare Imbrium (centered at 32 N, 344 )? [Remember that Plato is on the Northern edge of Mare Imbrium. After the Moon had cooled and solidified enough to preserve impact scars, it began to retain the huge signatures of basin-forming collisions with asteroid-sized bodies left over from the formation of the solar system. Part of Hall of the Universe. Urey 3. Published: September 14, 2012. 3 billion years ago, several hundred million years after the impact that created Imbrium. It is located in the outer rings of the Procellarum basin, just north of Mare Imbrium, and stretches east to north of Mare Serenitatis. The area is primarily composed of relatively low ridges and hills, between which exist undulating valleys. Arizona State University/GSFC/NASA. Sinus Iridum is his ear. The brightness of an astroid depends on. A map in orthographic projection, centered at 34. The flat region at the top of the image is Mare Serenitatis west of the landing side. This crater is bowl-shaped, with a small interior floor at the midpoint and a somewhat eroded outer rim. (Mare Imbrium) —Sea of Rains (Mare Imbrium) — Imbrium Basin, one of the largest impact basins on the Moon, formed when a huge impactor hit the lunar surface a little more than 3. Oceanus Procellarum, Mare Imbrium, and Mare Serenitatis) within 0. More targets to look out for. The Imbrium Basin formed from the collision of a proto-planet during the Late Heavy Bombardment. The Moon is believed to have been acquired or formed as a result of which of the following? Click the card to flip 👆. Sinus Iridum is the feature marked "A". 2 Lunar Highlands. However, the lunar ____ ("seas") are relatively recent features. Locate Mare Imbrium. 0 Ga. of the Moon have been computed, after applicationThe name Mare Insularum refers to the many islands of terra material in the mare. SCI 1301 Assignment 11: Meteorite Impacts and the Late Heavy Bombardment Mare Imbrium 1145 km Rocky 25. Download :. Extensive mare filling inside the basin is expected to retain a record of igneous activity through the thermal history of our Moon and Solar System. Image #3 is from the Lunar Orbiter IV. Carleton Chinner’s first novel, The Hills of Mare Imbrium, is an examination of what it means to be free, and what the cost of that freedom can be. Moon, the meandering lines outline maria and highlands. Scientists have found fresh evidence in lunar rocks showing that the moon was likely formed after a Mars-sized planet crashed into the proto-Earth more than 4 billion years ago. English: Mare Imbrium gravity map (red=high, blue=low) From description in JMARS: "digital map of the gravity anomaly derived from the JPL GL0660B model of the Moon's gravity field. 4 Gyr of each other. Aristarchus. Lava flow margins on the Moon are scarce [1,2], and the Here we map volcanic units in Mare Imbrium using high-resolution (200 m/pixel), Earth-based P band data. 6 billion years ago and mare basin-localized contractional deformation ended by about 1. The ejecta blanket. 9 billion years. Mare Frigoris is the fifth largest and almost northernmost mare located on the near side of the Moon. . Describe the similari- ties and differences. 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. S. The near side of the Moon is the only one we see from Earth. Volcanoes used to erupt on the moon when it was young and temperamental, between about 4. 0 Sea of Showers Mare Ingenii 33. After the Apollo and Luna missions, which were flown about 40 years ago, the Moon was explored only from orbit. MARIA: Imbrium, Crisium, Serenitatis, Tranquillitatis, Nectaris, Oceanus Procellarum. 59. Other authors, however, have. The lunar phase is full moon or, maybe, waxing gibbous moon just before full moon. All these answers: its distance from the sun, its size, the fraction of light it reflects and its distance from earth. 0 and 1. The CE-3 landing site is in northern Mare Imbrium and several tens of meters away from the rim. Its peaks rise to heights of about 5 kilometers. Messier and Messier A together form one of the most striking crater pairs on the nearside of the Moon. The Fra Mauro region is hilly, widespread geological area covering large portions of the lunar surface. Description. It constitutes a classic example of a relatively young, well-preserved lunar impact crater. The chemical compositions of relatively young mare lava flows have implications for the late volcanism on the Moon. 12°N on the Moon on 14 December 2013, and it released the Yutu (Jade Rabbit) rover the next morning . Considering its flat topography, Sinus Iridum has been selected as one of the important candidate landing areas for the future Chinese robotic and human exploration missions, e. The onboard lunar penetrating radar conducted a 114-m-long. This week we will highlight Mare Imbrium, viewable throughout the week. 雨海 （ 拉丁語 ： Mare Imbrium ， 拉丁文 的意思是" 淋浴之海 "或" 雨之海 "）是 月球 上布滿整个雨海 撞击盆地 的辽阔 月海 ，也是 太陽系中最大的撞击坑 之一。. The suggestion as adopted officially. They cover 17 percent of the surface area of the Moon. 1. The large crater near the center of the image is the 20 km diameter Pytheas, at 20. Mare Imbrium: [±NW/F8] The Imbrium basin was created 3. 55. , 2011; Wu et al. Mare Imbrium, Latin for “sea of showers,” is the name of a huge crater on the moon caused by a meteor hitting the lunar surface some 3. The formation ages of mare ridges. It was named after ancient Greek philosopher Plato. Since age is the primary control on surface roughness for surfaces outside cratering equilibrium, it is valid to run the model. et al. On its north-west edge lies the 32 km wide Aristarchus ray crater, the brightest feature on the Near side of the Moon. The basin material is of the Lower Imbrian epoch, with the mare material being of the Upper Imbrian and Eratosthenian epochs. In the Lunar geologic timescale, the Late Imbrian epoch occurred between 3800 million years ago to about 3200 million years ago. PROCEDURE III: The mountain Piton The eastern edge of Mare Imbrium has an interesting, isolated lunar mountain called Mount Piton. Mare Imbrium basin on the moon - the Man in the Moon's right eye - might have been made by a protoplanet-sized impact, 3. In addition, no samples were returned from the young and high-FeO and TiO 2 mare basalt in the northern Imbrium basin. It is named after ancient Greek astronomer Eratosthenes of Cyrene, [1] who estimated the circumference of the Earth, and the. Oceanus Procellarum, Mare Imbrium, Mare Insularum, and Mare Vaporum, located on the north-western portion of the lunar nearside (0 – 43 N, 2 – 51 W, Fig. The solid white box corresponds to the area in Figure 4 . 0°N, 22. C. Fra Mauro is a widespread hilly geological area covering large portions of the lunar surface around Mare Imbrium, and is thought to be composed of ejecta from the impact which formed Imbrium. Comments. The shock of the Imbrium impact melted many rocks. Moon craters are bowl-shaped landforms created by two processes: volcanism and cratering. 1 W. Find answers for LifeAfter on AppGamer. A guide to the Moon's Archimedes Crater - BBC Sky at Night Magazine. Lunar sunrise will be advancing along the peaks and ridges of the range on International Observe the Moon Night, with only the northern portion illuminated. We performed new crater size-frequency distribution measurements in order to investigate the stratigraphy of mare. The. They named the marePage 1 of 2 - Plato and environs: Mare Imbrium’s Northeast Rim - posted in Lunar Observing and Imaging: Surely the northeast rim of Mare Imbrium comprises some of the most magnificent, complex and recognizable set of features on the lunar surface. Study with Quizlet and memorize flashcards containing terms like Identify the following features on the near side of the Moon. The Imbrium Basin, an ancient impact basin that has been infilled by impact and volcanic materials since its formation, dominates the morphology of this region. We already have an answer for a similar question which you can see here: Which of these is an incorrect description of "Mare Imbrium" on the moon? If you have more answers to add you can do that below. Mare Insularum / ɪ n s ʊ ˈ l ɛər ə m / (Latin īnsulārum, the "sea of islands") is a lunar mare located in the Insularum basin just south of the western Mare Imbrium. The maria contain physical features such as pits and channels. 1992), which. Introduction. On Dec. Thicknesses of mare basalts on the Moon from gravity. English: Mare Imbrium sits in the Imbrium basin. Mare Imbrium, the ‘Sea of Showers’ (named by Riccioli) is the dominant feature of the northwestern quadrant of the Moon. B. Which of these is an incorrect description of Mare Imbrium on the moon?. 2. The inset image was taken by the descent camera mounted on the CE3 lander, and the solid black lines are the rover path. Sinus Iridum is a flat mare region located to the northwest Mare Imbrium on the nearside of the Moon. Category. Which of these is an incorrect description of the “Battle of Poitiers”? The campaign took place during World War I: Which of these is an incorrect description of the “Mare Imbrium” on the moon? It contains a certain amount of sedimentary water. Selenography is the study of the surface and physical features of the Moon (also known as geography of the Moon, or selenodesy ). , Mare Frigoris, the northeastern units of Mare Imbrium) exhibit very low TiO 2 values. This image of the moon at first quarter was taken by a small telescope on the ground (the Automated Telescope Facility). Dark-floored, 95 kilometer wide crater Plato is just left of the center. 7°N, 14. GILBERT 1 proposed that a large-scale collision occurred in Mare Imbrium and this hypothesis has been supported by R. Hadley–Apennine is a region on the near side of Earth's Moon that served as the landing site for the American Apollo 15 mission, the fourth crewed landing on the Moon and the first of the "J-missions", in July 1971. At a nomenclature meeting Hal Masursky said, "Well, there can only be one ocean on the moon" ( Oceanus Procellarum ). lava. The diameter of Archimedes is the largest of any crater on the Mare Imbrium. After its successful launch at 01:30 local time on December 2, 2013, CE. 8–3. This week we will highlight Mare Imbrium, viewable throughout the week. rovers, both of which explored the northwestern part of Mare Imbrium. This image shows details of the Apennine Mountains along the southeastern rim of Mare Imbrium. Mare Frigoris has an elongated shape, with a length of approximately 1500 km and a width of. The near side of the Moon is the lunar hemisphere that always faces towards Earth, opposite to the far side. 8–3. It is located on the northeastern shore of the Mare Imbrium, at the western extremity of the Montes Alpes mountain range. The material surrounding the mare is of the Lower Imbrian epoch, while the mare. Mare Imbrium, which is the largest basin on the nearside of the Moon and is filled with several basalt units estimated to date from 3. However, geological mapping indicates that it is intermediate in age between the Imbrium and Nectaris Basins, suggesting an age of about 3. A nice example of a sinuous rille, interpreted as a lava channel (4), runs out of the crater onto the mare surface. The onboard lunar penetrating radar conducted a 114-m-long profile, which measured a thickness of ∼5 m of the lunar regolith layer and detectedthreeunderlying basalt units at depths of 195, 215. Constraining mare volcanic history therefore provides a window into theDescription Moon (M. The crater Copernicus is just visible in the bottom of the photo, while Plato is clearly seen on the. Messier is a markedly oval crater that. Wikimedia Commons has media related to Mare Imbrium. Which of these is an incorrect description of Mare Imbrium on the moon?. the giant Imbrium Basin (Mare Imbrium) to the north—the largest impact basin (mare) on the Moon’s near side. Located at 10° N, 20° W, near the southern rim of the Imbrium Basin (Mare Imbrium) impact structure, Copernicus measures 93 km (58 miles) in diameter and is a source of radial bright rays, light. 1 - 3. Locate Mare Imbrium. Let us take a closer look at Mare Imbrium. It is also witness to one of the most violent upheavals to have rocked the Moon, the creation. Com Which of these is an incorrect description of the “Battle of Poitiers”? The campaign took place during World War I: Which of these is an incorrect description of the “Mare Imbrium” on the moon? It contains a certain amount of sedimentary water: Which of these is an incorrect description of wind energy? It is not a form of renewable energy Which of these is an incorrect description of the “Battle of Poitiers”? The campaign took place during World War I: Which of these is an incorrect description of the “Mare Imbrium” on the moon? It contains a certain amount of sedimentary water. Is a lunar mare located in the Moon's Crisium basin, just northeast of Mare Tranquillitatis. 9 billion years ago when an asteroid 60 miles in diameter slammed into the Moon at 10 miles per second and blasted out a 720-mile-wide crater! It was at one time a spectacular multi-ring basin like Mare Orientale (Day 13). 3-3. g. 54. These results suggest that late-stage volcanic evolution of the Moon might be revised. It was named after Swiss polymath Johann Heinrich Lambert. 3 billion years ago (7 am on our clock). Description. The most spectacular of the Moon’s mountain ranges stretches for 600 km along the southeast rim of the Imbrium Basin. Chang’e 3 vided unprecedented data sets of the Moon wlander and lunar rover Yutu landed in Mare Imbrium (44. This crater is bowl-shaped, with a small interior floor at the midpoint and a somewhat eroded outer rim. Figure 3: Lunar Mountain and Lunar Maria. The moon is by far the most luminous object in the night sky. Letronne/Hansteen. Mare Imbrium (37 N, 18. which covers the Moon at a 1:5,000,000 scale (fig. Figure 9. Stories of the Moon Apollo: The Epic Journey to the Moon. Single Frame of Mare Imbrium . Click the card to flip 👆. The LLM-1 Lunar Module (LM) lander would alight on a flat, relatively smooth basaltic plain known as a mare (Latin for "sea"). Its site functions include research, specialized containment and remote observation.