lava. 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. Category. - DannyCaes Jan 1,. 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. This was the first soft landing on the Moon since the Soviet Union’s Luna 24 mission in 1976 and is a new landing site in the north part of the Mare Imbrium (fig. New analysis of zircon grains in one lunar sample. A seminal cartographic achievement, this is the first Earthside Stereographic map of the Moon produced by the Army Map Service in anticipation of the lunar landing missions of the late 1960s. Lunar Orbiter IV imaged the Moon during May of 1967. 1–4. The last image of the moon captured by Lucy portrays Mare Imbrium, an ancient, lava-filled impact basin on the lunar terrain where the Apollo 15 mission made its landing in 1971 (the. , with all other units younger than 3. The highest TiO 2 values were found in Mare Tranquillitatis (∼12. 2. The chemical compositions of relatively young mare lava flows have implications for the late volcanism on the Moon. 7. 2 Ga, therefore, providing insights into the thermal and volcanic history of the Moon. The term, which in Latin means “sea,” was erroneously applied to such features by telescopic observers of the 17th century. Introduction. Find answers for LifeAfter on AppGamer. Features: This is an image Moon map with labels. However, geological mapping indicates that it is intermediate in age between the Imbrium and Nectaris Basins, suggesting an age of about 3. This oblique photograph was taken looking south across Mare Imbrium. The basin material is of the Lower Imbrian epoch, with the mare material being of the Upper Imbrian and Eratosthenian epochs. Sea of Crisis. It is a lava produced by an eruption on the Moon more than 3 billion years ago. A single frame Lucy image of the Mare Imbrium shows a roughly 600-mile wide portion of lunar terrain. Oceanus Procellarum, Mare Imbrium, and Mare Serenitatis) within 0. The Sinus Iridum basin (latitude 45° North. . The old, heavily cratered lunar highlands make up 83% of the Moon’s surface. The shock of the Imbrium impact melted many rocks. D. The oldest ages for returned lunar mare basalts are from Apollo 14 breccias; aluminous low-Ti basaltic clasts in these breccias range in age from 3. These results suggest that late-stage volcanic evolution of the Moon might be revised. Detail map of Mare Imbrium's features. The suggestion as adopted. , 2011; Wu et al. 3 billion years ago (Ga) and then declined or disappeared by 2. 8N 15. 6 billion years ago and mare basin-localized contractional deformation ended by about 1. The flow field originates in the southwest part of the basin from a fissure or series of fissures and cones located in the vicinity of Euler crater and erupted in three phases. g. 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. About 3. This week we will highlight Mare Imbrium, viewable throughout the week. 9 billion years ago when an asteroid 60 miles in diameter slammed into the Moon at 10 miles per. Situated within the heat-producing potassium, rare earth element, and phosphorus terrane, Mare Imbrium experienced some of the most long-lived (and recent) lunar volcanism, and its surface exhibits a significant diversity of basaltic chemistry. Oceanus Procellarum (/ oʊ ˈ s iː ə n ə s ˌ p r ɒ s ɛ ˈ l ɛər ə m / oh-SEE-ə-nəs PROSS-el-AIR-əm; from Latin: Ōceanus procellārum, lit. Users: In these collections Moon About. 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. : Mare Imbrium. The extent of the cratered highlands on the far side is very apparent. between the solar-illuminated and dark hemispheres. All these answers: its distance from the sun, its size, the fraction of light it reflects and its distance from earth. Hadley on the edge of Mare Imbrium was taken by Dave Scott, one of the Apollo 15 astronauts. That is, if a crater (or its ejecta) overlaid another, it must be the younger. On the Moon, we compare the dimensions of wrinkle ridges in the mascon basins (Mare Crisum, Mare Serenitatis, Mare Imbrium, Mare Humorum, and Mare Necataris) to wrinkle ridges in non-mascon settings. 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. 57. The following images illustrate three features from the surface of Mercury: (1) a large impact basin that is similar to Mare Imbrium on the Moon, (2) the highlands of Mercury, (3) and an example of a large geological fault. As a consequence, the surface of Mercury looks superficially like the Moon, but there are. Sinus Iridum. Samples from Mare Imbrium and the Ocean of Storms brought back by Apollo 11 and Apollo 12 are about 3. Rimmed grooves, lineations and elongate craters around Mare Imbrium shape much of the nearside Moon. W. 53b. The innermost raised ring is marked by isolated ridges and peaks within Mare Imbrium itself, including in the Plato. 7 N, 13. Thiessena,b, S. They cover 17 percent of the surface area of the Moon. SCP-3609 was identified following the Foundation's establishment of Lunar Area-32 in Mare Imbrium on / /1998. Figure 3: Lunar Mountain and Lunar Maria. 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. 9 billion years. The shock of the Imbrium impact melted many rocks. 9W 513. 0 Ga. Caroline Herschel was still winning. GameStop Moderna Pfizer Johnson & Johnson AstraZeneca Walgreens Best Buy Novavax SpaceX Tesla. Till now, three lunar missions, USSR’s Luna 17, American Apollo 15 and Chinese Chang’E-3, have successfully soft-landed and conducted surface investigation at this basin. The results of geochemical analyses of major and trace elements as well as isotopic ratios require the source reservoir for the mare basalts to be the mafic cumulates from the base of the lunar mantle (Walker et al. It begins just to the west of the prominent crater Eratosthenes, which abuts against the southern face of the range. 1 and 4. 251, has incorporated additional refinements (table 7. -This photo taken at low Sun angle emphasizes how common secondary impact craters are on the Moon. The origin of the Moon's craters as impact features became widely accepted only in the 1960s. 6 wt%) and Oceanus Procellarum (∼11. 0 Ga. Mare Nubium / ˈ nj uː b i ə m / (Latin nūbium, the "sea of clouds") is a lunar mare in the Nubium basin on the Moon's near side. 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. Here, employing UV-VIS data from the Clementine mission, we estimate mare thickness values in the Imbrium Basin by analyzing ejecta from large. 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. 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. Obique view looking west of Alpine Valley and Mare Imbrium on the Moon taken by Lunar Orbiter 5. 9 to 4. [1] The total volume of extrusive volcanism on the Moon provides a basic thermal and geologic constraint, and accurate volume assessments are contingent upon constraining lava flow depths. It was hoped that samples collected from these mountains would include ancient rocks that originated deep in the Moon's crust. The crater Copernicus is just visible in the bottom of the photo, while Plato is clearly seen on the. The valley is narrow at both ends and widens to about 10. Published: September 14, 2012. Team Moon: How 400,000 People Landed Apollo 11 on the Moon Earth and the Moon. Basaltic lava later flooded the giant crater to form the. This. Such samples are important to understand the formation and evolution of the Procellarum KREEP. The most spectacular of the Moon’s mountain ranges stretches for 600 km along the southeast rim of the Imbrium Basin. 2. The Fra Mauro region is hilly, widespread geological area covering large portions of the lunar surface. 61. 7. This large multi-ring impact basin is characterized by prolonged lunar volcanism ranging from the Imbrian age to the Eratosthenian period, forming the high-Ti mare unit, low-Ti mare basalts, and very low-Ti mare unit. SCP-2686 is itself not visibly biologically anomalous, though has claimed in past interviews to possess anomalous. On the Moon, mare basalt covers ~15% of the nearside and ~1% of the farside surface [Nelson et al. Note the old fractured terrain at the right and smoother textured and ridged mare terrain at center. Plain Language Summary The Chang'e‐3 spacecraft, which landed on the northern Mare Imbrium on the near side of the Moon, was equipped with lunar penetrating radar (LPR) on the Yutu rover and. Its youthfulness is confirmed by the freshness of the crater floor deposits and the characteristic shape of these deposits. Copernican‐age craters are among the most conspicuous features seen on the far side and western limb of the Moon in the Galileo multispectral images acquired in December 1990. This suggests that the infill history of the basin was punctuated and. pdf from AST 101 at Otero Junior College. The results of geochemical analyses of major and trace elements as well as isotopic ratios require the source reservoir for the mare basalts to be the mafic cumulates from the base of the lunar mantle (Walker et al. They were named by astronomer Johann Heinrich. The high-Th values of Aristillus impact ejecta and Timocharis crater ejecta, both located in the maria, show high Th even though the mare is many hundreds of me-ters thick. Before the Apollo missions landed humans on the Moon, NASA sent. 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. Mare Imbrium. Image #3 is from the Lunar Orbiter IV. Sinus Iridum is a flat mare region located to the northwest Mare Imbrium on the nearside of the Moon. Scientists say the asteroid was three times. 2 ). Did it land in a low area, or a high area? (2 points) Question #10: Compare the average elevation of the near-side of the Moon to that of the far. This pattern was coined the Imbrium Sculpture 1,. The Lunar Orbiter image has been subjected to a fast Fourier transformation in order to remove the stripes and has been map-projected. *Email: hughscot@isu. 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. Mare, any flat, dark plain of lower elevation on 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. Armstrong scanned the jumbled mare for a safe place to land. 5° N, 24. 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. Scientists investigated the area surrounding Mare Imbrium — Latin for "The Sea of Showers. It was named after ancient Greek philosopher Plato. 1007/978-1-4614-9213-9_226-1 # Springer Science+Business Media New York 2014These are substantial even in comparison with the well-studied mare Imbrium lobes, which range between 40 and 65 m 33,34. Credit: NASA/GSFC/Arizona State University. The near side of the Moon is the only one we see from Earth. Mare Frigoris / f r ɪ ˈ ɡ ɔːr ɪ s / (Latin frīgōris, the "Sea of Cold") is a lunar mare in the far north of the Moon. It is one of the largest craters on the moon. Single frame of Mare Imbrium. One of the loveliest features of the Moon has to be Sinus Iridum, which leads off the vast Mare Imbrium. The name is also applied to the extensive surrounding region, called the Fra Mauro Formation, which lunar scientists interpret to be material ejected from the impact that formed the giant Imbrium Basin (Mare Imbrium) to the north—the largest impact basin on the Moon’s near side. Lunar mare. The tech-141Copernicus, one of the most prominent craters on the Moon. The formation ages of mare ridges. , 2014]. The Imbrium basin was dated to be from 3. Copernicus is one of the most noticeable craters on the Moon. 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. Published: October 5, 2017. The Humorum basin is filled with a thick layer of mare basalt, believed to exceed 3 kilometers. Thicknesses of mare basalts on the Moon from gravity. Because of its small size, the Moon cooled quickly and was mostly dead volcanically Apollo 15 metric camera image of Southeastern Mare Imbrium. Mountain ranges with peaks up to 5500 meters above the mean lunar radius ( Montes Apenninus in the S-SE) define most of the circular morphology of the basin. 8 billion years ago. In the mare to the south are several rises collectively named the Montes Teneriffe. 85 Ga (Ryder, 1992,. Examine the images of the near and far sides of the moon on the website. 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. 830 000 km 2, it is. To prove him wrong, I suggested that a large expanse with a lot of terra islands be named Oceanus Insularum. Only one lunar basin, Imbrium, is generally agreed to be well dated at 3. On its north-west edge lies the 32 km wide Aristarchus ray crater, the brightest feature on the Near side of the Moon. Gruithuisen. 1 inches) long and is representative of the mare lavas that filled the basin 3. 0°N, 22. Team Moon: How 400,000 People Landed Apollo 11 on the Moon Earth and the Moon. Add your answer. The Moon is directly illuminated by the Sun, and the cyclically. 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. Alpine Valley is a sinuous rille, about 150 km long and 8 km wide running vertically through the center of the image. As an example, the age of the Imbrium Basin, filled with the ‘lunar sea’, the Mare Imbrium (visible in the top left of the Moon), which was probably created by the collision of an asteroid. The results of geochemical analyses of major and trace elements as well as isotopic ratios require the source reservoir for the mare basalts to be the mafic cumulates from the base of the lunar mantle (Walker et al. -D. English: Original description: Southward looking oblique view of Mare Imbrium and Copernicus crater on 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. The area is primarily composed of relatively low ridges and hills, between which exist undulating valleys. 1975; Shih and Schonfeld 1976; Taylor 1982; Snyder et al. English: Mare Imbrium sits in the Imbrium basin. 9 billion years. 0 Sea of Cleverness Mare Insularum 7. 1214°N, 340. Full description: "Southward looking oblique view of Mare. 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. which covers the Moon at a 1:5,000,000 scale (fig. 7 N, 20. -. 1 Ga (Neukum and Ivanov, 1994) to ∼3. 0°W. 0; -13. Mission planners chose. A map in orthographic projection, centered at 34. 5. The goal of the GRAIL mission was to map the Moon's gravity field in unprecedented detail in order to understand the structure of the lunar interior, place limits on the size of the Moon's core, and determine the subsurface structure of the lunar crust. •The Alpine Valley cuts through the Alpes Mountains near the 1 o'clock position around the Imbrium Basin. Moon craters are bowl-shaped landforms created by two processes: volcanism and cratering. Mare Imbrium is the dark, flat feature at the top. Figure 9. 1. Archimedes crater is the largest formation on Mare Imbrium. Scott and Mr. 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) -. Since age is the primary control on surface roughness for surfaces outside cratering equilibrium, it is valid to run the model. maxima. The crater is 107 km in diameter and is centered at 9. The Apollo 15 landing site is by far one of the most interesting that you can find on the surface of the Moon. ,. 0 N, longitude = 24 . 1 inches) long and is representative of the mare lavas that filled the basin 3. The setting of this sci-fi book is the hills of Mare Imbrium on the moon. As the development of space exploration technology, lunar gravity data has advantages of high accuracy and resolution, which can be used to invert the lunar crust and upper mantle. Irwin touched down, is a vast lava plain and impact crater that formed about 3. During. 3). The best developed lava flows on the Moon occur in Mare Imbrium where flow margins are traceable nearly their entire flow length. of the Moon have been computed, after applicationThe name Mare Insularum refers to the many islands of terra material in the mare. 4 billion years ago), the highlands are also extremely heavily cratered, bearing the scars of all those billions of years of impacts by interplanetary debris (Figure 9. North is at 4:00. This paper compares the morphology and relative ages of circular basins 300 km wide or wider and examines the relations between these basins and mare material on both the near and far sides of the Moon. I. Smith 1 Britney Smith 3-12-22 N/A Moon Observations 2-14-22 1. Yes. The Moon showing Mare Imbrium Another of the primary goals of the Apollo 15 mission was an examination of Hadley Rille, a channel-like depression in the lunar surface. Click the card to flip 👆. 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. However, the lunar ____ ("seas") are relatively recent features. C. the Moon formed from the impact of a rogue planet striking the Earth. 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. 8–3. 1 W, is partly visible at upper left. It constitutes a classic example of a relatively young, well-preserved lunar impact crater. 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. The Imbrium basin is one of the most prominent geologic units on the lunar nearside, and also significant exploration target for soft-landing missions. 3 Ga [e. The sea. In the mare to the south are several rises collectively named the Montes Teneriffe. There are hundreds of thousands of moon craters ranging from less than a mile across to giant basins called mare, which were once thought to be seas. (b) About 17% of the Moon’s surface consists of the maria—flat plains of basaltic lava. 49°E, 44. C. The structure of the regolith and those underneath young periods (Eratosthenian) and old periods (Imbrian). Their surface morphology is mare-like (“characterized by ‘ponded’ appearance” [Schafer 1981 ]), while their. The paler areas are the lunar highlands, and the darker areas are the lunar 'seas' or maria (singular: mare). The Earth, the Moon, and the other planets are the targets of a continuing bombardment of asteroids and comets from outer space. 2 ). About 3. , 2011), suggesting a long volcanic history for Mare Imbrium. The moon is by far the most luminous object in the night sky. The formation ages of tectonic structures and their spatial distributions were studied in the northwestern Imbrium and Sinus Iridum regions using images obtained by Terrain Camera and Multiband Imager on board the SELENE spacecraft and the images obtained by Narrow Angle Camera on board LRO. Bliss (crater) / 53. You will learn about the nearest planetary body to Earth, the long record of cratering on its surface, and about the ancient eruptions that flooded many low-lying areas. With an area of c. Lunar olivine basalt formed around 3. An excellent description of the basins on the near side of the Moon is that of Hartmann and Kuiper (1962). Messier is a markedly oval crater that. Mare Frigoris. 3 billion years ago (Ga) and then declined or disappeared by 2. To the north lies the wide. This crater is bowl-shaped, with a small interior floor at the midpoint and a somewhat eroded outer rim. A broad, shallow valley within the formation. In Fra Mauro. The solid white box corresponds to the area in Figure 4 . , 2018). I. The Moon is a key location for studying the geological evolution of planetary impact basins. Each point gives the Lunar gravity anomaly in milligals, which is the difference of the model gravity on the geoid from the gravity on a reference sphere with. Let us take a closer look at Mare Imbrium. Which of the above was the site where the first humans walked on the moon (Apollo 11 Mission:. 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 _____________. The. material around Mare Imbrium now given such rock-stratigraphic names as the Fra Mauro Formation (table 4. It is, therefore, the most magnetic region on the Moon. , Basaltic Volcanism Study Project (), 1981; Stöffler and Ryder, 2001; Taylor, 1982, and references therein]. On the basis of crater morphology measurement, Boyce, 1976, Boyce. Bliss (crater) / 53. Bugiolacchi et al. During their three-day stay on the Moon, Scott and Irwin traversed over 28km in the lunar rover – the first time a vehicle had been driven on the Moon's surface. GILBERT 1 proposed that a large-scale collision occurred in Mare Imbrium and this hypothesis has been supported by R. A powerful description of surroundings and life on the moon along with enjoyable characters and action kept my interest high all the way to the end. The Plato quadrangle in the north-central part of the Moon lies within a series of concentric depressed and raised rings surrounding the Imbrium basin, the center of which lies about 335 km southwest of Montes Teneriffe. e. On 14 December 2013 (UTC), China’s Chang’E-3 (CE-3) succeeded in landing on the Moon’s surface. SCI 1301 Assignment 11: Meteorite Impacts and the Late Heavy Bombardment Mare Imbrium 1145 km Rocky 25. Hadley Rille is located in the Montes Apenninus mountain range. 8 billion years ago. Oceanus Procellarum and Mare Imbrium, located in the north-western region of the lunar nearside, are the largest maria on the lunar surface and have experienced multiple episodes of large-scale volcanic eruptions and basaltic lava flow filling. Stuart Ross Taylor, in Encyclopedia of the Solar System (Second Edition), 2007. 49°E, 44. along the equator, between northern and southern. et al. Plato is a lava-filled lunar impact crater on the Moon. 1). In actuality, maria are huge basins containing lava flows marked by craters, ridges, faults, and straight and. The solid white box corresponds to the area in Figure 4 . The CE-3 landing site is in northern Mare Imbrium and several tens of meters away from the rim. ] [ 67] Areas of mare material occupy about 15 percent of the Moon's total surface. Mare Imbrium: [±NW/F8] The Imbrium basin was created 3. 9 Lunar Maria. 9–2. The LLM-1 Lunar Module (LM) lander would alight on a flat, relatively smooth basaltic plain known as a mare (Latin for "sea"). Thorium map of the Moon A map of the thorium content of the lunar surface based on Lunar Prospector data shows that a large area on the nearside of the Moon, including the Imbrium basin and Oceanus Procellarum, is enriched in thorium relative to the rest of the Moon. 3 Ga [e. There is also an area of enriched thorium on the farside, within the. It was not sampled by the Apollo program, so a precise age has not been determined. This month’s full. [Base map courtesy of the National Geographic Society. About 17% of the Moon’s surface consists of the maria—flat plains of basaltic lava. The image covers an area 15. Some investigators, however,. •This image provides an overview of the Mare Imbrium region, which occupies the upper left portion of the image. Gilbert, 1893, Stadermann et al. The Moon’s Long Memory. These features, known as the. At Knowth, a Neolithic site in County Meath, Ireland, for example, a 5,000-year-old rock carving depicts what appears to be Mare Imbrium, Mare Frigoris, and Mare Serenitatis, the Moon’s volcanic. 8 billion years ago. Bliss is small lunar impact crater that is located just to the west of the dark-floored crater Plato. Study with Quizlet and memorize flashcards containing terms like Identify the following features on the near side of the Moon. Wikimedia Commons has media related to Mare Imbrium. A guide to the Moon's Mare Imbrium and Sinus Iridium - BBC Sky at Night Magazine. In the foreground is Mare Imbrium, peppered with secondary crater chains and elongated craters due to the Copernicus impact. Southward view; in the background is Copernicus crater visible (near the horizon). Messier and Messier A together form one of the most striking crater pairs on the nearside of the Moon. The maria, which appear as mottled gray areas on the moon's white. Basalt from the Moon. Lunar Orbiter IV imaged the Moon during May of 1967. Both sites are within the dis- tinctive Eratosthenian-aged lava flow geologic unit and our comparisons showed that the. A broad, shallow valley within the formation about 50 km (30 miles). 3-3. Find answers for Survivors: The Quest® on AppGamer. (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. Smaller mare patches also occur in the floors of some. Now, there seems to be a man's face too, made by the combination of Mare Imbrium and Sinus Iridum. 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. 3 billion years. 1 / 15. Its site functions include research, specialized containment and remote observation. Kepler. The Sinus Iridum basin formed on the rim of the larger Imbrium basin, and provides an opportunity to investigate the interaction between mare basalt flows originating in different basins. The spacecraft and rover landed at the northern boundary of one of the best preserved flow fields on the lunar surface. The Latin word for it is Mare Imbrium. 5 × 10 −6 km 2 of basaltic flows that make up the lunar maria [Head, 1975] represent the most fundamental exogenic process to have resurfaced the face of the Moon. 8 billion years ago. Lunar mountains. The map was produced by the Army Map. A patchwork of stained and pasted bits of paper, the surface of Grossman’s collage captures the earth-bound view of light and shadows that cross the ancient. 5 in (130. Which of these is an incorrect description of Mare Imbrium on the moon?. Its diameter is 674 km (419 mi). Description. g. 7 N,. 85 Ga (e. 56. the giant Imbrium Basin (Mare Imbrium) to the north—the largest impact basin (mare) on the Moon’s near side. The description of maps and DEMs used for the regional geologic details of the 29 locations as. This location is designated as SCP-2686-1 and is detailed below. The landing site of the Apollo 14 mission in the Fra Mauro region. 3 b. Figure 3: Lunar Mountain and Lunar Maria. SCP-2686 is itself not visibly biologically anomalous, though has claimed in past interviews to possess anomalous.