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Chicxulub crater (8,252 words) [view diff] exact match in snippet view article find links to article

The Chicxulub crater (/tʃiːkʃuːˈluːb/ cheek-shoo-LOOB; Spanish: [tʃikʃuˈlub] ) is an impact crater buried underneath the Yucatán Peninsula in Mexico. Its

This is a partial list of craters on Mars. There are hundreds of thousands of impact craters on Mars, but only some of them have names. This list here

This is a list of craters on Mars. There are hundreds of thousands of impact craters on Mars, but only some of them have names. This list here contains

Impact craters in the Solar System An impact crater is a depression in the surface of a solid astronomical body formed by the hypervelocity impact of a

This is a partial list of craters on Mars. There are hundreds of thousands of impact craters on Mars, but only some of them have names. This list here

(crater) Debus (crater) Delporte (crater) Dyson (crater) Ellerman (crater) Emden (crater) Esnault-Pelterie (crater) Finsen (crater) Fleming (crater) Fowler

Crater Lake (Klamath: Giiwas) is a volcanic crater lake in south-central Oregon in the Western United States. It is the main feature of Crater Lake National

heavily cratered, with one of the craters near the equator having a central peak despite the moon's small size. The most prominent of these is the crater Stickney

Lunar craters are impact craters on Earth's Moon. The Moon's surface has many craters, all of which were formed by impacts. The International Astronomical

impact structure is the largest verified impact structure on Earth. The crater, which has since been eroded away, has been estimated at 170–300 kilometres

around 1.3 million years and has a long-lived lava lake in its inner summit crater that has been present since at least the early 1970s. On 28 November, 1979

started in Eagle crater in 2004, literally landing inside on the crater basin, then it travelled outward making its way to Endurance crater. After this it

Crater Lake National Park is a national park of the United States located in southern Oregon. Established in 1902, Crater Lake is the fifth-oldest national

Meteor Crater, or Barringer Crater, is an impact crater about 37 mi (60 km) east of Flagstaff and 18 mi (29 km) west of Winslow in the desert of northern

an impact crater in a solid planet or moon may be measured from the local surface to the bottom of the crater, or from the rim of the crater to the bottom

The Battle of the Crater took place during the American Civil War, part of the Siege of Petersburg. It occurred on Saturday, July 30, 1864, between the

(secondary coordinates) This list of impact structures (including impact craters) on Earth contains the majority of the 194+ confirmed impact structures

to dozens of kilometers in diameter). Although sometimes described as a crater, the feature is actually a type of sinkhole, as it is formed through subsidence

A volcanic crater lake is a lake in a crater that was formed by explosive activity or a collapse during a volcanic eruption. Lakes in calderas fill large

A volcanic crater is an approximately circular depression in the ground caused by volcanic activity. It is typically a bowl-shaped feature containing one

the 15.6-kilometre-diameter (9.7 mi) Karzok crater and the 10.4-kilometre-diameter (6.5 mi) Pangboche crater. They are two of several suspected source areas

1,624 craters (31.2%)   Martian: 1,092 craters (21.0%)   Venusian: 900 craters (17.3%)   Mercurian: 397 craters (7.6%)   Others: 1,198 craters (23.0%)

Gale is a crater, and probable dry lake, at 5°24′S 137°48′E / 5.4°S 137.8°E / -5.4; 137.8 in the northwestern part of the Aeolis quadrangle on Mars

A crater chain is a line of craters along the surface of an astronomical body. The descriptor term for crater chains is catena /kəˈtiːnə/, plural catenae

A concentric crater fill (CCF) is a landform where the floor of a crater is mostly covered with many parallel ridges. It is common in the mid-latitudes

crater Erebus crater Fram crater Naturaliste crater Nereus crater Santa Maria crater Victoria crater Cape Verde Vostok crater Block Island meteorite Bounce

is a crater on Mars in the Syrtis Major quadrangle, about 45.0 km (28.0 mi) in diameter. Thought to have once been flooded with water, the crater contains

impact crater on Mars, approximately 19 kilometers in diameter. It is located at 29.3°S, 103.8°W, north of the crater Virrat and northeast of the crater Dinorwic

impact crater on Mars, southwest of the crater Dinorwic and northeast of Clantas Fossae. Several Virrat crater radii to the north are the craters Koga and

Lomonosov is a crater on Mars, with a diameter close to 150 km. It is located in the Martian northern plains. Since it is large and found close (64.9°

80 km. It begins at the crater Béla, an elongated formation with the long axis oriented to the northwest. Four small craters near this rille have been

Puńsk is an impact crater on Mars, located in the Oxia Palus quadrangle at 20.8° N and 41.2° W. It measures 11.6 kilometers in diameter and was named after

Arusha Region, within the Crater Highlands geological area of northeastern Tanzania. The area is named after Ngorongoro Crater, a large volcanic caldera

Heimdal is a relatively recent impact crater on the planet Mars. It is a simple crater which lies in Vastitas Borealis, the northern plain. It is named

is a crater in the Ismenius Lacus quadrangle on Mars with a diameter of 130 km. It lies in the northern hemisphere south of the very large crater Lyot

Galle is a crater on Mars. It is located on the eastern rim of the huge impact basin Argyre Planitia in Argyre quadrangle. It is named after the German

is a crater on the planet Mars and is located at 14°30′S 175°24′E / 14.5°S 175.4°E / -14.5; 175.4 and is in the Aeolis quadrangle. The crater is about

Victoria is an impact crater on Mars located at 2.05°S, 5.50°W in the Meridiani Planum extraterrestrial plain, lying situated within the Margaritifer Sinus

Chincoteague is an impact crater in the Cebrenia quadrangle of Mars, located at 41.5° N and 236.0° W. It was named after Chincoteague, a town in Virginia

Escalante Crater is an impact crater in the Amenthes quadrangle of Mars. It is located at 0.2° N and 244.7° W. It is 79.3 km (49.3 mi) in diameter, and

Mädler is a crater on Mars. It was named in honor of the German astronomer Johann Heinrich Mädler by the IAU in 1973. Mädler and collaborator Wilhelm Beer

Burroughs is a large crater on Mars at latitude 72.5S / longitude 243.1W, with a diameter of 104.0 kilometres (64.6 mi). The crater is named after Edgar

Slipher is an impact crater in the Thaumasia quadrangle of Mars, located at 47.3°S latitude and 84.6°W longitude. It measures 127 kilometres (79 mi) in

Holden is a 140 km wide crater situated within the Margaritifer Sinus quadrangle (MC-19) region of the planet Mars, located with the southern highlands

Beer is a crater lying situated within the Margaritifer Sinus quadrangle (MC-19) region of the planet Mars, named in honor of the German astronomer, Wilhelm

Crommelin is an impact crater in the Oxia Palus quadrangle of Mars, located at 5.1°N latitude and 10.2°W longitude. It is 113.9 km in diameter. It was

Bernard is a large crater in the Memnonia quadrangle of Mars, located at 23.4° south latitude and 154.2° west longitude. It is 128 km in diameter and was

A Ring mold crater is a kind of crater on the planet Mars that looks like the ring molds used in baking. They are believed to be caused by an impact into

Bonneville is an impact crater on Mars. It is located within the much larger crater Gusev. Bonneville was visited by the Mars Exploration Rover Spirit

Crommelin is an impact crater in the Oxia Palus quadrangle of Mars, located at 5.1°N latitude and 10.2°W longitude. It is 113.9 km in diameter. It was

Saheki is a crater on Mars, located in the Iapygia quadrangle at 21.75° S and 286.97° W. It measures approximately 82 kilometers in diameter and was named

Sunset Crater is a cinder cone located north of Flagstaff in the U.S. state of Arizona. The crater is within the Sunset Crater Volcano National Monument

Erebus is a crater lying situated within the Margaritifer Sinus quadrangle (MC-19) region of the planet Mars, this extraterrestrial geological feature

impact crater on Mercury. With a diameter of 716 km it is the second-largest impact basin on the planet, after Caloris, and is one of the larger craters in

Main is an impact crater on Mars, located in the Mare Australe quadrangle at 76.6°S latitude and 310.9°W longitude. It measures 109.0 kilometers in diameter

Martian impact crater, approximately 22.99 kilometres (14.29 mi) in diameter. It is located at -31.1°S, 100.8°W, southeast of the crater Dinorwic and northeast

Impact craters generally have a rim with ejecta around them, in contrast volcanic craters usually do not have a rim or ejecta deposits. As craters get larger

Penticton is an impact crater in the Hellas quadrangle of Mars, located at 38.35° south latitude and 263.35° west longitude. Penticton is on the eastern

Korolev is an ice-filled impact crater in the Mare Boreum quadrangle of Mars, located at 73° north latitude and 165° east longitude. It is 81.4 kilometres

craters", Yuty-type craters have also been called petal or flower craters and fluidized ejecta craters. More commonly they are called rampart craters

Vishniac is the larger crater of the Martian surface feature called the Giant's Footprint. It was named after Wolf V. Vishniac, a microbiologist who died

The Chesapeake Bay impact crater is a buried impact crater, located beneath the mouth of Chesapeake Bay, United States. It was formed by a bolide that

Emma Dean is a small impact crater in the Meridiani Planum extraterrestrial plain situated within the Margaritifer Sinus quadrangle (MC-19) region of the

Lyot is a large peak ring crater in the Vastitas Borealis region of Mars, located at 50.8° north latitude and 330.7° west longitude within the Ismenius

Huygens is an impact crater on Mars named in honour of the Dutch astronomer, mathematician and physicist Christiaan Huygens. It is the fifth largest recognizable

Impact craters generally have a rim with ejecta around them, in contrast volcanic craters usually do not have a rim or ejecta deposits. As craters get larger

identified. Many craters once contained lakes. Some craters in Tikhonravov are classified as pedestal craters. A pedestal crater is a crater with its ejecta

Copernicus is a large crater on Mars, with a diameter close to 300 km. It is located south of the planet's equator in the heavily cratered highlands of Terra

Asimov Crater is an impact crater in the Noachis quadrangle of Mars, located at 47.0° S and 355.05° W. It is 84.0 km (52.2 mi) in diameter and was named

Santa Maria is an impact crater on Mars, located at 2.172°S, 5.445°W within the Meridiani Planum extraterrestrial plain, lying situated within the Margaritifer

Boeddicker is a crater in the Aeolis quadrangle of Mars, located at 15° south latitude and 197.7° west longitude. It is 109 km in diameter and was named

Miyamoto is a crater within the Margaritifer Sinus quadrangle (MC-19) region of the planet Mars, west of the Plains of Meridiani. It is 150 kilometers

Grindavik is an impact crater in the Oxia Palus quadrangle of Mars, located at 25.39° North and 39.07° West. It is 12 km (7.5 mi) in diameter and was named

Janssen Crater is an impact crater in the Arabia quadrangle on Mars at 2.7° N and 322.4° W. and is 154 km in diameter. Its name was approved in 1973, and

Endurance is an impact crater lying situated within the Margaritifer Sinus quadrangle (MC-19) region of the planet Mars. This crater was visited by the Opportunity

Joly is an impact crater on Mars, located at 74.7°S latitude and 42.7°W longitude in the Mare Australe quadrangle. It measures 79.9 kilometres (49.6 mi)

Denning Crater is a large Noachian-age impact crater in the southwestern Terra Sabaea region of the southern Martian highlands, within the Sinus Sabaeus

Beethoven is a crater at latitude 20°S, longitude 124°W on Mercury. It is 630 km in diameter and was named after Ludwig van Beethoven. It is the eleventh

were found in Vernal crater. MOLA map showing Vernal Crater and other nearby craters. Colors indicate elevations. Vernal Crater, as seen by CTX camera

Zunil is an impact crater near the Cerberus Fossae on Mars, with a diameter of 10.26 kilometres (6.38 miles). It is named after the town of Zunil in Guatemala

is a crater on Mars located at 46°N 0°E on the fringe of Acidalia Planitia near Arabia Terra. It is approximately 48 km in diameter. The crater's name

Apollo, also called the Apollo basin, is a large impact crater located on the far side of the Moon, in the southern hemisphere. It was previously known

Baltisk is a crater in the Argyre quadrangle of Mars. It was named after a town in Russia in 1976. Baltisk is located on the western edge of the Argyre

Gasa is an impact rayed crater in the Eridania quadrangle on Mars at 35.68° S and 230.72° W. and is 6.5 km in diameter. Its name was approved in 2009,

Bamberg is an impact crater in the Mare Acidalium quadrangle of Mars. It is named after the town Bamberg in Germany. CTX images and HiRISE images from

Cassini is a crater on Mars named in honour of the Italian astronomer Giovanni Cassini. The name was approved in 1973, by the International Astronomical

Beagle is a crater lying within the Margaritifer Sinus quadrangle (MC-19) portion of the planet Mars, the crater is one of multiple topographical depressions

Dawes Crater is located in the Sinus Sabaeus quadrangle of Mars, at 9.2 S and 38 E. It is about 191 km (119 mi) in diameter, and was named after William

Columbus is a crater in the Terra Sirenum of Mars. It is 119 km in diameter and was named after Christopher Columbus, Italian explorer (1451–1506). The

Ptolemaeus is a crater on Mars, found in the Phaethontis quadrangle. It measures approximately 165 kilometers in diameter and was named after Claudius

Dinorwic is a Martian impact crater, approximately 51 kilometers in diameter. It is named after the town in Ontario, Canada. Its name was approved by the

satellite crater Davy Y to the east, a formation which contains a crater chain designated Catena Davy. To the southeast of Davy is the prominent crater Alphonsus

Reynolds is an impact crater on Mars, located in the Mare Australe quadrangle at 75.1°S latitude and 157.9°W longitude and is in the southernmost portion

is a 150 km × 125 km (93 mi × 78 mi) crater at 35.7°S, 323.4°E on Mars, just north of Argyre basin. The crater is in the Argyre quadrangle. It was named

Becquerel is a 167 km-diameter crater at 22.1°N, 352.0°E on Mars, in Arabia Terra in Oxia Palus quadrangle. It is named after Antoine H. Becquerel. Photographs

Cruls is an impact crater in the Eridania quadrangle on Mars at 42.91° S and 163.03° E. and is 87.89 km in diameter. Its name was assigned in 1973 by the

Green is an impact crater in the Argyre quadrangle of Mars. It is named after Nathan E. Green, a British astronomer (1823-1899). Debris flows have been

Very is a crater on Mars, located south of the planet's equator in the heavily cratered highlands of Terra Sirenum in the Phaethontis quadrangle at 49

spherules at Eagle Crater. Spherule diameters are 3-6 mm. Close-up of sediment matrix with embedded hematite spherules at Eagle Crater. The central (partially

Cassini is a crater on Mars named in honour of the Italian astronomer Giovanni Cassini. The name was approved in 1973, by the International Astronomical

Dinorwic is a Martian impact crater, approximately 51 kilometers in diameter. It is named after the town in Ontario, Canada. Its name was approved by the

Becquerel is a 167 km-diameter crater at 22.1°N, 352.0°E on Mars, in Arabia Terra in Oxia Palus quadrangle. It is named after Antoine H. Becquerel. Photographs

Stokes is an impact crater on Mars, located on the Martian Northern plains at 55.9°N latitude and 188.8°W longitude. It measures approximately 62.74 kilometres

Very is a crater on Mars, located south of the planet's equator in the heavily cratered highlands of Terra Sirenum in the Phaethontis quadrangle at 49

Romania. Bopolu (crater) is west of Iazu and Endeavour crater. List of craters on Mars Geography of Mars "Planetary Names: Crater, craters: Iazu on Mars"

Garni is an impact crater on Mars, in which, according to NASA, there is evidence of liquid water. In the press release of its finding on 28 September

Mojave is a 58 km diameter impact crater in the Oxia Palus quadrangle of Mars, located at 7.5° N and 33.0° W. It was named after the town of Mojave in

a crater on Mars, approximately 90 kilometers in diameter, named after Dutch astronomer Jean Abraham Chrétien Oudemans (1827–1906). Oudemans crater is

Gledhill is an impact crater in the Hellas quadrangle of Mars, located at 53.2°S latitude and 87.1°E longitude. It is 78.5  km in diameter. It was named

lived from 1738 to 1815. Copley crater detail Copley crater region in exaggerated color Oblique view of Carducci crater (below center) and Copley with

Endeavour is an impact crater located in the Meridiani Planum extraterrestrial plain within the Margaritifer Sinus quadrangle (MC-19) region of the planet

Firsoff is an impact crater in the region called Meridiani Planum in the Oxia Palus quadrangle of Mars, located at 2.66°N latitude and 9.42°W longitude

Alphonsus is an ancient impact crater on the Moon that dates from the pre-Nectarian era. (Older sources state that it is Nectarian in age.) It is located

Airy-0 is a crater inside the larger Airy Crater on Mars, whose location historically defined the Martian prime meridian. It is about 0.5 km (0.3 mile)

South is an impact crater in the Mare Australe quadrangle of Mars, located at 76.9°S latitude and 21.9°E longitude. It measures 101.84 kilometres (63.28 mi)

Ritchey is a crater on Mars, located in the Coprates quadrangle at 28.8° South and 51° West. It measures 79 kilometers in diameter and was named after

Burton is an impact crater in the Memnonia quadrangle of Mars. It is 123.0 km in diameter and was named after British astronomer Charles E. Burton; the

Rahe is a crater on the planet Mars in the Tharsis quadrangle, positioned at 25.05° north latitude and 262.52° east longitude, between the volcanoes Ceraunius

Herschel is an impact crater in Mars's southern hemisphere. At roughly 304 kilometers in diameter, it is a moderately large impact crater. Located at 14.5°S

astronomers. Arago crater is to the east of Henry, Barth crater is to the southeast, and Pasteur crater is to the north. Henry crater has a large mound

SHAP-, US also /skiˌɑːp-/ skee-AHP-, Italian: [skjapaˈrɛlli]) is an impact crater on Mars, located near the planet's equator at latitude 3° south and longitude

partially buried impact crater in Margaritifer Terra, Mars. Eberswalde crater lies just to the north of Holden, a large crater that may have been a lake

Sinton is a crater in the Ismenius Lacus quadrangle on Mars. Sinton crater lies in the northern hemisphere, south of the very large crater Lyot and west

Dali is a crater on Mercury. It has a diameter of 176 kilometers. Its name was adopted by the International Astronomical Union in 2008. Dali is named for

Prokofiev is a crater near the north pole of the planet Mercury, named after the Russian composer Sergei Prokofiev. Data from the MESSENGER spacecraft

Martin crater in Manitoba, the Obolon' crater in Ukraine, and the Red Wing crater in North Dakota; however, more recent work has found that the craters formed

Terby is a crater on the northern edge of Hellas Planitia, Mars. It is in the Iapygia quadrangle. The 174-kilometre-diameter (108 mi) crater is centered

McMurdo is a crater in the Mare Australe quadrangle of Mars, located at 84.4° S and 359.1° W. It is 30.3 km in diameter and was named after McMurdo Station

363 ft (2,950 to 2,549 m), leaving a 1 mile (1.6 km) wide horseshoe-shaped crater. The debris avalanche was 0.6 cubic miles (2.5 km3) in volume. The 1980

Newton is a large crater on Mars, with a diameter close to 300 km. It is located south of the planet's equator in the heavily cratered highlands of Terra

Spallanzani is a crater on Mars, located in the Hellas quadrangle at 58.0° south latitude and 86.4° east longitude. It measures 71.69 kilometres (44.55 mi)

northeast of the large crater Praxiteles and south of Velázquez crater. Carvalho crater is to the southeast. Most of Kuan Han-Chʽing crater (right) Hollows within

Wislicenus is an impact crater on Mars, located in the Sinus Sabaeus quadrangle at 18.4° south latitude and 348.6° west longitude. It measures approximately

mountain in the western Mare Imbrium. It is located to the northeast of the crater Euler, and to the west-northwest of Lambert. The selenographic coordinates

Pangboche is a young impact crater on Mars, in the Tharsis quadrangle near the summit of Olympus Mons. It was named after a village in Nepal. It measures

In summer 1965, the first close-up images from Mars showed a cratered desert with no signs of water. However, over the decades, as more parts of the planet

Dvorák is a crater on Mercury. It has a diameter of 75 kilometers. Its name was adopted by the International Astronomical Union (IAU) in 1976. Dvorák is

instance, in 2021 the southeastern crater reached a height of 3,357 m (11,014 ft), but was then surpassed by the Voragine crater after the summer 2024 eruptions

Astronomical Union. The crater's extensive ejecta blanket and secondary crater field are superposed on plains materials and older craters. Verdi lies in the

Arandas is a crater in the Mare Acidalium quadrangle of Mars, located 42.77° North and 15.17° West. It is 24.76 km (15.39 mi) in diameter and is named

Tooting is an impact crater (of the type rampart crater) with volcanic features at 23.1°N, 207.1°E, in Amazonis Planitia (Amazonis quadrangle), due west

Baranauskas is a crater on Mercury. It has a diameter of 36 kilometres (22 miles). Its name was adopted by the International Astronomical Union (IAU) on

Sveinsdóttir is a large, elongated impact crater on Mercury. Its dimensions are 220 × 120 km. Sveinsdóttir crater is a distinctive feature on Mercury's landscape

Copland is an impact crater on Mercury. Its floor is flooded with volcanic smooth plains material, which could be related to the activity that formed the

Vyāsa is a crater on Mercury. It was named by the IAU in 1979, after the Hindu poet Vyasa. It is Tolstojan in age. Vyāsa is an ancient crater, overlain

chondrite meteorites. It is cratered, but the surface is noticeably smoother than that of Phobos, caused by the partial filling of craters with regolith.[citation

Danielson is an impact crater in the Oxia Palus quadrangle on Mars at 7.93° N and 7.11° W. and is 66.7 km in diameter, and is north of the Meridiani Planum

Wiktionary, the free dictionary. A maar is a broad, low-relief volcanic crater caused by a phreatomagmatic eruption (an explosion which occurs when groundwater

Hipparchus is an impact crater in the Phaethontis quadrangle of Mars, located at 44.8° S latitude and 151.4° W longitude. It is 93 kilometers (58 miles)

(/ˈiːəlɪs mɒnz/), is a mountain on Mars. It forms the central peak within Gale crater and is located around 5°05′S 137°51′E / 5.08°S 137.85°E / -5.08; 137

Tooting is an impact crater (of the type rampart crater) with volcanic features at 23.1°N, 207.1°E, in Amazonis Planitia (Amazonis quadrangle), due west

Trouvelot is a crater on Mars, located in the Oxia Palus quadrangle at 16.2° north latitude and 13.1° west longitude near the crustal dichotomy in the

Arandas is a crater in the Mare Acidalium quadrangle of Mars, located 42.77° North and 15.17° West. It is 24.76 km (15.39 mi) in diameter and is named

Chaikovskij (sometimes Tchaikovsky) is a crater on Mercury. It has a diameter of 171 kilometers. Its name was adopted by the International Astronomical

Copland is an impact crater on Mercury. Its floor is flooded with volcanic smooth plains material, which could be related to the activity that formed the

Hun Kal is a small (about 1.5 km in diameter) crater on Mercury that serves as the reference point for the planet's system of longitude. The longitude

002. Subrahmanya, K. R.; Prakash Narasimha, K. N. (October 2017). "Kaveri crater – An impact structure in the Precambrian terrain of southern India". Journal

Brahms is a crater on Mercury. It has a diameter of 100 kilometers. Its name was adopted by the International Astronomical Union (IAU) in 1979. Brahms

The Crater-class cargo ship were converted EC2-S-C1 type, Liberty cargo ships, constructed by the United States Maritime Commission (USMC) for use by the

age. The crater was first imaged by Mariner 10 in 1974. Unlike other Mercurian craters of similar size, Raphael is not multi-ringed. The crater Flaiano

Von Kármán is an impact crater in the Argyre quadrangle of Mars, located at 64.6°S latitude and 58.5°W longitude. It is 90 km (56 mi) in diameter. It was

spreads out and fills a large impact crater is likely to be younger than the crater. On the other hand, a small crater on top of the same lava flow is likely

Antoniadi is a crater on Syrtis Major Planum in the Syrtis Major quadrangle, Mars, located at 21.5° north latitude and 299.2° west longitude. It is 394 km

months. Opportunity was to leave Endurance crater, visit its discarded heat shield, and proceed to Victoria crater. Spirit was to attempt to climb to the

Flammarion is an impact crater in the Syrtis Major quadrangle on Mars at 25.2 ° N and 48.3 ° E. It is 173.0 km in diameter. Its name was approved in 1973

impact crater on Mercury, 90 kilometers in diameter. It is located at 10.4°, 21°W, south of the crater Abu Nuwas and southwest of the crater Molière

Angelou is a crater on Mercury. It has a diameter of 18 kilometers. Its name was adopted by the International Astronomical Union (IAU) on September 11

McLaughlin Crater is an old crater in the Oxia Palus quadrangle of Mars, located at 21°54′N 337°38′E / 21.9°N 337.63°E / 21.9; 337.63. It is 90.92 km

2 mi) Main Crater with a single crater lake formed from the 1911 eruption. The island consists of different overlapping cones and craters, of which forty-seven

Louth (/laʊð/) is an impact crater on Mars located at 70°11′N 103°14′E / 70.19°N 103.24°E / 70.19; 103.24 in the Mare Boreum quadrangle. Located within

layered material that reach above the crater's rim. Gale Crater and Crommelin (Martian crater) are two craters that hold large mounds. Such tall mounds

Bartók is a crater on Mercury. Its name was adopted by the International Astronomical Union (IAU) in 1979. Bartók is named for the Hungarian composer Béla

Chiang Kʻui is a crater on Mercury. It has a diameter of 41 kilometers. Its name was adopted by the International Astronomical Union (IAU) in 1976. Chiang

Aristoxenus is an impact crater near the north pole on Mercury. It was named by the IAU in 1979 after the Greek philosopher Aristoxenus. Aristoxenus is

The Lunar Crater Observation and Sensing Satellite (LCROSS) was a robotic spacecraft operated by NASA. The mission was conceived as a low-cost means of

Hargraves is a Hesperian-age complex double-layered ejecta impact crater on Mars. It was emplaced near the crustal dichotomy in the vicinity of the Nili

Lessing is a crater on Mercury. Its name was adopted by the International Astronomical Union in 1985. Lessing is named for the German writer Gotthold Ephraim

Alver is a crater on Mercury. It has a diameter of 151.49 kilometers. Its name was adopted by the International Astronomical Union (IAU) on March 15, 2013

Bashō is a crater on Mercury named after Matsuo Bashō, a 17th-century Japanese writer. Bashō crater is only 74.62 kilometers (46.37 mi) in diameter, but

Anguissola is a crater on Mercury. It has a diameter of 35.41 kilometres (22.00 miles). Its name was adopted by the International Astronomical Union (IAU)

Africanus Horton is a circular impact crater on Mercury. It was named by the IAU in 1976, after Africanus Horton, a Creole African nationalist writer and

Petrarch is a crater on Mercury. This crater is located within the distorted terrain on the opposite side of the planet from the Caloris Basin. It was

Apollodorus is an impact crater on Mercury. Its unusual appearance, with radiating dark troughs, led to a nickname of "the Spider" by scientists before

Al-Jāhiz is a crater on Mercury. It has a diameter of 83 kilometers. Its name was proposed by astrophysicist David Morrison and adopted by the International

Global Surveyor, they occur on steep slopes, especially on the walls of craters. Usually, each gully has a dendritic alcove at its head, a fan-shaped apron

augite and olivine crystals. Their crystallization ages, compared to a crater count chronology of different regions on Mars, suggest the nakhlites formed

Fet is a crater on Mercury that is named for the Russian poet Afanasy Fet, who lived from 1820 to 1892. Its name was adopted by the International Astronomical

Chu Ta is a crater on Mercury. It has a diameter of 100 kilometers. Its name was adopted by the International Astronomical Union in 1976. Chu Ta is named

pit-floored crater on Mercury, which was discovered in January 2008 during the first flyby of the planet by the MESSENGER spacecraft. The crater was named

several times the diameter of their originating crater, and are often accompanied by small secondary craters formed by larger chunks of ejecta. Ray systems

atmospheres mitigate many surface impacts through atmospheric entry. Impact craters and structures are dominant landforms on many of the Solar System's solid

Vivaldi is a crater on Mercury. It was named by the IAU after Italian composer Antonio Vivaldi in 1976. It has a prominent and nearly continuous inner

Bello is a crater on Mercury. It has a diameter of 129 kilometers. Its name was adopted by the International Astronomical Union (IAU) in 1976. Bello is

rayed impact crater on Mercury, which was discovered in 1991 by ground-based radar observations conducted at Goldstone Observatory. The crater was initially

Perepelkin Crater is an impact crater in the Arcadia quadrangle of the planet Mars. It is located at 52.8°N latitude and 64.6°W longitude. It is 77 km

Peace Vallis is an ancient stream valley on the northern rim of Gale Crater on the planet Mars. It is notable for its associated alluvial fan which lies

Dickens is a crater on Mercury. It has a diameter of 78 kilometers. Its name was adopted by the International Astronomical Union (IAU) in 1976. Dickens

is a crater on Mercury, named by the IAU in 1976 after Austrian composer Wolfgang Amadeus Mozart. The arc of dark hills visible on the crater's floor

Hovnatanian is a crater on Mercury. Its “butterfly” pattern of ejecta rays were created by an impact at an even lower angle than that which formed neighboring

Dickens is a crater on Mercury. It has a diameter of 78 kilometers. Its name was adopted by the International Astronomical Union (IAU) in 1976. Dickens

Amaral is a crater on the planet Mercury. With its smooth floor, surrounding ejecta, and small secondary craters, it appears noticeably younger than the

Chŏng Chʼŏl is a crater on Mercury. It has a diameter of 143 kilometers. Its name was adopted by the International Astronomical Union (IAU) in 1979. Chŏng

Nampeyo is a crater on Mercury. It has a diameter of 52 kilometers. Its name was adopted by the International Astronomical Union in 1976. Nampeyo is named

Located in the western edge of Mercury's giant Caloris basin, Kertész crater (named in 2008 for André Kertész, a Hungarian-born American photographer)

crater on Mercury 125 kilometers (78 mi) in diameter. Since there are very few later craters superposed on it, Eminescu appears to be a young crater formed

several times the diameter of their originating crater, and are often accompanied by small secondary craters formed by larger chunks of ejecta. Ray systems

Cunningham is a young crater on the western floor of the Caloris Basin, on Mercury. It is surrounded by a bright ray system. The crater's name was adopted

topography, chaos terrain, possible ancient rivers, pedestal craters, brain terrain, and ring mold craters. A new phenomenon known as slope streaks has been uncovered

Machaut is a crater on Mercury. Its name was adopted by the International Astronomical Union in 1976. Machaut is named for the French composer and poet

magma emptying the underlying magma chamber, formed a caldera that holds Crater Lake (Giiwas in the Native American language Klamath). Mount Mazama originally

is a crater on Mercury, named by the IAU in 1976 after Austrian composer Wolfgang Amadeus Mozart. The arc of dark hills visible on the crater's floor

Chekhov is a crater on Mercury. It has a diameter of 194 kilometers. Its name was adopted by the International Astronomical Union (IAU) in 1976. Chekhov

Hovnatanian is a crater on Mercury. Its “butterfly” pattern of ejecta rays were created by an impact at an even lower angle than that which formed neighboring

Meteor Crater, Odessa Meteor Crater, Wabar craters, and Wolfe Creek crater; iron meteorites are found in association with all of these craters. In contrast

geologists to believe the mountain is on the site of an ancient meteorite impact crater. Its proximity to Slide Mountain, the highest Catskill peak, the relatively

Burns is a crater on Mercury. It has a diameter of 43 kilometers. Its name was adopted by the International Astronomical Union (IAU) in 1985. Burns is

Ives is a crater on Mercury. Its name was adopted by the International Astronomical Union (IAU) in 1979. Ives is named for the American composer Charles

Coleridge is a crater on Mercury. Its name was adopted by the International Astronomical Union (IAU) in 1976. Coleridge is named for the English poet Samuel

Chao Meng-Fu is a 167 km (104 mi) diameter crater on Mercury named after the Chinese painter and calligrapher Zhao Mengfu (1254–1322). Due to its location

Darío is a crater on Mercury. It has a diameter of 151 kilometers. Its name was adopted by the International Astronomical Union (IAU) in 1976. Dario is

Bluff (or Gosse's Bluff) is thought to be the eroded remnant of an impact crater. Known as Tnorala to the Western Arrernte people of the surrounding region

Anyte is a crater on Mercury. It has a diameter of 20.92 kilometres (13.00 miles). Its name was adopted by the International Astronomical Union (IAU) on

Derain is a crater on Mercury named after André Derain, a French artist, painter, sculptor and co-founder of Fauvism with Henri Matisse. It has uncommonly

a crater on the planet Mercury. Its name was approved by the IAU on July 9, 2009. It was named after the modernist painter Sabri Berkel. The crater contains

Cézanne is a crater on Mercury. It has a diameter of 67 kilometers. Its name was adopted by the International Astronomical Union (IAU) in 1985. Cézanne

crater deposit that shows both impact craters and pit craters caused by collapse. Image taken by HiRISE under the HiWish program. A concentric crater

Andal is a crater on Mercury. Its name was adopted by the International Astronomical Union in 1976. Andal is named for the Tamil writer Andal, who lived

Firdousi is a crater on Mercury. It has a diameter of 98 kilometers. Its name was adopted by the International Astronomical Union (IAU) in 2010. Firdousi

Xiao Zhao crater is small in comparison with many other craters on Mercury. However, Xiao Zhao's long bright rays make it a readily visible feature. The

Sholem Aleichem is a crater on Mercury, named after the Yiddish writer Sholem Aleichem in 1979. The inter-crater plain deposits have been deformed by

the extinction coincided with a large meteorite impact at the Chicxulub crater and the generally accepted scientific theory is that this impact triggered

Janáček is a crater on Mercury. It has a diameter of 47 kilometers. Its name was adopted by the International Astronomical Union (IAU) in 1985. Janáček

Kenkō is a crater on Mercury. Its name was adopted by the International Astronomical Union (IAU) in 1976. Kenko is named for the Japanese author Yoshida

Donne is a crater on Mercury. It has a diameter of 86 kilometers. Its name was adopted by the International Astronomical Union (IAU) in 1976. Donne is

Akutagawa is a crater on Mercury. It has a diameter of 106 kilometers. Its name was adopted by the International Astronomical Union (IAU) in on September

Dürer is a crater on Mercury. It has a diameter of 195 kilometers. Its name was adopted by the International Astronomical Union (IAU) in 1976. Durer is

Barma is a crater on Mercury. It has a diameter of 128 kilometers. Its name was adopted by the International Astronomical Union in 1982. Barma is named

Grieg is a crater on Mercury. It has a diameter of 59 kilometers. Its name was adopted by the International Astronomical Union (IAU) in 1985. Grieg is

Al-Hamadhani is a crater on Mercury. It has a diameter of 186 kilometers. Its name was adopted by the International Astronomical Union in 1979. Al-Hamadhani

crater was first imaged by Mariner 10 in 1974. Balzac is one of the largest craters of the Kuiperian system on Mercury. The largest is Bartók crater.

Murasaki is a crater on Mercury located at 12 S, 31 W. It is 132 km in diameter. It was named after 10th-11th century Japanese writer Murasaki Shikibu

Kōshō is a crater on Mercury. Its name was adopted by the International Astronomical Union in 1985. Kōshō is named for the Japanese sculptor Kōshō, who

Carolan is a crater on Mercury. Its name was suggested by an Irishman, Fergal Donnelly, and two Americans, Joseph Brusseau and Deane Morrison, in a naming

Cervantes is a crater on Mercury. It has a diameter of 181 kilometers. Its name was adopted by the International Astronomical Union in 1976. Cervantes

Jókai is a crater on Mercury. Its name was adopted by the International Astronomical Union (IAU) in 1979. Jokai is named for the Hungarian novelist Mór

Bjornson is a crater on Mercury. Its name was adopted by the International Astronomical Union (IAU) in 1985. Bjornson is named for the Norwegian playwright

Melville is a crater on Mercury. It has a diameter of 154 kilometers. Its name was adopted by the International Astronomical Union (IAU) in 1976. Melville

Ōkyo is a crater on Mercury. Its name was adopted by the International Astronomical Union (IAU) in 1985. It is named for the Japanese painter Maruyama

Nureyev is a crater on Mercury. It has a diameter of 16 kilometers, and has a bright and extensive ray system. Its name was adopted by the International

Boccaccio is a crater on Mercury. It has a diameter of 151.95 kilometers. Its name was adopted by the International Astronomical Union (IAU) in 1976. Boccaccio

Burns is a crater on Mercury. It has a diameter of 43 kilometers. Its name was adopted by the International Astronomical Union (IAU) in 1985. Burns is

Dominici is a crater on Mercury. It was named by the IAU in 2010. Dominici's bright rays indicate that it is relatively young, and the young rays appear

Botticelli is a crater on Mercury. It has a diameter of 136.35 kilometres (84.72 mi). Its name was adopted by the International Astronomical Union (IAU)

Camões is a crater on Mercury. It has a diameter of 70 kilometers. Its name was adopted by the International Astronomical Union (IAU) in 1976. Camoes is

Benoit is a crater on Mercury. Its floor is quite unusual, with two mounds that have been suggested to be evidence of intrusive volcanic activity on Mercury

material blasted out during the crater's formation. Craters older than Degas are covered by the ray material, while younger craters are seen superimposed on

Fet is a crater on Mercury that is named for the Russian poet Afanasy Fet, who lived from 1820 to 1892. Its name was adopted by the International Astronomical

Navoi is a crater on Mercury. It contains uncommon reddish material that indicates a different rock composition from its surroundings. Navoi also appears

of the Arabian peninsula (the Gulf of Aden). Wislicenus Crater and the Schiaparelli basin crater contains layers, also called strata. Many places on Mars

Andal is a crater on Mercury. Its name was adopted by the International Astronomical Union in 1976. Andal is named for the Tamil writer Andal, who lived

Firdousi is a crater on Mercury. It has a diameter of 98 kilometers. Its name was adopted by the International Astronomical Union (IAU) in 2010. Firdousi

Hemingway is a crater on Mercury. It has a patch of very dark material located near its center. The dark color is likely due to rocks that have a different

Xiao Zhao crater is small in comparison with many other craters on Mercury. However, Xiao Zhao's long bright rays make it a readily visible feature. The

Larrocha is an impact crater on Mercury. It has a diameter of 196 km (122 mi), and it is one of 110 peak ring basins on Mercury. It is located in the Victoria

Possible ring mold crater, as seen by HiRISE under the HiWish program. Crater shape is due to impact into ice. Ring-mold craters form when an impact

Balagtas is a crater on Mercury. It has a diameter of 98 kilometers. Its name was adopted by the International Astronomical Union in 1976. Balagtas is

Mahler is a crater on Mercury. It has a diameter of 103 kilometers. Its name was adopted by the International Astronomical Union (IAU) in 1976. Mahler

Ibsen is a crater on Mercury. It is located near the antipode of the Caloris Basin. The name was approved by the IAU in 1976. It is named after Norwegian

Bernini is a crater on Mercury. It has a diameter of 146 kilometers. Its name was adopted by the International Astronomical Union (IAU) in 1976. Bernini

Derzhavin is a crater on Mercury. It has a diameter of 156 kilometers. Its name was adopted by the International Astronomical Union in 1979. Derzhavin

Munkácsy, named after Mihály Munkácsy, is a crater on Mercury. Munkácsy originally had a double-ring basin structure, but most of the inner ring was buried

Matisse is an impact crater on the southern hemisphere of Mercury. Matisse takes its name from the French artist Henri Matisse, and it was named by the

Mena is a crater in the Beethoven quadrangle on Mercury. Its name was adopted by the International Astronomical Union in 1976. Mena is named for the Spanish

Dostoevskij (sometimes Dostoevskii) is a crater on Mercury. It has a diameter of 430 kilometers. Its name was adopted by the International Astronomical

impact crater on Mercury. It was named after Leo Tolstoy by the IAU in 1976. The albedo feature Solitudo Maiae appears to be associated with this crater. The

Homer is a crater on Mercury. It is one of 110 peak ring basins on Mercury. It is Tolstojan in age. Deposits of material in and around this crater suggest

The crater Oskison is located in the far northern hemisphere of Mercury, in the plains north of Caloris basin. Oskison is a distinctive crater with a large

De Graft is a crater on Mercury. Its name was adopted by the International Astronomical Union in 2009, after Ghanaian playwright, poet, and novelist Joe

Atget crater is distinctive on the planet Mercury's surface due to its dark color. Atget crater is located within Caloris basin, near Apollodorus crater and

Despréz is a crater on Mercury with a diameter of 47.05 kilometers. Its name was adopted by the International Astronomical Union (IAU) in 1979. Despréz

geologists to believe the mountain is on the site of an ancient meteorite impact crater. Its proximity to Slide Mountain, the highest Catskill peak, the relatively

Mendes Pinto is a crater on Mercury. Its name was adopted by the International Astronomical Union (IAU) in 1976. Mendes Pinto is named for the Portuguese

Mansur is a crater on Mercury. Its name was adopted by the International Astronomical Union in 1979. Mansur is named for the Indian artist Ustad Mansur

Guido d'Arezzo is a crater on Mercury. It has a diameter of 58 kilometers. Its name was adopted by the International Astronomical Union (IAU) in 1976.

is an impact crater on the planet Mercury, 139 kilometers in diameter. It is located south of the crater Rodin, southeast of the crater Abu Nuwas, and

Titian is an impact crater on the planet Mercury. It was named by the IAU in 1976. In an enhanced color image, viewed from the MESSENGER spacecraft, the

Machaut is a crater on Mercury. Its name was adopted by the International Astronomical Union in 1976. Machaut is named for the French composer and poet

Alencar is a crater on Mercury. It has a diameter of 120 kilometers. Its name was adopted by the International Astronomical Union (IAU) in 1979. Alencar

Stravinsky is a crater on Mercury. It overlays the rim of the much older Vyāsa crater. It was named by the IAU in 1979 for the influential Russian composer

Voltaire is an impact crater on Mars's moon Deimos and is approximately 3 km (1.9 mi) across. Voltaire crater is named after François-Marie Arouet, a

Grieg is a crater on Mercury. It has a diameter of 59 kilometers. Its name was adopted by the International Astronomical Union (IAU) in 1985. Grieg is

Abu Nuwas is an impact crater on the planet Mercury, 116 kilometers in diameter. It is located at 17.4°N, 20.4°W. It is named after the Arab poet Abu Nuwas

Lau Crater. Heaviside Crater, as seen by CTX camera (on Mars Reconnaissance Orbiter). Gullies in a crater that is on the floor of Heaviside Crater, as

Nampeyo is a crater on Mercury. It has a diameter of 52 kilometers. Its name was adopted by the International Astronomical Union in 1976. Nampeyo is named

Bek is a crater on Mercury. It has a diameter of 32 kilometers. Its name was adopted by the International Astronomical Union (IAU) in 2010. Bek is named

Chekhov is a crater on Mercury. It has a diameter of 194 kilometers. Its name was adopted by the International Astronomical Union (IAU) in 1976. Chekhov

Byron is a crater on Mercury. It has a diameter of 106.58 kilometers. Its name was adopted by the International Astronomical Union (IAU) in 1976. Byron

Hitomaro is a crater on Mercury. It has a diameter of 105 kilometers. Its name was adopted by the International Astronomical Union (IAU) in 1976. Hitomaro

Gibran is a crater on Mercury and is in the east of the Shakespeare quadrangle. It was named after Lebanese-American poet Khalil Gibran in 2009. Gibran

Rachmaninoff is an impact crater on Mercury. This basin, first imaged in its entirety during MESSENGER's third Mercury flyby, was quickly identified as

Calvino is a crater on Mercury. Its name was adopted by the IAU in 2016, after the Italian writer Italo Calvino. Calvino lies in the center of Sihtu Planitia

Ailey is a crater on Mercury. It has a diameter of 21 kilometers. Its name was adopted by the International Astronomical Union (IAU) in on April 24, 2012

Schubert is a crater on Mercury. It was named after Franz Schubert, a famous Austrian composer, by the IAU in 1976. Schubert has been filled in by smooth

Bek is a crater on Mercury. It has a diameter of 32 kilometers. Its name was adopted by the International Astronomical Union (IAU) in 2010. Bek is named

Byron is a crater on Mercury. It has a diameter of 106.58 kilometers. Its name was adopted by the International Astronomical Union (IAU) in 1976. Byron

Brontë is a crater on Mercury. It has a diameter of 68 kilometres (42 miles). Its name was adopted by the International Astronomical Union in 1976. Bronte

Coleridge is a crater on Mercury. Its name was adopted by the International Astronomical Union (IAU) in 1976. Coleridge is named for the English poet Samuel

The Chryse Alien is a crater in the Chryse Planitia on Mars, named because of its resemblance to an "alien head". The crater is in a 712x935 image indexed

Li Chʻing-Chao is a crater on Mercury. It has a diameter of 61 kilometers. Its name was adopted by the International Astronomical Union (IAU) in 1976.

Monet is a crater on Mercury. Its name was adopted by the International Astronomical Union (IAU) in 1979. Monet is named for the French artist Claude Monet

Neruda is a crater on Mercury. It has a diameter of 112 kilometers. Its name was adopted by the International Astronomical Union (IAU) in 2008. Neruda

Nizāmī is a crater on Mercury. Its name was adopted by the International Astronomical Union (IAU) in 1979. Nizami is named for the Persian poet Nizami

Couperin is a crater on Mercury. It has a diameter of 80 kilometers. Its name was adopted by the International Astronomical Union (IAU) in 1979. Couperin

Mendes Pinto is a crater on Mercury. Its name was adopted by the International Astronomical Union (IAU) in 1976. Mendes Pinto is named for the Portuguese

Leopardi is a crater on Mercury. Its name was adopted by the International Astronomical Union in 1976. Leopardi is named for the Italian writer Giacomo

crater on Mercury. It was named by the IAU in 1976, after French composer Jean Philippe Rameau. The scarp Discovery Rupes cuts across Rameau crater.

Nāwahī is a crater on Mercury. Nāwahī crater is located within the large Caloris basin, near the western rim. The unusual dark material creating a halo

Ahmad Baba is a crater on Mercury. It has a diameter of 127 kilometers. Its name was adopted by the International Astronomical Union (IAU) in 1979. Ahmad

Gibran is a crater on Mercury and is in the east of the Shakespeare quadrangle. It was named after Lebanese-American poet Khalil Gibran in 2009. Gibran

Kālidāsā is a crater on Mercury. Its name was adopted by the International Astronomical Union in 1976. Kalidasa is named for the Indian writer Kālidāsa

Yeats is an impact crater on the planet Mercury. It is named after William Butler Yeats, an Irish poet and dramatist. The name was adopted by the International

Kipling is a crater on Mercury. It has a diameter of 164 kilometers. Its name was adopted by the International Astronomical Union (IAU) in 2010. Kipling

Mansart is a crater on Mercury. Its name was adopted by the International Astronomical Union (IAU) in 1979. Mansart is named for the French architect Jules

Husband Hill is one of the Columbia Hills in Gusev crater, Mars, which are close to the landing site of NASA's Spirit rover. It was named in honor of Rick

Inter-crater plains on Mercury are a land-form consisting of plains between craters on Mercury. Of the eight planets in the Solar System, Mercury is the

Brunelleschi is a crater on Mercury. It has a diameter of 128.57 kilometres (79.89 mi). Its name was adopted by the International Astronomical Union (IAU)

Hawthorne is a crater on Mercury. It has a diameter of 120 kilometers. Its name was adopted by the International Astronomical Union in 1979. Hawthorne

Equiano is a crater on Mercury. It has a diameter of 102 kilometers. Its name was adopted by the International Astronomical Union in 1976. Equiano is named

Murasaki is a crater on Mercury located at 12 S, 31 W. It is 132 km in diameter. It was named after 10th-11th century Japanese writer Murasaki Shikibu

crater was first imaged by Mariner 10 in 1974. Balzac is one of the largest craters of the Kuiperian system on Mercury. The largest is Bartók crater.

Faulkner is a crater on Mercury. It has a diameter of 168 kilometres (104 miles). Its name was adopted by the International Astronomical Union (IAU) on

an impact crater on the planet Mercury, 134 kilometers in diameter. It is located northeast of the crater Yeats and southeast of the crater Li Po. It

Melville is a crater on Mercury. It has a diameter of 154 kilometers. Its name was adopted by the International Astronomical Union (IAU) in 1976. Melville

Qi Baishi is a crater on Mercury. The crater was named after famed Chinese painter Qi Baishi. The crater has an asymmetric pattern of ejecta rays, which

Cervantes is a crater on Mercury. It has a diameter of 181 kilometers. Its name was adopted by the International Astronomical Union in 1976. Cervantes

Abedin is a crater on Mercury. It was named after the Bangladeshi artist Zainul Abedin by the IAU in 2009. Abedin exhibits a complex crater structure with

is a crater on the planet Mercury. It was named after Anicius Manlius Severinus Boethius, the Roman philosopher, by the IAU in 1976. The crater was first

Prime Meridian Argo Crater – Visited by Opportunity Beagle Crater – Visited by Opportunity Beer Crater Bopolu Crater Concepcion Crater - Visited by Opportunity

colonists. The abundance of volcanic features together with widespread cratering are strong evidence for a variety of ores. While nothing may be found

Delacroix is a crater on Mercury. Its name was adopted by the International Astronomical Union in 1979. Delacroix is named for the French painter Eugène

terrain Zumba crater, 29° S Small craters inset within Saheki crater, 22° S Crater in Arabia Terra, 13° N Sharp terrain in Radau crater, 17° N Softened

which is named after this crater. It is located at 48.1°N, 152.3°W and is named after playwright William Shakespeare. The crater was first imaged by Mariner

Keats is a crater on Mercury. The crater's name was adopted by the International Astronomical Union (IAU) in 1976 and named after an English poet. This

Polygnotus is a crater on Mercury, named by the IAU in 1976, after ancient Greek painter Polygnotus. The crater was first imaged by Mariner 10 in 1974

Bramante is a crater on Mercury. It has a diameter of 156 kilometers. Its name was adopted by the International Astronomical Union in 1976. Bramante is

Zola is a crater on Mercury. The crater was named after the French novelist and playwright Émile Zola by the IAU in 1979. Bright areas on the central

Haydn is a crater on Mercury. It has a diameter of 251 kilometers. Its name was adopted by the International Astronomical Union (IAU) in 1976. Haydn is

Lonar Lake, also known as Lonar crater, is a saline, soda lake, located at Lonar, 79 km from Buldhana city in Buldhana district, Maharashtra, India. It

Hiroshige is a crater on Mercury. Its name was adopted by the International Astronomical Union (IAU) in 1976, after the Japanese artist Andō Hiroshige

Milton is a crater on Mercury. It has a diameter of 186 kilometers. Its name was adopted by the International Astronomical Union in 1976. Milton is named

Qi Baishi is a crater on Mercury. The crater was named after famed Chinese painter Qi Baishi. The crater has an asymmetric pattern of ejecta rays, which

Abedin is a crater on Mercury. It was named after the Bangladeshi artist Zainul Abedin by the IAU in 2009. Abedin exhibits a complex crater structure with

Lermontov is an impact crater on the planet Mercury. The crater is named after Mikhail Yuryevich Lermontov, a 19th-century Russian poet. The name was approved

Kulthum is a crater on Mercury. It has a diameter of 31 kilometers. Its name was suggested by Molouk Ba-Isa from Saudi Arabia, Swiss individual Riana Rakotoarimanana

Li Po is a crater on Mercury. It has a diameter of 120 kilometers. Its name was adopted by the International Astronomical Union (IAU) in 1976. Li Po is

is a crater on Mercury. It has diameter about 77 km and is situated in northern part of Caloris Planitia. Hollows are scattered across Poe crater, and

Hugo is a crater on Mercury. Its name was adopted by the International Astronomical Union in 1979. Hugo is named for the French writer Victor Hugo, who

Dante is a lunar impact crater that is located on the far side of the Moon. It lies in the northern hemisphere exactly opposite the prime meridian facing

Praxiteles is a crater on Mercury. It is one of 110 peak ring basins on Mercury. MESSENGER's high-resolution images obtained during the mission's second

somewhat uneven, and it is surrounded by rugged lunar surface. Three tiny craters within this formation have been assigned names by the IAU. These are listed

Delacroix is a crater on Mercury. Its name was adopted by the International Astronomical Union in 1979. Delacroix is named for the French painter Eugène

Holbein is a crater on Mercury. Its name was adopted by the International Astronomical Union (IAU) in 1979. Holbein is named for the Germain painters Hans

Bramante is a crater on Mercury. It has a diameter of 156 kilometers. Its name was adopted by the International Astronomical Union in 1976. Bramante is

Lange is a crater on Mercury. It was named by the IAU in 2009 after American photographer Dorothea Lange. Lange appears to have been flooded by lava, with

Hodgkins is a crater on Mercury. It has a diameter of 19 kilometers. Its name was adopted by the International Astronomical Union in 2009. Hodgkins is

Handel is a crater on Mercury. It has a diameter of 166 kilometers. Its name was adopted by the International Astronomical Union in 1976. Handel is named

Hals is a crater on Mercury. It has a diameter of 93 kilometers. Its name was adopted by the International Astronomical Union (IAU) in 1985. Hals is named

from 1797 to 1856. Heine crater is to the southeast of the prominent Degas crater, and is overlain by rays and secondary craters from Degas. Heine is on

the southwestern edge of Kaupō Gap. In Hawaiian folklore, the depression (crater) at the summit of Haleakalā was home to the grandmother of the demigod Māui

Equiano is a crater on Mercury. It has a diameter of 102 kilometers. Its name was adopted by the International Astronomical Union in 1976. Equiano is named

Monteverdi is a crater on Mercury with a diameter of 138 kilometers. Its name was adopted by the International Astronomical Union (IAU) in 1979, from the

exploring and studying Victoria crater. The rover survived moderate dust storms and in 2011 reached Endeavour crater, which has been considered as a "second

continues to the present day. The Amazonian period has been dominated by impact crater formation and Aeolian processes with ongoing isolated volcanism occurring

Mussorgskij is a crater on Mercury. Its name was adopted by the International Astronomical Union (IAU) in 1979. Mussorgskij is named for the Russian composer

Eitoku is a crater on Mercury. It has a diameter of 101 kilometers. Its name was adopted by the International Astronomical Union in 1976. Eitoku is named

Mistral is a crater on Mercury. Its name was adopted by the International Astronomical Union (IAU) in 1976. Mistral is named for the Chilean poet Gabriela

Martí is a crater on Mercury. Its name was adopted by the International Astronomical Union (IAU) in 1976. Martí is named for the Cuban writer José Martí

Mickiewicz is a crater on Mercury. Its name was adopted by the International Astronomical Union (IAU) in 1976. Mickiewicz is named for the Polish poet

Harunobu is a crater on Mercury. It has a diameter of 107 kilometers. Its name was adopted by the International Astronomical Union in 1976. Harunobu is

Enheduanna is a crater on Mercury. It has a diameter of 105 kilometers. Its name was suggested by Gagan Toor from India in a naming contest which was eventually

Lu Hsun is a crater on Mercury. It has a diameter of 98 kilometers. Its name was adopted by the International Astronomical Union (IAU) in 1976. Lu Hsun

Moody is an impact crater on Mercury. Moody features a complex central peak and an annulus of dark material on its outer floor. The area inward of the

Ma Chih-Yuan is a crater on Mercury. Its name was adopted by the International Astronomical Union (IAU) in 1976. Ma Chih-Yuan is named for the Chinese

Villa-Lobos is a crater on Mercury. Its name was adopted by the International Astronomical Union (IAU) on September 25, 2015. Villa-Lobos is named for

Goya is a crater on Mercury. It has a diameter of 135 kilometers. Its name was adopted by the International Astronomical Union (IAU) in 1976. Goya is named

Crater Lake Lodge

Aksakov is a crater on Mercury. It has a diameter of 174 kilometers. Its name was adopted by the International Astronomical Union (IAU) on April 24, 2012

separating the Two Solitudes Main (lunar crater), located near the north pole of the Moon Main (Martian crater) Main (surname), a list of people with this

short-lived community Mount Darwin (Tasmania) Darwin Crater, a suspected meteorite impact crater Cordillera Darwin, Tierra del Fuego, a mountain range

Kurosawa is a crater on Mercury. Its name was adopted by the International Astronomical Union (IAU) in 1976. Kurosawa is named for the Japanese composer

Gogol is a crater on Mercury. Its name was adopted by the International Astronomical Union (IAU) in 1985. Gogol is named for the Russian playwright Nikolai

Hiroshige is a crater on Mercury. Its name was adopted by the International Astronomical Union (IAU) in 1976, after the Japanese artist Andō Hiroshige

Molokini is a crescent-shaped, partially submerged volcanic crater which forms a small, uninhabited islet located in ʻAlalākeiki Channel between the islands

filled in by sediments and clay-rich ejecta from a nearby giant impact crater, the Isidis basin. It is at approximately 22°N, 75°E, and has an elevation

Horace is a crater on Mercury. Its name was adopted by the International Astronomical Union (IAU) in 1976. Horace is named for the Ancient Roman poet Horace

Diophantus is a lunar impact crater that lies in the southwestern part of the Mare Imbrium, named after the ancient Greek mathematician Diophantus. It

(2,751 m). The deep, active crater is between the peaks and fills with water between major eruptions, being known as Crater Lake (Māori: Te Wai ā-moe)

Swift is an impact crater on Mars's moon Deimos. It is about 3 km (1.9 mi) in diameter. Swift is named after Jonathan Swift, whose 1726 book Gulliver's

Raden Saleh is a crater on Mercury. Its name was approved by the IAU in 2008, and it is named after a famous Indonesian painter named Raden Saleh. Oblique

Ovid is a crater on Mercury. Its name was adopted by the International Astronomical Union (IAU) in 1976. Ovid is named for the Roman poet Ovid, who lived

Sander is a crater on Mercury within Caloris Basin. It has dark walls and bright patches on its floor. Unlike the rays of Bashō crater, the bright areas

Mistral is a crater on Mercury. Its name was adopted by the International Astronomical Union (IAU) in 1976. Mistral is named for the Chilean poet Gabriela

Hesiod is a crater on Mercury. It has a diameter of 101 kilometers. Its name was adopted by the International Astronomical Union (IAU) in 1976. Hesiod

Kurosawa is a crater on Mercury. Its name was adopted by the International Astronomical Union (IAU) in 1976. Kurosawa is named for the Japanese composer

impact structures on Earth. The structure, the eroded remnant of an impact crater, was formed by the impact of an asteroid 1.849 billion years ago in the

Myron is a crater on Mercury. It has a diameter of 31 kilometers. Its name was adopted by the International Astronomical Union in 1979. Myron is named

separating the Two Solitudes Main (lunar crater), located near the north pole of the Moon Main (Martian crater) Main (surname), a list of people with this

Izquierdo is a crater on Mercury. Its name was adopted by the International Astronomical Union (IAU) in 2009, for the Mexican painter María Izquierdo.

Gogol is a crater on Mercury. Its name was adopted by the International Astronomical Union (IAU) in 1985. Gogol is named for the Russian playwright Nikolai

short-lived community Mount Darwin (Tasmania) Darwin Crater, a suspected meteorite impact crater Cordillera Darwin, Tierra del Fuego, a mountain range

Diophantus is a lunar impact crater that lies in the southwestern part of the Mare Imbrium, named after the ancient Greek mathematician Diophantus. It

Molokini is a crescent-shaped, partially submerged volcanic crater which forms a small, uninhabited islet located in ʻAlalākeiki Channel between the islands

filled in by sediments and clay-rich ejecta from a nearby giant impact crater, the Isidis basin. It is at approximately 22°N, 75°E, and has an elevation

(2,751 m). The deep, active crater is between the peaks and fills with water between major eruptions, being known as Crater Lake (Māori: Te Wai ā-moe)

Munch is a crater on Mercury. It was discovered on the first flyby of Mercury by the MESSENGER spacecraft on 14 January 2008, and was named after Edvard

Glinka is a pit-floored crater on Mercury, which was discovered in 1974 by Mariner 10 spacecraft. It was named by the IAU in 2008, after Russian composer

Rivera is a crater on Mercury. It has a diameter of 40 kilometers. Its name was suggested by Mexican residents Ricardo Martinez and Arturo Gutierrez, and

Gainsborough is a crater on Mercury. It has a diameter of 95 kilometers. Its name was adopted by the International Astronomical Union (IAU) in 1985. Gainsborough

Complex craters are a type of large impact crater morphology. Complex craters are classified into two groups: central-peak craters and peak-ring craters. Peak-ring

Firnas is a lunar impact crater on the far side of the Moon. Attached to the exterior of its southwestern rim is the prominent crater King. Only a few kilometers

Flaiano is a crater on Mercury. It has a diameter of 43 kilometres (27 miles). Its name was adopted by the International Astronomical Union (IAU) on March

units. The crater Verdi, 122 km (76 mi) in diameter, is the largest of the younger craters. Its extensive ejecta blanket and secondary crater field are

Crater is a small constellation in the southern celestial hemisphere. Its name is the latinization of the Greek krater, a type of cup used to water down

Khansa is a crater on Mercury. Its name was adopted by the International Astronomical Union (IAU) in 1976. Khansa is named after the Arab poet al-Khansa

Gluck is a crater on Mercury. It has a diameter of 100 kilometers. Its name was adopted by the International Astronomical Union (IAU) in 1979. Gluck is

Liszt is a crater on Mercury. It has a diameter of 85 kilometers. Its name was adopted by the International Astronomical Union (IAU) in 1985. Liszt is

the Michelangelo quadrangle of Mercury, which is named after this crater. The crater itself was named by the IAU in 1979 after the Italian painter, sculptor

Holst is a crater on Mercury. Its name was adopted by the International Astronomical Union (IAU) on April 24, 2012. Holst is one of 110 peak ring basins

Renoir is a crater on the planet Mercury. Its name, after the French painter Pierre-Auguste Renoir (1841–1919), was adopted by the International Astronomical

Scarlatti is a pit-floored crater on Mercury, which was discovered in 1974 by the Mariner 10 spacecraft. It has a prominent peak ring, and it is one of

The Nördlinger Ries is an impact crater and large circular depression in western Bavaria and eastern Baden-Württemberg. It is located north of the Danube

Imhotep is a crater on Mercury. It has a diameter of 159 kilometers. Its name was adopted by the International Astronomical Union in 1976. Imhotep is named

Karsh is a crater on Mercury. It has a diameter of 58 kilometers. Its name was suggested by American resident Elizabeth Freeman Rosenzweig in a naming

Ghiberti is a crater on Mercury, with a diameter of 110 kilometers. Its name, Ghiberti, was adopted by the International Astronomical Union (IAU) in 1976;

Gauguin is a crater on Mercury. It has a diameter of 70 kilometers. Its name was adopted by the International Astronomical Union (IAU) in 1979. Gauguin

Eratosthenes crater is a relatively deep lunar impact crater that lies on the boundary between the Mare Imbrium and Sinus Aestuum mare regions. It forms

Judah Ha-Levi is a crater on Mercury. Its name was adopted by the International Astronomical Union (IAU) in 1976. Judah Ha-Levi is named for the Spanish-Jewish

Hauptmann is a crater on Mercury. It has a diameter of 118 kilometers. Its name was adopted by the International Astronomical Union (IAU) in 1985. Hauptmann

Han Kan is a crater on Mercury. It has a diameter of 50 kilometers. Its name was adopted by the International Astronomical Union (IAU) in 1985. Han Kan

Ictinus is a crater on Mercury. Its depth from crater floor to rim is 4.8 km. Its name was adopted by the International Astronomical Union in 1976. Ictinus

Kunisada is a crater on Mercury. It has a diameter of 241 km (150 mi). Its name was adopted by the International Astronomical Union in 2009. Kunisada is

Fahrenheit is a tiny lunar impact crater located in the southeast part of the Mare Crisium. This area of the surface is nearly devoid of impact features

March is a crater on Mercury. Its name was adopted by the International Astronomical Union in 1979. March is named for the Valencian poet in Catalan language

Kamensk crater is an impact crater located 10 to 15 kilometres (6.2 to 9.3 mi) to the north of Kamensk-Shakhtinsky town in Rostov Oblast, Russia. It is

The Popigai impact structure is the eroded remnant of an impact crater in northern Siberia, Russia. It is tied with the Manicouagan structure as the fourth

impact crater in the eastern part of the Mare Imbrium. It was named after French natural scientist Louis Feuillée. It lies less than a half crater diameter

Mark Twain is a crater on Mercury. Its name was adopted by the International Astronomical Union (IAU) in 1976. Mark Twain is named for the American author

Daedalus is a prominent crater located near the center of the far side of the Moon. The inner wall is terraced, and there is a cluster of central peaks

impact crater, according to research from the Planetary Science Institute in Tucson, led by Joseph R. Michalski. The research postulated the crater was formed

impact crater that is located in the northern hemisphere on the far side of the Moon. It is named after Jacob Robert Emden (1862-1940). The crater lies

a tiny lunar impact crater. It is roughly circular and cup-shaped, with interior walls that slope down to the midpoint. The crater lies in the Palus Somni

is a lunar impact crater on the far side of the Moon, located to the north of the huge walled plain Korolev. The satellite crater Engelʹgardt B is attached

boundaries. Mayon is a classic stratovolcano with a small central summit crater. It is one of the world's most symmetrical volcanic cones. The concave profile

lake, 25 km (16 mi) in diameter, located within a 52 km (32 mi) impact crater. It is located in the Tajik National Park in the Pamir Mountains in Tajikistan

Douglass is a lunar impact crater on the far side of the Moon. It lies to the southwest of the crater Frost and south-southwest of the large walled plain

impact crater, according to research from the Planetary Science Institute in Tucson, led by Joseph R. Michalski. The research postulated the crater was formed

Ictinus is a crater on Mercury. Its depth from crater floor to rim is 4.8 km. Its name was adopted by the International Astronomical Union in 1976. Ictinus

Eratosthenes crater is a relatively deep lunar impact crater that lies on the boundary between the Mare Imbrium and Sinus Aestuum mare regions. It forms

largest crater in this quadrangle is Huygens. Some interesting features in this quadrangle are dikes. the many layers found in Terby crater, and the

is a lunar impact crater on the far side of the Moon. It lies less than a crater diameter to the east-southeast of the larger crater Langemak. To the east-northeast

including Gale Crater. Gale Crater - Landing site is within Aeolis Palus near Aeolis Mons ("Mount Sharp") - North is down. Gale Crater - Landing site

impact crater that is located on the far side of the Moon. The crater floor is bisected by the lunar equator, and it lies about three crater diameters

The Yarrabubba impact structure is the eroded remnant of an impact crater, situated in the northern Yilgarn Craton near Yarrabubba Station between the

Mark Twain is a crater on Mercury. Its name was adopted by the International Astronomical Union (IAU) in 1976. Mark Twain is named for the American author

Boltysh crater or Bovtyshka crater is a buried impact crater in the Kirovohrad Oblast of Ukraine, near the village of Bovtyshka. The crater is 24 kilometres

Daedalus is a prominent crater located near the center of the far side of the Moon. The inner wall is terraced, and there is a cluster of central peaks

Cantor is a lunar impact crater that is located on the northern hemisphere on the far side of the Moon. The outer rim of the crater has a distinctly hexagonal

overestimating the depth of craters, so as to make them have shadows at higher sun angles. Fortunately he was able to see four craters, Matthew, Mark, Luke and

craters. However, a few large craters do stand out. The giant impact crater, Lyot, is easy to see in the northern part of Ismenius Lacus. Lyot Crater

years old to less than 1,000 years (Miocene to Holocene), of which Sunset Crater is the youngest. The highest peak in the field is Humphreys Peak, at Flagstaff's

is a lunar impact crater located on the lunar far side near the northern pole. The crater is located in between the prominent craters Haskin and Nansen

large lunar impact crater on the far side of the Moon. It lies to the west-southwest of the crater Cockcroft, and about two crater diameters to the northeast

March is a crater on Mercury. Its name was adopted by the International Astronomical Union in 1979. March is named for the Valencian poet in Catalan language

The Bench Crater meteorite is a meteorite discovered on the Moon by Apollo 12 astronauts in 1969. It is part of the friable basalt lunar sample 12037.

Cooper is a lunar impact crater that is located in the northern hemisphere on the far side of the Moon. It lies to the east of the large walled plain D'Alembert

Mjølnir is a meteorite crater on the floor of Barents Sea off the coast of Norway. It is 40 km (25 mi) in diameter and the age is estimated to be 142.0

da Vinci is a lunar impact crater that is located in the eastern part of the Moon, to the northwest of Mare Fecunditatis. It lies along the eastern shore

streaks, pit crater chains, and large troughs (called fossae). Research published in the journal Icarus has found pits in Zumba Crater are caused by

Dugan is a lunar impact crater that is located on the northern part of the Moon's far side. It lies to the southwest of the large walled plain Schwarzschild

crater Tralles and the prominent Cleomedes. This crater is joined to the oval-shaped Debes A through a break in the southern rim. The latter crater is

Dufay is a lunar impact crater that is located on the far side of the Moon. It lies about one crater diameter to the east of the large walled plain Mandel'shtam

Bianchini is a lunar impact crater that lies along the northern Jura Mountains that ring the Sinus Iridum, in the northwestern part of the near side of

Perseverance is a car-sized Mars rover designed to explore the Jezero crater on Mars as part of NASA's Mars 2020 mission. It was manufactured by the Jet

Draper is a small lunar impact crater in the southern part of the Mare Imbrium. It is a circular, cup-shaped formation, with a tiny craterlet intruding

old lunar impact crater that is located in the northern hemisphere on the far side of the Moon. It lies to the southeast of the crater Chernyshev, and

impact crater that lies just beyond the northwest rim of the Moon, on the far side as seen from the Earth. It lies to the northeast of the crater Rynin

Fermat is a lunar impact crater located to the west of the Rupes Altai escarpment. To the west-southwest is the larger crater Sacrobosco, and to the southwest

a pseudocrater, is a volcanic landform which resembles a true volcanic crater, but differs in that it is not an actual vent from which lava has erupted

Southeast and Peary crater (diameter of 73 km) to the North. The crater is named after Australian scientist Howard Florey. The crater was named by the IAU

crater remnant Weiss. The crater is named after Italian astronomer Cecco d'Ascoli. The rim of this crater is only slightly worn, although the crater Cichus

is a small lunar impact crater that is located to the south of Mare Smythii, near the eastern limb of the Moon. This crater is seen at a highly oblique

Clavius is one of the largest crater formations on the Moon and the second largest crater on the visible near side (very close in size to Deslandres)

a small lunar impact crater on the Moon's far side. The northwest part of its rim is intruded upon by the somewhat larger crater Shirakatsi, and the outer

Carrillo is a small lunar impact crater located near the eastern limb of the Moon. In this location the crater is subject to lunar libration effects,

Ring) is an impact structure, the deeply eroded remnant of a former impact crater, situated in arid central Western Australia, about 100 kilometres (62 mi)

lunar impact crater located on the northwest edge of Mare Nectaris. Intruding into the northeast rim is the slightly larger, and younger crater Theophilus

Dyson is a lunar impact crater, 63 kilometers in diameter, that lies on the far side of the Moon, past the northwest limb. It is located in the northern

Cassini is a lunar impact crater that is located in the Palus Nebularum, at the eastern end of Mare Imbrium. The crater was named after astronomers Giovanni

Damoiseau is a lunar impact crater that is located just to the west of the Oceanus Procellarum, in the western part of the Moon's near side. It lies due

lunar impact crater located on the northwest edge of Mare Nectaris. Intruding into the northeast rim is the slightly larger, and younger crater Theophilus

Cassini is a lunar impact crater that is located in the Palus Nebularum, at the eastern end of Mare Imbrium. The crater was named after astronomers Giovanni

Southeast and Peary crater (diameter of 73 km) to the North. The crater is named after Australian scientist Howard Florey. The crater was named by the IAU

impact crater in the western part of the Mare Imbrium. It was named after French astronomer Joseph-Nicolas Delisle. It lies to the north of the crater Diophantus

lunar impact crater that is located near the northern limb of the Moon, on the western hemisphere. It lies nearly due south of the crater Pascal, and southeast

appears to be weak because of few boulders. Among a group of large craters is Mariner Crater, first observed by the Mariner 4 spacecraft in the summer of 1965

Clark is a lunar impact crater that lies in the southern hemisphere of the Moon's far side. It is located midway between the larger walled plain Van der

Presqu'île is a meteorite crater in the territory equivalent to a regional county municipality (TE) of Jamésie in the Nord-du-Québec region of Quebec,

Haughton impact crater is located on Devon Island, Nunavut in far Northern Canada. It is about 23 km (14 mi) in diameter and was formed 31–32 million years

Collins is a tiny lunar impact crater located on the southern part of the Mare Tranquillitatis. It is located about 25 kilometers to the north of the Apollo

Dugan is a lunar impact crater that is located on the northern part of the Moon's far side. It lies to the southwest of the large walled plain Schwarzschild

Denning is a lunar impact crater that is located on the far side of the Moon. It lies about midway between the craters Levi-Civita to the south and Marconi

crater Tralles and the prominent Cleomedes. This crater is joined to the oval-shaped Debes A through a break in the southern rim. The latter crater is

southern rim are the co-joined craters Bonpland and Parry, which intrude into the formation forming inward-bulging walls. The crater is named after Italian geographer

Dyson is a lunar impact crater, 63 kilometers in diameter, that lies on the far side of the Moon, past the northwest limb. It is located in the northern

Damoiseau is a lunar impact crater that is located just to the west of the Oceanus Procellarum, in the western part of the Moon's near side. It lies due

impact crater that is located near the southern limb of the Moon. The north-northeast rim of the crater overlies a portion of the slightly larger crater Klaproth

Puchezh-Katunki is a meteor crater located in the Nizhny Novgorod Oblast of the Volga Federal District, Russia. It is 80 km (50 mi) in diameter. Argon–argon

stratigraphic relations and on visual comparisons of the density of superposed craters. Crater ages are established by relative freshness of appearance, as indicated

Cabeus is a lunar impact crater that is located about 100 km (62 mi) from the south pole of the Moon. At this location the crater is seen obliquely from

the eastern edge of the Mare Imbrium. It is located to the west of the crater Conon. To the west of this peak is the Rima Bradley rille. (See below.)

hills, which suggests the ring of hills are not the rim of the original crater but a peak ring within a much larger structure. The Carswell Formation,

impact crater that is located within the northeast part of the walled plain Janssen. Attached to the north-northwest rim is the slightly larger crater Metius

lies less than one crater diameter to the south-southwest of the crater Zagut, and due north of Büsching. This is a heavily worn crater with a southwest

crater remnant Weiss. The crater is named after Italian astronomer Cecco d'Ascoli. The rim of this crater is only slightly worn, although the crater Cichus

lunar impact crater located in the wide straight between Mare Serenitatis and Mare Tranquilitatis. To its southwest lies the larger crater Plinius, and

Einstein is a large lunar impact crater that lies along the western limb of the Moon, which makes it difficult to observe from the Earth. The visibility

Obolon' crater (Ukrainian: Оболонь) is a 20 km (12 mi) diameter buried meteorite impact crater situated about 200 km (120 mi) southeast of Kyiv in Ukraine

lunar impact crater that is located on the far side of the Moon. It lies to the northeast of the walled plain Fersman, and north of the crater Weyl. This

lunar impact crater that is located in the southeastern part of the Moon, to the south of the crater Peirescius. To the northwest lie the craters Vega and

Carrillo is a small lunar impact crater located near the eastern limb of the Moon. In this location the crater is subject to lunar libration effects,

Carrel is a small lunar crater on the Mare Tranquillitatis. It has a somewhat distorted appearance, having a slight protruding bulge in the northwest rim

Caloris impact event. The crater Fet is near the center of Tir Planitia. Hovnatanian crater is southwest of Fet. The craters Amru Al-Qays and Nureyev are

point of the volcanic caldera and ends at the interesting crater Rahe (an oblique impact crater with measures of 35 × 18 km), just north from the volcano

Euclides is a small lunar impact crater located near the eastern edge of Oceanus Procellarum, about 30 kilometers to the west of the Montes Riphaeus mountains

(disambiguation) Lake Henry (disambiguation) Henry (Apollo lunar crater) Henry (lunar crater) Henry (Martian crater) HMS Henry (1660), English Royal Navy vessel Henry

Moons Phobos Stickney crater Limtoc crater Monolith Deimos Swift crater Voltaire crater Transits Solar eclipses on Mars Satellite transits Phobos Deimos

Caventou is a tiny lunar impact crater located in the western part of the Mare Imbrium. It is a circular, cup-shaped formation surrounded by the lunar

Aeolis Palus, between Peace Vallis and Aeolis Mons ("Mount Sharp"), in Gale crater on the planet Mars. The outcrop was encountered by the Curiosity rover on

the existence of an impact crater on the Earth, Meteor Crater in Arizona. The site has been renamed the Barringer Crater in his honor, which is the preferred

Bernoulli is a lunar impact crater that is located in the northeast part of the Moon. It lies to the south of the crater Messala, and east of Geminus.

Pot of Gold is the nickname for a knobby, softball-sized rock in Gusev Crater on Mars. During an examination by the Mars Exploration Rover Spirit on June

lunar impact crater that is located in the rugged southern highlands of the Moon's near side. It lies directly to the south of the crater Maurolycus and

impact crater that lies on the western edge of the Mare Tranquillitatis. It was named after Dionysius the Areopagite. To the southeast is the crater pair

Amelia Creek crater is an impact structure (or astrobleme), the eroded remnant of a former impact crater, located in the Davenport Range, Northern Territory

Mistastin crater is a meteorite crater in Labrador, Canada which contains the roughly circular Mistastin Lake. The lake is approximately 16 km (9.9 mi)

Fauth is a small double-crater located at the edge of the rough southern ramparts of the prominent ray crater Copernicus on the Moon. It lies in the Mare

heavily worn lunar impact crater that is located in the rugged south-central highlands of the Moon. To the southwest is the crater Abulfeda. It is named after

a small lunar impact crater that lies on the far side of the Moon, just past the southwestern limb. In this location the crater is occasionally brought

occur on steep slopes, especially craters. Gullies are believed to be relatively young because they have few, if any craters, and they lie on top of sand dunes