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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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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%)

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

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

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

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

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

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

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

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°

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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,

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

Zumba is a very young crater on Mars, located in the Phoenicis Lacus quadrangle at 28.68 South and 133.18 West. It measures approximately 2.93 kilometres

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

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

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

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

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

Wegener is an impact crater in the Argyre quadrangle of Mars, located at 64.6°S latitude and 4.0°W longitude. It measures approximately 68.51 kilometres

a large crater in the Noachis quadrangle of Mars. It was named in 1973 after Richard A. Proctor, a British astronomer (1837–1888). The crater contains

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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)

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

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)

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

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

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

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

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)

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

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

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

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

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

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"

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

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

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

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

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

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)

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

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

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

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

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

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

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

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

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

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)

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

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

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

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

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

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

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

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

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

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

Bowditch is a lunar impact crater that lies on the far side of the Moon, just beyond the eastern limb. It is located on a region of the lunar surface that

Chopin is a crater on Mercury. It has a diameter of 131 kilometers. Chopin is named for the Polish composer Frédéric Chopin (lived 1810–49). Its name was

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

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

(/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

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

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

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

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

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

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

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

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

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

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

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)

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

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

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

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

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

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

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

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

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)

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

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

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

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

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

A maar is a broad, low-relief volcanic crater caused by a phreatomagmatic eruption (an explosion which occurs when groundwater comes into contact with

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

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

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

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

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

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

Aeolis Palus is a plain between the northern wall of Gale crater and the northern foothills of Aeolis Mons (Mount Sharp) on Mars. It is located at 4°28′S

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

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

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

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

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

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

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

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

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

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

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

crater on Phobos, which is a satellite of Mars. It is 9 km (5.6 mi) in diameter, taking up a substantial proportion of the moon's surface. The crater

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

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

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

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

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

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

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

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

in 1976. The crater was first imaged by Mariner 10 in 1974. Bach is one of 110 peak ring basins on Mercury. MESSENGER image Bach crater interior Bach

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

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

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

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

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

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

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

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

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

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

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

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

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

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

Sullivan is a crater on Mercury. Its name was adopted by the International Astronomical Union (IAU) in 1976, and is named for the American architect Louis

Carducci is a crater on Mercury. It has a diameter of 108.19 kilometers. Its name was adopted by the International Astronomical Union (IAU) in 1976. Carducci

Al-Akhtal is a crater on Mercury. Its name was adopted by the International Astronomical Union (IAU) in 1985. Al-Akhtal is named for the Arab poet Akhtal

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

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

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

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

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

Debussy is a rayed impact crater on Mercury, which was discovered in 1969 by low resolution ground-based radar observations obtained by the Goldstone Observatory

Bruegel is a crater on Mercury. It has a diameter of 72 kilometers. Its name was adopted by the International Astronomical Union in 1985. Bruegel is named

Liang Kʻai is a crater on Mercury. It has a diameter of 140 kilometers. Its name was adopted by the International Astronomical Union in 1979. Liang Kʻai

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

Belinskij (sometimes Belinskii) is a crater on Mercury. It has a diameter of 70 kilometers. Its name was adopted by the International Astronomical Union

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

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

Kuiper is a moderate-size crater with a central peak cluster located at 11°21′S 31°14′W / 11.35°S 31.23°W / -11.35; -31.23 on Mercury. It is 62 kilometers

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

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

Balanchine is an impact crater on the planet Mercury. It possesses a ray system of slightly blue rays which inspired its name due to resembling the tutu

Amru Al-Qays is a crater on Mercury. The crater was first imaged by Mariner 10 in 1974. Its name was adopted by the IAU in 1976, after the pre-Islamic

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

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

relation to First Crater and Crater Hill, but the name has fallen into disuse. Twin Crater, alluding to the nested cones in the crater, was applied as early

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

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

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

is a crater on Mercury. On the floor of Rudaki and also in a broad region surrounding it to the west are smooth plains, which are far less cratered than

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

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

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

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

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

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

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

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

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

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

To Ngoc Van is a pit-floored crater on Mercury, named after the Vietnamese artist Tô Ngọc Vân. It was discovered in January 2008 during the first flyby

Balanchine is an impact crater on the planet Mercury. It possesses a ray system of slightly blue rays which inspired its name due to resembling the tutu

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.

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

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

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

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

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

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

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

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

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

is a crater on Mercury. On the floor of Rudaki and also in a broad region surrounding it to the west are smooth plains, which are far less cratered than

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

Giotto is a crater on Mercury. It has a diameter of 144 kilometers. Its name was adopted by the International Astronomical Union (IAU) in 1976. Giotto

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

Callicrates is a crater on Mercury. Its name was adopted by the International Astronomical Union in 1976. Callicrates is named for the Greek architect

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

Dowland is a crater on Mercury. It has a diameter of 158 kilometers. Its name was adopted by the International Astronomical Union in 1979, and refers to

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

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

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

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

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

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

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

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

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

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

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

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

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

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

Aneirin is a crater on Mercury. It has a diameter of 467 kilometers. Its name was adopted by the International Astronomical Union (IAU) on June 13, 2014

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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.

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

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

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

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

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

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)

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

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

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

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

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

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

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

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

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

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

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

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

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

through several craters, before ending at Holden crater. Part of Uzboi Vallis along with nearby craters. Colors relate to elevation. Bond crater (bottom), Uzboi

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

is an impact crater on the planet Mercury. It is named in honor of Ben Enwonwu, the modernist Nigerian sculptor and painter. The crater displays a central

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.

lunar impact crater located in eastern Oceanus Procellarum. It was named after the astronomer Nicolaus Copernicus. It typifies craters that formed during

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

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

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

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

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

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

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

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

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

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

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

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

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

disappeared over time in a crater. Crater on left is before ice disappeared. Crater is 6 meters in diameter. Impact craters generally have a rim with ejecta

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

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

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

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

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

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

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

impact crater on Mercury. It has a set of dark rays. Dark rays are rare on Mercury, but other occurrences have been identified, such as at Mozart crater. Mozart

Holberg is a crater on Mercury. Its name was adopted by the International Astronomical Union in 1976. Holberg is named for the Dano-Norwegian writer Ludvig

Mofolo is a crater on Mercury. Its name was adopted by the International Astronomical Union in 1976. Mofolo is named for the Basotho writer Thomas Mofolo

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

Crater Lake Lodge

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

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

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

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

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

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

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

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

Flaubert is a crater on Mercury. Its name was adopted by the International Astronomical Union (IAU) in 1985. Flaubert is named for the French novelist

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

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

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

through several craters, before ending at Holden crater. Part of Uzboi Vallis along with nearby craters. Colors relate to elevation. Bond crater (bottom), Uzboi

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

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

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

through several craters, before ending at Holden crater. Part of Uzboi Vallis along with nearby craters. Colors relate to elevation. Bond crater (bottom), Uzboi

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

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

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

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

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

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

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

175.4785°E / -14.5718; 175.4785) in Gusev crater (January 4, 2004), and the Curiosity rover in Gale Crater (4°35′31″S 137°26′25″E / 4.591817°S 137.440247°E

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

Phidias is a crater on Mercury. Its name was adopted by the International Astronomical Union (IAU) in 1976. Phidias is named for the Greek artist Phidias

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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.

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

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

180°. The western part of Memnonia is a highly cratered highland region that exhibits a large range of crater degradation. Memnonia includes these topographical

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

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

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

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

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;

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

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

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

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

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

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)

impact crater that lies in the southern hemisphere on the far side of the Moon. The rim has been worn by subsequent impacts, with a smaller crater overlying

Raditladi is a large impact crater on Mercury with a diameter of 263 km. Inside its peak ring there is a system of concentric extensional troughs (graben)

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

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

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

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

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

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

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

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

low hills inside Gusev crater on Mars. They were observed by the Mars Exploration Rover Spirit when it landed within the crater in 2004. They were promptly

Cauchy is a small lunar impact crater on the eastern Mare Tranquillitatis. It was named after French mathematician Augustin-Louis Cauchy. It is circular

Eötvös is the remains of a lunar impact crater on the far side of the Moon. It lies to the north-northwest of the walled plain Roche, and east-southeast

Chrétien is a lunar impact crater that is located in the southern hemisphere on the far side of the Moon from the Earth. It lies due south of the Mare

of 15 islands in total, was created by a meteorite impact which formed a crater about 32 km (20 mi) wide. In 1985, the Ontario government established the

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

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

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

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

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

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

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

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

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

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

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

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

The Araguainha crater or Araguainha dome is an impact crater on the border of Mato Grosso and Goiás states, Brazil, between the villages of Araguainha

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

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

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

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

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

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

Curtis is a very small lunar impact crater that lies in the western Mare Crisium, to the east of the crater Picard. It is a circular, cup-shaped formation

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

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

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

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

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

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

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

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

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

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

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

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

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

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

impact crater that lies on the far side of the Moon. It lies due east of the huge walled plain Gagarin, and to the north of the somewhat smaller crater Barbier

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

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

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

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

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

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

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

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

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

impact crater that lies on the far side of the Moon. It lies due east of the huge walled plain Gagarin, and to the north of the somewhat smaller crater Barbier

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

impact crater on the far side of the Moon, named after the English solar astronomer John Evershed. It is located to the northeast of the larger crater Cockcroft

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 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

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,

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

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

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

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

is a small lunar impact crater located in the Mare Imbrium. It was named after Italian astronomer Francesco Carlini. The crater is bowl-shaped with a small

Deutsch is a lunar impact crater on the far side of the Moon. It lies to the southwest of the larger crater Seyfert. About one crater to the east-northeast

Couder is a small lunar impact crater that is located just behind the western limb of the Moon, in a region of the surface that is brought into view during

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

is a lunar impact crater that lies to the southwest of Mare Tranquillitatis, in the central highland region. To the west is the crater pair of Theon Junior

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,

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

lunar impact crater in the northern part of the Moon, relatively close to the limb (as viewed from earth). At this position the crater is foreshortened

Crüger is a lunar impact crater that is located in the western part of the Moon, to the northeast of the much larger walled plain Darwin. The most distinctive

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

lunar impact crater that is located on the far side of the Moon, due east of the walled plain Van der Waals. To the northeast is the crater Rosseland, and

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

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

small lunar impact crater on the far side of the Moon. It is situated across the northeastern rim of the older and larger crater Danjon. To the west

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

Eddington is the lava-flooded remnant of a lunar impact crater, located on the western part of Oceanus Procellarum. The western rim is attached to the

impact crater that is located in the northeastern part of the Moon's near side, about a crater diameter east-southeast of the prominent crater Atlas.

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.

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

Belopolʹskiy is a lunar impact crater that is located on the far side of the Moon. It lies to the west of the crater Houzeau, and northeast of Strömgren

Flamsteed is a small lunar impact crater located on the Oceanus Procellarum, which is named after British astronomer John Flamsteed. It lies almost due

Ching-Te is a small lunar impact crater located in a mountainous area to the east of the Mare Serenitatis. It is a circular, bowl-shaped formation with

Dewar is a lunar impact crater that lies on the Moon's far side. Less than one crater diameter to the south-southwest is the crater Stratton. Vening Meinesz

Daly is a small lunar impact crater that is located in the eastern part of the Moon, to the northwest of the crater Apollonius. This formation is relatively

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

lunar impact crater on the far side of the Moon. It overlies part of the northwestern rim of the huge walled plain Fermi, and the crater Litke is nearly

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

Chandler is a lunar impact crater in the northern hemisphere, on the Moon's far side. It lies to the southeast of the large walled plain D'Alembert, and

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,

is a small lunar impact crater that is located in the central region of the Moon, midway between the crater D'Arrest two crater diameters to the south

is a largely degraded lunar impact crater that is located near the eastern limb of the Moon. Banachiewicz crater is located near the eastern limb of

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