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Rille on the Moon
Rimae Atlas are rilles on the crater of Atlas, on the Moon. The naming of the rilles were derived from the Atlas crater that was named after Atlas, the
Rimae_Atlas
Lunar impact crater
northeast and southeast walls. A system of slender clefts named the Rimae Atlas crosses the crater floor, and were created by volcanism. Along the north
Atlas_(crater)
found on lunar maria. These features form a cape or headland on a mare. Rimae (singular rima) are lunar rilles. These are escarpments in the surface.
List_of_lunar_features
System of rilles on the Moon
Rimae Secchi is a system of rilles on the Moon, in northwestern Mare Fecunditatis. They are approximately 40 km long and run along the shore of the mare
Rimae_Secchi
Crater on the Moon
Just to the northwest of Littrow is a system of rilles designated the Rimae Littrow. These are located at selenographic coordinates 22.1° N, 29.9° E
Littrow_(crater)
Crater on the Moon
Aristarchus. Just to the north of Prinz is a system of rilles designated the Rimae Prinz. These are sinuous in nature and extend for up to 80 kilometers. The
Prinz_(crater)
Crater on the Moon
There is a group of rilles located to the west of the crater named the Rimae Bode. Its name comes from the name of the crater. Due to the interesting
Bode_(crater)
Lunar impact crater
central peak, but the floor is hilly and laced with a rille system named the Rimae Posidonius. The floor is also slightly bulged due to the past lava uplift
Posidonius_(crater)
Small circular depression on the Moon
contacts Rimae Herigonius. Oblique image also from Apollo 16 Regional map Most of the Rimae Herigonius and Herigonius K crater (below center). The rimae (rilles)
Herigonius_(crater)
Rille on the Moon
Rimae Sirsalis is a lunar rille. It is located at 15°42′S 61°42′W / 15.7°S 61.7°W / -15.7; -61.7 and is 426 km long. It was formed by extension of
Rimae_Sirsalis
Fissure, especially on the Moon
surface of the Moon that resemble channels. The Latin term is rima, plural rimae. Typically, a rille can be several kilometers wide and hundreds of kilometers
Rille
Crater on the Moon
of higher-albedo material. Just to the south lies the rille system named Rimae Hypatia. These follow a course running roughly east-southeast to west-northwest
Moltke_(crater)
Crater on the Moon
by lava, and is now cross-crossed by a system of small clefts named the Rimae Hevelius. There is a low, one-km-high central peak offset to the northwest
Hevelius_(crater)
which: 19 are craters, 8 are Regiones, 3 are Labes, 2 are Fossae, 2 are Rimae, 2 are Rupes, and 1 is a Dorsum. 21 Lutetia was flown by in July 2010 by
List of geological features on 21 Lutetia
List_of_geological_features_on_21_Lutetia
Crater on the Moon
(43 mi) to the north of Hypatia is a system of linear rilles designated Rimae Hypatia, running about 180 kilometers (110 mi) across the Mare Tranquillitatis
Hypatia_(crater)
Crater on the Moon
of Grimaldi is a system of rilles named the Rimae Grimaldi. To the northwest, rilles belonging to the Rimae Riccioli approach the western edge of Grimaldi's
Grimaldi_(crater)
Crater on the Moon
surrounding surface. This system of clefts in the surface is designated Rimae de Gasparis, and they span an area of about 47 km (29 mi) in diameter. The
De_Gasparis_(crater)
Crater on the Moon
during their LMP ascent. To the northwest is a rille system designated the Rimae Sulpicius Gallus. These extend to the northwest for a distance of about
Sulpicius_Gallus_(crater)
Lunar impact crater
To the east on the mare is a formation of parallel rilles designated the Rimae Sosigenes. These follow a course to the north, and have a length of about
Sosigenes_(crater)
Crater on the Moon
of the crater is designated Rimae Maclear, while the rilles to the south-southwest are named Rimae Sosigenes. The Rimae Maclear stretches for about 100
Maclear_(crater)
Mountain range on the Moon
designated Rimae Plinius. 100 km farther to the west the craters Menelaus and Auwers are embedded within the range, and to their northeast are the Rimae Menelaus
Montes_Haemus
Feature on the moon
(110 mi). In the southern part of this area is a rille system designated Rimae Archimedes. To the south is a prominent linear rille named Rima Bradley
Palus_Putredinis
Crater on the Moon
Wikimedia Commons has media related to Schroter (crater). Lunar Orbiter 1 images 113 and 114, showing parts of Rimae Schröter Schröter at The Moon Wiki
Schröter_(lunar_crater)
Lunar surface depression
satellite crater Vasco da Gama R contains a system of rilles designated the Rimae Vasco da Gama. By convention these features are identified on lunar maps
Vasco_da_Gama_(crater)
Lunar impact crater
the northeast is Dawes. Just to the north is a system of rilles named the Rimae Plinius and touching it is the Brackett crater which is more than a crater
Plinius_(crater)
NASA orbiter mission to the Moon (1967–1968)
Schroteri, Marius Hills, Montes Apenninus, Rimae Plato, Sinus Aestuum, Hipparchus, Rimae Sulpicius Gallus, Rimae Calippus, Censorinus, Dionysius, and the
Lunar_Orbiter_5
Lunar crater
by high-albedo ejecta. To the west is a system of rilles designated the Rimae Menelaus. It was named after Brabantian mathematician André Tacquet (1612-1660)
Tacquet_(crater)
Crater on the Moon
Archived from the original on June 14, 2011. Wood, Chuck (August 12, 2006). "Rimae Weird". Lunar Photo of the Day. Archived from the original on June 14, 2011
Pallas_(crater)
Circular depression on the Moon
There is also a system of fractures that criss-crosses the floor, named the Rimae Gassendi. The fresh crater Gassendi A is adjacent to Gassendi to the north
Gassendi_(crater)
Crater on the Moon
Väisälä lies just to the west of the Rupes Toscanelli fault line, and the Rimae Aristarchus rille system. To the southwest is the notable Vallis Schröteri
Väisälä_(crater)
Wrinkle ridge system on the Moon
Dorsum Buckland. It is also roughly in line with Rimae Sulpicius Gallus to the northwest and with Rimae Menelaus to the southeast. "Dorsa Sorby". Gazetteer
Dorsa_Sorby
Crater on the Moon
north of Opelt on the lunar mare is a sinuous system of rilles designated Rimae Opelt. These occupy a diameter of about 70 kilometers. By convention these
Opelt_(crater)
Lunar impact crater
to the southwest contains a number of rilles belonging to the Rimae Aristarchus and Rimae Prinz rille systems. Further to the east-southeast are the Montes
Krieger_(crater)
Crater on the Moon
crater. The interior floor of Repsold contains a prominent rille named the Rimae Repsold. It begins in the northeastern part of the floor and crosses to
Repsold_(crater)
Crater on the Moon
submerged by the mare. South of this feature is a system of linear rilles named Rimae Maestlin. The mare surface around Maestlin is dusted with ray material from
Maestlin_(crater)
Mountain range on the Moon
eastern rim of the dark-floored crater Plato. The system of rilles named Rimae Plato may be found in between the eastern edge of Plato and the western
Montes_Alpes
Crater on the Moon
two form a distinctive feature. To the east is a rille system named the Rimae Sirsalis. The longest of these rilles follows a line running approximately
Sirsalis_(crater)
Impact crater on the Moon
Putredinis, a lava-flooded plain containing a system of rilles named the Rimae Archimedes, which extends over 150 kilometers. North-northwest of Archimedes
Archimedes_(crater)
Crater on the Moon
southwest lies Ramsden. This feature lies in a system of rilles named the Rimae Ramsden, and an interrupted branch passes only a few kilometers to the south
Marth_(lunar_crater)
Crater on the Moon
crater, among the Montes Alpes, are several rilles collectively named the Rimae Plato. On the lunar geologic timescale, Plato is one of the largest craters
Plato_(crater)
Crater on the Moon
difficult to find. The southern rim is contacting a rille system named Rimae Plinius. The crater is named after American physicist Frederick Sumner Brackett
Brackett_(crater)
Crater on the Moon
several small rilles to the southwest of Wollaston, forming part of the Rimae Prinz. The crater was formally named by the IAU in 1935. This is a circular
Wollaston_(crater)
Lunar crater
the prominent crater Plinius. South of the crater are the rilles of the Rimae Maclear. The rim of this crater is rich in high calcium pyroxene, while
Al-Bakri_(crater)
Rille on the Moon
(186.4 mi) long, is a fault system similar to those on Earth. "Straight Rimae". www.hq.nasa.gov. Archived from the original on 2018-05-30. Retrieved 2018-10-01
Rima_Ariadaeus
Crater on the Moon
irregular. To the northeast of this crater is a system of rilles designated Rimae Maupertuis. These are considered to have formed through geological activity
Maupertuis_(crater)
Lunar crater
northwest of Santos-Dumont is a 90-km-wide system of rilles designated the Rimae Fresnel, being named for the Promontorium Fresnel that lies to the north
Santos-Dumont_(crater)
Lunar impact crater
Palus Epidemiarum reaches the west rim of Mercator, and a rille from the Rimae Ramsden reaches the western rim at the site of the craterlet Mercator C
Mercator_(crater)
Crater on the Moon
lava) within the larger Gerard Q Outer, and a system of rilles named the Rimae Gerard. These extend for a distance of about 100 kilometers. Like many craters
Gerard_(crater)
Crater on the Moon
Fabricius. The floor of this inner depression contains a rille system named the Rimae Janssen. The rille curves from the rim of Fabricius to the southeast of
Janssen_(lunar_crater)
Lunar impact crater
is designated Rimae Maclear, after the crater Maclear just to the east of the bay. At the southern end of the bay entrance is the Rimae Sosigenes, named
Sinus_Honoris
Crater on the Moon
the patch of highland containing Lubbock is the rille system designated Rimae Goclenius. The parallel rays from the crater pair of Messier and Messier
Lubbock_(crater)
Feature on the moon
This mare is notable for a system of rilles in the western end named the Rimae Ramsden, and for the wide Rima Hesiodus that extends from near the midpoint
Palus_Epidemiarum
Crater on the Moon
Somniorum. To the south-southeast is the much larger crater Posidonius. The Rimae Daniell rille system is to the west of Daniell crater, and consists of a
Daniell_(crater)
Crater on the Moon
Other rille systems lie in the vicinity, including the Rimae Ritter to the southeast and Rimae Sosigenes to the northeast. The crater was named after
Ariadaeus_(crater)
Crater on the Moon
contains low hills in the east and a system of slender clefts named the Rimae Pitatus. The larger and more spectacular of these rilles follow the edges
Pitatus_(crater)
Crater on the Moon
east is the larger crater Ramsden, within a system of rilles named the Rimae Ramsden. This is an elongated crater feature that is longer in the north–south
Lepaute_(crater)
Crater on the Moon
broken across the northeast by a pair of clefts that form a part of the Rimae Goclenius. These extend northwest from the Goclenius region. The central
Gutenberg_(crater)
Lunar impact crater
region that has a number of rille systems, with the Rimae Hippalus to the northwest, and the Rimae Ramsden to the south and east. By convention these features
Dunthorne_(crater)
Lunar impact crater
the International Astronomical Union in 1935. A rille system, called the Rimae Parry, crosses the region in a series of graben. One rille crosses the southeast
Parry_(crater)
Crater on the Moon
running for a length of up to 240 kilometers. This feature is named the Rimae Goclenius. The rim of this crater is worn, distorted and irregular, having
Goclenius_(crater)
Crater on the Moon
northeast wall in that part of the crater. A system of rilles named the Rimae Riccioli lies across the interior, and crosscut the ejecta ridges. In the
Riccioli_(crater)
Crater on the Moon
light-hued outer rim and a darker interior floor. A rille belonging to the Rimae Parry almost connects with the north-northwestern rim of Tolansky. It was
Tolansky_(crater)
Lunar impact crater
has been resurfaced by lava flow, and displays a rille system named the Rimae Petavius. The large central mountains are a prominent formation with multiple
Petavius_(crater)
Crater on the Moon
the level interior floor is offset slightly to the east. A rille from the Rimae Repsold system crosses the northeastern rim and traverses the interior,
Galvani_(crater)
Crater on the Moon
the surface and edges of the Mare Humorum is a rille system designated Rimae Mersenius. These rilles are generally parallel and run to the north-northeast
Mersenius_(crater)
Lunar impact crater
it intersects the lunar mare. To the southwest is a rille system named Rimae Grimaldi, named after the crater. This continues to the west and south,
Damoiseau_(crater)
Escarpment on the Moon
Rimae Fresnel is a 90km-long arcuate escarpment on the Moon at 28°00′N 4°00′E / 28.0°N 4.0°E / 28.0; 4.0. Both the escarpment and the nearby Promontorium
Rimae_Fresnel
Crater on the Moon
the north. This rille is part of a nearby system that has the designation Rimae Aristarchus. Just to the south of Toscanelli is a fault line in the surface
Toscanelli_(crater)
Genus of leguminous plants
Hend. Lupinus revolutus C.P. Sm. Lupinus richardianus C.P. Sm. Lupinus rimae Eastw. Lupinus rivularis Lindl. – riverbank lupin Lupinus romasanus Ulbr
Lupinus
Crater on the Moon
across the crater floor. To the south is a pair of rilles designated the Rimae Secchi. These lie near the edge of the mare, and have a combined length
Secchi_(lunar_crater)
Crater on the Moon
distance to the southeast is Mersenius. A system of faint rilles named the Rimae Zupus lie to the northwest, following a course to the north-northwest towards
Zupus_(crater)
Crater on the Moon
To the northwest of the crater is a prominent system of rilles named the Rimae Römer. These follow a course to the north from the western rim of the crater
Römer_(crater)
Crater on the Moon
even smaller Daubrée. To the northeast is a faint rille system named the Rimae Menelaus. The wall of Menelaus is slightly irregular in outline, with a
Menelaus_(crater)
Crater on the near side of Earth's Moon
Vallis Schröteri, and south of a system of narrow sinuous rilles named Rimae Aristarchus. Aristarchus is bright because it is a relatively young formation
Aristarchus_(crater)
Crater on the Moon
easy to recognize. The surface is crossed by the rille system designated Rimae Boscovich that extends for a diameter of 32 kilometres. Two of these rilles
Boscovich_(crater)
Crater on the Moon
eastern edge of Mare Serenitatis in the midst of a rille system named the Rimae Littrow after the crater Littrow to the east. This crater is roughly circular
Clerke_(crater)
Crater on the Moon
Astronomical Union in 1935. Cauchy lies between the Rupes Cauchy and the Rimae Cauchy. To the south of Cauchy is a 150-km fault in the surface named the
Cauchy_(crater)
Crater on the Moon
Triesnecker (crater). Triesnecker at the Moon Wiki Rimae Triesnecker at the Moon Wiki Lunar Orbiter 2 Closeup of Rimae Triesnecker (Lunar and Planetary Institute)
Triesnecker_(crater)
Feature on the moon
the southern half of this border area lies a rille system designated the Rimae Daniell, which consists of a set of graben oriented along a NNW-SSE direction
Lacus_Somniorum
Crater on the Moon
surface between this pair and Leakey is a system of rilles designated the Rimae Gutenberg that follow a course to the southeast. Leakey is a circular, bowl-shaped
Leakey_(crater)
Crater on the Moon
ridges. To the northwest of Ritter is a system of parallel rilles designated Rimae Ritter. These follow a course to the northwest. Ranger 8 flew over Ritter
Ritter_(crater)
Lunar impact crater
of Campanus is the rille system named Rimae Hippalus. Another rille system lies to the south, designated Rimae Ramsden. This formation is named after
Campanus_(crater)
Crater on the Moon
lava-flooded floor of Hippalus is bisected by a wide rille belonging to the Rimae Hippalus. This rille follows a course to the south before curving gently
Hippalus_(crater)
Feature on the moon
contains an extensive system of criss-crossing rilles collectively designated Rimae Bürg, spanning a length of 140 km. The rilles are suspected to have formed
Lacus_Mortis
Lunar surface depression
the east are Hippalus crater and Promontorium Kelvin. To the west are the Rimae Doppelmayer and the Rupes Liebig, which are cliffs near Liebig itself which
Mare_Humorum
Crater on the Moon
Liebig and de Gasparis. The floor is marked by a system of rilles named the Rimae Palmieri that continue to the north and southeast beyond the crater perimeter
Palmieri_(crater)
Crater on the Moon
Ritter and Sabine. Just to the northwest is the system of rilles designated Rimae Ritter. These clefts follow a generally northwest direction. The rim of
Dionysius_(crater)
Feature on the moon
surface between Liebig and de Gasparis, is a system of rilles named the Rimae de Gasparis. These cover an area with a diameter of 130 km. By convention
Liebig_(crater)
Headland on the near side of the Moon
Mare Serenitatis and Mare Imbrium. Just west of the mountainous cape is Rimae Fresnel. Both features were named after the French physicist Augustin-Jean
Promontorium_Fresnel
Crater on the Moon
lava-flooded remains of De Vico T. Beyond is a linear rille designated Rimae Sirsalis that follows a path to the northeast past the rim of Sirsalis.
De_Vico_(crater)
Crater on the Moon
a ray system. The crater lies directly across a rille system named the Rimae Ramsden. These span an area 130 kilometers across, sprawling over the western
Ramsden_(crater)
Lunar impact crater
crater Zupus. Midway between Fontana and Zupus is a rille system designated Rimae Zupus. This is a low-rimmed crater with an interior floor that is marked
Fontana_(lunar_crater)
Lunar impact crater
broken by a series of narrow clefts. These are collectively designated the Rimae Parry. The clefts cross the rim to the south and also to the north, with
Bonpland_(crater)
Lunar impact crater
Furnerius. To the southwest of Adams is a system of rilles designated the Rimae Hase. The longest of these rilles follows a course to the southeast. Adams
Adams_(lunar_crater)
Former RNLI Lifeboat station in North Ayrshire, Scotland
The Lifeboat. X (103): 22. 1 February 1877. Retrieved 19 October 2024. "Rimae". The Lifeboat. XIII (139): 10. 1 February 1886. Retrieved 19 October 2024
Kildonan_Lifeboat_Station
Feature on the moon
eastward to the edge of the Mare Tranquillitatis. At longitudes 4-6° E is the Rimae Triesnecker rille system, named after the crater Triesnecker just to the
Sinus_Medii
Lunar impact crater
the central Cavendish crater floor from east to west. A rille from the Rimae de Gasparis reaches the eastern rim of Cavendish. The crater only has one
Cavendish_(crater)
Crater on the Moon
irregular. To the southeast of Hase D is a system of linear rilles designated Rimae Hase. Their north-western extension transects western part of Hase and Hase
Hase_(crater)
Crater on the Moon
irregular and uneven, and contains a system of faint rilles called the Rimae Chacornac, which cross the crater wall to the south. There is one distinct
Chacornac_(crater)
Crater on the Moon
crater Fabbroni, and to the northeast is Littrow. North of Ching-Te is the Rimae Littrow rille system as well as the crater Clerke. Between Ching-Te and
Ching-Te_(crater)
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