「craters」の共起表現(1語右で並び替え)

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craters

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were proponents for a volcanic origin of the craters, a theory that was later proved incorrect.
It is located at 21.1°N, 18.2°W, north of the craters Abu Nuwas and Moliere, and east of the crater
There are two small subsidiary craters adjacent to the main cone and some lava flows
The craters' age is estimated as 4,000-5,000 years.
Each group often containing several large craters all of which were the result of explosions ca
A characteristic feature of both craters, almost identical in size, is the "pedestal"
A crater chain is a line of craters along the surface of an astronomical body.
There are several tiny craters along the rim edge and the inner walls, but n
to the south, and there is a pair of smaller craters along the western rim and inner wall.
ons that a new surface forms with zero impact craters, and that impact craters accumulate at some c
Diamond Craters and the nearby Diamond post office were named
ns seen on the Moon often radiate from larger craters, and are thought to be either caused by secon
The craters and the area around contain numerous fragment
ules will likely differ from those for impact craters, and thus "Copland" would probably not be an
tly misplaced shot; thick rough that features craters and mounds; tall, shot-obstructing palm trees
These may be related impact craters, and if correct, Aorounga may be part of a cr
called axalpazcos, lying in shallow volcanic craters and sustained by underground water.
There were huge craters and gas flames blazing high in the air and ta
It contains seven meteor craters, and was created in 1976 with an area of 55 h
s, animated solar flares and prominences, 3-D craters and mountains, and historic collision events.
elatively young because they have few, if any craters, and they lie on top of sand dunes which are
ns suggest the presence of many recent impact craters and landforms such as chevrons which are thou
ozen nitrogen and methane sprinkled by impact craters and openings of geysers.
d about 30 small shield volcanoes, along with craters and lava flows.
The engineers filled bomb craters and laid Pierced Steel Planking over the dama
Bomb craters and long strings of strafing bullet marks fro
He placed them in the shelter of shell craters and then alone faced a strong enemy counterat
oes not have the circular shape of most lunar craters, and instead has the overall shape of three o
Furthermore, both craters appear crisp and feature terraces.
The ejecta deposit surrounding the craters appears very bright on the bright terrain.
These pit craters are thought to be evidence of shallow volcani
Ghost craters are unusual forms that occur in the Suisei Pl
The nearest named craters are Lichtenberg to the southwest and Nielsen
face is striated by cracks and streaks, while craters are relatively infrequent.
Many chains of secondary craters are visible radiating from Oskison outward on
Nearby named craters are Clark to the east, and Pogson to the sout
Fossae/pit craters are common near volcanoes in the Tharsis and
ken under higher sun illumination angle, both craters are shown to have extended bright rays, espec
he extensive flows, unique to Venusian impact craters, are a continuing subject of study for a numb
Complex craters are distinguished by having a raised central
The eastern and western craters are 26 km (16 mi) and 36 km (22 mi) in diamet
The two craters are believed to have formed nearly simultaneo
A pair of small craters are also attached to the outside of the west
The craters are believed to have formed simultaneously as
The closest named craters are Vashakidze to the southeast on the far si
The Arkenryu craters are a pair of eroded impact craters in Libya.
ause fresh and rough surfaces of young impact craters are good scatterers of radio waves.
Secondary craters are impact craters formed by the ejecta that
nce turned into a morass of mud, trenches and craters as had happened during the First World War.
ientists to map the size and shape of as many craters as possible using data from the NASA Lunar Re
The Meteorite Craters at Henbury Central Australia by A.R. Alderman
Many craters at equatorial and mid-latitudes on Mars have
The discovery of multiple pit-floor craters augments evidence that volcanic activity has
Two craters bear his name.
Small craters belonging to the Catena Abulfeda intrude slig
Two parasitic craters, both about 90 x 45 m (300 x 150 ft) wide, ar
nitials to distinguish them from the existing craters called Anderson, Brown and Clark.
uptions occasionally create broad, low-relief craters called maars.
Spasmodic Geyser's eruptions from the two craters can be up to 15 feet (4.6 m) high.
Black Buck Two's craters can be seen more clearly to the left.
The craters can still be seen.
ng to and from Liverpool and a number of bomb craters can still be seen today.
About 20 small craters can be found today.
The outer wall is bordered by the craters Carnot to the south, Rowland along the west r
on Mars expose stratified layers on slopes in craters, channels, and hillsides, it would be extreme
forms the southern-most member of a chain of craters consisting of Vogel, Argelander, and Airy.
The craters, containing iron masses, were reported in 157
Rowley has said that the chance that these craters could be aligned like this due to chance are
terior is relatively flat, with multiple tiny craters covering parts of the floor.
owed that shocked quartz is also found inside craters created by meteor impact, such as the Barring
estimates vary), it is one of the most recent craters created by an impact event and the only known
t to the northeast are the small, bowl-shaped craters De Morgan and Cayley.
A linear formation of craters designated Catena Artamonov lies alongside th
However, a few large craters do stand out.
e Range of western North America, and at Inyo Craters east of the Sierra Nevada in California.
spot-shaped telescopic features (later called craters) eponyms of noted astronomers and philosopher
It lies near the mid-point between the craters Euler to the west and Lambert to the east.
e life, and could be an important analogue to craters filled with sediment in a similar way on Mars
ction left large areas filled with debris and craters for decades.
The Enki craters formed across the sharp boundary between area
rt crater shows many long chains of secondary craters, formed by impact of material thrown out duri
the Open University, discovered that the five craters formed a chain, indicating the breakup and su
Even though all the craters formed nearly simultaneously, it is difficult
If these secondary craters formed from a single, large, nearby impact, t
and are often accompanied by small secondary craters formed by larger chunks of ejecta.
The smallest craters found have been microscopic in size, found in
nter of Vepriai Meteor Crater, the largest of craters found in Lithuania.
oring terrain (except for the small secondary craters from the large, fresh crater to the west of R
brium (foreground) is peppered with secondary craters from the impact that formed Copernicus crater
y to be confused with quarries, although bomb craters from WW2 can occasionally lead the landscape
along with the entire village; several large craters from underground mines were blown over the co
It lies between the craters Goclenius to the northwest and Crozier to the
All of the craters had previously been known and studied, but th
cted since previous drillings on large impact craters had not produced such fragments, and it was t
One of these craters has cut a notch in the southeast wall, and th
To the northwest are the craters Hase and Petavius, and to the southwest is Fu
he crater is located in between the prominent craters Haskin and Hansen.
Very few impact craters have been found in Diyar, demonstrating the y
Many of these smaller craters have also been eroded, leaving little more th
Both craters have the same age, 290 ± 20 million years (Pe
The following craters have been renamed by the IAU.
Several of the more notable craters have received names.
Multiple examples of pit craters have been observed on Mercury on the floors o
6 including actions in battle at the St. Eloi Craters, Hill 62, Mount Sorrel and Sanctuary Wood.
the position of Opportunity and names for the craters Iazu, Endeavour, and Victoria
e reflective features appear to coincide with craters imaged by Mariner 10, with the largest featur
The craters in the catena seem to have formed from east t
Orbiter Laser Altimeter - counted some 50,000 craters in one 20-kilometer area.
leads scientists to believe that some of the craters in Arabia may have held huge lakes.
nomer in Ottawa and made a study of meteorite craters in Canada.
iameter, making it one of the smallest impact craters in the world.
eroded, and the surface reshaped by multiple craters in the interior and along the rim.
th) paraboloidal streaks were observed around craters in earlier Magellan images, but this is a rar
All of the craters in the cluster would appear to be equally ero
July 2010 showed that is one of at least nine craters in the northern lowlands that contains hydrat
Some craters in Tikhonravov are classified as pedestal cra
younger and less eroded than the other large craters in the surroundings.
For meteorite-created craters in general, see Impact crater.
Among the largest and most famous metal craters in antiquity were one in the possession of th
Some craters in Thaumasia show dark blotches in them.
There are three possible meteorite craters in Smiltene.
Nearby craters include the irregular Meton formation to the
Nearby craters include Watts to the southeast and Lawrence t
A pair of small craters, including Fabry H, lies along the eastern ri
internal structure typical of complex impact craters, including an uplifted centre, and suggests t
cross the surrounding surface and neighboring craters, indicating that Enwonwu crater was formed co
Diamond Craters is a volcanic field or small shield volcano i
Unlike other young craters, it is very flat, so if it is of impact origi
Unlike many Finnish craters, it does not seem to have been buried under l
Although it has few craters, it is believed that this is the oldest terra
the crater [one of Mauna Loa's lower volcanic craters, Kilauea] and walked on the dome's hot surfac
eral Virrat crater radii to the north are the craters Koga and Nhill.
The craters La Caille to the southwest and Faye to the no
The eruptions from the Four Craters Lava Field were accompanied by a slight sinki
It is located in the southwest corner of Four Craters Lava Field in the Deschutes National Forest.
this crater is a series of valleys and impact craters leading a couple of hundred kilometres to the
Smaller craters lie along many parts of this remaining rim, m
A cluster of small craters lie across the south-southwest rim and inner
A pair of craters lie across the southwestern rim, and two smal
r has been worn by impacts, and multiple tiny craters lie along the rim.
t escaped the bombardment, and multiple small craters lie across the interior, in some places overl
A combination of three small craters lie across the northern rim, at the eastern e
Multiple small craters lie across the rim and inner wall, leaving a
and eroded, and a pair of small, bowl-shaped craters lies across the western rim.
Shell craters littered the ground all around the buildings
Kaali is a group of 9 meteorite craters located on the Estonian island of Saaremaa.
an eroded crater formation with several small craters lying long the rim.
r wall of Abbe is somewhat eroded, with small craters lying across the northwest and southwest rim
There are small craters lying along the inside and attached to the ex
n end of the interior floor, and several tiny craters mark the surviving rim.
, with the usual accompaniment of tiny impact craters marking the surface.
The images revealed river beds, craters, massive extinct volcanoes (such as Olympus M
noes are less than 60,000 years old, and some craters may be as recent as 6,000 years based on the
Pit-floor craters may provide an indication of internal igneous
When hiking here early in summer, some of the craters may be filled with runoff water (called maars
The secondary craters may be in clusters.
On the same walled basin are the craters Moissan to the south and Richards to the west
Incidentally, craters named after Ghanim's father, Ayyub, and siste
rater is the eastern-most of the row of three craters named in honor of the Apollo 11 crew members.
crater is the western-most of a row of three craters named in honor of the Apollo 11 crew members.
ter is the central member of the row of three craters named in honor of the Apollo 11 crew members.
Incidentally, craters named Ghanim and Fitnah are found near Ayyub.
Incidentally, craters named Ghanim and Ayyub are found near Fitnah.
A chain of craters named the Catena Abulfeda runs between the so
southern rim is overlain by a pair of smaller craters named Cyrillus B and C. The crater floor is r
ad about 60 new names to anonymous craters near the edge of the moon that had been broug
There is a cluster of small craters near the mid-point of the interior, and the w
es from Mars Global Surveyor, surveying small craters never before cataloged.
The nearest craters of note are Larmor to the north and Morse to
All three were satellite craters of Langrenus before being renamed by the IAU.
e things seen by Galileo Galilei, such as the craters of Earth's Moon, four of Jupiter's moons, and
escopes in 1609, which they used to study the craters of the Moon and Halley's Comet.
The rim is pock-marked by small craters of various dimensions.
e interior floor is covered in a multitude of craters of various sizes.
, particularly at sea, by observing peaks and craters of the Moon as they appear and disappear, not
Nearby craters of note include Maxwell and Lomonosov to the
Craters of this dimension typically form cup-shaped e
Craters of the Sac is a semi-official MP3-only album
worn, being covered in a multitude of smaller craters of various sizes.
terrain, and is not overlain by other impact craters of note.
He is an authority on the meteor craters of Brazil and known for the Crosta method/tec
No craters of note overlie the rim, although some format
Nearby craters of note include Tikhov, which is nearly attac
d and rounded, but is not marked by any small craters of significance.
ned outer rim that is not overlain by smaller craters of note.
Craters of the Moon National Monument
The Craters of the Moon, a steamfield close-by, created b
Conrad et al. (2007) show that craters of this size "can be expected from the impact
There are two small impact craters of note within the interior: Banachiewicz B i
woods surrounding the village has three large craters often mistakenly attributed to World War II b
Craters on the Moon and on Mars were named in his hon
Craters on Mars and the Moon are named in his honor.
Craters on the Moon and Mars were named in his and hi
onception of the world forever: mountains and craters on the Moon, a plethora of stars invisible to
is probably one of the youngest large impact craters on Titania.
Because there are few craters on this mantle, the mantle is relatively youn
Craters on Mars and on the Moon were named in his hon
a Artamonov is a 134 km (83 mi)-long chain of craters on the Moon.
ate tectonics, have destroyed most multi-ring craters on Earth.

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