「Craters」の共起表現一覧(1語右で並び替え)
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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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