Wiki User
∙ 14y agoThe whole Moon has a diameter of about 30 arc-minutes, as seen from us; the real diameter is about 3400 kilometers. You can write a ratio or proportion with those numbers.
Wiki User
∙ 14y agoThe diameter of a lunar crater with 1 minute of arc is roughly 1.6 kilometers. The actual size of lunar craters can vary widely, so this is just an approximate value.
lenpollock
1 minute of arc is 1 nautical mile. (Not( land) miles).
That is 1/60 of a degree.
This in turn is 1852 m. or 1.852 km/
A crater or a rill.
Lunar craters are found on the surface of the Moon. They are formed by impacts from meteoroids, asteroids, or comets hitting the Moon's surface. Some well-known lunar craters include Tycho, Copernicus, and Aristarchus.
Two of the larger craters on the moon are the Mare Orientale, located on the moon's western limb, and the South Pole–Aitken basin, located near the south pole. Mare Orientale is about 920 km in diameter and is one of the most prominent lunar impact basins, while the South Pole–Aitken basin is one of the largest and deepest impact craters in the solar system, with a diameter of about 2,500 km.
The Copernicus crater on the moon was formed by a large impact event, likely from an asteroid or comet colliding with the lunar surface. The impact created a circular depression that we see as the crater today.
Without a telescope, you can see the different phases of the moon, lunar craters, and dark patches known as lunar seas or maria. You may also see some of the moon's prominent features, such as the Tycho crater or the Apennine Mountains.
The craters on the Moon's maria can vary in size, but some can be several kilometers in diameter. The largest known crater on a lunar mare is the Orientale Basin, which is about 930 kilometers in diameter.
One name of a crater on the moon is Tycho. Tycho Crater is a prominent lunar impact crater with a diameter of about 85 kilometers and is located in the southern highlands of the moon. It is easily recognizable due to its bright rays that extend across the lunar surface.
A crater or a rill.
Lunar craters are found on the surface of the Moon. They are formed by impacts from meteoroids, asteroids, or comets hitting the Moon's surface. Some well-known lunar craters include Tycho, Copernicus, and Aristarchus.
Not surprisingly Sacrobosco Crater. It is an irregular lunar impact crater [See Link] that is located in the southern highlands to the west of the Rupes Altai escarpment.
Two of the larger craters on the moon are the Mare Orientale, located on the moon's western limb, and the South Pole–Aitken basin, located near the south pole. Mare Orientale is about 920 km in diameter and is one of the most prominent lunar impact basins, while the South Pole–Aitken basin is one of the largest and deepest impact craters in the solar system, with a diameter of about 2,500 km.
The lunar crater Hase is located in the rugged southeast part of the moon, to the south-southwest of the prominent walled plain petavius, the palitzsch and vallis palitzsch are attached to the northeastern rim of the haze.
The scientific term for the light colored crater filled highland areas of the lunar surface is called the lunar highlands. These areas are characterized by their rugged terrain, abundant impact craters, and lighter-colored surface material compared to the lunar maria.
It's a crater on the surface of the Moon, probably the result of an asteroid impact.
Assuming that the moon is spherical and the orbit is circular: Lunar diameter = 3,475 km Orbital diameter = 3,475 + 42 = 3,517 km Orbital circumference = (pi) times diameter = 3,517(pi) = 11,048.981 km (rounded)
1) A house built of "Sod" 2) An eroded Lunar Impact Crater
LCROSS stands for Lunar Crater Observation and Sensing Satellite. It was a NASA mission launched in 2009 to study the permanently shadowed regions of the moon's polar regions by impacting a spacecraft into a crater to expose subsurface materials.