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In contrast, the Lunar distance (LD or ), or Earth–Moon characteristic distance, is a unit of measure in astronomy. More technically, it is the semi-major axis of the geocentric lunar orbit . The average lunar distance is approximately 385,000 km (239,000 mi), or 1.28 light-seconds ; this is roughly 30 times Earth's diameter .
Modern Lunar Laser Ranging data can be fit with a 1 cm weighted rms residual. The center of Earth to center of Moon distance is computed by a program that numerically integrates the lunar and planetary orbits accounting for the gravitational attraction of the Sun, planets, and a selection of asteroids. [36] [23]
In celestial navigation, lunar distance, also called a lunar, is the angular distance between the Moon and another celestial body. The lunar distances method uses this angle and a nautical almanac to calculate Greenwich time if so desired, or by extension any other time. That calculated time can be used in solving a spherical triangle.
The Lunar Instrumentation for Subsurface Thermal Exploration with Rapidity (LISTER) is designed to measure heat flow from the interior of the Moon. The probe will attempt to drill 2.13 to 3.05 meters (7 to 10 ft) into the lunar regolith to investigate the Moon's thermal properties at different depths.
[36] [37] To determine this value, Ptolemy started by measuring the Moon's parallax, finding what amounted to a horizontal lunar parallax of 1° 26′, which was much too large. He then derived a maximum lunar distance of 64 + 1 / 6 Earth radii. Because of cancelling errors in his parallax figure, his theory of the Moon's orbit, and ...
The Lunar Traverse Gravimeter was a lunar science experiment, deployed by astronauts on the lunar surface in 1972 as part of Apollo 17.The goal of the experiment was to use relative gravity measurements to infer potential attributes about the geological substrata near the Apollo 17 landing site.
To determine the distance to the reflector to 1 mm precision, or 7 ps, by averaging, the measurement needs at least (400/7) 2 ≈ 3000 photons. This explains why a much larger system is needed to improve the existing measurements—the pre-APOLLO 2 cm RMS range precision required only about 10 photons, even at the worst-case orientation of the ...
The Earth appears in the Moon's sky with an apparent size of 1° 48 ′ to 2°, [295] three to four times the size of the Moon or Sun in Earth's sky, or about the apparent width of two little fingers at an arm's length away. Observations from the Moon started as early as 1966 with the first images of Earth from the Moon, taken by Lunar Orbiter 1.
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