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Geological studies of the Moon are based on a combination of Earth-based telescope observations, measurements from orbiting spacecraft, lunar samples, and geophysical data. . Six locations were sampled directly during the crewed Apollo program landings from 1969 to 1972, which returned 382 kilograms (842 lb) of lunar rock and lunar soil to Earth [8] In addition, three robotic Soviet Luna ...
Lunar maria (singular mare) are large, dark, regions of the Moon. They do not contain any water, but are believed to have been formed from molten rock from the Moon's mantle coming out onto the surface of the Moon. This list also includes the one oceanus and the features known by the names lacus, palus and sinus.
A Blue Moon is the term for the second full moon in a month. Typically full moons come once a month (every 30 or so days), but in the event of a Blue Moon, it happens twice.
The Moon is Earth's only natural satellite.It orbits at an average distance of 384,400 km (238,900 mi), about 30 times the diameter of Earth. Tidal forces between Earth and the Moon have synchronized the Moon's orbital period (lunar month) with its rotation period at 29.5 Earth days, causing the same side of the Moon to always face Earth.
Tuesday’s moon followed the Aug. 19 super blue moon. A blue moon does not describe the color of the moon; instead, it refers to the third full moon occurring in a season with four full moons.
The first of these three is pretty well known to us: a phase in the lunar cycle in which the Earth, sun, and moon are aligned with the Earth in the middle, so the moon is fully illuminated on Earth.
The US has been studying the Moon for decades and in 2019 it started to implement the Commercial Lunar Payload Services (CLPS) program to support the crewed Artemis program, both aimed at scouting and exploiting lunar resources to facilitate a long-term crewed base on the Moon, and depending on the lessons learned, then move on to a crewed ...
A transient lunar phenomenon (TLP) or lunar transient phenomenon (LTP) is a short-lived change in light, color or appearance on the surface of the Moon. The term was created by Patrick Moore in his co-authorship of NASA Technical Report R-277 Chronological Catalog of Reported Lunar Events , published in 1968.