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New finding reveals billions of years of lunar history. China’s Chang’e-4 mission rover has helped scientists visualise “hidden” structures deep below the surface of the moon’s far side ...
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 ...
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. The modern system of lunar nomenclature was introduced in 1651 by Riccioli. [1]
In the same year, the first Complete Map of the Moon (1: 5 000 000 scale [26]) and updated complete globe (1: 10 000 000 scale), featuring 95 percent of the lunar surface, [26] were released in the Soviet Union. [31] [32] As many prominent landscape features of the far side were discovered by Soviet space probes, Soviet scientists selected ...
This week, explore the mysterious far side of the moon, see the reconstructed face of a Neanderthal woman, decipher the story of Plato’s final night, and more. New mission could shed light on ...
The pit is located at 8.3355°N, 33.222°E on the moon's surface. Radar imaging indicated that the pit's funnel is roughly 20 meters deep, while the inner pit has a depth of approximately 105 meters. The diameter of the pit's funnel was between 140 and 146 meters long while the diameter of the inner pit is 88–100 meters long.
The 842 pounds (382 kilograms) of lunar rocks and soil returned to Earth by the Apollo missions in the late 1960s and early 1970s disproved ideas that the moon was a celestial body caught in Earth ...
The near side of the Moon is the lunar hemisphere that always faces towards Earth, opposite to the far side. Only one side of the Moon is visible from Earth because the Moon rotates on its axis at the same rate that the Moon orbits the Earth—a situation known as tidal locking .