Earth's rocky orbit neighbour could have once been part of the Moon

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International
Image by UKT2 from Pixabay
Image by UKT2 from Pixabay

A large chunk of rock orbiting the Sun very close to Earth, known as Kamo'oalewa, might have been formed by an ancient impact on the moon. International researchers have analysed the light reflected from Kamo'oalewa and found that it seems to be made from the same material as the minerals on the Moon's surface. Kamo'oalewa is the most stable of five known 'quasi-satellites' of Earth, with a very Earth-like one-year orbit around the sun, and the researchers found that the orbital path is indicative of an object which originated from the Moon. 

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From: Springer Nature

Planetary science: Earth’s quasi-satellite Kamo’oalewa could be made of Moon material

One of Earth’s quasi-satellites, known as Kamo’oalewa, could be comprised of lunar-like material and may have been formed by an ancient impact on the Moon, according to an article published in Communications Earth & Environment.

Quasi-satellites are small objects that remain close to the Earth whilst they orbit the sun. Despite being close to Earth, they are difficult to observe and so little is known about their origin or composition.

Benjamin Sharkey and colleagues examined the light reflected from Kamo’oalewa using the Large Binocular Telescope and the Lowell Discovery Telescope. The authors found that it had a red reflectance spectrum, very similar to that of minerals on the Moon’s surface. This finding, coupled with an assessment of Kamo’oalewa’s orbital path, suggests that it most likely originated as a part of the Earth-Moon system, perhaps as debris from an impact event or from the gravitational break-up of a larger body during a close encounter with the Earth and Moon. The findings offer rare insights into the formation of Earth’s quasi-satellite population.

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conference:
Nature Communications
Research:Paper
Organisation/s: University of Arizona, USA
Funder: B.N.L. Sharkey and V. Reddy’s work presented in this paper is supported by NASA Near-Earth Object Observations Program Grant NNX17AJ19G (PI: Reddy). This paper uses data taken with the MODS spectrographs built with funding from NSF grant AST-9987045 and the NSF Telescope System Instrumentation Program (TSIP), with additional funds from the Ohio Board of Regents and the Ohio State University Office of Research.
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