A lunar lander named for the Chinese goddess of the moon may have lessened the mystery of the far side of the moon. The fourth probe of Chang'E(CE-4) was the first mission to land on the far side of the moon, and it has collected new evidence from the largest crater in the solar system,clarifying how the moon may have evolved.
The results were published on May 16, 2019, in Nature.
A theory emerged in the 1970s that in the moon’s infancy, an ocean made of magma covered its surface. As the molten ocean began to calm and cool, lighter minerals floated to the top, while heavier components sank. The top crusted over in a sheet of mare basalt, encasing a mantle of dense minerals, such as olivine and pyroxene.
As asteroids and space junk crashed into the surface of the moon, they cracked through the crust and kicked up pieces of the lunar mantel.
“Understanding the composition of the lunar mantel is critical for testing whether a magma ocean ever existed, as postulated,” said corresponding author Chunlai Li, a professor of the National Astronomical Observatories of Chinese Academy of Sciences (NAOC). “It also helps advance our understanding of the thermal and magmatic evolution of the moon.”
The evolution of the moon may provide a window into the evolution of Earth and other terrestrial planets, according to Li, because its surface is relatively untouched compared to, say, the early planetary surface of Earth.
Li and his team landed CE-4 in the moon’s South Pole-Aitken (SPA) basin, which stretches about 2,500 kilometres—about half the width of China. CE-4 collected spectral data samples from the flat stretches of the basin, as well as from other, smaller but deeper impact craters within the basin.
Fig.1: Image captured by Chang’E 4 showed the landscape near the landing site. (Image credit: NAOC/CNSA)
The researchers expected to find a wealth of excavated mantle material on the flat floor of the SPA basin, since the originating impact would have penetrated well into and past the lunar crust. Instead, they found mere traces of olivine, the primary component of the Earth’s upper mantle.
“The absence of abundant olivine in the SPA interior remains a conundrum,” Li said. “Could the predictions of an olivine-rich lunar mantle be incorrect?”
Not quite. As it turns out, more olivine appeared in the samples from deeper impacts. One theory, according to Li, is that the mantle consists of equal parts olivine and pyroxene, rather than being dominated by one over the other.
Fig.2: Image captured by Chang'E 4 showed the landscape near the landing site. (Image credit: NAOC/CNSA)
CE-4 will need to explore more to better understand the geology of its landing site, as well as collect much more spectral data to validate its initial findings and to fully understand the composition of the lunar mantle.
This work was supported by the Chang’E-4 mission of the Chinese Lunar Exploration Program. Other contributors from the Key Laboratory of Lunar and Deep Space Exploration in the National Astronomical Observatories of the Chinese Academy of Sciences include Dawei Liu, Bin Liu, Xin Ren, Jianjun Liu, Wei Zuo, Xingguo Zeng, Xu Tan, Xiaoxia Zhang, Wangli Chen, Weibin Wen, Yan Su, Hongbo Zhang, and Ziyuan Ouyang, who is also affiliated with the Institute of Geochemistry. Zhiping He, Rui Xu, and Rong Shu of the Shanghai Institute of Technical Physics also contributed.
About The National Astronomical Observatories of Chinese Academy of Sciences (NAOC):
The National Astronomical Observatories of Chinese Academy of Sciences (NAOC) was officially founded in April 2001 through the merger of observatories, stations and research center under Chinese Academy of Sciences. It is headquartered in Beijing and has four subordinate units across the country: the Yunnan Observatory (YNAO), the Nanjing Institute of Astronomical Optics and Technology (NIAOT), the Xinjiang Astronomical Observatory (XAO) and the Changchun Observatory. NAOC conducts cutting-edge astronomical studies, and operates major national facilities including The Large Sky Area Multi-Object Fiber Spectroscopy Telescope (LAMOST), the Five-hundred-meter Aperture Spherical Telescope (FAST) etc.
NAOC’s main research involves cosmological large-scale structures, the formation and evolution of galaxies and stars, high-energy astrophysics, solar magnetism and activity, lunar and deep space exploration, and astronomical instrumentation. NAOC has seven major research divisions in the areas of optical astronomy, radio astronomy, galaxies and cosmology, space science, solar physics, lunar and deep space exploration, and applications in astronomy.
The paper can be accessed at https://doi.org/10.1038/s41586-019-1189-0
01 20, 2017
01 20, 2017
Address: 20A Datun Road, Chaoyang District, Beijing, China code: 100012
Tel: 010-64888708 E-mail: firstname.lastname@example.org