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'바로가기를 만드시겠습니까?'라고 묻는 창이 나오면, 아이콘의 이름을 확인한 후 '만들기' 버튼을 눌러 주세요.
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NWA 16788 is roofed in the reddish-brown fusion crust providing it an unmistakable Martian hue. Regmaglypts, or surface depressions shaped by frictional heating for the duration of fast descent via Earth’s ambiance, can also be seen on the floor of the meteorite.
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바탕화면 하단 작업표시줄에 유튜브 바로가기 아이콘이 고정된 것을 확인할 수 있습니다. 만약 작업표시줄이 아니라 바탕화면에 놓고 싶으면 마우스로 아이콘을 바탕화면으로 끌어서 원하는 위치에 놓으면 됩니다.
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It is actually all over 70% more substantial in comparison to the preceding most significant acknowledged Martian meteorite, and it is referred to as having a "deep pink hue" and also a "glassy crust," As outlined by Sotheby's.
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NWA 16788 is undoubtedly an olivine-microgabbroic shergottite, fashioned within the slow cooling of Martian magma and characterized by a system-grained texture composed mainly of pyroxene, maskelynite, and olivine. Only 5.4% of Martian meteorites are at the moment labeled as possibly gabbroic or microgabbroic, making this a rare form of rock inside the already particularly unusual category of Martian meteorites.
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Given the severity of influence necessary to eject any product off the Martian area and into Room, researchers believe there are only about 19 craters massive sufficient to become the probable origination points for Martian meteorites.