NASA's Curiosity finds how water helps shape Mars mountain
US space agency NASA said Monday that Mars' Mount Sharp, where its Curiosity rover is exploring, was built by sediments deposited in a large lake bed over tens of millions of years.
The formation of Mount Sharp, a five-kilometer-high layered mountain at the center of Gale Crater, has been a challenging question for researchers.
Curiosity landed inside Gale Crater in 2012 and its primary destination was Mount Sharp, which it arrived at three months ago. Currently, the rover is investigating the lowest sedimentary layers of Mount Sharp, a section of rock 150 meters high dubbed the Murray formation.
Observations by Curiosity showed that the mountain was created by sediments from the crater rim highlands and transported toward the center of the crater in alluvial fans, deltas, and wind-blown drifts, NASA said.
"During wet periods, water pooled in lakes where sediments settled out in the center of crater," it said.
"Even during dry periods in the crater center, groundwater would have existed beneath the surface. Then, during the next wet period it would resurface to form the next lake. This alternation of lakes, rivers and deserts could have represented a long-lasting habitable environment."
Later, after the crater had at least partially filled with sediment, erosion of previously deposited sedimentary layers occurred, exposing the ancient sequence of lake, river and desert environments as a series of bands, or layers, along the lower flanks of Mount Sharp.
"We are making headway in solving the mystery of Mount Sharp," Curiosity Project Scientist John Grotzinger of the California Institute of Technology in Pasadena, California, said in a statement. "Where there's now a mountain, there may have once been a series of lakes."
As Curiosity climbs higher on Mount Sharp, the researchers will have a series of experiments to show patterns in how the atmosphere and the water and the sediments interact, Grotzinger said.
The findings also indicated that ancient Mars maintained a climate that could have produced long-lasting lakes at many locations on the Red Planet.
"If our hypothesis for Mount Sharp holds up, it challenges the notion that warm and wet conditions were transient, local, or only underground on Mars," said Ashwin Vasavada, Curiosity deputy project scientist at NASA's Jet Propulsion Laboratory.
"A more radical explanation is that Mars' ancient, thicker atmosphere raised temperatures above freezing globally, but so far we don't know how the atmosphere did that."
Despite earlier evidence from several Mars missions that pointed to wet environments on ancient Mars, modeling of the ancient climate has yet to identify the conditions that could have produced long periods warm enough for stable water on the surface.
NASA said the new findings could also help guide plans for future missions to seek signs of Martian life.
“好奇”號(hào)破解火星夏普山成因之謎
美國航天局8日說,“好奇”號(hào)火星車破解了火星夏普山的形成之謎。這座位于一個(gè)巨大隕石坑中心的高山,可能是由一個(gè)大型湖床的沉淀物長期累積與風(fēng)化所形成的。
夏普山海拔約5000米,位于直徑154公里的蓋爾隕石坑的中心位置。為什么隕石坑中心會(huì)形成一座高山,一直是個(gè)令科學(xué)家感興趣的話題。“好奇”號(hào)2012年在蓋爾隕石坑著陸,主要任務(wù)就是探索夏普山,并于今年9月成功抵達(dá)山腳下。
“好奇”號(hào)的觀察表明,30億年前,蓋爾隕石坑可能曾多次變成湖泊又多次蒸發(fā)干涸。在這種循環(huán)中,湖泊沉淀物以及源自隕石坑邊緣高地、被水和風(fēng)帶來的河流沉淀物和風(fēng)化沉淀物層層交替累積。當(dāng)沉淀物沉積到一定高度,又遭風(fēng)侵蝕被“雕刻”成山的形狀。在有水的時(shí)候,這樣的高峰可能作為島嶼在湖泊中出現(xiàn)。
這項(xiàng)研究還表明,古代火星的氣候曾足以支持在許多地點(diǎn)產(chǎn)生湖泊,它們的存在時(shí)間也比以前認(rèn)為的要更長久。“好奇”號(hào)項(xiàng)目科學(xué)家阿斯溫·瓦薩瓦達(dá)在此研究的基礎(chǔ)上猜測說,古代火星的平均氣溫曾高于零攝氏度,而現(xiàn)在的火星年平均氣溫只有零下55攝氏度左右。
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