Mashable 2024年10月02日
This nearby dwarf planet's ice may be left over from a dirty ocean
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谷神星,这颗位于小行星带的矮行星,可能比冥王星更容易被地球人访问。尽管它只有不到600英里宽,但谷神星似乎富含水冰,来自普渡大学和美国宇航局喷气推进实验室的新研究证实,它曾经被流动的水覆盖。多年来,谷神星的陨石坑表面让专家们感到困惑。这些陨石坑似乎太深太硬,不可能存在于一个退役的水世界。科学家现在认为,如果考虑到一个关键因素:泥土——也许还有很多泥土,这可能并不矛盾。

🧑‍🚀谷神星曾经是一个类似于木卫二(木星的卫星)的“海洋世界”,但它的海洋是泥泞的。随着时间的推移,这个泥泞的海洋逐渐冻结,形成了一个冰冷的地壳,其中夹杂着少量的岩石物质。

🧊科学家们通过计算机模型发现,混合在谷神星古老海洋中的泥土可能加强了这颗矮行星的冰,保持了陨石坑的形状,并保存了它的一些地质特征,使其能够在很长一段时间内保持稳定。

🧂美国宇航局的黎明号宇宙飞船在2015年至2018年期间对谷神星表面进行了更近距离的观察,发现其表面有明亮的斑块,这些斑块是由碳酸钠的盐壳组成,与人们用作软化水的盐类型相同。

🌊科学家们认为,这些盐可能是地下约25英里、数百英里宽的巨大咸水库的残留物。陨石撞击要么融化了地表以下的泥浆,要么在矮行星上形成了巨大的裂缝,使盐水从冰火山中渗出。

🔭由于谷神星是距离地球最近的冰冻海洋世界,平均距离为2.6亿英里,天体生物学家一直想知道,简单的微生物生命是否可能存在于谷神星。美国国家科学院的行星科学十年调查最近建议美国宇航局返回谷神星收集样本。

🚀未来对谷神星的更多机器人任务可以提供更多洞察力,并为外太阳系的冰卫星(如土卫二、木卫二和木卫三)提供比较点。谷神星表面的一些明亮特征是谷神星泥泞海洋的残余物,现在大部分或全部都已冻结,并喷发到地表。所以我们有一个地方可以从一个古老海洋世界的海洋中收集样本,而这个海洋并不难到达。

Pluto is the most famous dwarf planet, due in part to its very public demotion from ninth planet of the solar system two decades ago. 

But a relatively obscure dwarf planet in the main asteroid belt could be the most accessible icy world to Earthlings in space. Though it's less than 600 miles wide, Ceres appears to be rich in water ice, and new research from Purdue University and NASA's Jet Propulsion Laboratory is helping to confirm it was once drenched in flowing water. 

For years, Ceres confounded experts with its cratered surface. These pits seemed too deep and rigid to exist on a retired water world. Scientists now think that may not be a contradiction after all, if they account for a key ingredient: mud — and maybe lots of it. 

"Our interpretation of all this is that Ceres used to be an 'ocean world' like Europa (one of Jupiter's moons), but with a dirty, muddy ocean," said Mike Sori, a planetary geophysicist at Purdue, in a statement. "As that muddy ocean froze over time, it created an icy crust with a little bit of rocky material trapped in it."

NASA's Dawn spacecraft observed craters on the dwarf planet Ceres between 2015 and 2018. Credit: NASA / JPL-Caltech / UCLA / MPS / DLR / IDA / ASI / INAF

Using computer models, the team discovered that dirt mixed into Ceres' ancient ocean could have reinforced the dwarf planet's ice, holding the craters' shapes and preserving some of its other geology for long periods of time. This mixture would allow the surface to be both icy and strong. The study appears in the journal Nature Astronomy.

Previous thinking suggested that if the dwarf planet were icy, the craters would deform easily, like glaciers flowing on Earth — or like gooey honey, Sori said. 

The paper, led by doctoral student Ian Pamerleau, posits that Ceres' surface is, in fact, loaded with ice — perhaps as much as 90 percent of it. Through simulations, the team tested different crust scenarios and found that dirty ice could keep the crust from "flowing" over billions of years. With this structure, the dwarf planet would get gradually muddier and less frozen at lower depths. 

A NASA spacecraft got a closer look at Ceres' surface between 2015 and 2018 through the Dawn mission. Those observations revealed the dwarf planet's unusual bright patches as a salty crust of sodium carbonate, the same type of salt people use as a water softener. 

After looking at the mission data, scientists thought perhaps the salt was the residue of a vast, briny reservoir about 25 miles underground and hundreds of miles wide. Meteorite impacts either melted slush just below the surface or created large fractures in the dwarf planet, allowing salt water to ooze out of ice volcanoes.

Bright features on the surface of dwarf planet Ceres are a salty crust of sodium carbonate, the same type of salt people use as a water softener. Credit: NASA / JPL-Caltech / UCLA / MPS / DLR / IDA

Astrobiologists have wondered if simple, microbial life could exist on Ceres, the closest frozen ocean world to Earth at an average of 260 million miles away. The National Academies Planetary Science Decadal Survey recently recommended that NASA return to Ceres to collect samples.

More robotic missions to the dwarf planet could provide greater insights and points of comparison for the icy moons of the outer solar system, such as Saturn's Enceladus and Jupiter's Europa and Ganymede, Sori said. 

"Some of the bright features we see at Ceres' surface are the remnants of Ceres' muddy ocean, now mostly or entirely frozen, erupted onto the surface," he said. "So we have a place to collect samples from the ocean of an ancient ocean world that is not too difficult to send a spacecraft to."

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谷神星 矮行星 冰冻海洋 泥土 水冰
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