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“1 Ceres” Asteroid Might Have An ‘Ice Volcano’ And Other Signs Of Water, NASA’s Dawn mission Reveals




The entrance of NASA’s Dawn mission at the enormous asteroid “1 Ceres” in early 2015 has turned out to have been well worth to come for. This dwarf planet is the biggest body in the asteroid belt between Mars and Jupiter and was the first to be found. But, until recently, we have only had evidence from ground and space centered telescopes, which have given us tempting sights of a dark, maybe water-rich object.


Now the NASA’s Dawn space probe has sent back a mammoth harvest of answers, shortened in six new exploration papers printed in a special issue of the journal Science. We now have a map of Ceres that discloses uncommon minerals, a surface sprinkled with craters, and water in the form of ice and perhaps an external atmosphere of vapour. There is also sufficient uncertainty in the answers to sow the seeds for yet to come researches.

The data delivers a global geographical map of the asteroid displaying that its whole surface seems to be covered in phyllosilicates, a significant set of clay minerals. Two particular clays are discovered: one that is totally magnesium-rich, the second an ammonium-rich types. There appears to be little or no pattern to the scattering of the two minerals, they are both nearly everywhere.


This ubiquity is what is essential. The minerals could not have been produced in an ordinary incident, such as an impact into an ice-filled crater. They must have been formed by planet-wide adaptation, probably denoting there must have been volumes of water. It is clear that huge amounts of liquid water are not present on Ceres currently. But the signal of water-ice has been spotted in at least one crater.

The temperature of Ceres is reasonably warm (between -93to -33), water-ice visible at the surface would quickly convert into a gas in such a low pressure surroundings. So the discovered traces of water-ice propose some underground ice was just out and that there must be some mechanism to describe how the surface was bothered in this way. Some scientists think that the solution is cry volcanism, where subsurface coatings of mixed ice and minerals percolate gradually to the surface through fractures and cracks, or more quickly following an effect. If the minerals are chlorides, then  low temperature brine can keep the subsurface coating move-able.

As well as a geographical map of Ceres, we also have an image of Ceres’overall geomorphology (its surface types). This demonstrates that the surface of Ceres is interspersed with impact craters, though the craters are not scattered equally over the surface. Much more fascinating are the three different types of mineral drift across the landscape, formed by the movement of ice-rich material, mudslides or layers of ejected particles following impact into the ice-rich material. The scattering of the flow types differs with latitude, and the scientists consider this means different surface coatings of the asteroid contain different quantities of ice.

One of the most extraordinary results is the discovery of an unexpected burst of extremely energetic electrons over a period of nearly a week in June 2015, corresponding with a solar proton storm. The scientists consider the protons fired out by the sun intermingled with particles in Ceres' feeble atmosphere, generating a shock wave that speeded the electrons. Based on explanations by the Hubble Space Telescope, Ceres is assumed to have a feeble exo-sphere (external atmosphere) of water vapour. The results from Dawn propose that this may actually be the case.

Monica Grady, Professor of Planetary and Space Sciences, The Open UniversityThis article was initially published on The Conversation.

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