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Dwarf Planet Ceres Up To 30 Percent Water
After 4 billion years, the dwarf planet Ceres is still carrying a surprising amount of water weight — as much as 30 percent.
The finding, which was published in the Jan. 6 edition of the journal Science, is consistent with earlier models, and provides valuable clues to how Ceres formed.
NASA’s Dawn spacecraft found the water using an instrument — the Gamma Ray and Neutron Detector (GRaND) — that matches chemical elements to patterns of gamma rays and neutrons, which Ceres emits as cosmic rays strike its surface.
“The gammas and neutrons give you a fingerprint of the elemental composition of the surface to a depth of about a meter,” said Tom Prettyman, GRaND team leader and a senior scientist at the Tucson-based Planetary Science Institute.
The key word is elements. Prettyman explained that GRaND cannot detect molecules per se, so researcher have to infer the presence of water based on what they know about how the compound affects the makeup of similar objects, such as the groups of meteorites known as carbonaceous chondrites.
“So, when I’m talking about water, as seen by GRaND, we’re making kind of a leap — we’re making an assumption that the hydrogen is in — mostly in — the form of water."
The accumulated research on Ceres indicates that water has played a significant role in the dwarf plant’s history, from the formation of a 13,000-foot volcano formed from the action of salty, muddy ice, to existing ice deposits that sit in the “cold traps” of shadowy craters. At least one study has shown that ice might “hop” around Ceres — or escape it, as heating processes sublimate surface ice into water vapor.
Prettyman said that ice distribution on Ceres is uneven due to that way exposure to the sun’s heat varies by latitude.
“If you went there and you got a shovel and dug a little hole at the north pole, you would probably immediately find water ice whereas, at the equator, you’d have to dig a little bit deeper — almost a meter beneath the surface,” said Prettyman.
The GRaND team found that, beyond the H2O in this ice table, a surprising amount of Ceres’s water remains locked up in non-icy minerals. Prettyman explained that water altered material in the dwarf Ceres’s interior as the dwarf planet developed, and became in mineral lattices in the process.
“And so, if you add up all the sources of water that we see on Ceres, as inferred from GRaND observations, we get almost, but not quite, 30 percent. That’s very similar to what we expected going in, but still is a surprise to see it in the different forms that we found it," Prettyman said.
Dawn is the only spacecraft ever to orbit two destinations beyond Earth. After training its instruments on the giant asteroid Vesta from July 2011 to September 2012, it traveled to Ceres, where it has orbited since 2015.
(Photo courtesy of NASA/JPL-Caltech/UCLA/MPS/DLR/IDA/PSI)
NASA's Dawn spacecraft determined the hydrogen content of the upper yard, or meter, of Ceres' surface. Blue indicates where hydrogen content is higher, near the poles, while red indicates lower content at lower latitudes.