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UH-led Team Uses Dawn Mission To Identify Icy Craters on Ceres

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Dr. Norbert Schorghofer
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Dr. Roy Gal
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Might the dwarf planet Ceres have permanent ice deposits? Using NASA's Dawn mission, a team led by Norbert Schorghofer, an astronomer at the University of Hawaii Institute for Astronomy, has identified permanently shadowed regions on the dwarf planet Ceres. Most of these areas likely have been cold enough to trap water ice for a billion years, suggesting that ice deposits could exist there now.

"The conditions on Ceres are right for accumulating deposits of water ice," said Schorghofer. "Ceres has just enough mass to hold on to water molecules, and the permanently shadowed regions we identified are extremely cold - colder than most that exist on the moon or Mercury."

Permanently shadowed regions do not receive direct sunlight but get indirect radiation. These regions are typically located on a crater floor or along a section of the crater wall facing the pole. If the temperature stays below minus 243 degrees Fahrenheit (minus 153 degrees Celsius), the area is a cold trap - a good place for water ice to accumulate and remain stable. Cold traps were predicted for Ceres, but this is the first time they have been identified.


Ceres' frozen craters
Shadowed Craters on Ceres

At the poles of Ceres, scientists have found craters that are permanently in shadow (indicated by blue markings). Such craters are called "cold traps" if they remain below about minus 240 degrees Fahrenheit (minus 151 degrees Celsius). These shadowed craters may have been collecting ice for billions of years because they are so cold. This image was created using data from NASA's Dawn spacecraft.

In this study, Schorghofer and colleagues studied Ceres' northern hemisphere. Images from Dawn's cameras were combined to map the dwarf planet's shape, showing craters, plains and other features in three dimensions. Using this input, a sophisticated computer model developed at NASA's Goddard Space Flight Center, Greenbelt, Maryland, was used to determine which areas receive direct sunlight, how much solar radiation reaches the surface, and how the conditions change over the course of a year on Ceres.

The researchers found dozens of sizeable, permanently shadowed regions across the northern hemisphere. The largest one is inside a 10-mile-wide (16-kilometer) crater located less than 40 miles (65 kilometers) from Ceres' north pole. Taken together, all of these regions on Ceres cover about 695 square miles (1,800 square kilometers) - much less than 1 percent of the surface area of the northern hemisphere.

The team expects the permanently shadowed regions on Ceres to be colder than those on Mercury or the moon. That's because Ceres is quite far from the sun, and the shadowed parts of its craters receive little indirect radiation.

"On Ceres, these regions act as cold traps down to relatively low latitudes," said Erwan Mazarico, a Dawn guest investigator at Goddard. "On the moon and Mercury, only the permanently shadowed regions very close to the poles get cold enough for ice to be stable on the surface."

The situation on Ceres is quite similar to that on Mercury, where permanently shadowed regions account for roughly the same fraction of the northern hemisphere. The trapping efficiency - the ability to accumulate water ice - is also comparable.

By the team's calculations, about 1 out of every 1000 water molecules generated on the surface of Ceres will end up in a cold trap during a year on Ceres (1,680 days). That's enough to build up thin but detectable ice deposits over 100,000 years or so.

"While cold traps may provide surface deposits of water ice as have been seen at the moon and Mercury, Ceres may have been formed with a relatively greater reservoir of water," said Chris Russell, principal investigator of the Dawn mission, based at the University of California, Los Angeles. "Some observations indicate Ceres may be a volatile-rich world that is not dependent on current-day external sources."

The findings are available online in a Geophysical Research Letters paper published today.


Dawn's mission is managed by JPL for NASA's Science Mission Directorate in Washington. Dawn is a project of the directorate's Discovery Program, managed by NASA's Marshall Space Flight Center in Huntsville, Alabama. UCLA is responsible for overall Dawn mission science. Orbital ATK Inc., in Dulles, Virginia, designed and built the spacecraft. The German Aerospace Center, Max Planck Institute for Solar System Research, Italian Space Agency and Italian National Astrophysical Institute are international partners on the mission team. For a complete list of mission participants, visit:
http://dawn.jpl.nasa.gov/mission
More information about Dawn is available at the following sites:
http://dawn.jpl.nasa.gov
http://www.nasa.gov/dawn

Founded in 1967, the Institute for Astronomy at the University of Hawaii at Manoa conducts research into galaxies, cosmology, stars, planets, and the sun. Its faculty and staff are also involved in astronomy education, deep space missions, and in the development and management of the observatories on Haleakala and Maunakea. The Institute operates facilities on the islands of Oahu, Maui, and Hawaii.