A group of scientists from NASA's Dawn mission suggests that when sunlight reaches Ceres' Occator Crater, a kind of thin haze of dust and evaporating water forms there. This haze only becomes dense enough to be seen by looking at it laterally, as in this image, the scientists wrote in the journal Nature in December 2015.
Occator measures about 60 miles (90 kilometers) wide, and contains the brightest material seen on Ceres.
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, the Max Planck Institute for Solar System Research, the Italian Space Agency and the Italian National Astrophysical Institute are international partners on the mission team. For a complete list of acknowledgments, see http://dawn.jpl.nasa.gov/mission .
For more information about the Dawn mission, visit http://dawn.jpl.nasa.gov .
Name | Value | Additional Values |
---|---|---|
Target | 1 Ceres | |
System | Main Belt | |
Target Type | Dwarf Planet | Asteroid |
Mission | Dawn | |
Instrument Host | Dawn | |
Host Type | Orbiter | |
Instrument | Framing Camera (FC) | |
Detector | ||
Extra Keywords | Atmosphere, Crater, Dust, Grayscale, Haze, Water | |
Acquisition Date | ||
Release Date | 2015-12-09 | |
Date in Caption | ||
Image Credit | NASA/JPL-Caltech/UCLA/MPS/DLR/IDA | |
Source | photojournal.jpl.nasa.gov/catalog/PIA20181 | |
Identifier | PIA20181 |