The geologic context of red organic-rich materials (ROR) found across an elongated 200 km region on Ceres is evaluated with spectral information from the multispectral framing camera (FC) and the visible and near-infrared mapping spectrometer (VIR) of Dawn. Discrete areas of ROR materials are found to be associated with small fresh craters less than a few hundred meters in diameter. Regions with the highest concentration of discrete ROR areas exhibit a weaker diffuse background of ROR materials. The observed pattern could be consistent with a field of secondary impacts, but no appropriate primary crater has been found. Both endogenic and exogenic sources are being considered for these distinctive organic materials
The otherwise homogeneous surface of Ceres is dotted with hundreds of anomalously bright, predominan...
Linear features are very common on asteroid surfaces. They are generally formed after impact and pro...
We present a global spectrophotometric characterization of the Ceres surface using Dawn Framing Came...
International audienceCeres is the largest object in the main belt and is a wet body with a complex ...
The NASA/Dawn mission has acquired unprecedented measurements of the surface of the dwarf planet Cer...
International audienceThe NASA/Dawn mission has acquired unprecedented measurements of the surface o...
International audienceOrganic matter directly observed at the surface of an inner planetary body is ...
In March 2015, the NASA Dawn spacecraft entered orbit around Ceres, the largest object in the main a...
Variations and spatial distributions of bright and dark material on dwarf planet Ceres play a key ro...
After more than one year orbit around Ceres, Dawn spacecraft covered large part of its surface, allo...
Ceres’ surface has commonly been linked with carbonaceous chondrites (CCs) by ground‐based telescopi...
Impact craters of different geological ages, sizes and morphologies are not only the most obvious su...
Ceres’ surface has commonly been linked with carbonaceous chondrites (CCs) by ground‐based telescopi...
International audienceThe dwarf planet Ceres is an airless body composed of Mg-phyllosilicates, NH4-...
The dwarf planet Ceres (equatorial diameter 963km) is the largest object that has remained in the ma...
The otherwise homogeneous surface of Ceres is dotted with hundreds of anomalously bright, predominan...
Linear features are very common on asteroid surfaces. They are generally formed after impact and pro...
We present a global spectrophotometric characterization of the Ceres surface using Dawn Framing Came...
International audienceCeres is the largest object in the main belt and is a wet body with a complex ...
The NASA/Dawn mission has acquired unprecedented measurements of the surface of the dwarf planet Cer...
International audienceThe NASA/Dawn mission has acquired unprecedented measurements of the surface o...
International audienceOrganic matter directly observed at the surface of an inner planetary body is ...
In March 2015, the NASA Dawn spacecraft entered orbit around Ceres, the largest object in the main a...
Variations and spatial distributions of bright and dark material on dwarf planet Ceres play a key ro...
After more than one year orbit around Ceres, Dawn spacecraft covered large part of its surface, allo...
Ceres’ surface has commonly been linked with carbonaceous chondrites (CCs) by ground‐based telescopi...
Impact craters of different geological ages, sizes and morphologies are not only the most obvious su...
Ceres’ surface has commonly been linked with carbonaceous chondrites (CCs) by ground‐based telescopi...
International audienceThe dwarf planet Ceres is an airless body composed of Mg-phyllosilicates, NH4-...
The dwarf planet Ceres (equatorial diameter 963km) is the largest object that has remained in the ma...
The otherwise homogeneous surface of Ceres is dotted with hundreds of anomalously bright, predominan...
Linear features are very common on asteroid surfaces. They are generally formed after impact and pro...
We present a global spectrophotometric characterization of the Ceres surface using Dawn Framing Came...