The surface of the dwarf planet Ceres is considered to be dominated by geological processes typical of small bodies or medium-sized icy bodies, such as impact cratering; there are also features of putative cryovolcanic origin as well as those related to flow of near-surface ice. Extensional features include regional linear troughs, fractures and pit chains, fractures associated with impact craters and with crater floors, and polygonal craters whose walls seem to be structurally controlled. However, no contractional features, which are related to thrust fault activity more typical of large silicate bodies, have been described. Here we report the presence of scarps, ridges and fractures associated with thrust faults, tectonically raised terra...
Craters on Ceres, such as Haulani, Kupalo, Ikapati, and Occator show postimpact modification by the ...
I analyze landslides on Ceres using several quantitative approaches to constrain the composition and...
Ceres, the largest body in the asteroid belt (940 km diameter), provides a unique opportunity to stu...
The surface of the dwarf planet Ceres is considered to be dominated by geological processes typical ...
Some craters on Ceres show post-impact modifications, like the deposition of extended plains laced w...
The Dawn Science Team is conducting a geological mapping campaign at Ceres during the nominal missio...
We present a comprehensive global catalog of the geomorphological features with clear orpotential re...
Analysis of Dawn spacecraft Framing Camera image data allows evaluation of the topography and geomor...
We present a comprehensive global catalog of the geomorphological features with clear or potential r...
Dawn is the first spacecraft to visit and orbit Ceres, the largest object in the asteroid belt and t...
### INTRODUCTION Observations of Ceres, the largest object in the asteroid belt, have suggested that...
Analysis of Dawn spacecraft Framing Camera image data allows evaluation of the topography and geomor...
Ceres´ surface is affected by numerous impact craters and some of them show features such as channel...
Floor-fractured craters are one of the most distinct features on Ceres. Most of the fractures are lo...
The otherwise homogeneous surface of Ceres is dotted with hundreds of anomalously bright, predominan...
Craters on Ceres, such as Haulani, Kupalo, Ikapati, and Occator show postimpact modification by the ...
I analyze landslides on Ceres using several quantitative approaches to constrain the composition and...
Ceres, the largest body in the asteroid belt (940 km diameter), provides a unique opportunity to stu...
The surface of the dwarf planet Ceres is considered to be dominated by geological processes typical ...
Some craters on Ceres show post-impact modifications, like the deposition of extended plains laced w...
The Dawn Science Team is conducting a geological mapping campaign at Ceres during the nominal missio...
We present a comprehensive global catalog of the geomorphological features with clear orpotential re...
Analysis of Dawn spacecraft Framing Camera image data allows evaluation of the topography and geomor...
We present a comprehensive global catalog of the geomorphological features with clear or potential r...
Dawn is the first spacecraft to visit and orbit Ceres, the largest object in the asteroid belt and t...
### INTRODUCTION Observations of Ceres, the largest object in the asteroid belt, have suggested that...
Analysis of Dawn spacecraft Framing Camera image data allows evaluation of the topography and geomor...
Ceres´ surface is affected by numerous impact craters and some of them show features such as channel...
Floor-fractured craters are one of the most distinct features on Ceres. Most of the fractures are lo...
The otherwise homogeneous surface of Ceres is dotted with hundreds of anomalously bright, predominan...
Craters on Ceres, such as Haulani, Kupalo, Ikapati, and Occator show postimpact modification by the ...
I analyze landslides on Ceres using several quantitative approaches to constrain the composition and...
Ceres, the largest body in the asteroid belt (940 km diameter), provides a unique opportunity to stu...