entered orbit around the Main Belt asteroid 4 Vesta. Dawn has been designed to map the asteroid Vesta and later in the mission the dwarf planet 1 Ceres from var-ious altitudes utilizing three different instruments [1]
Dawn's main objective is to characterize two of the largest bodies in the main asteroid belt: aste...
The DAWN mission to asteroids (4) Vesta and (1) Ceres was the ninth mission in NASA’s low cost Disco...
The objective of the Dawn topography investigation is to derive the detailed shapes of 4 Vesta and 1...
In July 2011 the Dawn spacecraft entered orbit around the Main Belt asteroid 4 Vesta. Dawn has been ...
Dawn space mission will provide the first, detailed data of two of the major bodies in the Main Belt...
In July 2011 the Dawn spacecraft entered orbit around the Main Belt asteroid 4 Vesta utilizing three...
The NASA Dawn mission has extensively examined the surface of asteroid Vesta, the second most massiv...
The Dawn spacecraft now in orbit has revealed the asteroid 4 Vesta to be a heavily cratered object, ...
We derived model functions for the crater production size-frequency distribution and chronology of t...
The geologic objectives of the Dawn Mission are to derive Vesta's shape, map the surface geology, un...
Context. The forthcoming arrival of the NASA’s Dawn spacecraft to Ceres and Vesta means that these u...
In this paper, we present a global database of craters larger than 0.7 km in diameter on the surface...
The Dawn mission mapped the surface of the asteroid 4 Vesta over a period of nearly ten months from ...
Vesta is a large differentiated rocky body in the main asteroid belt that accreted within the first ...
Dawn maps the surface of Vesta and Ceres and probes their internal density distributions, during one...
Dawn's main objective is to characterize two of the largest bodies in the main asteroid belt: aste...
The DAWN mission to asteroids (4) Vesta and (1) Ceres was the ninth mission in NASA’s low cost Disco...
The objective of the Dawn topography investigation is to derive the detailed shapes of 4 Vesta and 1...
In July 2011 the Dawn spacecraft entered orbit around the Main Belt asteroid 4 Vesta. Dawn has been ...
Dawn space mission will provide the first, detailed data of two of the major bodies in the Main Belt...
In July 2011 the Dawn spacecraft entered orbit around the Main Belt asteroid 4 Vesta utilizing three...
The NASA Dawn mission has extensively examined the surface of asteroid Vesta, the second most massiv...
The Dawn spacecraft now in orbit has revealed the asteroid 4 Vesta to be a heavily cratered object, ...
We derived model functions for the crater production size-frequency distribution and chronology of t...
The geologic objectives of the Dawn Mission are to derive Vesta's shape, map the surface geology, un...
Context. The forthcoming arrival of the NASA’s Dawn spacecraft to Ceres and Vesta means that these u...
In this paper, we present a global database of craters larger than 0.7 km in diameter on the surface...
The Dawn mission mapped the surface of the asteroid 4 Vesta over a period of nearly ten months from ...
Vesta is a large differentiated rocky body in the main asteroid belt that accreted within the first ...
Dawn maps the surface of Vesta and Ceres and probes their internal density distributions, during one...
Dawn's main objective is to characterize two of the largest bodies in the main asteroid belt: aste...
The DAWN mission to asteroids (4) Vesta and (1) Ceres was the ninth mission in NASA’s low cost Disco...
The objective of the Dawn topography investigation is to derive the detailed shapes of 4 Vesta and 1...
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