[1] Venus impact craters larger than 5 km in diameter (90 % of all craters) have been classified based on the presence and prominence of associated radar-dark deposits. Approximate estimates of the absolute age of craters of different morphologic classes are made. Analysis of age relations of dated craters and volcanic and tectonic structures permits the estimation of the age and duration of different volcanic and tectonic events. INDEX TERMS
Abstract. On the basis of regional and global stratigraphic analyses, we outline the major events in...
The images of the asteroid 951 Gaspra obtained by Galileo show impact craters down th the resolution...
Counting impact craters on surfaces of terrestrial bodies is currently the only way to estimate the ...
[1] We use the degree of degradation of crater-associated radar-dark deposits on Venus to estimate t...
A central question for any planet is the age of its surface. Based on comparative planetological arg...
The average surface age of a planet is a major indicator of the level of its geologic activity and t...
The determination of the timing of impact events and the ages of cratered planetary surfaces is a co...
The consensus regarding interpretation of Magellan radar imagery assigns Venus a young volcanic surf...
Compared with volcanism and tectonism, impact cratering on Venus has played an overall minor role in...
Use of impact crater ejects at time-stratigraphic markers was established during lunar geologic mapp...
A first-order impact crater aging model is presented based on observations of the global crater popu...
Ein polygonaler Einschlagskrater ist ein Krater, der inder Draufsicht mehr oder weniger eckig ersche...
[1] We investigated the possibility of significant variations in the rates and styles of volcanism a...
The relationship between sudden catastrophic events and sudden mass extinctions on Earth has attract...
Mariner 9 images of the four great volcanic shields of the Tharsis region of Mars show many circular...
Abstract. On the basis of regional and global stratigraphic analyses, we outline the major events in...
The images of the asteroid 951 Gaspra obtained by Galileo show impact craters down th the resolution...
Counting impact craters on surfaces of terrestrial bodies is currently the only way to estimate the ...
[1] We use the degree of degradation of crater-associated radar-dark deposits on Venus to estimate t...
A central question for any planet is the age of its surface. Based on comparative planetological arg...
The average surface age of a planet is a major indicator of the level of its geologic activity and t...
The determination of the timing of impact events and the ages of cratered planetary surfaces is a co...
The consensus regarding interpretation of Magellan radar imagery assigns Venus a young volcanic surf...
Compared with volcanism and tectonism, impact cratering on Venus has played an overall minor role in...
Use of impact crater ejects at time-stratigraphic markers was established during lunar geologic mapp...
A first-order impact crater aging model is presented based on observations of the global crater popu...
Ein polygonaler Einschlagskrater ist ein Krater, der inder Draufsicht mehr oder weniger eckig ersche...
[1] We investigated the possibility of significant variations in the rates and styles of volcanism a...
The relationship between sudden catastrophic events and sudden mass extinctions on Earth has attract...
Mariner 9 images of the four great volcanic shields of the Tharsis region of Mars show many circular...
Abstract. On the basis of regional and global stratigraphic analyses, we outline the major events in...
The images of the asteroid 951 Gaspra obtained by Galileo show impact craters down th the resolution...
Counting impact craters on surfaces of terrestrial bodies is currently the only way to estimate the ...