There are no large-scale sedimentation and erosion processes on Venus, therefore the observed deformation must be formed on the surface or close to it, and in the ellipsoids of stresses one of the main axes must be perpendicular to the surface. According to the deformation visible on photography from Venera-15, 16, the orientations of the ellipsoids of stresses are established in the different sections of the Montes Maxwell and the northern parquet. A geological model is established, according to which the Montes Maxwell is an arched vault and the region to the south a conjugate bend, separated by a shift zone
analyzed to provide a basis for understanding the nature of geologic processes operating there. The ...
High-resolution radar images from the Magellan spacecraft have revealed the first details of the mor...
Gravitational spreading is expected to lead to rapid relaxation of high relief due to the high surfa...
Large-scale mapping of tectonic structures on Venus shows that there is an organized global distribu...
Preliminary tectonic mapping of Venus from Venera 15/16 images shows unquestionable evidence of at l...
While the Pioneer Venus altimeter, Earth-based radar observatories, and the Venera 15-16 orbital ima...
Tesserae are regions of elevated terrain characterized by two or more sets of ridges and grooves tha...
High-resolution radar images from the Magellan spacecraft have revealed the first details of the mor...
The relationship between the dominant global heat loss mechanism and planetary size has motivated th...
High resolution radar images from the Magellan spacecraft have revealed the first details of the mor...
In previous studies, extensional models were used that incorporated realistic rheologies in order to...
Initial examination of the Magellan coverage of Venus has revealed between 150 and 300 large, radial...
The objectives of this research project were to (1) compile a comprehensive database of the occurren...
Venus has been thought to possess a globally continuous lithosphere, in contrast to the mosaic of mo...
Compared with volcanism and tectonism, impact cratering on Venus has played an overall minor role in...
analyzed to provide a basis for understanding the nature of geologic processes operating there. The ...
High-resolution radar images from the Magellan spacecraft have revealed the first details of the mor...
Gravitational spreading is expected to lead to rapid relaxation of high relief due to the high surfa...
Large-scale mapping of tectonic structures on Venus shows that there is an organized global distribu...
Preliminary tectonic mapping of Venus from Venera 15/16 images shows unquestionable evidence of at l...
While the Pioneer Venus altimeter, Earth-based radar observatories, and the Venera 15-16 orbital ima...
Tesserae are regions of elevated terrain characterized by two or more sets of ridges and grooves tha...
High-resolution radar images from the Magellan spacecraft have revealed the first details of the mor...
The relationship between the dominant global heat loss mechanism and planetary size has motivated th...
High resolution radar images from the Magellan spacecraft have revealed the first details of the mor...
In previous studies, extensional models were used that incorporated realistic rheologies in order to...
Initial examination of the Magellan coverage of Venus has revealed between 150 and 300 large, radial...
The objectives of this research project were to (1) compile a comprehensive database of the occurren...
Venus has been thought to possess a globally continuous lithosphere, in contrast to the mosaic of mo...
Compared with volcanism and tectonism, impact cratering on Venus has played an overall minor role in...
analyzed to provide a basis for understanding the nature of geologic processes operating there. The ...
High-resolution radar images from the Magellan spacecraft have revealed the first details of the mor...
Gravitational spreading is expected to lead to rapid relaxation of high relief due to the high surfa...