๐”– Bobbio Scriptorium
โœฆ   LIBER   โœฆ

On the nature and visibility of crater-associated streaks on Mars

โœ Scribed by J. Veverka; P. Thomas; Carl Sagan


Publisher
Elsevier Science
Year
1978
Tongue
English
Weight
312 KB
Volume
36
Category
Article
ISSN
0019-1035

No coin nor oath required. For personal study only.


๐Ÿ“œ SIMILAR VOLUMES


Interpreting the Elliptical Crater Popul
โœ William F. Bottke Jr.; Stanley G. Love; David Tytell; Timothy Glotch ๐Ÿ“‚ Article ๐Ÿ“… 2000 ๐Ÿ› Elsevier Science ๐ŸŒ English โš– 379 KB

Asteroids or comets striking a planetary surface at very shallow angles produce elliptical-shaped craters. According to laboratory impact experiments (D. E. Gault and J. A. Wedekind 1978, Proc. Lunar Planet. Sci. Conf. 9th, 3843-3875), elliptical craters result from impact angles within โˆผ5 โ€ข of hori

"Softened" Impact Craters on Mars: Impli
โœ David G. Jankowski; Steven W. Squyres ๐Ÿ“‚ Article ๐Ÿ“… 1993 ๐Ÿ› Elsevier Science ๐ŸŒ English โš– 788 KB

"Terrain softening" is a distinct style of landform degradation observed on Mars. The morphology and distribution of softened terrain have led to the hypothesis that it is the result of quasiviscous relaxation of topology due to the creep deformation of subsurface ice. In order to test this hypothes

On the satellites of mars
โœ A. Marth ๐Ÿ“‚ Article ๐Ÿ“… 1879 ๐Ÿ› John Wiley and Sons ๐ŸŒ English โš– 455 KB ๐Ÿ‘ 2 views

J denoting the inclination of the plane of the satellite's orbit ta the plane of the equator of the epoch, N the rightascension of the node, uo the longitude of the satellite in its orbit reckoned from the node and n the daily. motion. The eccentricities are here disregarded on account of their unce