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Additional info for Acceleration of the Center of Mass of an Extended Body in a Weak Gravitational Field
The most obvious deformational features are those associated with the Tharsis bulge. Around the bulge is a vast system of radial grabens that affects about a third of the planet’s surface. Circumferential wrinkle ridges are also present in places, particularly on the east side of the bulge in Lunae Planum. Both the fractures and the compressional ridges are believed to be the result of stresses in the lithosphere caused by the presence of the Tharsis bulge. No comparably extensive system of deformational features occurs around Elysium, but Overview fractures occur in other places where the crust has been differentially loaded, as around large impact basins, such as Hellas and Isidis, or around large volcanoes, such as Elysium Mons and Pavonis Mons.
A bouldery, smooth to hummocky rim transitions outward, at about one crater radius from the rim, to terrain with a strong radial fabric (MOC R1502146). higher rates of erosion and burial on Mars. Detailed characteristics of a prominent 10 km diameter ray crater are described by McEwen et al. (2005). 1 km in diameter, is a familiar example of a simple terrestrial impact crater. It is thought to have formed 50,000 years ago by the impact of a 30 m diameter object moving at 20 km sÀ1 (Melosh, 1989).
Being on highly elliptical orbits, longperiod comets move rapidly through the inner Solar System and typically have impact velocities at Mars of a few tens of kilometers per second (Hartmann, 1977). Short-period comets are divided into two groups. Halley-type comets have orbital periods of 20À200 years and random inclinations like the Impact craters long-term comets. Jupiter-family comets have periods less than 20 years and orbit inclinations that are close to the plane of the ecliptic. Impact velocities at Mars for short-period comets are around 10 km sÀ1.
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