WebAug 13, 2015 · Being a large object in the solar system means getting brutalized over the years, pummeled by millions of impacts. Some objects wear it well; Earth, for … WebConditions of crater saturation and equilibrium have been simulated with a Monte Carlo computer program which utilizes a generating function of the form N = b·D −a.The …
Planetary cratering 2: Studies of saturation equilibrium
Web3333 S. Crater Road, Suite 5 Petersburg, VA 23805 Phone: (804) 861-1606 Fax: (804) 862-1254 Phenix City, AL. Address: 1023 13th St. Phenix City, AL 36867 Phone: (706) 257 … WebJul 3, 2013 · In general, we find that the spatial density of craters from the lunar and Mercurian terrains in Fig. 2b approaches empirical saturation equilibrium, which is thought to occur at R = 0.2–0.3 ... need to cancel order
Cratering saturation and equilibrium: A new model looks at
WebCelsius is a small lunar impact crater that is located in the rugged terrain in the southern hemisphere on the Moon's near side. It is named after Swedish astronomer, physicist … WebAug 9, 2024 · This finding suggests that a more realistic cratering record could be attained through detailed porosity analysis, even in areas with crater saturation where it is impossible to determine the true number of craters formed. The lunar impact record constrains rates of impact events throughout the inner solar system. WebDec 1, 2009 · Although of limited dynamic (crater-size) range, this model demonstrated that crater density equilibrium conditions generally occur at an overall density level of 1–10% of what Gault termed ‘geometric saturation:’ the crater density achieved when craters of … Although of limited dynamic (crater-size) range, this model demonstrated that … Cratering saturation and equilibrium: A new model looks at an old problem. James … need to center screen