Tests of random density models of terrestrial planets

• Published in: Geophysical research letters Vol. 18; no. 5; pp. 909 - 912
• Main Authors: Kaula, William M., Asimow, Paul D.
• Format: Journal Article
• Language: English
• Published: Washington, DC Blackwell Publishing Ltd 01.05.1991; American Geophysical Union
• Subjects: 640107 - Astrophysics & Cosmology- Planetary Phenomena; Astronomy; CLASSICAL AND QUANTUM MECHANICS, GENERAL PHYSICS; DATA ANALYSIS; Density; EARTH PLANET; Earth, ocean, space; Exact sciences and technology; General, solar nebula, and cosmogony; Geophysics; GRAVITATION; Gravitational fields; HARMONICS; Mars; MARS PLANET; MATHEMATICAL MODELS; MOMENT OF INERTIA; MOON; OSCILLATIONS; PLANETS; PROBABILISTIC ESTIMATION; SATELLITES; Solar system; Terrestrial planets; TESTING; Venus; VENUS PLANET; Earth; Stochastic model; Gravitational field; Terrestrial planet; Moon; Venus; Mars planet; Probability density function; Density distribution; Moment of inertia
• ISSN: 0094-8276; 1944-8007
• DOI: 10.1029/91GL01064

Random density models are analyzed to determine the low degree harmonics of the gravity field of a planet, and therefrom two properties: an axiality Pl, the percent of the degree variance in the zonal term referred to an axis through the maximum for degree l; and an angularity Eln, the angle between the maxima for two degrees l, n. The random density distributions give solutions reasonably consistent with the axialities and angularities for the low degrees, l < 5, of Earth, Venus, and Moon, but not for Mars, which has improbably large axialities and small angularities. Hence the random density model is an unreliable predictor for the non‐hydrostatic second‐degree gravity of Mars, and thus for the moment‐of‐inertia, which is more plausibly close to 0.365MR2.