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A critical approach to the concept of a polar, low-altitude LARES satellite

2002/07/25 by Lorenzo Iorio · 4 citations
Earth and Planetary Sciences · Engineering · Physics and Astronomy · #GNSS positioning and interference #Geophysics and Gravity Measurements #Solar and Space Plasma Dynamics #astro-ph #gr-qc #physics.space-ph

paper · pdf · doi:10.1088/0264-9381/19/17/103

published as Class.Quant.Grav. 19 (2002) L175-L183 · LaTex2e, 11 pages, 4 figures, 1 table. Accepted for publication in Classical and Quantum Gravity

arxiv created 2002/07/25 · openalex publication_date 2002/08/15 · arxiv updated 2009/11/30 · openalex created_date 2025/10/10 · openalex updated_date 2026/07/30

Abstract

According to very recent developments of the LARES mission, which is devoted to the measurement of the general relativistic Lense–Thirring effect in the gravitational field of the Earth with satellite laser ranging, it seems that the LARES satellite might be finally launched in a polar, low-altitude orbit by means of a relatively low-cost rocket. The observable would be the node only. The Lense–Thirring effect on it would consist of a secular linear trend. The biasing classical secular nodal precessions due to the even zonal harmonics of the geopotential, which represent the major source of uncertainty, vanish if and only if the orbit is exactly polar. Due to the small altitude, even small possible deviations from the projected inclination, which might be induced by the orbital injection errors, should yield a rather large systematic error due to the mismodelled even zonal harmonics of geopotential in the measurement of the relativistic nodal shift. So, in this paper we show how such a configuration, in fact, to the present level of knowledge of the terrestrial gravitational field according to the EGM96 gravity model, should be of relatively little utility in increasing the obtainable accuracy in measuring the Lense–Thirring effect with respect not only to the originally proposed supplementary LARES–LAGEOS configuration, but also to the present LAGEOS–LAGEOS II experiment which has a total accuracy of the order of 20–30%. Maybe the situation will improve, at least to a certain extent, when the new, more accurate Earth gravity models from the CHAMP and GRACE missions become available.

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