Authors: Weinwurm Gudrun
Year: 2006
Title: Gravity field of Jupiter’s moon Amalthea and the implication on a spacecraft trajectory
Journal: Advances in Space Research
Volume: 38
Number: 9
Pages: 2125-2130
Keywords: Jupiter, small, theory, parameter, analytical, model
Abstract: Before its final plunge into Jupiter in September 2003, GALILEO made a last ‘visit’ to one of Jupiter’s moons ᾢ Amalthea. This final flyby of the spacecraft’s successful mission occurred on November 5, 2002. In order to analyse the spacecraft data with respect to Amalthea’s gravity field, interior models of the moon had to be provided. The method used for this approach is based on the numerical integration of infinitesimal volume elements of a three-axial ellipsoid in elliptic coordinates. To derive the gravity field coefficients of the body, the second method of Neumann was applied. Based on the spacecraft trajectory data provided by the Jet Propulsion Laboratory, GALILEO’s velocity perturbations at closest approach could be calculated. The harmonic coefficients of Amalthea’s gravity field have been derived up to degree and order six, for both homogeneous and reasonable heterogeneous cases. Founded on these numbers the impact on the trajectory of GALILEO was calculated and compared to existing Doppler data. Furthermore, predictions for future spacecraft flybys were derived. No two-way Doppler-data was available during the flyby and the harmonic coefficients of the gravity field are buried in the one-way Doppler-noise. Nevertheless, the generated gravity field models reflect the most likely interior structure of the moon and can be a basis for further exploration of the Jovian system.
%F: Institute of Geodesy and Geophysics, Vienna University of Technology, A-1040 Vienna, Austria. Present address: Diamond Airborne Sensing, A-2700 Wr. Neustadt, Austria. Tel.: +43 664 1045981.
Bibliogaphic Code: 2006AdSpR..38.2125W
Return to previous page