Gravity field of Jupiter’s moon Amalthea and the implication on a spacecraft trajectory

Details Gravity field of Jupiter’s moon Amalthea and the implication on a spacecraft trajectory Gravity field of Jupiter’s moon Amalthea and the implication on a spacecraft trajectory

Jan 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006adspr..38.2125w&link_type=abstract

Advances in Space Research, Volume 38, Issue 9, p. 2125-2130.

Computer Science

Scientific paper

Before its final plunge into Jupiter in September 2003, GALILEO made a last ‘visit’ to one of Jupiter’s moons 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.

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