Mercury's rotational parameters from MESSENGER image and laser altimeter data: A feasibility study. (November 2015)

• Record Type: Journal Article
• Authors: Stark, Alexander; Oberst, Jürgen; Preusker, Frank; Gwinner, Klaus; Peale, Stanton J.; Margot, Jean-Luc; Phillips, Roger J.; Zuber, Maria T.; Solomon, Sean C.
• Is Part Of: Planetary and space science. Volume 117(2015)
• Page Start: 64
• Page End: 72
• Publication Date: 2015-11
• Subjects: Mercury -- Rotation -- MESSENGER -- Laser altimetry -- Stereo photogrammetry -- Co-registration; Space sciences -- Periodicals; Atmosphere, Upper -- Periodicals; Sciences spatiales -- Périodiques; Haute atmosphère -- Périodiques; 523
• DOI: 10.1016/j.pss.2015.05.006
• Languages: English
• ISSNs: 0032-0633

Abstract

Abstract: A novel method has been developed to determine the rotational parameters of Mercury from data acquired by the MESSENGER spacecraft. We exploit the complementarity of laser altimeter tracks taken at different rotational phases and rigid stereo terrain models to determine a Mercury rotational model. In particular, we solve for the orientation of the spin axis, the rotation rate, and the amplitude of the forced libration. In this paper, we verify the proposed method and carry out an extensive simulation of MESSENGER data acquisition with assumed rotational parameters. To assess the uncertainty in the rotational parameters we use mission-typical assumptions for spacecraft attitude and position knowledge as well as for small-scale terrain morphology. We find that the orientation of the spin axis and the libration amplitude can be recovered with an accuracy of a few arc seconds from three years of MESSENGER orbital observations. The rotation rate can be determined to within 5 arc seconds per year. The method developed here serves as a framework for the ongoing analysis of data from the MESSENGER spacecraft. The rotational parameters of Mercury hold important constraints on the internal structure and evolution of the planet. Highlights: We developed a novel method for measurement of the rotational elements of Mercury. We solved for spin pole position, mean spin rate, and libration amplitude. Studies with simulated data verified the proposed method and its expected accuracy.