Mercury’s gravity, tides, and spin from MESSENGER radio science data

Ashok Kumar Verma, Jean-Luc Margot
(Submitted on 3 Aug 2016)

We analyze radio tracking data obtained during 1311 orbits of the MESSENGER spacecraft in the period March 2011 to April 2014. A least-squares minimization of the residuals between observed and computed values of two-way range and Doppler allows us to solve for a model describing Mercury’s gravity, tidal response, and spin state. We use a spherical harmonic representation of the gravity field to degree and order 40 and report error bars corresponding to 10 times the formal uncertainties of the fit. Our estimate of the product of Mercury’s mass and the gravitational constant, GM=(22031.87404±9×10−4) km3s−2, is in excellent agreement with published results. Our solution for the geophysically important second-degree coefficients (C¯2,0=−2.25100×10−5±1.3×10−9, C¯2,2=1.24973×10−5±1.2×10−9) confirms previous estimates to better than 0.4\% and, therefore, inferences about Mercury’s moment of inertia and interior structure. Our estimate of the tidal Love number k2=0.464±0.023 indicates that Mercury’s mantle may be hotter and weaker than previously thought. Our spin state solution suggests that gravity-based estimates of Mercury’s spin axis orientation are marginally consistent with previous measurements of the orientation of the crust.

Comments: Accepted for publication in J. Geophys. Res. – planets
Subjects: Earth and Planetary Astrophysics (astro-ph.EP); Geophysics (physics.geo-ph)
Cite as: arXiv:1608.01360 [astro-ph.EP] (or arXiv:1608.01360v1 [astro-ph.EP] for this version)
Submission history
From: Ashok Kumar Verma
[v1] Wed, 3 Aug 2016 21:17:20 GMT (4299kb,D)
http://arxiv.org/abs/1608.01360