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Geodetic Evidence That Mercury Has A Solid Inner Core.

Authors :
Genova, Antonio
Goossens, Sander
Mazarico, Erwan
Lemoine, Frank G.
Neumann, Gregory A.
Kuang, Weijia
Sabaka, Terence J.
Hauck, Steven A.
Smith, David E.
Solomon, Sean C.
Zuber, Maria T.
Source :
Geophysical Research Letters. 4/16/2019, Vol. 46 Issue 7, p3625-3633. 9p.
Publication Year :
2019

Abstract

Geodetic analysis of radio tracking measurements of the MErcury Surface, Space ENvironment, GEochemistry, and Ranging spacecraft while in orbit about Mercury has yielded new estimates for the planet's gravity field, tidal Love number, and pole coordinates. The derived right ascension (α = 281.0082° ± 0.0009°; all uncertainties are 3 standard deviations) and declination (δ = 61.4164° ± 0.0003°) of the spin pole place Mercury in the Cassini state. Confirmation of the equilibrium state with an estimated mean (whole planet) obliquity ϵ of 1.968 ± 0.027 arcmin enables the confident determination of the planet's normalized polar moment of inertia (0.333 ± 0.005), which indicates a high degree of internal differentiation. Internal structure models generated by a Markov Chain Monte Carlo process and consistent with the geodetic constraints possess a solid inner core with a radius (ric) between 0.3 and 0.7 that of the outer core (roc). Key Points: New solution for Mercury's gravity field provides crucial information on the planet's tidal response and orientationNew determination of Mercury's pole position fully satisfies the equilibrium Cassini stateNew estimate of Mercury's polar moment of inertia supports the presence of a large solid inner core [ABSTRACT FROM AUTHOR]

Details

Language :
English
ISSN :
00948276
Volume :
46
Issue :
7
Database :
Academic Search Index
Journal :
Geophysical Research Letters
Publication Type :
Academic Journal
Accession number :
136089450
Full Text :
https://doi.org/10.1029/2018GL081135