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Compared to the previous INPOP versions, the INPOP10a planetary and lunarephemeris has several improvements. For the planets of our solar system, no bigchange was brought in the dynamics but improvements were implemented in thefitting process, the data sets used in the fit and in the selection of fittedparameters. We report here the main characteristics of the planetary part ofINPOP10a like the fit of the product of the Solar mass with the gravitationalconstant (GM$_{\odot}$) instead of the astronomical unit. Determinations of PPNparameters as well as adjustments of the Sun J2 and of asteroid masses are alsopresented. New advances of nodes and perihelia of planets were also estimatedand are given here. As for INPOP08, INPOP10a provides to the user, positionsand velocities of the planets, the moon, the rotation angles of the Earth andthe Moon as well as TT-TDB chebychev polynomials at http://www.imcce.fr/inpop

The INPOP10a planetary ephemeris and its applications in fundamental physics