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VI/81 Planetary Solutions VSOP87 (Bretagnon+, 1988) ================================================================================ Planetary Theories in rectangular and spherical variables: VSOP87 solution. Bretagnon P., Francou G. <Astron. Astrophys. 202, 309 (1988)> =1988A&A...202..309B Theorie du mouvement de l'ensemble des planetes (VSOP82). Bretagnon P. <Astron. Astrophys. 114, 278 (1982)> =1982A&A...114..278B ================================================================================ ADC_Keywords: Ephemerides ; Keywords: planets - ephemerides - celestial mechanics Description: The Planetary solutions VSOP87 (Variations Seculaires des Orbites Planetaires) are analytical solutions of the motion of the planets in different versions. The main version VSOP87 consists of the series in elliptic elements as in the case of VSOP82 solution and the other versions VSOP87 (A-B-C-D-E) are built in in rectangular and spherical variables. Authors' Address: P. Bretagnon, G. Francou Bureau des Longitudes, CNRS URA 707 77, Avenue Denfert-Rochereau 75014, Paris, France Tel : (33) 1 40 51 22 69 (33) 1 40 51 22 60 Fax : (33) 1 46 33 28 34 E-mail : pierre@bdl.fr francou@bdl.fr Contents: The main version of VSOP87 is similar to the previous theory VSOP82. In the both cases the constants of integration have been determined by fitting to the numerical integration DE200 of the Jet Propulsion Laboratory. The various versions of VSOP87 are different from one to another in the type of coordinates and the reference frame. VSOP87 : heliocentric elliptic variables; equinox and ecliptic J2000. VSOP87A : heliocentric rectangular variables; equinox and ecliptic J2000. VSOP87B : heliocentric spherical variables; equinox and ecliptic J2000. VSOP87C : heliocentric rectangular variables; equinox and ecliptic of date. VSOP87D : heliocentric spherical variables; equinox and ecliptic of date. VSOP87E : barycentric rectangular variables; equinox and ecliptic J2000. A program EXAMPLE (Fortran 77) is provided which makes use of the subroutine VSOP87 which substitutes the time in the series of the solutions VSOP87. File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file vsop87.txt 80 338 Notice for use of VSOP87 files vsop87.f 72 231 Fortran77 subroutine VSOP87 (time substitution) example.f 72 781 Fortran77 program example of use of VSOP87 vsop87.chk 77 2000 Results of substitution of time in VSOP87 series VSOP87.mer 132 4843 Mercury Heliocentric elliptic elements J2000 VSOP87.ven 132 3018 Venus Heliocentric elliptic elements J2000 VSOP87.emb 132 4233 Earth-Moon Heliocentric elliptic elements J2000 VSOP87.mar 132 7540 Mars Heliocentric elliptic elements J2000 VSOP87.jup 132 6109 Jupiter Heliocentric elliptic elements J2000 VSOP87.sat 132 12375 Saturn Heliocentric elliptic elements J2000 VSOP87.ura 132 15212 Uranus Heliocentric elliptic elements J2000 VSOP87.nep 132 8049 Neptune Heliocentric elliptic elements J2000 VSOP87A.mer 132 6377 Mercury Heliocentric rectangular var. J2000 VSOP87A.ven 132 2375 Venus Heliocentric rectangular var. J2000 VSOP87A.ear 132 3556 Earth Heliocentric rectangular var. J2000 VSOP87A.emb 132 3340 Earth-Moon Heliocentric rectangular var. J2000 VSOP87A.mar 132 7091 Mars Heliocentric rectangular var. J2000 VSOP87A.jup 132 4452 Jupiter Heliocentric rectangular var. J2000 VSOP87A.sat 132 7530 Saturn Heliocentric rectangular var. J2000 VSOP87A.ura 132 5303 Uranus Heliocentric rectangular var. J2000 VSOP87A.nep 132 2650 Neptune Heliocentric rectangular var. J2000 VSOP87B.mer 132 7141 Mercury Heliocentric spherical var. J2000 VSOP87B.ven 132 1728 Venus Heliocentric spherical var. J2000 VSOP87B.ear 132 2582 Earth Heliocentric spherical var. J2000 VSOP87B.mar 132 6418 Mars Heliocentric spherical var. J2000 VSOP87B.jup 132 3643 Jupiter Heliocentric spherical var. J2000 VSOP87B.sat 132 6383 Saturn Heliocentric spherical var. J2000 VSOP87B.ura 132 5283 Uranus Heliocentric spherical var. J2000 VSOP87B.nep 132 2037 Neptune Heliocentric spherical var. J2000 VSOP87C.mer 132 8173 Mercury Heliocentric rectangular var. of date VSOP87C.ven 132 2922 Venus Heliocentric rectangular var. of date VSOP87C.ear 132 4211 Earth Heliocentric rectangular var. of date VSOP87C.mar 132 8321 Mars Heliocentric rectangular var. of date VSOP87C.jup 132 5573 Jupiter Heliocentric rectangular var. of date VSOP87C.sat 132 8801 Saturn Heliocentric rectangular var. of date VSOP87C.ura 132 7010 Uranus Heliocentric rectangular var. of date VSOP87C.nep 132 2898 Neptune Heliocentric rectangular var. of date VSOP87D.mer 132 6845 Mercury Heliocentric spherical var. of date VSOP87D.ven 132 1700 Venus Heliocentric spherical var. of date VSOP87D.ear 132 2442 Earth Heliocentric spherical var. of date VSOP87D.mar 132 5501 Mars Heliocentric spherical var. of date VSOP87D.jup 132 3501 Jupiter Heliocentric spherical var. of date VSOP87D.sat 132 5777 Saturn Heliocentric spherical var. of date VSOP87D.ura 132 4005 Uranus Heliocentric spherical var. of date VSOP87D.nep 132 1946 Neptune Heliocentric spherical var. of date VSOP87E.mer 132 7898 Mercury Barycentric rectangular var. J2000 VSOP87E.ven 132 4675 Venus Barycentric rectangular var. J2000 VSOP87E.ear 132 5574 Earth Barycentric rectangular var. J2000 VSOP87E.mar 132 7593 Mars Barycentric rectangular var. J2000 VSOP87E.jup 132 4560 Jupiter Barycentric rectangular var. J2000 VSOP87E.sat 132 7540 Saturn Barycentric rectangular var. J2000 VSOP87E.ura 132 5139 Uranus Barycentric rectangular var. J2000 VSOP87E.nep 132 2403 Neptune Barycentric rectangular var. J2000 VSOP87E.sun 132 6652 Sun Barycentric rectangular var. J2000 -------------------------------------------------------------------------------- See also: VI/88 : Ephemerides of Pluto based on DE200 (Chapront+ 1995) VI/87 : Planetary Ephemerides based on DE403 (Chapront+ 1996) Remarks: The subroutine VSOP87 and the program EXAMPLE (Fortran 77) are provided to simply illustrate the computation of a planetary ephemeris. If the user wants to improve the rapidity of computation, it is recommended to transform files in direct access or to read series in memory once for all. ================================================================================ (End) Gerard Francou [BDL], Francois Ochsenbein [CDS] 31-May-1995
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