| 1 | /* Position of outer planets; straightforward from:
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| 2 | ftp://adc.gsfc.nasa.gov/pub/adc/archives/journal_tables/A+AS/109/181:
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| 3 | 
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| 4 | J/A+AS/109/181                            Planetary ephemerides (Chapront, 1995)
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| 5 | ===============================================================================
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| 6 | Representation of planetary ephemerides by frequency analysis. Application to
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| 7 | the five outer planets.
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| 8 |        CHAPRONT J.
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| 9 |       <Astron. Astrophys. Suppl. Ser. 109, 181 (1995)>
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| 10 |       =1995A&AS..109..181C      (SIMBAD/NED Reference)
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| 11 | ===============================================================================
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| 12 | 
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| 13 | Keywords: ephemerides - planets and satellites: general - methods: numerical
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| 14 | 
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| 15 | Contents:
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| 16 |   Heliocentric equatorial rectangular coordinates of the five outer planets
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| 17 |   (X, Y and Z). The source is based on DE200 (tables 4 to 7) or a reconstruction
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| 18 |   of DE200 by numerical integration (tables 9 to 13). The reference frame is
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| 19 |   the mean equator and equinox J2000 of DE200.
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| 20 | 
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| 21 |   The general formulation of the series X is:
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| 22 |   X = SUM[i=1,Records] T**n_i*(CX_i*cos(Nu_k*t)+SX_i*sin(Nu_k*t))
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| 23 |   The formulation is identical for Y and Z.
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| 24 |   T is the time (TDB) in Julian centuries from J2000:
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| 25 |         T = (JulianDate - 2451545.0)/36525
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| 26 |   t is the time (TDB) in Julian years from J2000:
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| 27 |         t = (JulianDate - 2451545.0)/365.25
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| 28 |   Nu is the frequency. Frequencies are identical for all terms of rank k:
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| 29 |                 Nu_k = Nu_i when n_i = 0
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| 30 |                 For purely secular terms k = 0 and Nu_0 = 0
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| 31 | 
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| 32 | ===============================================================================
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| 33 | (End)                                          Patricia Bauer [CDS] 03-Oct-1994
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| 34 | */
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| 35 | 
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| 36 | #define CHAP_SCALE      1e10
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| 37 | 
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| 38 | /* JDs of validity period */
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| 39 | #define CHAP_BEGIN      (2338032.5 - MJD0)      /* 1689/3/19 */
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| 40 | #define CHAP_END        (2542032.5 - MJD0)      /* 2247/10/1 */
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| 41 | 
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| 42 | /* coding flags */
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| 43 | /* calculating rates increases time by about 10%
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| 44 |  *
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| 45 |  * On an HP715/75, for pluto the times per step are 0.00049 s and 0.00057 s
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| 46 |  * This method is quite fast.
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| 47 |  */
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| 48 | #define CHAP_GETRATE    1
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| 49 | 
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| 50 | typedef struct {
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| 51 |         short n;        /* order of time; "-1" marks end of list */
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| 52 |         double amp[6];  /* amplitudes of cosine and sine terms for x,y,z */
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| 53 |                         /* in original order [CX,SX,CY,SY,CZ,SZ] */
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| 54 |         double Nu;      /* Frequency Nu_k; given only at n=0 */
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| 55 | } chap95_rec;
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| 56 | 
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| 57 | extern chap95_rec chap95_jupiter[];
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| 58 | extern chap95_rec chap95_saturn[];
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| 59 | extern chap95_rec chap95_uranus[];
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| 60 | extern chap95_rec chap95_neptune[];
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| 61 | extern chap95_rec chap95_pluto[];
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| 62 | 
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| 63 | extern int chap95 (double m, int obj, double prec, double *ret);
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| 64 | 
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| 65 | 
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| 66 | /* For RCS Only -- Do Not Edit
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| 67 |  * @(#) $RCSfile: chap95.h,v $ $Date: 2011-09-21 16:17:48 $ $Revision: 1.9 $ $Name: not supported by cvs2svn $
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| 68 |  */
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