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987 lines
37 KiB
Plaintext
987 lines
37 KiB
Plaintext
KPL/PCK
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\begindata
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CASSINI_PCK_VERSION = ( '2004-MAR-05' )
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\begintext
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P_constants (PcK) SPICE kernel file
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Refer to the notes at the bottom of the file for help, contacts, version history,
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references, and Cassini-specific parameter descriptions. All radii and orientation
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values are from reference [1] unless otherwise noted.
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-------- SUN
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Value for the Sun radii is from [2], page K7. BODY10_GM from [10].
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\begindata
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BODY10_GM = ( 132712440017.9870 )
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BODY10_RADII = ( 696000. 696000. 696000. )
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BODY10_POLE_RA = ( 286.13 0. 0. )
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BODY10_POLE_DEC = ( 63.87 0. 0. )
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BODY10_PM = ( 84.10 +14.18440 0. )
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BODY10_LONG_AXIS = ( 0. )
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\begintext
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-------- VENUS
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BODY299_GM from [10].
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\begindata
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BODY2_GM = ( 324858.5988264598 )
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BODY299_GM = ( 324858.5988264598 )
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BODY299_RADII = ( 6051.8 6051.8 6051.8 )
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BODY299_POLE_RA = ( 272.76 0. 0. )
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BODY299_POLE_DEC = ( +67.16 0. 0. )
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BODY299_PM = ( 160.20 -1.4813688 0. )
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BODY299_LONG_AXIS = ( 0. )
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\begintext
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-------- EARTH
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BODY3_GM, BODY399_GM from [10]. Northern hemisphere projection of the
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Earth's magnetic dipole: coordinates are planetocentric, values are from [3].
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\begindata
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BODY3_GM = ( 403503.2334790870 )
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BODY399_GM = ( 398600.4328969392 )
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BODY399_RADII = ( 6378.140 6378.140 6356.75 )
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BODY399_POLE_RA = ( 0. -0.641 0. )
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BODY399_POLE_DEC = ( +90. -0.557 0. )
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BODY399_PM = ( 190.147 +360.9856235 0. )
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BODY399_LONG_AXIS = ( 0. )
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BODY3_NUT_PREC_ANGLES = ( 125.045 -1935.5364525000
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250.089 -3871.0729050000
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260.008 475263.3328725000
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176.625 487269.6299850000
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357.529 35999.0509575000
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311.589 964468.4993100001
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134.963 477198.8693250000
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276.617 12006.3007650000
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34.226 63863.5132425000
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15.134 -5806.6093575000
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119.743 131.8406400000
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239.961 6003.1503825000
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25.053 473327.7964200000 )
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BODY399_MAG_NORTH_POLE_LON = ( -69.761 )
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BODY399_MAG_NORTH_POLE_LAT = ( 78.565 )
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\begintext
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-------- JUPITER
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BODY599_GM value = BODY5_GM - Sum(BODY5xx_gm) where xx = 01,16. BODY5_GM
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value from [10].
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\begindata
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BODY5_GM = ( 126712767.8577960 )
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BODY599_GM = ( 126686536.9637693 )
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BODY599_RADII = ( 71492. 71492. 66854. )
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BODY599_POLE_RA = ( 268.05 -0.009 0. )
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BODY599_POLE_DEC = ( +64.49 +0.003 0. )
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BODY599_PM = ( 284.95 +870.5366420 0. )
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BODY599_LONG_AXIS = ( 0. )
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BODY5_NUT_PREC_ANGLES = ( 73.32 +91472.9
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24.62 +45137.2
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283.90 +4850.7
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355.80 +1191.3
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119.90 +262.1
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229.80 +64.3
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352.35 +2382.6
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113.35 +6070.0 )
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\begintext
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-------- SATURN
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BODY6_GM value from [10]. BODY699_GM value = BODY6_GM - Sum(BODY6xx_gm)
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where xx = 1,9. Nonzero gravitational harmonics listed below are J2, J4, J6, C22,
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S22 from [7]. In the future, the navigation team may track and report these
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values. The first seven angles given in NUT_PREC are the angles S1
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through S7 from the 2000 IAU report; the eighth and ninth angles are 2*S1
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and 2*S2, respectively.
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Ring models are from a variety of sources, but are documented in references
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[11] and [12]. F Ring Data are from [8]. MIMI zone reflects the old flight rule
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for MIMI INCA, +/- 30000 km thickness inside of 8.74 Rs.
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The optical altitude is for PDT to determine at what altitude delta (km)
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from the RADII that Saturn first starts to cast a discernible shadow.
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Eventually three different magnetospheric models will be provided. This
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section currently serves as a placeholder.
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BODY699_RADII_RS keyword is provided since the value 60330 is a standard number
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for most ring scientists.
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BODY699_MAG_NORTH_POLE_LON = ( 0.0 )
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BODY699_MAG_NORTH_POLE_LAT = ( +90.0 )
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BODY699_M1COEF = ( 0.0 0.0 0.0 0.0)
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BODY699_G1COEF = ( 0.0 0.0 0.0 0.0)
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BODY699_H1COEF = ( 0.0 0.0 0.0 0.0)
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BODY699_M2COEF = ( 0.0 0.0 0.0 0.0)
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BODY699_G2COEF = ( 0.0 0.0 0.0 0.0)
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BODY699_H2COEF = ( 0.0 0.0 0.0 0.0)
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BODY699_M3COEF = ( 0.0 0.0 0.0 0.0)
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BODY699_G3COEF = ( 0.0 0.0 0.0 0.0)
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BODY699_H3COEF = ( 0.0 0.0 0.0 0.0)
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\begindata
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BODY6_GM = ( 37940629.764 )
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BODY699_GM = ( 37931267.73 )
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BODY699_RADII = ( 60268. 60268. 54364. )
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BODY699_RADII_1BAR = ( 60268. 60268. 54364. )
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BODY699_RADII_OPTICAL = ( 60430. 60430. 54508. )
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BODY699_RADII_RS = ( 60330. 60330. 60330. )
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BODY699_POLE_RA = ( 40.589 -0.036 0. )
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BODY699_POLE_DEC = ( +83.537 -0.004 0. )
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BODY699_PM = ( 38.90 +810.7939024 0. )
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BODY699_LONG_AXIS = ( 0. )
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BODY699_JCOEF = ( 0.0, 0.016298, 0.0, -0.000915, 0.0, 0.000103 )
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BODY699_CCOEF = ( 0.0, 0.0, 0.00000070 )
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BODY699_SCOEF = ( 0.0, 0.0, -0.00000020 )
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BODY6_NUT_PREC_ANGLES = ( 353.32 75706.7
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28.72 75706.7
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177.40 -36505.5
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300.00 -7225.9
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316.45 506.2
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345.20 -1016.3
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29.80 -52.1
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706.64 151413.4
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57.44 151413.4 )
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BODY699_RING1_NAME = 'A Ring'
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BODY699_RING1 = (122170.0 136780.0 0.1 0.1 0.5)
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BODY699_RING1_1_NAME = 'Encke Gap'
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BODY699_RING1_1 = (133405.0 133730.0 0.0 0.0 0.0)
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BODY699_RING2_NAME = 'Cassini Division'
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BODY699_RING2 = (117580.0 122170.0 0.0 0.0 0.0)
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BODY699_RING3_NAME = 'B Ring'
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BODY699_RING3 = (92000.0 117580.0 0.1 0.1 1.5)
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BODY699_RING4_NAME = 'C Ring'
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BODY699_RING4 = (74510.0 92000.0 0.1 0.1 0.1)
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BODY699_RING5_NAME = 'D Ring'
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BODY699_RING5 = (66970.0 74510.0 0.1 0.1 0.00001)
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BODY699_RING6_NAME = 'E ring'
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BODY699_RING6_A = (189870.0 256900.0 9000.0 9000.0 0.000003)
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BODY699_RING6_B = (256900.0 420000.0 9000.0 17000.0 0.000003)
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BODY699_RING7_NAME = 'F Ring'
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BODY699_RING7 = (140180.0 140270.0 6.5 6.5 0.1)
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BODY699_RING7_FCENTER = (140223.7, 0.00254, 24.1, 2.7001, 0.0065, 16.1, -2.6876)
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BODY699_RING8_NAME = 'G Ring'
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BODY699_RING8 = (165000.0 176000.0 280.0 280.0 0.000001)
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BODY699_MIMI_DUST_ZONE = ( 0.0 527284.2 60000.0 60000.0 )
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\begintext
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-------- URANUS
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BODY7_GM value from [10].
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\begindata
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BODY7_GM = ( 5794549.007071874 )
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BODY799_GM = ( 5793939.2128179700 )
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BODY799_RADII = ( 25559. 25559. 24973. )
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BODY799_POLE_RA = ( 257.311 0. 0. )
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BODY799_POLE_DEC = ( -15.175 0. 0. )
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BODY799_PM = ( 203.81 -501.1600928 0. )
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BODY799_LONG_AXIS = ( 0. )
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\begintext
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-------- MOON
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BODY301_GM from [10].
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\begindata
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BODY301_GM = ( 4902.800582147764 )
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BODY301_RADII = ( 1737.4 1737.4 1737.4 )
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BODY301_POLE_RA = ( 269.9949 0.0031 0. )
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BODY301_POLE_DEC = ( 66.5392 0.0130 0. )
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BODY301_PM = ( 38.3213 13.17635815 -1.4D-12 )
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BODY301_LONG_AXIS = ( 0. )
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BODY301_NUT_PREC_RA = ( -3.8787 -0.1204 +0.0700 -0.0172
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0. +0.0072 0. 0.
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0. -0.0052 0. 0.
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+0.0043 )
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BODY301_NUT_PREC_DEC = ( 1.5419 0.0239 -0.0278 +0.0068
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0. -0.0029 +0.0009 0.
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0. +0.0008 0. 0.
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-0.0009 )
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BODY301_NUT_PREC_PM = ( 3.5610 +0.1208 -0.0642 +0.0158
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+0.0252 -0.0066 -0.0047 -0.0046
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+0.0028 +0.0052 +0.0040 +0.0019
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-0.0044 )
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\begintext
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-------- IO
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BODY501_GM value from [5].
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\begindata
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BODY501_GM = ( 5959.92 )
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BODY501_RADII = ( 1829.4 1819.3 1815.7 )
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BODY501_POLE_RA = ( 268.05 -0.009 0. )
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BODY501_POLE_DEC = ( +64.50 +0.003 0. )
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BODY501_PM = ( 200.39 +203.4889538 0. )
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BODY501_LONG_AXIS = ( 0. )
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BODY501_NUT_PREC_RA = ( 0. 0. +0.094 +0.024 )
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BODY501_NUT_PREC_DEC = ( 0. 0. +0.040 +0.011 )
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BODY501_NUT_PREC_PM = ( 0. 0. -0.085 -0.022 )
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\begintext
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-------- EUROPA
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BODY502_GM value from [5].
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\begindata
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BODY502_GM = ( 3202.72 )
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BODY502_RADII = ( 1564.13 1561.23 1560.93 )
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BODY502_POLE_RA = ( 268.08 -0.009 0. )
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BODY502_POLE_DEC = ( +64.51 +0.003 0. )
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BODY502_PM = ( 36.022 +101.3747235 0. )
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BODY502_LONG_AXIS = ( 0. )
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BODY502_NUT_PREC_RA = ( 0. 0. 0. +1.086 +0.060 +0.015 +0.009 )
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BODY502_NUT_PREC_DEC = ( 0. 0. 0. +0.468 +0.026 +0.007 +0.002 )
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BODY502_NUT_PREC_PM = ( 0. 0. 0. -0.980 -0.054 -0.014 -0.008 )
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\begintext
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-------- GANYMEDE
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BODY503_GM value from [5].
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\begindata
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BODY503_GM = ( 9887.83 )
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BODY503_RADII = ( 2632.4 2632.29 2632.35 )
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BODY503_POLE_RA = ( 268.20 -0.009 0. )
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BODY503_POLE_DEC = ( +64.57 +0.003 0. )
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BODY503_PM = ( 44.04 +50.3176081 0. )
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BODY503_LONG_AXIS = ( 0. )
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BODY503_NUT_PREC_RA = ( 0. 0. 0. -0.037 +0.431 +0.091 )
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BODY503_NUT_PREC_DEC = ( 0. 0. 0. -0.016 +0.186 +0.039 )
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BODY503_NUT_PREC_PM = ( 0. 0. 0. +0.033 -0.389 -0.082 )
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\begintext
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-------- CALLISTO
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BODY504_GM value from [5].
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\begindata
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BODY504_GM = ( 7179.29 )
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BODY504_RADII = ( 2409.4 2409.2 2409.3 )
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BODY504_POLE_RA = ( 268.72 -0.009 0. )
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BODY504_POLE_DEC = ( +64.83 +0.003 0. )
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BODY504_PM = ( 259.51 +21.5710715 0. )
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BODY504_LONG_AXIS = ( 0. )
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BODY504_NUT_PREC_RA = ( 0. 0. 0. 0. -0.068 +0.590 0. +0.010 )
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BODY504_NUT_PREC_DEC = ( 0. 0. 0. 0. -0.029 +0.254 0. -0.004 )
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BODY504_NUT_PREC_PM = ( 0. 0. 0. 0. +0.061 -0.533 0. -0.009 )
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\begintext
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-------- HIMALIA
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BODY506_GM values from [7].
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\begindata
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BODY506_GM = ( 0.45 )
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BODY506_RADII = ( 85 85 85 )
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BODY506_POLE_RA = ( 268.72 -0.009 0. )
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BODY506_POLE_DEC = ( +64.83 +0.003 0. )
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BODY506_PM = ( 259.51 +21.5710715 0. )
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BODY506_LONG_AXIS = ( 0. )
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\begintext
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-------- MIMAS
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BODY601_GM from [6].
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\begindata
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BODY601_GM = ( 2.5 )
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BODY601_RADII = ( 209.1 196.2 191.4 )
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BODY601_POLE_RA = ( 40.66 -0.036 0. )
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BODY601_POLE_DEC = ( +83.52 -0.004 0. )
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BODY601_PM = ( 337.46 +381.9945550 0. )
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BODY601_LONG_AXIS = ( 0. )
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BODY601_NUT_PREC_RA = ( 0. 0. +13.56 0. 0. 0. 0. 0. 0. )
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BODY601_NUT_PREC_DEC = ( 0. 0. -1.53 0. 0. 0. 0. 0. 0. )
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BODY601_NUT_PREC_PM = ( 0. 0. -13.48 0. -44.85 0. 0. 0. 0. )
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\begintext
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-------- ENCELADUS
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BODY602_GM from [6].
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\begindata
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BODY602_GM = ( 4.9 )
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BODY602_RADII = ( 256.3 247.3 244.6 )
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BODY602_POLE_RA = ( 40.66 -0.036 0. )
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BODY602_POLE_DEC = ( +83.52 -0.004 0. )
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BODY602_PM = ( 2.82 +262.7318996 0. )
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BODY602_LONG_AXIS = ( 0. )
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\begintext
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-------- TETHYS
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BODY603_GM from [6].
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\begindata
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BODY603_GM = ( 41.808 )
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BODY603_RADII = ( 535.6 528.2 525.8 )
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BODY603_POLE_RA = ( 40.66 -0.036 0. )
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BODY603_POLE_DEC = ( +83.52 -0.004 0. )
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BODY603_PM = ( 10.45 +190.6979085 0. )
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BODY603_LONG_AXIS = ( 0. )
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BODY603_NUT_PREC_RA = ( 0. 0. 0. +9.66 0. 0. 0. 0. 0. )
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BODY603_NUT_PREC_DEC = ( 0. 0. 0. -1.09 0. 0. 0. 0. 0. )
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BODY603_NUT_PREC_PM = ( 0. 0. 0. -9.60 +2.23 0. 0. 0. 0. )
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\begintext
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-------- DIONE
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BODY604_GM from [6].
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\begindata
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BODY604_GM = ( 73.156 )
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BODY604_RADII = ( 560. 560. 560. )
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BODY604_POLE_RA = ( 40.66 -0.036 0. )
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BODY604_POLE_DEC = ( +83.52 -0.004 0. )
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BODY604_PM = ( 357.00 +131.5349316 0. )
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BODY604_LONG_AXIS = ( 0. )
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\begintext
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-------- RHEA
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BODY605_GM from [6].
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\begindata
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BODY605_GM = ( 154.000 )
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BODY605_RADII = ( 764. 764. 764. )
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BODY605_POLE_RA = ( 40.38 -0.036 0. )
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BODY605_POLE_DEC = ( +83.55 -0.004 0. )
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BODY605_PM = ( 235.16 +79.6900478 0. )
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BODY605_LONG_AXIS = ( 0. )
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BODY605_NUT_PREC_RA = ( 0. 0. 0. 0. 0. +3.10 0. 0. 0. )
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BODY605_NUT_PREC_DEC = ( 0. 0. 0. 0. 0. -0.35 0. 0. 0. )
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BODY605_NUT_PREC_PM = ( 0. 0. 0. 0. 0. -3.08 0. 0. 0. )
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\begintext
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-------- TITAN
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BODY606_GM from [6].
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\begindata
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BODY606_GM = ( 8978.2 )
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BODY606_RADII = ( 2575. 2575. 2575. )
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BODY606_POLE_RA = ( 36.41 -0.036 0. )
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BODY606_POLE_DEC = ( +83.94 -0.004 0. )
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BODY606_PM = ( 189.64 +22.5769768 0. )
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BODY606_LONG_AXIS = ( 0. )
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BODY606_NUT_PREC_RA = ( 0. 0. 0. 0. 0. 0. +2.66 0. 0. )
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BODY606_NUT_PREC_DEC = ( 0. 0. 0. 0. 0. 0. -0.30 0. 0. )
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|
BODY606_NUT_PREC_PM = ( 0. 0. 0. 0. 0. 0. -2.64 0. 0. )
|
|
BODY606_ATMOSPHERE = ( 175.0 10.0
|
|
0.000006350 11400.0 76.0
|
|
0.000000513 8030.0 -429.0
|
|
0.000073500 15000.0 44.0 )
|
|
\begintext
|
|
|
|
|
|
-------- HYPERION
|
|
|
|
|
|
BODY607_GM from [6].
|
|
|
|
|
|
While Hyperion's spin state is chaotic, Voyager and ground-based
|
|
observations suggest some states are common (Thomas et al 1995,
|
|
Icarus 117, 128-148). The spin pole orientation is from the
|
|
Voyager observations; both the spin pole orientation and spin rate
|
|
will probably differ during Cassini's mission. Hyperion radii and
|
|
orientation from Peter Thomas @ Cornell
|
|
|
|
|
|
\begindata
|
|
BODY607_GM = ( 0.99 )
|
|
BODY607_RADII = ( 164. 130. 107. )
|
|
BODY607_POLE_RA = ( 226. 0 0 )
|
|
BODY607_POLE_DEC = ( 35. 0 0 )
|
|
BODY607_PM = ( 20.02 72.0 0 )
|
|
BODY607_LONG_AXIS = ( 0. )
|
|
\begintext
|
|
|
|
|
|
-------- IAPETUS
|
|
|
|
|
|
BODY608_GM from [6].
|
|
|
|
|
|
\begindata
|
|
BODY608_GM = ( 106.0 )
|
|
BODY608_RADII = ( 718. 718. 718. )
|
|
BODY608_POLE_RA = ( 318.16 -3.949 0. )
|
|
BODY608_POLE_DEC = ( +75.03 -1.143 0. )
|
|
BODY608_PM = ( 350.20 +4.5379572 0. )
|
|
BODY608_LONG_AXIS = ( 0. )
|
|
\begintext
|
|
|
|
|
|
-------- PHOEBE
|
|
|
|
|
|
BODY609_GM from [6].
|
|
BODY609_PM from [13].
|
|
|
|
|
|
\begindata
|
|
BODY609_GM = ( 0.48 )
|
|
BODY609_RADII = ( 115. 110. 105. )
|
|
BODY609_POLE_RA = ( 355.00 0. 0. )
|
|
BODY609_POLE_DEC = ( +68.70 0. 0. )
|
|
BODY609_PM = ( 178.58 +931.639 0. )
|
|
BODY609_LONG_AXIS = ( 0. )
|
|
\begintext
|
|
|
|
|
|
-------- JANUS
|
|
|
|
|
|
BODY610_GM is from [7].
|
|
|
|
|
|
\begindata
|
|
BODY610_GM = ( 0.1284 )
|
|
BODY610_RADII = ( 97. 95. 77. )
|
|
BODY610_POLE_RA = ( 40.58 -0.036 0. )
|
|
BODY610_POLE_DEC = ( 83.52 -0.004 0. )
|
|
BODY610_PM = ( 58.83 +518.2359876 0. )
|
|
BODY610_LONG_AXIS = ( 0. )
|
|
BODY610_NUT_PREC_RA = ( 0. -1.623 0. 0. 0. 0. 0. 0. +0.023 )
|
|
BODY610_NUT_PREC_DEC = ( 0. -0.183 0. 0. 0. 0. 0. 0. +0.001 )
|
|
BODY610_NUT_PREC_PM = ( 0. +1.613 0. 0. 0. 0. 0. 0. -0.023 )
|
|
\begintext
|
|
|
|
|
|
-------- EPIMETHEUS
|
|
|
|
|
|
BODY611_GM is from [7].
|
|
|
|
|
|
\begindata
|
|
BODY611_GM = ( .0357 )
|
|
BODY611_RADII = ( 69. 55. 55. )
|
|
BODY611_POLE_RA = ( 40.58 -0.036 0. )
|
|
BODY611_POLE_DEC = ( 83.52 -0.004 0. )
|
|
BODY611_PM = ( 293.87 +518.4907239 0. )
|
|
BODY611_LONG_AXIS = ( 0. )
|
|
BODY611_NUT_PREC_RA = ( -3.153 0. 0. 0. 0. 0. 0. +0.086 0. )
|
|
BODY611_NUT_PREC_DEC = ( -0.356 0. 0. 0. 0. 0. 0. +0.005 0. )
|
|
BODY611_NUT_PREC_PM = ( +3.133 0. 0. 0. 0. 0. 0. -0.086 0. )
|
|
\begintext
|
|
|
|
|
|
-------- HELENE
|
|
|
|
|
|
BODY612_GM is from [7].
|
|
|
|
|
|
Only the subplanetary equatorial radius and polar radius for Helene
|
|
(body 612) are listed in the 2000 IAU report, i.e.:
|
|
|
|
|
|
BODY612_RADII = ( 17.5 --- 0.7 )
|
|
|
|
|
|
The mean radius is 16km; we use the mean radius for each axis when all
|
|
three are not available.
|
|
|
|
|
|
\begindata
|
|
BODY612_GM = ( .0017 )
|
|
BODY612_RADII = ( 16 16 16 )
|
|
BODY612_POLE_RA = ( 40.85 -0.036 0. )
|
|
BODY612_POLE_DEC = ( 83.34 -0.004 0. )
|
|
BODY612_PM = ( 245.12 +131.6174056 0. )
|
|
BODY612_LONG_AXIS = ( 0. )
|
|
\begintext
|
|
|
|
|
|
-------- TELESTO
|
|
|
|
|
|
BODY613_GM is from [7].
|
|
|
|
|
|
\begindata
|
|
BODY613_GM = ( .00048 )
|
|
BODY613_RADII = ( 15 12.5 7.5 )
|
|
BODY613_POLE_RA = ( 50.51 -0.036 0. )
|
|
BODY613_POLE_DEC = ( 84.06 -0.004 0. )
|
|
BODY613_PM = ( 56.88 +190.6979332 0. )
|
|
BODY613_LONG_AXIS = ( 0. )
|
|
\begintext
|
|
|
|
-------- CALYPSO
|
|
|
|
|
|
BODY614_GM is from [7].
|
|
|
|
|
|
\begindata
|
|
BODY614_GM = ( 0.00024 )
|
|
BODY614_RADII = ( 15 8 8 )
|
|
BODY614_POLE_RA = ( 36.41 -0.036 0. )
|
|
BODY614_POLE_DEC = ( 85.04 -0.004 0. )
|
|
BODY614_PM = ( 153.51 +190.6742373 0. )
|
|
BODY614_LONG_AXIS = ( 0. )
|
|
\begintext
|
|
|
|
|
|
-------- ATLAS
|
|
|
|
|
|
BODY615_GM is from [7].
|
|
|
|
|
|
\begindata
|
|
BODY615_GM = ( 0.00072 )
|
|
BODY615_RADII = ( 18.5 17.2 13.5 )
|
|
BODY615_POLE_RA = ( 40.58 -0.036 0. )
|
|
BODY615_POLE_DEC = ( 83.53 -0.004 0. )
|
|
BODY615_PM = ( 137.88 +598.3060000 0. )
|
|
BODY615_LONG_AXIS = ( 0. )
|
|
\begintext
|
|
|
|
|
|
-------- PROMETHEUS
|
|
|
|
|
|
BODY616_GM is from [7].
|
|
|
|
|
|
\begindata
|
|
BODY616_GM = ( 0.022 )
|
|
BODY616_RADII = ( 74 50 34 )
|
|
BODY616_POLE_RA = ( 40.58 -0.036 0. )
|
|
BODY616_POLE_DEC = ( 83.53 -0.004 0. )
|
|
BODY616_PM = ( 296.14 +587.2890000 0. )
|
|
BODY616_LONG_AXIS = ( 0. )
|
|
\begintext
|
|
|
|
|
|
-------- PANDORA
|
|
|
|
|
|
BODY617_GM is from [7].
|
|
|
|
|
|
\begindata
|
|
BODY617_GM = ( 0.013 )
|
|
BODY617_RADII = ( 55 44 31 )
|
|
BODY617_POLE_RA = ( 40.58 -0.036 0. )
|
|
BODY617_POLE_DEC = ( 83.53 -0.004 0. )
|
|
BODY617_PM = ( 162.92 +572.7891000 0. )
|
|
BODY617_LONG_AXIS = ( 0. )
|
|
\begintext
|
|
|
|
|
|
-------- PAN
|
|
|
|
|
|
BODY618_GM is from [7]. For Pan, only a mean radius is given in the 2000 IAU report.
|
|
|
|
|
|
\begindata
|
|
BODY618_GM = ( 0.00018 )
|
|
BODY618_RADII = ( 10 10 10 )
|
|
BODY618_POLE_RA = ( 40.6 -0.036 0. )
|
|
BODY618_POLE_DEC = ( 83.5 -0.004 0. )
|
|
BODY618_PM = ( 48.8 +626.0440000 0. )
|
|
BODY618_LONG_AXIS = ( 0. )
|
|
\begintext
|
|
|
|
|
|
-------- CONSTANTS AND NOTES FOR PDT USERS
|
|
|
|
|
|
The astronomical unit AU, given in kilometers.
|
|
|
|
|
|
\begindata
|
|
AU = ( 149597870.7 )
|
|
\begintext
|
|
|
|
|
|
|
|
Saturn reference radius (Rs) is the base for measuring body
|
|
distances and ring radial distances in mulitples of saturn radius.
|
|
|
|
|
|
\begindata
|
|
RS = ( 60330.0 )
|
|
\begintext
|
|
|
|
|
|
Note that GM values >= 1.0 are packaged as is into 7CONIC_VEC
|
|
commands for AACS to propagate the body's ephemeris.
|
|
For GM values < 1.0, the value in the G_MASS parameter
|
|
of the 7CONIC_VEC command is set to 1.0. One is the minimum
|
|
value for the G_MASS parameter. The resetting of the G_MASS
|
|
parameter to the minimum acceptable where the actual
|
|
GM is < 1.0 is acceptable since CAS will not pass close enough
|
|
to any of the affected bodies for the gravitational mass
|
|
to have an effect.
|
|
|
|
-------- OBLATE SPHEROIDS VERSUS TRIAXIAL ELLIPSOIDS
|
|
|
|
|
|
Some Cassini software cannot model triaxial ellipsoids, where the
|
|
RADII are all different. Instead, they model bodies as oblate
|
|
spheroids, where the equatorial RADII values (the first two) must
|
|
be identical. In cases here where the equatorial radii are not
|
|
identical, the average of the two should be used when constructing
|
|
an oblate spheroid. The polar radius (the third RADII) can be used
|
|
as given in both cases.
|
|
|
|
|
|
-------- CONSTANTS AND NOTES FOR CASPER USERS
|
|
|
|
|
|
\begindata
|
|
BODY601_GM/PRIMARY = ( 6.59087D-08 )
|
|
BODY602_GM/PRIMARY = ( 1.29181D-07 )
|
|
BODY603_GM/PRIMARY = ( 1.1022D-06 )
|
|
BODY604_GM/PRIMARY = ( 1.92865D-06 )
|
|
BODY605_GM/PRIMARY = ( 4.05998D-06 )
|
|
BODY606_GM/PRIMARY = ( 2.36697D-04 )
|
|
BODY607_GM/PRIMARY = ( 2.60998D-08 )
|
|
BODY608_GM/PRIMARY = ( 2.79453D-06 )
|
|
BODY609_GM/PRIMARY = ( 1.26545D-08 )
|
|
BODY610_GM/PRIMARY = ( 3.38507D-09 )
|
|
BODY611_GM/PRIMARY = ( 9.41176D-10 )
|
|
BODY612_GM/PRIMARY = ( 4.48179D-11 )
|
|
BODY613_GM/PRIMARY = ( 1.26545D-11 )
|
|
BODY614_GM/PRIMARY = ( 6.32723D-12 )
|
|
BODY615_GM/PRIMARY = ( 1.89817D-11 )
|
|
BODY616_GM/PRIMARY = ( 5.79996D-10 )
|
|
BODY617_GM/PRIMARY = ( 3.42725D-10 )
|
|
BODY618_GM/PRIMARY = ( 4.74543D-12 )
|
|
\begintext
|
|
|
|
-------- URLS AND CONTACTS
|
|
|
|
|
|
Description of PCK format and contents can be found in NAIF's PCK "required
|
|
reading" document, at:
|
|
|
|
ftp://naif.jpl.nasa.gov/pub/naif/toolkit_docs/C/ascii/individual_docs/pck.req
|
|
|
|
|
|
NAIF tutorial on PCK formatting and use at:
|
|
|
|
ftp://naif.jpl.nasa.gov/pub/naif/toolkit_docs/Tutorials/office/individual_docs/16_pck.ppt
|
|
ftp://naif.jpl.nasa.gov/pub/naif/toolkit_docs/Tutorials/office/packages/
|
|
SPICE_tutorials_Oct-12-2003.zip
|
|
|
|
|
|
The Cassini PCK & ephemeris files can be found on the DOM, and at:
|
|
|
|
ftp://naif.jpl.nasa.gov/pub/naif/CASSINI/kernels/
|
|
|
|
|
|
Questions regarding this file can be directed to:
|
|
|
|
Diane Conner (818)354-8586 Diane.Conner@jpl.nasa.gov
|
|
David Seal (818)354-2707 David.Seal@jpl.nasa.gov
|
|
|
|
|
|
-------- VERSION HISTORY
|
|
|
|
|
|
Only the noted versions were officially published; the others were
|
|
created and circulated for internal review only.
|
|
|
|
2004 Mar 05 (published)
|
|
|
|
Updated descriptive text preceeding RS keyword.
|
|
Updated contact information and verified URLs.
|
|
|
|
Updates per ECR 103313:
|
|
Change 1: Update the values for Pheobe Prime Meridian
|
|
TO:
|
|
BODY609_PM = ( 178.58 +931.639 0. )
|
|
|
|
Reference: Bauer, Simonelli, Buratti, IAU Circular 8279,
|
|
1/30/2004; re-reduced by Owen 2/5/2004
|
|
|
|
Change 2: Saturn Reference Radius
|
|
ADD:
|
|
BODY699_RADII_RS = ( 60330. 60330. 60330. )
|
|
60330 is such a standard number for almost all ring scientists
|
|
and is needed in the PCK.
|
|
Date: Tue, 25 Nov 2003 16:22:41 -0700
|
|
From: Carolyn Porco <carolyn@ciclops.org>
|
|
|
|
2002 Oct 01 (published)
|
|
Changed BODY699_RADII_OPTICAL to be consistent with recommendation of Phil
|
|
Nicholson dated 24 Sep. Added notes in the version history as to which
|
|
versions were published to the DOM, as opposed to the versions that were
|
|
intermediate for review.
|
|
|
|
2002 Aug 28
|
|
Expanded some version histories. Added radii for alternate models of Saturn.
|
|
Added notes on oblate spheroids vs. triaxial ellipsoids. Fixed the reference
|
|
for BODY10_GM. Provided more description of URL links.
|
|
|
|
|
|
2002 Aug 12
|
|
Added notes on gravitational harmonics. Added link to NAIF required reading
|
|
document. Removed unused references.
|
|
|
|
|
|
2002 Jun 21
|
|
Made cosmetic changes to organization. Added begindata flag to Venus area
|
|
so that Venus data would not be lost. Copied Venus GM to Venus system GM
|
|
(since Venus has no satellites). Removed entries for small Jovian
|
|
satellites except for Himalia (no small satellites were observed by Cassini
|
|
except Himalia). Added dummy orientation values for Himalia (since
|
|
IAU_HIMALIA is a possible coordinate frame). Removed last two NUT_PREC entries
|
|
for Jupiter (big 4 satellites + Himalia only require 8 angles, not 10). Fixed
|
|
the BODY3_NUT_PREC angles to the full set that is required for Earth and Moon
|
|
orientation. Corrected errors in the orientation for Callisto and Jupiter.
|
|
Removed BODY7_NUT_PREC angles since no Uranian satellites are present.
|
|
Adjusted Jovian satellite radii to match IAU 2000 report. Added LONG_AXIS
|
|
statement for Hyperion.
|
|
By: David Seal
|
|
|
|
|
|
2002 Jun 20
|
|
Added BODY299_GM and BODY299_RADII.
|
|
By: John Aiello
|
|
|
|
|
|
2002 Jun 17
|
|
Changes to reflect values listed in IAU/IAG/COSPAR 2000 report:
|
|
BODY399_PM, BODY502_PM, BODY504_PM, BODY505_RADII, BODY514_RADII,
|
|
BODY515_RADII, BODY516_RADII, BODY607_RADII.
|
|
By: John Aiello
|
|
|
|
|
|
2002 Jun 10
|
|
Updated BODY5_GM, BODY599_GM, and BODY301_GM per NAV OD solution SM828D.
|
|
By: John Aiello
|
|
|
|
|
|
2002 Jun 06
|
|
Reference added for Saturn gravitational field.
|
|
By: John Aiello
|
|
|
|
|
|
2002 May 02
|
|
Corrected values for: BODY3_NUT_PREC_ANGLES, BODY599_PM (rotation rate was missing
|
|
last four digits), BODY610_PM (rotation rate was missing last digit). These values
|
|
were changed to be consistent with the IAU 2000 report.
|
|
By: John Aiello
|
|
2 May 2002
|
|
|
|
|
|
2001 Dec 14 (published)
|
|
Corrected typo in BODY699_RING1
|
|
By: John Aiello
|
|
14 Dec 2001
|
|
|
|
|
|
2001 Nov 20 (published)
|
|
Saturn ring model (updated version per series of telecons between PDT software
|
|
architects and Mark Showalter, Jeff Cuzzi, Carolyn Porco, Linda Spilker, John Aiello)
|
|
By: John Aiello
|
|
20 Nov 2001
|
|
|
|
|
|
2001 Oct 26 (published)
|
|
First release. Contents as follows.
|
|
GM values for Sun, Earth, Moon, Jupiter, Saturn, Mimas, Enceladus,
|
|
Tethys, Dione, Rhea, Titan, Hyperion, Iapetus, Phoebe
|
|
Saturn ring model
|
|
Saturn magnetosphere model
|
|
Titan atmosphere model
|
|
Dummy values for Himalia froim Kevin Yau (Cassini PDT) 2000 May 11
|
|
Based on pck0007.tpc by Nat Bachman (NAIF) 2000 April 24
|
|
By: Dave Seal, John Aiello (Cassini Mission Planning)
|
|
|
|
|
|
|
|
-------- FORMATTING FOR SPECIAL PARAMETERS
|
|
|
|
|
|
BODYNNN_GM
|
|
GM in km^3/s^2
|
|
|
|
BODYNNN_RADII_OPTICAL
|
|
BODYNNN_RADII_1BAR
|
|
BOYDNNN_RADII_RS
|
|
Alternate radii that are required for modeling purposes. These radii are
|
|
not necessarily identical to the IAU standard, and may have to be updated
|
|
during tour at a frequency not compatible with the IAU standard update
|
|
process. (For this reason, these were added so that Cassini would not be
|
|
required to use the existing RADII for not-IAU-approved values.) The OPTICAL
|
|
radii are typically used to determine the point at which Saturn's atmosphere
|
|
begins to attenuate light rays (e.g. for shadowing). The 1 bar radii may be
|
|
used as a markpoint for some radio or atmospheric observations. The RS radii
|
|
may be used by ring scientists that model Saturn as a sphere.
|
|
|
|
|
|
BODYNNN_ATMOSPHERE
|
|
Exponential atmospheric model in the form of one set of
|
|
two values To, f, followed by any number of sets of
|
|
three numbers Do, K, Zo. The atmospheric density in g/cm3
|
|
can be calculated as follows:
|
|
Z = height above surface (km)
|
|
R = radius of body (km)
|
|
T = thermospheric temperature (K) = To + f * sigma, where
|
|
sigma is the number of standard deviations (conservatism)
|
|
desired. If f > 0, positive sigma will result in a hotter
|
|
thermosphere and higher density.
|
|
H = scale height of atmosphere (km) = T * ( R + Z ) / K
|
|
(K is a curve-fit parameter with units of degrees K)
|
|
D = density (g/cm3) = Do * exp( - ( Z - Zo ) / H )
|
|
If there are more than one set of Do, K, Zo, sum each
|
|
value to get the total atmospheric density.
|
|
|
|
|
|
BODYNNN_RING*
|
|
The ring identification scheme is numeric with keyword-associated names.
|
|
The defnition of a ring is in a set of keywords. The BODYNNN_RING...
|
|
keyword set includes
|
|
|
|
|
|
1) a required NAME keyword (BODYNNN_RING<n>_NAME),
|
|
2) either a complete ring keyword (BODYNNN_RING<n>) or a set of segmented
|
|
ring keywords (BODYNNN_RING<n>_<X>), and
|
|
3) optional embedded ringlet/gap keywords (BODYNNN_RING<n>_<n>) with
|
|
required names (BODYNNN_RING<n>_<n>_NAME).
|
|
|
|
|
|
The total number of rings (BODYNNN_RING<n>) that can be defined is from
|
|
01 to 99. A complete ring can be segmented (BODYNNN_RING<n>_<X>) in upto
|
|
26 (A-Z) sub-segments. Embedded ringlets/gaps (BODYNNN_RING<n>_<n>) can
|
|
be defined from 1 to 99. Ring geometry is defined in the form of one set
|
|
of R1, R2, Z1, Z2, OD where R1 and R2 are inner and outer radii
|
|
respectively of the ring (in kilometers), Z1 and Z2 are the vertical
|
|
heights of the ring at R1 and R2 respectively (also in km, equal to
|
|
one-half of the total thickness of the ring), and OD is the average optical
|
|
depth of the ring sub-segment/gap across R1 to R2. A complex ring
|
|
thickness model is pieced together by sub-segmenting Rs, Zs, & ODs; each
|
|
sub-segment is uniquely numbered.
|
|
|
|
|
|
BODYNNN_*COEF
|
|
Where * = J, C, or S. These coefficients are the normalized gravity field
|
|
coefficients. J's are 1 to N, C's and S's have two indexes. Index 1 goes from
|
|
1 to N, and Index 2 goes from 1 to (Index 1). E.g. C11, C21, C22, C31, C32,
|
|
C33, C41, etc.
|
|
|
|
|
|
BODY699_RING7_FCENTER
|
|
Elliptical orbital characteristics for the F Ring: The array items (and
|
|
units) are (in order):
|
|
|
|
|
|
SEMIMAJOR_AXIS (km)
|
|
ECCENTRICITY (degrees)
|
|
LONGITUDE_PERICENTER_EPOCH (degrees)
|
|
PERICENTER_PRECESSION_RATE (degrees)
|
|
INCLINATION (degrees)
|
|
LONGITUDE_ASCENDING_NODE_EPOCH (degrees)
|
|
NODAL_REGRESSION_RATE (degrees).
|
|
|
|
|
|
The epoch for the elements is J2000 (noon UTC on 1/1/2000) at the ring
|
|
(i.e., with no light-time correction). Longitudes are measured in the
|
|
prograde direction from the ascending node of Saturn's equatorial plane
|
|
on Earth's J2000 equator.
|
|
|
|
|
|
-------- REFERENCES
|
|
|
|
1. "Report of the IAU/IAG/COSPAR Working Group on
|
|
Cartographic Coordinates and Rotational Elements of
|
|
the Planets and Satellites: 2000."
|
|
2. "The Astronomical Almanac," 2002.
|
|
3. Russell, Christopher T., "Geophysical Coordinate Transformations,"
|
|
Cosmic Electrodynamics 2 (1971) 184-186.
|
|
4. Showalter, Mark R. "Properties of Saturn's E and G Rings from the
|
|
1995 Ring Plane Crossings", presented at Ames ring hazard
|
|
workshop, 25 January 1996.
|
|
5. Jacobson, R. A., JPL IOM 312.F-00-102, 29 Jun 2000, "Jup171"
|
|
ephemeris file
|
|
6. Jacobson, R.A., JPL IOM 312.F-99-084, 13 Oct 1999, "Sat105"
|
|
ephemeris file
|
|
7. Jacobson, R., private communication; data will be presented in
|
|
forthcoming web site listing Satellite Physical Properties
|
|
8. Bosh, A. S., et. al., (2002) Icarus 157, 57.
|
|
9. Campbell, J.K. and Anderson, J.D. (1989) Astron J. 97, 1485.
|
|
10. Cassini NAV OD solution SM828D.
|
|
11. Cassini Mission Plan, JPL D-5564, Cassini document 699-100,
|
|
revision N, May 2002.
|
|
12. Cassini Dust Protection Plan, JPL D-24251, Cassini document 699-525,
|
|
revision A, October 2002.
|
|
13. Bauer, Simonelli, Buratti, IAU Circular 8279, 1/30/2004;
|
|
re-reduced by Owen 2/5/2004
|
|
|
|
Most values are from the "IAU/IAG/COSPAR Working Group on
|
|
Cartographic Coordinates and Rotational Elements of the
|
|
Planets and Satellites: 2000." All exceptions are commented
|
|
where they occur in this file.
|
|
|