KPL/PCK P_constants (PCK) SPICE kernel file pck00011_n0066.tpc =========================================================================== By: Nat Bachman (NAIF) 2022 December 27 Data Accuracy Warning -------------------------------------------------------- This file provides reduced accuracy Phobos rotation data compared to those provided in the file pck00011.tpc. This reduction was needed to make this file usable with the N0066 and older versions of the SPICE Toolkit. See the sections "Version Description" and "Software limitations" below. All other data in this file match those provided in pck00011.tpc. Purpose -------------------------------------------------------- This file makes available for use in SPICE-based application software orientation and size/shape data for natural bodies. The principal source of the data is a published report by the IAU Working Group on Cartographic Coordinates and Rotational Elements [1]. Orientation and size/shape data not provided by this file may be available in mission-specific PCK files. Such PCKs may be the preferred data source for mission-related applications. Mission-specific PCKs can be found in PDS archives or on the NAIF web site at URL: https://naif.jpl.nasa.gov/naif/data.html Version Description -------------------------------------------------------- This file was created on December 27, 2022 by NASA's Navigation and Ancillary Information Facility (NAIF) group, located at the Jet Propulsion Laboratory, Pasadena, CA. This file contains the same data as the file pck00011.tpc except that in this file, data for the orientation of Phobos have been modified, at the expense of some loss of accuracy, so that the file is usable by the N0066 and older versions of the SPICE Toolkit. Specifically, in this file, the polynomial defining the M5 phase angle of the Mars system is truncated to first order, and all of the phase angle polynomial coefficient sets for the Mars system have two coefficients. Only the model of the orientation of Phobos is affected by this change. Over the time period 2000 : 2040 the maximum angular error of Phobos' orientation relative to that given by the original model is approximately 0.041 degrees. The maximum error occurs at year 2040. The previous version of the file was pck00010.tpc That file was published October 21, 2011. This version incorporates data from sources listed under "Sources and References" below. The primary sources are [1] and [2]. This file contains size, shape, and orientation data for all objects covered by the previous version of the file. New objects covered by this file but not by the previous version are: Asteroid 52 Europa Comet 67P/Churyumov-Gerasimenko Aegaeon (Saturn LIII) Comet Hartley 2 Asteroid Psyche Orientation data for the following objects provided by this file differ from those provided by the previous version: Mercury Mars Deimos Phobos Neptune Ceres Steins Vesta Borrelly Tempel 1 Radii for the following objects provided by this file differ from those provided by the previous version: Sun Mercury Anthe Atlas Calypso Daphnis Epimetheus Helene Janus Methone Pallene Pan Pandora Prometheus Telesto Pluto Charon Itokawa File Organization -------------------------------------------------------- The contents of this file are as follows. Introductory Information: -- Purpose -- Version description -- File Organization -- Disclaimer -- Sources -- Explanatory notes -- Body numbers and names PcK Data: Orientation Data ---------------- -- Orientation constants for the Sun, planets, and Pluto. Additional items included in this section: - North geomagnetic centered dipole value for the year 2023 -- Orientation constants for satellites -- Orientation constants for asteroids 52 Europa Davida Eros Gaspra Hartley 2 (data shown in comments only) Ida Itokawa Lutetia Pallas Steins Vesta -- Orientation constants for comets 19P/Borrelly 67P/Churyumov-Gerasimenko Hartley 2 (data shown in comments only) 9P/Tempel 1 Orientation data provided in this file are used by the SPICE Toolkit to evaluate the orientation of body-fixed, body-centered reference frames with respect to the ICRF frame ("J2000" in SPICE documentation). These body-fixed frames have names of the form IAU_ for example IAU_JUPITER See the PCK Required Reading file pck.req for details. Radii of Bodies --------------- -- Radii of Sun, planets, and Pluto -- Radii of satellites, where available -- Radii of asteroids 52 Europa Ceres Davida Eros Gaspra Ida Itokawa Lutetia Mathilde Psyche Steins Toutatis Vesta -- Radii of comets 19P/Borrelly 67P/Churyumov-Gerasimenko 81P/Wild 2 9P/Tempel 1 Halley Hartley 2 Disclaimer -------------------------------------------------------- Applicability of Data This P_constants file (PCK) may not contain the parameter values that you prefer. NAIF suggests that you inspect this file visually before proceeding with any critical or extended data processing. File Modifications by Users Note that this file may be readily modified by you to change values or add/delete parameters. NAIF requests that you update the "by line," date, version description section, and file name if you modify this file. A user-modified file should be thoroughly tested before being published or otherwise distributed. P_constants files must conform to the standards described in the two SPICE technical reference documents: PCK Required Reading Kernel Required Reading Known Limitations and Caveats Accuracy -------- In general, the orientation models given here are claimed by the IAU Working Group Report [1] to be accurate to 0.1 degree ([1], p. 9). However, NAIF notes that orientation models for natural satellites and asteroids have in some cases changed substantially with the availability of new observational data, so users are urged to investigate the suitability for their applications of the models presented here. Earth orientation ----------------- The IAU report [1] no longer provides rotational elements for the Earth. Data in this file are from [3]. NAIF strongly cautions against using the earth rotation model presented here, corresponding to the SPICE reference frame name IAU_EARTH, for work demanding high accuracy. This model has been determined by NAIF to have an error in the prime meridian location of magnitude at least 150 arcseconds, with a local minimum occurring during the year 1999. Regarding availability of better earth orientation data for use with the SPICE system: Earth orientation data are available from NAIF in the form of binary earth PCK files. These files provide orientation data for the ITRF93 (terrestrial) reference frame relative to the ICRF. NAIF employs an automated process to create these files; each time JPL's Tracking Systems and Applications Section produces a new earth orientation parameter (EOP) file, a new PCK is produced. These PCKs cover a roughly 23 year time span starting at Jan. 1, 2000. In these PCK files, the following effects are accounted for in modeling the earth's rotation: - Precession: 1976 IAU model - Nutation: 1980 IAU model, plus interpolated EOP nutation corrections - Polar motion: interpolated from EOP file - True sidereal time: UT1 - UT1R (if needed): given by analytic formula + TAI - UT1 (or UT1R): interpolated from EOP file + UT1 - GMST: given by analytic formula + equation of equinoxes: given by analytic formula where TAI = International Atomic Time UT1 = Greenwich hour angle of computed mean sun - 12h UT1R = Regularized UT1 GMST = Greenwich mean sidereal time These kernels are available from the NAIF web site https://naif.jpl.nasa.gov/pub/naif/generic_kernels/pck At this time, these kernels have file names of the form earth_000101_yymmdd_yymmdd.bpc The first date in the file name, meaning 2000 January 1, is the file's coverage begin time. The second and third dates are, respectively, the file's coverage end time and the epoch of the last datum. These binary PCK files are very accurate (error < 0.1 microradian) for epochs preceding the epoch of the last datum. For later epochs, the error rises to several microradians. Binary PCK files giving accurate earth orientation from 1972 to 2007 and *low accuracy* predicted earth orientation from 2020 to 2099 are also available in the same location. Characteristics and names of the binary kernels described here are subject to change. See the aareadme.txt file at the URL above for details. Lunar orientation ----------------- The IAU report [1] no longer provides rotational elements for the Moon. Data in this file are from [3]. The lunar orientation formula provided by this file is a trigonometric polynomial approximation yielding the orientation of the lunar "Mean Earth/Polar Axis" (ME) reference frame. The SPICE reference frame name corresponding to this model is IAU_MOON. A more accurate approximation can be obtained by using both the latest NAIF lunar frame kernel and the latest binary lunar orientation PCK file. These files provide orientation data for the both the Mean Earth/Polar Axis frame, which has the SPICE name MOON_ME, and the Lunar Principal Axes frame, which has the SPICE name MOON_PA. These files are available on the NAIF web site; lunar PCKs are located at the PCK URL above; lunar frame kernels are located at https://naif.jpl.nasa.gov/pub/naif/generic_kernels/fk/satellites The latest lunar frame kernel has a name of the form moon_dennn_yymmdd.tf The latest binary lunar PCK has a name of the form moon_pa_dennn_yymmdd.bpc See the "aareadme.txt" files in the paths shown above for details on file contents and versions. We also suggest you refer to the SPICE tutorial named "lunar_earth_pck-fk," which is available from the NAIF web site. Geomagnetic dipole ------------------ The SPICE Toolkit doesn't currently contain software to model the north geomagnetic centered dipole as a function of time. As a convenience for users, this dipole's location at the epoch 2023.0 was selected as a representative datum, and the planetocentric longitude and latitude of this location have been associated with the keywords BODY399_N_GEOMAG_CTR_DIPOLE_LON BODY399_N_GEOMAG_CTR_DIPOLE_LAT Older values for the north geomagnetic centered dipole are presented in comments as a discrete time series for the time range 1945-2000. For details concerning the geomagnetic field model from which these values were derived, including a discussion of the model's accuracy, see [9] and [11]. Prime meridian offsets ---------------------- Prime meridian offset kernel variables, which have names of the form BODYnnn_LONG_AXIS are not used by SPICE geometry software. These variables should be considered deprecated; however, they will be retained for backwards compatibility. Users wishing to specify an offset reflecting the orientation of a reference ellipsoid relative to a body-fixed reference frame specified here should do so by creating a constant-offset frame (also called a "TK" frame) specification. See the Frames Required Reading frames.req for details. The Mars prime meridian offset given by [6] is provided for informational purposes only. Software limitations -------------------- SPICE Toolkits prior to version N0067 cannot make use of the Mars system orientation data provided in the file pck00011.tpc These older Toolkits are unable to detect and signal a SPICE error if they are used to compute orientation of Mars, Phobos, or Deimos using these data: memory corruption will occur in user applications linked these Toolkits if the applications attempt such computations. Any results, including those of unrelated computations, may be invalid after such memory corruption occurs. NAIF provides this PCK file pck00011_n0066.tpc for use with older Toolkits. In this file, one of the phase angle polynomials for Phobos is truncated so as to be usable with older Toolkits. See the "Version Description" above for details. Sources and References -------------------------------------------------------- Sources and background references for the constants listed in this file are: [1] Archinal, B.A., Acton, C.H., A'Hearn, M.F., Conrad, A., Consolmagno, G.J., Duxbury, T., Hestroffer, D., Hilton, J.L., Kirk, R.L., Klinoner, S.A., McCarthy, D., Meech, K., Oberst, J., Ping., J., Seidelmann, P.K., Tholen, D.J., Thomas, P.C., and Williams, I.P., "Report of the IAU Working Group on Cartographic Coordinates and Rotational Elements: 2015," Celestial Mechanics and Dynamical Astronomy 130, Article number 22 (2018). DOI: https://doi.org/10.1007/s10569-017-9805-5 [2] Archinal, B.A., Acton, C.H., Conrad, A., Duxbury, T., Hestroffer, D., Hilton, J.L., Jorda, L., Kirk, R.L., Klinoner, Margot, J.-L., S.A., Meech, K., Oberst, Paganelli, F., J., Ping., J., Seidelmann, P.K., Stark, A., Tholen, Wang, Y., and Williams, I.P., "Correction to: Report of the IAU Working Group on Cartographic Coordinates and Rotational Elements: 2015." [3] Archinal, B.A., A'Hearn, M.F., Bowell, E., Conrad, A., Consolmagno, G.J., Courtin, R., Fukushima, T., Hestroffer, D., Hilton, J.L., Krasinsky, G.A., Neumann, G., Oberst, J., Seidelmann, P.K., Stooke, P., Tholen, D.J., Thomas, P.C., and Williams, I.P. "Report of the IAU Working Group on Cartographic Coordinates and Rotational Elements: 2009." [4] Archinal, B.A., A'Hearn, M.F., Conrad, A., Consolmagno, G.J., Courtin, R., Fukushima, T., Hestroffer, D., Hilton, J.L., Krasinsky, G.A., Neumann, G., Oberst, J., Seidelmann, P.K., Stooke, P., Tholen, D.J., Thomas, P.C., and Williams, I.P. "Erratum to: Reports of the IAU Working Group on Cartographic Coordinates and Rotational Elements: 2006 & 2009." [5] Seidelmann, P.K., Archinal, B.A., A'Hearn, M.F., Conrad, A., Consolmagno, G.J., Hestroffer, D., Hilton, J.L., Krasinsky, G.A., Neumann, G., Oberst, J., Stooke, P., Tedesco, E.F., Tholen, D.J., and Thomas, P.C. "Report of the IAU/IAG Working Group on Cartographic Coordinates and Rotational Elements: 2006." [6] Duxbury, Thomas C. (2001). "IAU/IAG 2000 Mars Cartographic Conventions," presentation to the Mars Express Data Archive Working Group, Dec. 14, 2001. [7] Russell, C.T. and Luhmann, J.G. (1990). "Earth: Magnetic Field and Magnetosphere." . Originally published in "Encyclopedia of Planetary Sciences," J.H. Shirley and R.W. Fainbridge, eds. Chapman and Hall, New York, pp 208-211. [8] Russell, C.T. (1971). "Geophysical Coordinate Transformations," Cosmic Electrodynamics 2 184-186. NAIF document 181.0. [9] ESA/ESTEC Space Environment Information System (SPENVIS) (2003). Web page: "Dipole approximations of the geomagnetic field." . [10] Davies, M.E., Abalakin, V.K., Bursa, M., Hunt, G.E., and Lieske, J.H. (1989). "Report of the IAU/IAG/COSPAR Working Group on Cartographic Coordinates and Rotational Elements of the Planets and Satellites: 1988," Celestial Mechanics and Dynamical Astronomy, v.46, no.2, pp. 187-204. [11] International Association of Geomagnetism and Aeronomy Web page: "International Geomagnetic Reference Field." Discussion URL: http://www.ngdc.noaa.gov/IAGA/vmod/igrf.html Coefficients URL: https://www.ngdc.noaa.gov/IAGA/vmod/coeffs/igrf13coeffs.txt [12] Email communication from Dr. Brent Archinal (IAU WGCCRE Chair, USGS): "Re: Shape of comet Hartley 2." Dated December 22, 2022. [13] Seidelmann, P.K., Archinal, B.A., A'Hearn, M.F., Cruikshank, D.P., Hilton, J.L., Keller, H.U., Oberst, J., Simon, J.L., Stooke, P., Tholen, D.J., and Thomas, P.C. "Report of the IAU/IAG Working Group on Cartographic Coordinates and Rotational Elements of the Planets and Satellites: 2003," Unpublished. Most values are from [1]. All exceptions are commented where they occur in this file. The exceptions are: -- Phobos prime meridian constants are from [2]. -- Lunar orientation data are from [3]. -- Earth orientation data are from [3]. -- North geomagnetic centered dipole values were computed by Nat Bachman from the 13th generation IGRF. The data source was [11]. "Old values" listed are from the SPICE PCK file pck00010.tpc dated October 21, 2011. Most of these values came from the 2009 IAU report [3]. Explanatory Notes -------------------------------------------------------- This file, which is logically part of the SPICE P-kernel, contains constants used to model the orientation, size and shape of the Sun, planets, natural satellites, and selected comets and asteroids. The orientation models express the direction of the pole and location of the prime meridian of a body as a function of time. The size/shape models ("shape models" for short) represent all bodies as ellipsoids, using two equatorial radii and a polar radius. Spheroids and spheres are obtained when two or all three radii are equal. The SPICE Toolkit routines that use this file are documented in the SPICE "Required Reading" file pck.req. They are also documented in the "PCK" SPICE tutorial, which is available on the NAIF web site. File Format A terse description of the PCK file format is given here. See the SPICE "Required Reading" files pck.req and kernel.req for a detailed explanation of the SPICE text kernel file format. The files pck.req and kernel.req are included in the documentation provided with the SPICE Toolkit. The file starts out with the ``ID word'' string KPL/PCK This string identifies the file as a text kernel containing PCK data. This file consists of a series of comment blocks and data blocks. Comment blocks, which contain free-form descriptive or explanatory text, are preceded by a \begintext token. Data blocks follow a \begindata token. In order to be recognized, each of these tokens must be placed on a line by itself. The portion of the file preceding the first data block is treated as a comment block; it doesn't require an initial \begintext token. This file identifies data using a series of KEYWORD = VALUE assignments. The left hand side of each assignment is a "kernel variable" name; the right hand side is an associated value or list of values. SPICE kernel pool access routines (see kernel.req) enable other SPICE routines and user applications to retrieve the set of values associated with each kernel variable name. Kernel variable names are case-sensitive and are limited to 32 characters in length. Numeric values may be integer or floating point. String values are normally limited to 80 characters in length; however, SPICE provides a mechanism for identifying longer, "continued" strings. See the SPICE routine STPOOL for details. String values are single quoted. When the right hand side of an assignment is a list of values, the list items may be separated by commas or simply by blanks. The list must be bracketed by parentheses. Example: BODY399_RADII = ( 6378.1366 6378.1366 6356.7519 ) Any blanks preceding or following keyword names, values and equal signs are ignored. Assignments may be spread over multiple lines, for example: BODY399_RADII = ( 6378.1366 6378.1366 6356.7519 ) This file may contain blank lines anywhere. Non-printing characters including TAB should not be present in the file: the presence of such characters may cause formatting errors when the file is viewed. Time systems and reference frames The 2015 IAU Working Group Report [1] states the time scale used as the independent variable for the rotation formulas is Barycentric Dynamical Time (TDB) and that the epoch of variable quantities is J2000 TDB (2000 Jan 1 12:00:00 TDB, Julian ephemeris date 2451545.0 TDB). Throughout SPICE documentation and in this file, we use the names "J2000 TDB" and "J2000" for this epoch. The name "J2000.0" is equivalent. SPICE documentation refers to the time system used in this file as either "ET" or "TDB." SPICE software makes no distinction between TDB and the time system associated with the independent variable of the JPL planetary ephemerides T_eph. The inertial reference frame used for the rotational elements in this file is identified by [1] as the ICRF (International Celestial Reference Frame). The SPICE PCK software that reads this file uses the label "J2000" to refer to the ICRF; this is actually a mislabeling which has been retained in the interest of backward compatibility. Using data from this file, by means of calls to the SPICE frame transformation routines, will actually compute orientation relative to the ICRF. The difference between the J2000 frame and the ICRF is on the order of 100 milliarcseconds and is well below the accuracy level of the formulas in this file. Orientation models All of the complete orientation models use three Euler angles to describe the orientation of the coordinate axes of the "Body Equator and Prime Meridian" system with respect to an inertial system. By default, the inertial system is the ICRF (labeled as "J2000"), but other inertial frames can be specified in the file. See the PCK Required Reading for details. The first two angles, in order, are the ICRF right ascension and declination (henceforth RA and DEC) of the north pole of a body as a function of time. The third angle is the prime meridian location (represented by "W"), which is expressed as a rotation about the north pole, and is also a function of time. For each body, the expressions for the north pole's right ascension and declination, as well as prime meridian location, are sums (as far as the models that appear in this file are concerned) of quadratic polynomials and trigonometric polynomials, where the independent variable is time. In this file, the time arguments in expressions always refer to Barycentric Dynamical Time (TDB), measured in centuries or days past a reference epoch. By default, the reference epoch is the J2000 epoch, which is Julian ephemeris date 2451545.0 (2000 Jan 1 12:00:00 TDB), but other epochs can be specified in the file. See the PCK Required Reading for details. Orientation models for satellites and some planets (including Jupiter) involve both polynomial terms and trigonometric terms. The arguments of the trigonometric terms are linear or quadratic polynomials. In this file, we call the arguments of these trigonometric terms "nutation precession angles" or "phase angles." Example: 2015 IAU Model for orientation of Jupiter. Note that these values are used as an example only; see the data area below for current values. Right ascension --------------- alpha = 268.056595 - 0.006499 T + 0.000117 sin(Ja) 0 + 0.000938 sin(Jb) + 0.001432 sin(Jc) + 0.000030 sin(Jd) + 0.002150 sin(Je) Declination ----------- delta = 64.495303 + 0.002413 T + 0.000050 cos(Ja) 0 + 0.000404 cos(Jb) + 0.000617 cos(Jc) - 0.000013 cos(Jd) + 0.000926 cos(Je) Prime meridian -------------- W = 284.95 + 870.5366420 d Here T represents centuries past J2000 ( TDB ), d represents days past J2000 ( TDB ). Ja-Je are nutation precession angles. In this file, the polynomials' coefficients above are assigned to kernel variable names (left-hand-side symbols) as follows BODY599_POLE_RA = ( 268.056595 -0.006499 0. ) BODY599_POLE_DEC = ( 64.495303 0.002413 0. ) BODY599_PM = ( 284.95 870.5360000 0. ) and the trigonometric polynomials' coefficients are assigned as follows BODY599_NUT_PREC_RA = ( 0. 0. 0. 0. 0. 0. 0. 0. 0. 0. 0.000117 0.000938 0.001432 0.000030 0.002150 ) BODY599_NUT_PREC_DEC = ( 0. 0. 0. 0. 0. 0. 0. 0. 0. 0. 0.000050 0.000404 0.000617 -0.000013 0.000926 ) BODY599_NUT_PREC_PM = ( 0. 0. 0. 0. 0. 0. 0. 0. 0. 0. 0.0 0.0 0.0 0.0 0.0 ) Note the number "599"; this is the NAIF ID code for Jupiter. In this file, the polynomial expressions for the nutation precession angles are listed along with the planet's RA, DEC, and prime meridian terms. Below are the 2006 IAU nutation precession angles for the Jupiter system. J1 = 73.32 + 91472.9 T J2 = 24.62 + 45137.2 T J3 = 283.90 + 4850.7 T J4 = 355.80 + 1191.3 T J5 = 119.90 + 262.1 T J6 = 229.80 + 64.3 T J7 = 352.25 + 2382.6 T J8 = 113.35 + 6070.0 T J9 = 146.64 + 182945.8 T J10 = 49.24 + 90274.4 T Ja = 99.360714 + 4850.4046 T Jb = 175.895369 + 1191.9605 T Jc = 300.323162 + 262.5475 T Jd = 114.012305 + 6070.2476 T Je = 49.511251 + 64.3000 T Here T represents centuries past J2000 ( TDB ) J1-J10 and Ja-Je are the nutation precession angles. The angles J9 and J10 are equal to 2*J1 and 2*J2, respectively. Angles J9 and J10 are not present in [1]; they have been added to fit the terms 2*J1 and 2*J2, which appear in the orientation models of several satellites, into a form that can be accepted by the PCK system. The assignment of the nutation precession angles for the Jupiter system is as follows: BODY5_NUT_PREC_ANGLES = ( 73.32 91472.9 24.62 45137.2 283.90 4850.7 355.80 1191.3 119.90 262.1 229.80 64.3 352.25 2382.6 113.35 6070.0 146.64 182945.8 49.24 90274.4 99.360714 4850.4046 175.895369 1191.9605 300.323162 262.5475 114.012305 6070.2476 49.511251 64.3000 ) You'll see an additional symbol grouped with the ones listed above; it is BODY599_LONG_AXIS This is a deprecated feature; see the note on "Prime meridian offsets" under "Known Limitations and Caveats" above. The pattern of the formulas for satellite orientation is similar to that for Jupiter. Example: 2006 IAU values for Io. Again, these values are used as an example only; see the data area below for current values. Right ascension --------------- alpha = 268.05 - 0.009 T + 0.094 sin(J3) + 0.024 sin(J4) 0 Declination ----------- delta = 64.50 + 0.003 T + 0.040 cos(J3) + 0.011 cos(J4) 0 Prime meridian -------------- W = 200.39 + 203.4889538 d - 0.085 sin(J3) - 0.022 sin(J4) d represents days past J2000. J3 and J4 are nutation precession angles. The polynomial terms are assigned to symbols by the statements BODY501_POLE_RA = ( 268.05 -0.009 0. ) BODY501_POLE_DEC = ( 64.50 0.003 0. ) BODY501_PM = ( 200.39 203.4889538 0. ) The coefficients of the trigonometric terms are assigned to symbols by the statements BODY501_NUT_PREC_RA = ( 0. 0. 0.094 0.024 ) BODY501_NUT_PREC_DEC = ( 0. 0. 0.040 0.011 ) BODY501_NUT_PREC_PM = ( 0. 0. -0.085 -0.022 ) 501 is the NAIF ID code for Io. SPICE software expects the models for satellite orientation to follow the form of the model shown here: the polynomial portions of the RA, DEC, and W expressions are expected to be quadratic, the trigonometric terms for RA and W (satellite prime meridian) are expected to be linear combinations of sines of nutation precession angles, the trigonometric terms for DEC are expected to be linear combinations of cosines of nutation precession angles, and the polynomials for the nutation precession angles themselves are expected to be linear or quadratic. Eventually, the software will handle more complex expressions, we expect. Shape models There is only one kind of shape model supported by the SPICE Toolkit software at present: the triaxial ellipsoid. The 2015 IAU report [1] does not use any other models, except in the case of Mars, where separate values are given for the north and south polar radii. In this file, we provide as a datum the mean Mars polar radius provided by [1]. The North and South values are included as comments. For each body, three radii are listed: The first number is the largest equatorial radius, the second number is the smaller equatorial radius, and the third is the polar radius. Example: Radii of the Earth. BODY399_RADII = ( 6378.1366 6378.1366 6356.7519 ) Body Numbers and Names -------------------------------------------------------- The following NAIF body ID codes and body names appear in this file. See the NAIF IDs Required Reading file naif_ids.req for a detailed discussion and a complete list of ID codes and names. 1 Mercury barycenter 2 Venus barycenter 3 Earth barycenter 4 Mars barycenter 5 Jupiter barycenter 6 Saturn barycenter 7 Uranus barycenter 8 Neptune barycenter 9 Pluto barycenter 10 Sun 199 Mercury 299 Venus 399 Earth 301 Moon 499 Mars 401 Phobos 402 Deimos 599 Jupiter 501 Io 502 Europa 503 Ganymede 504 Callisto 505 Amalthea 506 Himalia 507 Elara 508 Pasiphae 509 Sinope 510 Lysithea 511 Carme 512 Ananke 513 Leda 514 Thebe 515 Adrastea 516 Metis 699 Saturn 601 Mimas 602 Enceladus 603 Tethys 604 Dione 605 Rhea 606 Titan 607 Hyperion 608 Iapetus 609 Phoebe 610 Janus 611 Epimetheus 612 Helene 613 Telesto 614 Calypso 615 Atlas 616 Prometheus 617 Pandora 618 Pan 632 Methone 633 Pallene 634 Polydeuces 635 Daphnis 649 Anthe 653 Aegaeon 799 Uranus 701 Ariel 702 Umbriel 703 Titania 704 Oberon 705 Miranda 706 Cordelia 707 Ophelia 708 Bianca 709 Cressida 710 Desdemona 711 Juliet 712 Portia 713 Rosalind 714 Belinda 715 Puck 899 Neptune 801 Triton 802 Nereid 803 Naiad 804 Thalassa 805 Despina 806 Galatea 807 Larissa 808 Proteus 999 Pluto 901 Charon 1000005 Comet 19P/Borrelly 1000012 Comet 67P/Churyumov-Gerasimenko 1000036 Comet Halley 1000041 Comet Hartley 2 1000093 Comet 9P/Tempel 1 1000107 Comet 81P/Wild 2 2000001 Asteroid Ceres 2000002 Asteroid Pallas 2000016 Asteroid Psyche 2000004 Asteroid Vesta 2000021 Asteroid Lutetia 2000052 Asteroid 52 Europa 2000216 Asteroid Kleopatra 2000253 Asteroid Mathilde 2000433 Asteroid Eros 2000511 Asteroid Davida 2002867 Asteroid Steins 2004179 Asteroid Toutatis 2025143 Asteroid Itokawa 2431010 Asteroid Ida 9511010 Asteroid Gaspra Orientation Constants for the Sun and Planets -------------------------------------------------------- Sun Old values: Values are unchanged in the 2015 IAU report. Current values: \begindata BODY10_POLE_RA = ( 286.13 0. 0. ) BODY10_POLE_DEC = ( 63.87 0. 0. ) BODY10_PM = ( 84.176 14.18440 0. ) BODY10_LONG_AXIS = ( 0. ) \begintext Mercury Old values: Values are from the 2009 IAU report. body199_pole_ra = ( 281.0097 -0.0328 0. ) body199_pole_dec = ( 61.4143 -0.0049 0. ) body199_pm = ( 329.5469 6.1385025 0. ) body199_long_axis = ( 0. ) body199_nut_prec_ra = ( 0. 0. 0. 0. 0. ) body199_nut_prec_dec = ( 0. 0. 0. 0. 0. ) body199_nut_prec_pm = ( 0.00993822 -0.00104581 -0.00010280 -0.00002364 -0.00000532 ) Current values: \begindata BODY199_POLE_RA = ( 281.0103 -0.0328 0. ) BODY199_POLE_DEC = ( 61.4155 -0.0049 0. ) BODY199_PM = ( 329.5988 6.1385108 0. ) BODY199_LONG_AXIS = ( 0. ) BODY199_NUT_PREC_RA = ( 0. 0. 0. 0. 0. ) BODY199_NUT_PREC_DEC = ( 0. 0. 0. 0. 0. ) BODY199_NUT_PREC_PM = ( 0.01067257 -0.00112309 -0.00011040 -0.00002539 -0.00000571 ) \begintext The linear coefficients have been scaled up from degrees/day to degrees/century, because the SPICELIB PCK reader expects these units. The original constants were: 174.7910857 4.092335 349.5821714 8.184670 164.3732571 12.277005 339.1643429 16.369340 153.9554286 20.461675 \begindata BODY1_NUT_PREC_ANGLES = ( 174.7910857 0.14947253587500003E+06 349.5821714 0.29894507175000006E+06 164.3732571 0.44841760762500006E+06 339.1643429 0.59789014350000012E+06 153.9554286 0.74736267937499995E+06 ) \begintext Venus Old values: Values are unchanged in the 2015 IAU report. Current values: \begindata BODY299_POLE_RA = ( 272.76 0. 0. ) BODY299_POLE_DEC = ( 67.16 0. 0. ) BODY299_PM = ( 160.20 -1.4813688 0. ) BODY299_LONG_AXIS = ( 0. ) \begintext Earth Old values: The values shown below are those from the 2009 IAU report. The 2015 report does not provide orientation data for the Earth or Moon. \begindata BODY399_POLE_RA = ( 0. -0.641 0. ) BODY399_POLE_DEC = ( 90. -0.557 0. ) BODY399_PM = ( 190.147 360.9856235 0. ) BODY399_LONG_AXIS = ( 0. ) \begintext Nutation precession angles for the Earth-Moon system: The linear coefficients have been scaled up from degrees/day to degrees/century, because the SPICELIB PCK reader expects these units. The original constants were: 125.045D0 -0.0529921D0 250.089D0 -0.1059842D0 260.008D0 13.0120009D0 176.625D0 13.3407154D0 357.529D0 0.9856003D0 311.589D0 26.4057084D0 134.963D0 13.0649930D0 276.617D0 0.3287146D0 34.226D0 1.7484877D0 15.134D0 -0.1589763D0 119.743D0 0.0036096D0 239.961D0 0.1643573D0 25.053D0 12.9590088D0 \begindata BODY3_NUT_PREC_ANGLES = ( 125.045 -1935.5364525000 250.089 -3871.0729050000 260.008 475263.3328725000 176.625 487269.6299850000 357.529 35999.0509575000 311.589 964468.4993100000 134.963 477198.8693250000 276.617 12006.3007650000 34.226 63863.5132425000 15.134 -5806.6093575000 119.743 131.8406400000 239.961 6003.1503825000 25.053 473327.7964200000 ) \begintext North geomagnetic centered dipole: The north dipole location is time-varying. The values shown below, taken from [9], represent a discrete sampling of the north dipole location from 1945 to 2000. The terms DGRF and IGRF refer to, respectively, "Definitive Geomagnetic Reference Field" and "International Geomagnetic Reference Field." See references [9] and [11] for details. Coordinates are planetocentric. Data source Lat Lon ----------- ----- ------ DGRF 1945 78.47 291.47 DGRF 1950 78.47 291.15 DGRF 1955 78.46 290.84 DGRF 1960 78.51 290.53 DGRF 1965 78.53 290.15 DGRF 1970 78.59 289.82 DGRF 1975 78.69 289.53 DGRF 1980 78.81 289.24 DGRF 1985 78.97 289.10 DGRF 1990 79.13 288.89 IGRF 1995 79.30 288.59 IGRF 2000 79.54 288.43 Original values: Values are from [8]. Note the year of publication was 1971. body399_mag_north_pole_lon = ( -69.761 ) body399_mag_north_pole_lat = ( 78.565 ) Previous values: body399_n_geomag_ctr_dipole_lon = ( 287.62 ) body399_n_geomag_ctr_dipole_lat = ( 80.13 ) Current values: Values are given for the epoch 2023.0 and were derived by Nat Bachman from constants taken from IGRF-13. See [11]. \begindata BODY399_N_GEOMAG_CTR_DIPOLE_LON = ( 287.34 ) BODY399_N_GEOMAG_CTR_DIPOLE_LAT = ( 80.74 ) \begintext Mars Old values: Values are from the 2009 IAU report. body499_pole_ra = ( 317.68143 -0.1061 0. ) body499_pole_dec = ( 52.88650 -0.0609 0. ) body499_pm = ( 176.630 350.89198226 0. ) body499_long_axis = ( 252. ) Below, the linear terms are scaled by 36525.0: -0.4357640000000000 --> -15916.28010000000 1128.409670000000 --> 41215163.19675000 -1.8151000000000000E-02 --> -662.9652750000000 We also introduce a fourth nutation precession angle, which is the pi/2-complement of the third angle. This angle is used in computing the prime meridian location for Deimos. See the discussion of this angle below in the section containing orientation constants for Deimos. body4_nut_prec_angles = ( 169.51 -15916.2801 192.93 41215163.19675 53.47 -662.965275 36.53 662.965275 ) Current values: \begindata BODY499_POLE_RA = ( 317.269202 -0.10927547 0. ) BODY499_POLE_DEC = ( 54.432516 -0.05827105 0. ) BODY499_PM = ( 176.049863 +350.891982443297 0. ) BODY499_NUT_PREC_RA = ( 0 0 0 0 0 0 0 0 0 0 0.000068 0.000238 0.000052 0.000009 0.419057 ) BODY499_NUT_PREC_DEC = ( 0 0 0 0 0 0 0 0 0 0 0 0 0 0 0 0.000051 0.000141 0.000031 0.000005 1.591274 ) BODY499_NUT_PREC_PM = ( 0 0 0 0 0 0 0 0 0 0 0 0 0 0 0 0 0 0 0 0 0.000145 0.000157 0.000040 0.000001 0.000001 0.584542 ) \begintext SPICE support for quadratic phase angle polynomials was introduced in the N0067 Toolkit version. Older Toolkits cannot use the constants for the Mars phase angles given by [1]. In this file, the polynomial for the M5 phase angle has been truncated to first order. Only the model of the orientation of Phobos is degraded by this change. See the SPICE server at https://naif.jpl.nasa.gov/naif/ for the file pck00011.tpc, which has the original model given by [1]. \begindata BODY4_NUT_PREC_ANGLES = ( 190.72646643 15917.10818695 21.46892470 31834.27934054 332.86082793 19139.89694742 394.93256437 38280.79631835 189.63271560 41215158.18420050 121.46893664 660.22803474 231.05028581 660.99123540 251.37314025 1320.50145245 217.98635955 38279.96125550 196.19729402 19139.83628608 198.991226 19139.4819985 226.292679 38280.8511281 249.663391 57420.7251593 266.183510 76560.6367950 79.398797 0.5042615 122.433576 19139.9407476 43.058401 38280.8753272 57.663379 57420.7517205 79.476401 76560.6495004 166.325722 0.5042615 129.071773 19140.0328244 36.352167 38281.0473591 56.668646 57420.9295360 67.364003 76560.2552215 104.792680 95700.4387578 95.391654 0.5042615 ) \begintext Jupiter Old values: Values are unchanged in the 2015 IAU report. Current values: The number of nutation precession angles is 15. The ninth and tenth are twice the first and second, respectively. The eleventh through fifteenth correspond to angles JA-JE in the 2015 IAU report. \begindata BODY599_POLE_RA = ( 268.056595 -0.006499 0. ) BODY599_POLE_DEC = ( 64.495303 0.002413 0. ) BODY599_PM = ( 284.95 870.5360000 0. ) BODY599_LONG_AXIS = ( 0. ) BODY599_NUT_PREC_RA = ( 0. 0. 0. 0. 0. 0. 0. 0. 0. 0. 0.000117 0.000938 0.001432 0.000030 0.002150 ) BODY599_NUT_PREC_DEC = ( 0. 0. 0. 0. 0. 0. 0. 0. 0. 0. 0.000050 0.000404 0.000617 -0.000013 0.000926 ) BODY599_NUT_PREC_PM = ( 0. 0. 0. 0. 0. 0. 0. 0. 0. 0. 0.0 0.0 0.0 0.0 0.0 ) BODY5_NUT_PREC_ANGLES = ( 73.32 91472.9 24.62 45137.2 283.90 4850.7 355.80 1191.3 119.90 262.1 229.80 64.3 352.25 2382.6 113.35 6070.0 146.64 182945.8 49.24 90274.4 99.360714 4850.4046 175.895369 1191.9605 300.323162 262.5475 114.012305 6070.2476 49.511251 64.3000 ) \begintext Saturn Old values: Values are unchanged in the 2015 IAU report. Current values: \begindata BODY699_POLE_RA = ( 40.589 -0.036 0. ) BODY699_POLE_DEC = ( 83.537 -0.004 0. ) BODY699_PM = ( 38.90 810.7939024 0. ) BODY699_LONG_AXIS = ( 0. ) \begintext The first six angles given here are the angles S1 through S6 from the 2015 IAU report; the seventh and eighth angles are 2*S1 and 2*S2, respectively. \begindata BODY6_NUT_PREC_ANGLES = ( 353.32 75706.7 28.72 75706.7 177.40 -36505.5 300.00 -7225.9 316.45 506.2 345.20 -1016.3 706.64 151413.4 57.44 151413.4 ) \begintext Uranus Old values: Values are unchanged in the 2015 IAU report. Current values: \begindata BODY799_POLE_RA = ( 257.311 0. 0. ) BODY799_POLE_DEC = ( -15.175 0. 0. ) BODY799_PM = ( 203.81 -501.1600928 0. ) BODY799_LONG_AXIS = ( 0. ) \begintext The first 16 angles given here are the angles U1 through U16 from the 2000 report; the 17th and 18th angles are 2*U11 and 2*U12, respectively. \begindata BODY7_NUT_PREC_ANGLES = ( 115.75 54991.87 141.69 41887.66 135.03 29927.35 61.77 25733.59 249.32 24471.46 43.86 22278.41 77.66 20289.42 157.36 16652.76 101.81 12872.63 138.64 8061.81 102.23 -2024.22 316.41 2863.96 304.01 -51.94 308.71 -93.17 340.82 -75.32 259.14 -504.81 204.46 -4048.44 632.82 5727.92 ) \begintext Neptune Old values are from the 2009 IAU report: body899_pole_ra = ( 299.36 0. 0. ) body899_pole_dec = ( 43.46 0. 0. ) body899_pm = ( 253.18 536.3128492 0. ) body899_long_axis = ( 0. ) body899_nut_prec_ra = ( 0.70 0. 0. 0. 0. 0. 0. 0. ) body899_nut_prec_dec = ( -0.51 0. 0. 0. 0. 0. 0. 0. ) body899_nut_prec_pm = ( -0.48 0. 0. 0. 0. 0. 0. 0. ) Current values: \begindata BODY899_POLE_RA = ( 299.36 0. 0. ) BODY899_POLE_DEC = ( 43.46 0. 0. ) BODY899_PM = ( 249.978 541.1397757 0. ) BODY899_LONG_AXIS = ( 0. ) BODY899_NUT_PREC_RA = ( 0.70 0. 0. 0. 0. 0. 0. 0. ) BODY899_NUT_PREC_DEC = ( -0.51 0. 0. 0. 0. 0. 0. 0. ) BODY899_NUT_PREC_PM = ( -0.48 0. 0. 0. 0. 0. 0. 0. ) \begintext The 2015 IAU report defines the nutation precession angles N, N1, N2, ... , N7 and also uses the multiples of N1 and N7 2*N1 and 2*N7, 3*N7, ..., 9*N7 In this file, we treat the angles and their multiples as separate angles. In the kernel variable BODY8_NUT_PREC_ANGLES the order of the angles is N, N1, N2, ... , N7, 2*N1, 2*N7, 3*N7, ..., 9*N7 Each angle is defined by a linear polynomial, so two consecutive array elements are allocated for each angle. The first term of each pair is the constant term, the second is the linear term. \begindata BODY8_NUT_PREC_ANGLES = ( 357.85 52.316 323.92 62606.6 220.51 55064.2 354.27 46564.5 75.31 26109.4 35.36 14325.4 142.61 2824.6 177.85 52.316 647.840 125213.200 355.700 104.632 533.550 156.948 711.400 209.264 889.250 261.580 1067.100 313.896 1244.950 366.212 1422.800 418.528 1600.650 470.844 ) \begintext Orientation Constants for the Dwarf Planet Pluto -------------------------------------------------------- Pluto Old values: Values are unchanged in the 2015 IAU report. Current values: \begindata BODY999_POLE_RA = ( 132.993 0. 0. ) BODY999_POLE_DEC = ( -6.163 0. 0. ) BODY999_PM = ( 302.695 56.3625225 0. ) BODY999_LONG_AXIS = ( 0. ) \begintext Orientation constants for the satellites -------------------------------------------------------- Satellites of Earth Old values: The values shown below are those from the 2009 IAU report. The 2015 report does not provide orientation data for the Earth or Moon. \begindata BODY301_POLE_RA = ( 269.9949 0.0031 0. ) BODY301_POLE_DEC = ( 66.5392 0.0130 0. ) BODY301_PM = ( 38.3213 13.17635815 -1.4D-12 ) BODY301_LONG_AXIS = ( 0. ) BODY301_NUT_PREC_RA = ( -3.8787 -0.1204 0.0700 -0.0172 0.0 0.0072 0.0 0.0 0.0 -0.0052 0.0 0.0 0.0043 ) BODY301_NUT_PREC_DEC = ( 1.5419 0.0239 -0.0278 0.0068 0.0 -0.0029 0.0009 0.0 0.0 0.0008 0.0 0.0 -0.0009 ) BODY301_NUT_PREC_PM = ( 3.5610 0.1208 -0.0642 0.0158 0.0252 -0.0066 -0.0047 -0.0046 0.0028 0.0052 0.0040 0.0019 -0.0044 ) \begintext Satellites of Mars Phobos Old values are from the 2009 IAU report. body401_pole_ra = ( 317.68 -0.108 0. ) body401_pole_dec = ( 52.90 -0.061 0. ) body401_pm = ( 35.06 1128.8445850 6.6443009930565219e-09 ) body401_long_axis = ( 0. ) body401_nut_prec_ra = ( 1.79 0. 0. 0. ) body401_nut_prec_dec = ( -1.08 0. 0. 0. ) body401_nut_prec_pm = ( -1.42 -0.78 0. 0. ) The quadratic prime meridian term is scaled by 1/36525**2: 8.864000000000000 ---> 6.6443009930565219E-09 Current values: Values from the 2015 IAU report [1] were corrected by [2], which is used as the source for the data below. The quadratic prime meridian term is scaled by 1/36525**2: 12.72192797000000000000 ---> 9.536137031212154e-09 \begindata BODY401_POLE_RA = ( 317.67071657 -0.10844326 0. ) BODY401_POLE_DEC = ( 52.88627266 -0.06134706 0. ) BODY401_PM = ( 35.18774440 1128.84475928 9.536137031212154e-09 ) BODY401_LONG_AXIS = ( 0. ) BODY401_NUT_PREC_RA = ( -1.78428399 0.02212824 -0.01028251 -0.00475595 ) BODY401_NUT_PREC_DEC = ( -1.07516537 0.00668626 -0.00648740 0.00281576 ) BODY401_NUT_PREC_PM = ( 1.42421769 -0.02273783 0.00410711 0.00631964 -1.143 ) \begintext Deimos Old values: Values are from the 2009 IAU report. The Deimos prime meridian expression from that report is: 2 W = 79.41 + 285.1618970 d - 0.520 T - 2.58 sin M 3 + 0.19 cos M . 3 At the present time, the PCK kernel software (the routine BODEUL in particular) cannot handle the cosine term directly, but we can represent it as 0.19 sin M 4 where M = 90.D0 - M 4 3 Therefore, the old nutation precession angle assignments for Phobos and Deimos contain four coefficients rather than three. The quadratic prime meridian term is scaled by 1/36525**2: -0.5200000000000000 ---> -3.8978300049519307E-10 body402_pole_ra = ( 316.65 -0.108 0. ) body402_pole_dec = ( 53.52 -0.061 0. ) body402_pm = ( 79.41 285.1618970 -3.897830d-10 ) body402_long_axis = ( 0. ) body402_nut_prec_ra = ( 0. 0. 2.98 0. ) body402_nut_prec_dec = ( 0. 0. -1.78 0. ) body402_nut_prec_pm = ( 0. 0. -2.58 0.19 ) New values: \begindata BODY402_POLE_RA = ( 316.65705808 -0.10518014 0. ) BODY402_POLE_DEC = ( 53.50992033 -0.05979094 0. ) BODY402_PM = ( 79.39932954 285.16188899 0. ) BODY402_LONG_AXIS = ( 0. ) BODY402_NUT_PREC_RA = ( 0 0 0 0 0 3.09217726 0.22980637 0.06418655 0.02533537 0.00778695 ) BODY402_NUT_PREC_DEC = ( 0 0 0 0 0 1.83936004 0.14325320 0.01911409 -0.01482590 0.00192430 ) BODY402_NUT_PREC_PM = ( 0 0 0 0 0 -2.73954829 -0.39968606 -0.06563259 -0.02912940 0.01699160 ) \begintext Satellites of Jupiter Io Old values: Values are unchanged in the 2015 IAU report. Current values: \begindata BODY501_POLE_RA = ( 268.05 -0.009 0. ) BODY501_POLE_DEC = ( 64.50 0.003 0. ) BODY501_PM = ( 200.39 203.4889538 0. ) BODY501_LONG_AXIS = ( 0. ) BODY501_NUT_PREC_RA = ( 0. 0. 0.094 0.024 ) BODY501_NUT_PREC_DEC = ( 0. 0. 0.040 0.011 ) BODY501_NUT_PREC_PM = ( 0. 0. -0.085 -0.022 ) \begintext Europa Old values: Values are unchanged in the 2015 IAU report. Current values: \begindata BODY502_POLE_RA = ( 268.08 -0.009 0. ) BODY502_POLE_DEC = ( 64.51 0.003 0. ) BODY502_PM = ( 36.022 101.3747235 0. ) BODY502_LONG_AXIS = ( 0. ) BODY502_NUT_PREC_RA = ( 0. 0. 0. 1.086 0.060 0.015 0.009 ) BODY502_NUT_PREC_DEC = ( 0. 0. 0. 0.468 0.026 0.007 0.002 ) BODY502_NUT_PREC_PM = ( 0. 0. 0. -0.980 -0.054 -0.014 -0.008 ) \begintext Ganymede Old values: Values are unchanged in the 2015 IAU report. Current values: \begindata BODY503_POLE_RA = ( 268.20 -0.009 0. ) BODY503_POLE_DEC = ( 64.57 0.003 0. ) BODY503_PM = ( 44.064 50.3176081 0. ) BODY503_LONG_AXIS = ( 0. ) BODY503_NUT_PREC_RA = ( 0. 0. 0. -0.037 0.431 0.091 ) BODY503_NUT_PREC_DEC = ( 0. 0. 0. -0.016 0.186 0.039 ) BODY503_NUT_PREC_PM = ( 0. 0. 0. 0.033 -0.389 -0.082 ) \begintext Callisto Old values: Values are unchanged in the 2015 IAU report. Current values: \begindata BODY504_POLE_RA = ( 268.72 -0.009 0. ) BODY504_POLE_DEC = ( 64.83 0.003 0. ) BODY504_PM = ( 259.51 21.5710715 0. ) BODY504_LONG_AXIS = ( 0. ) BODY504_NUT_PREC_RA = ( 0. 0. 0. 0. -0.068 0.590 0. 0.010 ) BODY504_NUT_PREC_DEC = ( 0. 0. 0. 0. -0.029 0.254 0. -0.004 ) BODY504_NUT_PREC_PM = ( 0. 0. 0. 0. 0.061 -0.533 0. -0.009 ) \begintext Amalthea Old values: Values are unchanged in the 2015 IAU report. Current values: \begindata BODY505_POLE_RA = ( 268.05 -0.009 0. ) BODY505_POLE_DEC = ( 64.49 0.003 0. ) BODY505_PM = ( 231.67 722.6314560 0. ) BODY505_LONG_AXIS = ( 0. ) BODY505_NUT_PREC_RA = ( -0.84 0. 0. 0. 0. 0. 0. 0. 0.01 0. ) BODY505_NUT_PREC_DEC = ( -0.36 0. 0. 0. 0. 0. 0. 0. 0. 0. ) BODY505_NUT_PREC_PM = ( 0.76 0. 0. 0. 0. 0. 0. 0. -0.01 0. ) \begintext Thebe Old values: Values are unchanged in the 2015 IAU report. Current values: \begindata BODY514_POLE_RA = ( 268.05 -0.009 0. ) BODY514_POLE_DEC = ( 64.49 0.003 0. ) BODY514_PM = ( 8.56 533.7004100 0. ) BODY514_LONG_AXIS = ( 0. ) BODY514_NUT_PREC_RA = ( 0. -2.11 0. 0. 0. 0. 0. 0. 0. 0.04 ) BODY514_NUT_PREC_DEC = ( 0. -0.91 0. 0. 0. 0. 0. 0. 0. 0.01 ) BODY514_NUT_PREC_PM = ( 0. 1.91 0. 0. 0. 0. 0. 0. 0. -0.04 ) \begintext Adrastea Old values: Values are unchanged in the 2015 IAU report. Current values: \begindata BODY515_POLE_RA = ( 268.05 -0.009 0. ) BODY515_POLE_DEC = ( 64.49 0.003 0. ) BODY515_PM = ( 33.29 1206.9986602 0. ) BODY515_LONG_AXIS = ( 0. ) \begintext Metis Old values: Values are unchanged in the 2015 IAU report. Current values: \begindata BODY516_POLE_RA = ( 268.05 -0.009 0. ) BODY516_POLE_DEC = ( 64.49 0.003 0. ) BODY516_PM = ( 346.09 1221.2547301 0. ) BODY516_LONG_AXIS = ( 0. ) \begintext Satellites of Saturn Mimas Old values: Values are unchanged in the 2015 IAU report. Current values: \begindata BODY601_POLE_RA = ( 40.66 -0.036 0. ) BODY601_POLE_DEC = ( 83.52 -0.004 0. ) BODY601_PM = ( 333.46 381.9945550 0. ) BODY601_LONG_AXIS = ( 0. ) BODY601_NUT_PREC_RA = ( 0. 0. 13.56 0. 0. 0. 0. 0. ) BODY601_NUT_PREC_DEC = ( 0. 0. -1.53 0. 0. 0. 0. 0. ) BODY601_NUT_PREC_PM = ( 0. 0. -13.48 0. -44.85 0. 0. 0. ) \begintext Enceladus Old values: Values are unchanged in the 2015 IAU report. Current values: \begindata BODY602_POLE_RA = ( 40.66 -0.036 0. ) BODY602_POLE_DEC = ( 83.52 -0.004 0. ) BODY602_PM = ( 6.32 262.7318996 0. ) BODY602_LONG_AXIS = ( 0. ) \begintext Tethys Old values: Values are unchanged in the 2015 IAU report. Current values: \begindata BODY603_POLE_RA = ( 40.66 -0.036 0. ) BODY603_POLE_DEC = ( 83.52 -0.004 0. ) BODY603_PM = ( 8.95 190.6979085 0. ) BODY603_LONG_AXIS = ( 0. ) BODY603_NUT_PREC_RA = ( 0. 0. 0. 9.66 0. 0. 0. 0. ) BODY603_NUT_PREC_DEC = ( 0. 0. 0. -1.09 0. 0. 0. 0. ) BODY603_NUT_PREC_PM = ( 0. 0. 0. -9.60 2.23 0. 0. 0. ) \begintext Dione Old values: Values are unchanged in the 2015 IAU report. Current values: \begindata BODY604_POLE_RA = ( 40.66 -0.036 0. ) BODY604_POLE_DEC = ( 83.52 -0.004 0. ) BODY604_PM = ( 357.6 131.5349316 0. ) BODY604_LONG_AXIS = ( 0. ) \begintext Rhea Old values: Values are unchanged in the 2015 IAU report. Current values: \begindata BODY605_POLE_RA = ( 40.38 -0.036 0. ) BODY605_POLE_DEC = ( 83.55 -0.004 0. ) BODY605_PM = ( 235.16 79.6900478 0. ) BODY605_LONG_AXIS = ( 0. ) BODY605_NUT_PREC_RA = ( 0. 0. 0. 0. 0. 3.10 0. 0. ) BODY605_NUT_PREC_DEC = ( 0. 0. 0. 0. 0. -0.35 0. 0. ) BODY605_NUT_PREC_PM = ( 0. 0. 0. 0. 0. -3.08 0. 0. ) \begintext Titan Old values: Values are unchanged in the 2015 IAU report. Current values: Note removal of dependence on the nutation precession angles. \begindata BODY606_POLE_RA = ( 39.4827 0. 0. ) BODY606_POLE_DEC = ( 83.4279 0. 0. ) BODY606_PM = ( 186.5855 22.5769768 0. ) BODY606_LONG_AXIS = ( 0. ) BODY606_NUT_PREC_RA = ( 0. 0. 0. 0. 0. 0. 0. 0 ) BODY606_NUT_PREC_DEC = ( 0. 0. 0. 0. 0. 0. 0. 0 ) BODY606_NUT_PREC_PM = ( 0. 0. 0. 0. 0. 0. 0. 0 ) \begintext Hyperion The IAU report does not give an orientation model for Hyperion. Hyperion's rotation is in chaotic and is not predictable for long periods. Iapetus Old values: Values are unchanged in the 2015 IAU report. Current values: \begindata BODY608_POLE_RA = ( 318.16 -3.949 0. ) BODY608_POLE_DEC = ( 75.03 -1.143 0. ) BODY608_PM = ( 355.2 4.5379572 0. ) BODY608_LONG_AXIS = ( 0. ) \begintext Phoebe Old values: Values are unchanged in the 2015 IAU report. Current values: \begindata BODY609_POLE_RA = ( 356.90 0. 0. ) BODY609_POLE_DEC = ( 77.80 0. 0. ) BODY609_PM = ( 178.58 931.639 0. ) BODY609_LONG_AXIS = ( 0. ) \begintext Janus Old values: Values are unchanged in the 2015 IAU report. Current values: \begindata 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. 0.023 ) BODY610_NUT_PREC_DEC = ( 0. -0.183 0. 0. 0. 0. 0. 0.001 ) BODY610_NUT_PREC_PM = ( 0. 1.613 0. 0. 0. 0. 0. -0.023 ) \begintext Epimetheus Old values: Values are unchanged in the 2015 IAU report. Current values: \begindata 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. 0.086 0. ) BODY611_NUT_PREC_DEC = ( -0.356 0. 0. 0. 0. 0. 0.005 0. ) BODY611_NUT_PREC_PM = ( 3.133 0. 0. 0. 0. 0. -0.086 0. ) \begintext Helene Old values: Values are unchanged in the 2015 IAU report. Current values: \begindata 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 Old values: Values are unchanged in the 2015 IAU report. Current values: \begindata 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 Old values: Values are unchanged in the 2015 IAU report. Current values: \begindata 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 Old values: Values are unchanged in the 2015 IAU report. Current values: \begindata 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 Old values: Values are unchanged in the 2015 IAU report. Current values: \begindata BODY616_POLE_RA = ( 40.58 -0.036 ) BODY616_POLE_DEC = ( 83.53 -0.004 ) BODY616_PM = ( 296.14 587.289000 ) BODY616_LONG_AXIS = ( 0. ) \begintext Pandora Old values: Values are unchanged in the 2015 IAU report. Current values: \begindata 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 Old values: Values are unchanged in the 2015 IAU report. Current values: \begindata 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 Satellites of Uranus Ariel Old values: Values are unchanged in the 2015 IAU report. Current values: \begindata BODY701_POLE_RA = ( 257.43 0. 0. ) BODY701_POLE_DEC = ( -15.10 0. 0. ) BODY701_PM = ( 156.22 -142.8356681 0. ) BODY701_LONG_AXIS = ( 0. ) BODY701_NUT_PREC_RA = ( 0. 0. 0. 0. 0. 0. 0. 0. 0. 0. 0. 0. 0.29 ) BODY701_NUT_PREC_DEC = ( 0. 0. 0. 0. 0. 0. 0. 0. 0. 0. 0. 0. 0.28 ) BODY701_NUT_PREC_PM = ( 0. 0. 0. 0. 0. 0. 0. 0. 0. 0. 0. 0.05 0.08 ) \begintext Umbriel Old values: Values are unchanged in the 2015 IAU report. \begindata BODY702_POLE_RA = ( 257.43 0. 0. ) BODY702_POLE_DEC = ( -15.10 0. 0. ) BODY702_PM = ( 108.05 -86.8688923 0. ) BODY702_LONG_AXIS = ( 0. ) BODY702_NUT_PREC_RA = ( 0. 0. 0. 0. 0. 0. 0. 0. 0. 0. 0. 0. 0. 0.21 ) BODY702_NUT_PREC_DEC = ( 0. 0. 0. 0. 0. 0. 0. 0. 0. 0. 0. 0. 0. 0.20 ) BODY702_NUT_PREC_PM = ( 0. 0. 0. 0. 0. 0. 0. 0. 0. 0. 0. -0.09 0. 0.06 ) \begintext Titania Old values: Values are unchanged in the 2015 IAU report. Current values: \begindata BODY703_POLE_RA = ( 257.43 0. 0. ) BODY703_POLE_DEC = ( -15.10 0. 0. ) BODY703_PM = ( 77.74 -41.3514316 0. ) BODY703_LONG_AXIS = ( 0. ) BODY703_NUT_PREC_RA = ( 0. 0. 0. 0. 0. 0. 0. 0. 0. 0. 0. 0. 0. 0. 0.29 ) BODY703_NUT_PREC_DEC = ( 0. 0. 0. 0. 0. 0. 0. 0. 0. 0. 0. 0. 0. 0. 0.28 ) BODY703_NUT_PREC_PM = ( 0. 0. 0. 0. 0. 0. 0. 0. 0. 0. 0. 0. 0. 0. 0.08 ) \begintext Oberon Old values: Values are unchanged in the 2015 IAU report. Current values: \begindata BODY704_POLE_RA = ( 257.43 0. 0. ) BODY704_POLE_DEC = ( -15.10 0. 0. ) BODY704_PM = ( 6.77 -26.7394932 0. ) BODY704_LONG_AXIS = ( 0. ) BODY704_NUT_PREC_RA = ( 0. 0. 0. 0. 0. 0. 0. 0. 0. 0. 0. 0. 0. 0. 0. 0.16 ) BODY704_NUT_PREC_DEC = ( 0. 0. 0. 0. 0. 0. 0. 0. 0. 0. 0. 0. 0. 0. 0. 0.16 ) BODY704_NUT_PREC_PM = ( 0. 0. 0. 0. 0. 0. 0. 0. 0. 0. 0. 0. 0. 0. 0. 0.04 ) \begintext Miranda Old values: Values are unchanged in the 2015 IAU report. Current values: \begindata BODY705_POLE_RA = ( 257.43 0. 0. ) BODY705_POLE_DEC = ( -15.08 0. 0. ) BODY705_PM = ( 30.70 -254.6906892 0. ) BODY705_LONG_AXIS = ( 0. ) BODY705_NUT_PREC_RA = ( 0. 0. 0. 0. 0. 0. 0. 0. 0. 0. 4.41 0. 0. 0. 0. 0. -0.04 0. ) BODY705_NUT_PREC_DEC = ( 0. 0. 0. 0. 0. 0. 0. 0. 0. 0. 4.25 0. 0. 0. 0. 0. -0.02 0. ) BODY705_NUT_PREC_PM = ( 0. 0. 0. 0. 0. 0. 0. 0. 0. 0. 1.15 -1.27 0. 0. 0. 0. -0.09 0.15 ) \begintext Cordelia Old values: Values are unchanged in the 2015 IAU report. Current values: \begindata BODY706_POLE_RA = ( 257.31 0. 0. ) BODY706_POLE_DEC = ( -15.18 0. 0. ) BODY706_PM = ( 127.69 -1074.5205730 0. ) BODY706_LONG_AXIS = ( 0. ) BODY706_NUT_PREC_RA = ( -0.15 0. 0. 0. 0. 0. 0. 0. 0. 0. 0. 0. 0. 0. 0. 0. 0. 0. ) BODY706_NUT_PREC_DEC = ( 0.14 0. 0. 0. 0. 0. 0. 0. 0. 0. 0. 0. 0. 0. 0. 0. 0. 0. ) BODY706_NUT_PREC_PM = ( -0.04 0. 0. 0. 0. 0. 0. 0. 0. 0. 0. 0. 0. 0. 0. 0. 0. 0. ) \begintext Ophelia Old values: Values are unchanged in the 2015 IAU report. Current values: \begindata BODY707_POLE_RA = ( 257.31 0. 0. ) BODY707_POLE_DEC = ( -15.18 0. 0. ) BODY707_PM = ( 130.35 -956.4068150 0. ) BODY707_LONG_AXIS = ( 0. ) BODY707_NUT_PREC_RA = ( 0. -0.09 0. 0. 0. 0. 0. 0. 0. 0. 0. 0. 0. 0. 0. 0. 0. 0. ) BODY707_NUT_PREC_DEC = ( 0. 0.09 0. 0. 0. 0. 0. 0. 0. 0. 0. 0. 0. 0. 0. 0. 0. 0. ) BODY707_NUT_PREC_PM = ( 0. -0.03 0. 0. 0. 0. 0. 0. 0. 0. 0. 0. 0. 0. 0. 0. 0. 0. ) \begintext Bianca Old values: Values are unchanged in the 2015 IAU report. Current values: \begindata BODY708_POLE_RA = ( 257.31 0. 0. ) BODY708_POLE_DEC = ( -15.18 0. 0. ) BODY708_PM = ( 105.46 -828.3914760 0. ) BODY708_LONG_AXIS = ( 0. ) BODY708_NUT_PREC_RA = ( 0. 0. -0.16 0. 0. 0. 0. 0. 0. 0. 0. 0. 0. 0. 0. 0. 0. 0. ) BODY708_NUT_PREC_DEC = ( 0. 0. 0.16 0. 0. 0. 0. 0. 0. 0. 0. 0. 0. 0. 0. 0. 0. 0. ) BODY708_NUT_PREC_PM = ( 0. 0. -0.04 0. 0. 0. 0. 0. 0. 0. 0. 0. 0. 0. 0. 0. 0. 0. ) \begintext Cressida Old values: Values are unchanged in the 2015 IAU report. Current values: \begindata BODY709_POLE_RA = ( 257.31 0. 0. ) BODY709_POLE_DEC = ( -15.18 0. 0. ) BODY709_PM = ( 59.16 -776.5816320 0. ) BODY709_LONG_AXIS = ( 0. ) BODY709_NUT_PREC_RA = ( 0. 0. 0. -0.04 0. 0. 0. 0. 0. 0. 0. 0. 0. 0. 0. 0. 0. 0. ) BODY709_NUT_PREC_DEC = ( 0. 0. 0. 0.04 0. 0. 0. 0. 0. 0. 0. 0. 0. 0. 0. 0. 0. 0. ) BODY709_NUT_PREC_PM = ( 0. 0. 0. -0.01 0. 0. 0. 0. 0. 0. 0. 0. 0. 0. 0. 0. 0. 0. ) \begintext Desdemona Old values: Values are unchanged in the 2015 IAU report. Current values: \begindata BODY710_POLE_RA = ( 257.31 0. 0. ) BODY710_POLE_DEC = ( -15.18 0. 0. ) BODY710_PM = ( 95.08 -760.0531690 0. ) BODY710_LONG_AXIS = ( 0. ) BODY710_NUT_PREC_RA = ( 0. 0. 0. 0. -0.17 0. 0. 0. 0. 0. 0. 0. 0. 0. 0. 0. 0. 0. ) BODY710_NUT_PREC_DEC = ( 0. 0. 0. 0. 0.16 0. 0. 0. 0. 0. 0. 0. 0. 0. 0. 0. 0. 0. ) BODY710_NUT_PREC_PM = ( 0. 0. 0. 0. -0.04 0. 0. 0. 0. 0. 0. 0. 0. 0. 0. 0. 0. 0. ) \begintext Juliet Old values: Values are unchanged in the 2015 IAU report. Current values: \begindata BODY711_POLE_RA = ( 257.31 0. 0. ) BODY711_POLE_DEC = ( -15.18 0. 0. ) BODY711_PM = ( 302.56 -730.1253660 0. ) BODY711_LONG_AXIS = ( 0. ) BODY711_NUT_PREC_RA = ( 0. 0. 0. 0. 0. -0.06 0. 0. 0. 0. 0. 0. 0. 0. 0. 0. 0. 0. ) BODY711_NUT_PREC_DEC = ( 0. 0. 0. 0. 0. 0.06 0. 0. 0. 0. 0. 0. 0. 0. 0. 0. 0. 0. ) BODY711_NUT_PREC_PM = ( 0. 0. 0. 0. 0. -0.02 0. 0. 0. 0. 0. 0. 0. 0. 0. 0. 0. 0. ) \begintext Portia Old values: Values are unchanged in the 2015 IAU report. Current values: \begindata BODY712_POLE_RA = ( 257.31 0. 0. ) BODY712_POLE_DEC = ( -15.18 0. 0. ) BODY712_PM = ( 25.03 -701.4865870 0. ) BODY712_LONG_AXIS = ( 0. ) BODY712_NUT_PREC_RA = ( 0. 0. 0. 0. 0. 0. -0.09 0. 0. 0. 0. 0. 0. 0. 0. 0. 0. 0. ) BODY712_NUT_PREC_DEC = ( 0. 0. 0. 0. 0. 0. 0.09 0. 0. 0. 0. 0. 0. 0. 0. 0. 0. 0. ) BODY712_NUT_PREC_PM = ( 0. 0. 0. 0. 0. 0. -0.02 0. 0. 0. 0. 0. 0. 0. 0. 0. 0. 0. ) \begintext Rosalind Old values: Values are unchanged in the 2015 IAU report. Current values: \begindata BODY713_POLE_RA = ( 257.31 0. 0. ) BODY713_POLE_DEC = ( -15.18 0. 0. ) BODY713_PM = ( 314.90 -644.6311260 0. ) BODY713_LONG_AXIS = ( 0. ) BODY713_NUT_PREC_RA = ( 0. 0. 0. 0. 0. 0. 0. -0.29 0. 0. 0. 0. 0. 0. 0. 0. 0. 0. ) BODY713_NUT_PREC_DEC = ( 0. 0. 0. 0. 0. 0. 0. 0.28 0. 0. 0. 0. 0. 0. 0. 0. 0. 0. ) BODY713_NUT_PREC_PM = ( 0. 0. 0. 0. 0. 0. 0. -0.08 0. 0. 0. 0. 0. 0. 0. 0. 0. 0. ) \begintext Belinda Old values: Values are unchanged in the 2015 IAU report. Current values: \begindata BODY714_POLE_RA = ( 257.31 0. 0. ) BODY714_POLE_DEC = ( -15.18 0. 0. ) BODY714_PM = ( 297.46 -577.3628170 0. ) BODY714_LONG_AXIS = ( 0. ) BODY714_NUT_PREC_RA = ( 0. 0. 0. 0. 0. 0. 0. 0. -0.03 0. 0. 0. 0. 0. 0. 0. 0. 0. ) BODY714_NUT_PREC_DEC = ( 0. 0. 0. 0. 0. 0. 0. 0. 0.03 0. 0. 0. 0. 0. 0. 0. 0. 0. ) BODY714_NUT_PREC_PM = ( 0. 0. 0. 0. 0. 0. 0. 0. -0.01 0. 0. 0. 0. 0. 0. 0. 0. 0. ) \begintext Puck Old values: Values are unchanged in the 2015 IAU report. Current values: \begindata BODY715_POLE_RA = ( 257.31 0. 0. ) BODY715_POLE_DEC = ( -15.18 0. 0. ) BODY715_PM = ( 91.24 -472.5450690 0. ) BODY715_LONG_AXIS = ( 0. ) BODY715_NUT_PREC_RA = ( 0. 0. 0. 0. 0. 0. 0. 0. 0. -0.33 0. 0. 0. 0. 0. 0. 0. 0. ) BODY715_NUT_PREC_DEC = ( 0. 0. 0. 0. 0. 0. 0. 0. 0. 0.31 0. 0. 0. 0. 0. 0. 0. 0. ) BODY715_NUT_PREC_PM = ( 0. 0. 0. 0. 0. 0. 0. 0. 0. -0.09 0. 0. 0. 0. 0. 0. 0. 0. ) \begintext Satellites of Neptune Triton Old values: Values are unchanged in the 2015 IAU report. Current values: \begindata BODY801_POLE_RA = ( 299.36 0. 0. ) BODY801_POLE_DEC = ( 41.17 0. 0. ) BODY801_PM = ( 296.53 -61.2572637 0. ) BODY801_LONG_AXIS = ( 0. ) BODY801_NUT_PREC_RA = ( 0. 0. 0. 0. 0. 0. 0. -32.35 0. -6.28 -2.08 -0.74 -0.28 -0.11 -0.07 -0.02 -0.01 ) BODY801_NUT_PREC_DEC = ( 0. 0. 0. 0. 0. 0. 0. 22.55 0. 2.10 0.55 0.16 0.05 0.02 0.01 0. 0. ) BODY801_NUT_PREC_PM = ( 0. 0. 0. 0. 0. 0. 0. 22.25 0. 6.73 2.05 0.74 0.28 0.11 0.05 0.02 0.01 ) \begintext Nereid Old values: The 2009 IAU report [3] states that values for Nereid are not given because Nereid is not in synchronous rotation with Neptune (notes following table 2). Current values: The 2015 IAU report does not provide values for Nereid. Naiad Old values: Values are unchanged in the 2015 IAU report. Current values: \begindata BODY803_POLE_RA = ( 299.36 0. 0. ) BODY803_POLE_DEC = ( 43.36 0. 0. ) BODY803_PM = ( 254.06 +1222.8441209 0. ) BODY803_LONG_AXIS = ( 0. ) BODY803_NUT_PREC_RA = ( 0.70 -6.49 0. 0. 0. 0. 0. 0. 0.25 0. 0. 0. 0. 0. 0. 0. 0. ) BODY803_NUT_PREC_DEC = ( -0.51 -4.75 0. 0. 0. 0. 0. 0. 0.09 0. 0. 0. 0. 0. 0. 0. 0. ) BODY803_NUT_PREC_PM = ( -0.48 4.40 0. 0. 0. 0. 0. 0. -0.27 0. 0. 0. 0. 0. 0. 0. 0. ) \begintext Thalassa Old values: Values are unchanged in the 2015 IAU report. Current values: \begindata BODY804_POLE_RA = ( 299.36 0. 0. ) BODY804_POLE_DEC = ( 43.45 0. 0. ) BODY804_PM = ( 102.06 1155.7555612 0. ) BODY804_LONG_AXIS = ( 0. ) BODY804_NUT_PREC_RA = ( 0.70 0. -0.28 0. 0. 0. 0. 0. 0. 0. 0. 0. 0. 0. 0. 0. 0. ) BODY804_NUT_PREC_DEC = ( -0.51 0. -0.21 0. 0. 0. 0. 0. 0. 0. 0. 0. 0. 0. 0. 0. 0. ) BODY804_NUT_PREC_PM = ( -0.48 0. 0.19 0. 0. 0. 0. 0. 0. 0. 0. 0. 0. 0. 0. 0. 0. ) \begintext Despina Old values: Values are unchanged in the 2015 IAU report. Current values: \begindata BODY805_POLE_RA = ( 299.36 0. 0. ) BODY805_POLE_DEC = ( 43.45 0. 0. ) BODY805_PM = ( 306.51 +1075.7341562 0. ) BODY805_LONG_AXIS = ( 0. ) BODY805_NUT_PREC_RA = ( 0.70 0. 0. -0.09 0. 0. 0. 0. 0. 0. 0. 0. 0. 0. 0. 0. 0. ) BODY805_NUT_PREC_DEC = ( -0.51 0. 0. -0.07 0. 0. 0. 0. 0. 0. 0. 0. 0. 0. 0. 0. 0. ) BODY805_NUT_PREC_PM = ( -0.49 0. 0. 0.06 0. 0. 0. 0. 0. 0. 0. 0. 0. 0. 0. 0. 0. ) \begintext Galatea Old values: Values are unchanged in the 2015 IAU report. Current values: \begindata BODY806_POLE_RA = ( 299.36 0. 0. ) BODY806_POLE_DEC = ( 43.43 0. 0. ) BODY806_PM = ( 258.09 839.6597686 0. ) BODY806_LONG_AXIS = ( 0. ) BODY806_NUT_PREC_RA = ( 0.70 0. 0. 0. -0.07 0. 0. 0. 0. 0. 0. 0. 0. 0. 0. 0. 0. ) BODY806_NUT_PREC_DEC = ( -0.51 0. 0. 0. -0.05 0. 0. 0. 0. 0. 0. 0. 0. 0. 0. 0. 0. ) BODY806_NUT_PREC_PM = ( -0.48 0. 0. 0. 0.05 0. 0. 0. 0. 0. 0. 0. 0. 0. 0. 0. 0. ) \begintext Larissa Old values: Values are unchanged in the 2015 IAU report. Current values: \begindata BODY807_POLE_RA = ( 299.36 0. 0. ) BODY807_POLE_DEC = ( 43.41 0. 0. ) BODY807_PM = ( 179.41 +649.0534470 0. ) BODY807_LONG_AXIS = ( 0. ) BODY807_NUT_PREC_RA = ( 0.70 0. 0. 0. 0. -0.27 0. 0. 0. 0. 0. 0. 0. 0. 0. 0. 0. ) BODY807_NUT_PREC_DEC = ( -0.51 0. 0. 0. 0. -0.20 0. 0. 0. 0. 0. 0. 0. 0. 0. 0. 0. ) BODY807_NUT_PREC_PM = ( -0.48 0. 0. 0. 0. 0.19 0. 0. 0. 0. 0. 0. 0. 0. 0. 0. 0. ) \begintext Proteus Old values: Values are unchanged in the 2015 IAU report. Current values: \begindata BODY808_POLE_RA = ( 299.27 0. 0. ) BODY808_POLE_DEC = ( 42.91 0. 0. ) BODY808_PM = ( 93.38 +320.7654228 0. ) BODY808_LONG_AXIS = ( 0. ) BODY808_NUT_PREC_RA = ( 0.70 0. 0. 0. 0. 0. -0.05 0. 0. 0. 0. 0. 0. 0. 0. 0. 0. ) BODY808_NUT_PREC_DEC = ( -0.51 0. 0. 0. 0. 0. -0.04 0. 0. 0. 0. 0. 0. 0. 0. 0. 0. ) BODY808_NUT_PREC_PM = ( -0.48 0. 0. 0. 0. 0. 0.04 0. 0. 0. 0. 0. 0. 0. 0. 0. 0. ) \begintext Satellites of Pluto Charon Old values: Values are unchanged in the 2015 IAU report. Current values: \begindata BODY901_POLE_RA = ( 132.993 0. 0. ) BODY901_POLE_DEC = ( -6.163 0. 0. ) BODY901_PM = ( 122.695 56.3625225 0. ) BODY901_LONG_AXIS = ( 0. ) \begintext Orientation constants for Selected Comets and Asteroids -------------------------------------------------------- Ceres Old values are from the 2009 IAU report. body2000001_pole_ra = ( 291. 0. 0. ) body2000001_pole_dec = ( 59. 0. 0. ) body2000001_pm = ( 170.90 952.1532 0. ) body2000001_long_axis = ( 0. ) Current values: \begindata BODY2000001_POLE_RA = ( 291.418 0. 0. ) BODY2000001_POLE_DEC = ( 66.764 0. 0. ) BODY2000001_PM = ( 170.650 952.1532 0. ) BODY2000001_LONG_AXIS = ( 0. ) \begintext Pallas Old values: Values are unchanged in the 2015 IAU report. Current values: \begindata BODY2000002_POLE_RA = ( 33. 0. 0. ) BODY2000002_POLE_DEC = ( -3. 0. 0. ) BODY2000002_PM = ( 38. 1105.8036 0. ) BODY2000002_LONG_AXIS = ( 0. ) \begintext Vesta Old values: Values are from the 2009 IAU report. body2000004_pole_ra = ( 305.8 0. 0. ) body2000004_pole_dec = ( 41.4 0. 0. ) body2000004_pm = ( 292. 1617.332776 0. ) body2000004_long_axis = ( 0. ) Current values: \begindata BODY2000004_POLE_RA = ( 309.031 0. 0. ) BODY2000004_POLE_DEC = ( 42.235 0. 0. ) BODY2000004_PM = ( 285.39 1617.3329428 0. ) BODY2000004_LONG_AXIS = ( 0. ) \begintext 52 Europa (asteroid) Current values: Values are provided for the first time in the 2015 IAU report. \begindata BODY2000052_POLE_RA = ( 257.0 0. 0. ) BODY2000052_POLE_DEC = ( 12.0 0. 0. ) BODY2000052_PM = ( 55.0 1534.6472187 0. ) BODY2000052_LONG_AXIS = ( 0. ) \begintext Lutetia Old values: Values are from the 2009 IAU report. Current values: \begindata BODY2000021_POLE_RA = ( 52. 0. 0. ) BODY2000021_POLE_DEC = ( 12. 0. 0. ) BODY2000021_PM = ( 94. 1057.7515 0. ) BODY2000021_LONG_AXIS = ( 0. ) \begintext Ida Old values are from the 2009 IAU report. body2431010_pole_ra = ( 168.76 0. 0. ) body2431010_pole_dec = ( -2.88 0. 0. ) body2431010_pm = ( 274.05 +1864.6280070 0. ) body2431010_long_axis = ( 0. ) The PM constant W0 is from [4]. Current values: \begindata BODY2431010_POLE_RA = ( 168.76 0. 0. ) BODY2431010_POLE_DEC = ( -87.12 0. 0. ) BODY2431010_PM = ( 274.05 +1864.6280070 0. ) BODY2431010_LONG_AXIS = ( 0. ) \begintext Eros Old values: Values are unchanged in the 2015 IAU report. Current values: \begindata BODY2000433_POLE_RA = ( 11.35 0. 0. ) BODY2000433_POLE_DEC = ( 17.22 0. 0. ) BODY2000433_PM = ( 326.07 1639.38864745 0. ) BODY2000433_LONG_AXIS = ( 0. ) \begintext Davida Old values: Values are unchanged in the 2015 IAU report. Current values: \begindata BODY2000511_POLE_RA = ( 297. 0. 0. ) BODY2000511_POLE_DEC = ( 5. 0. 0. ) BODY2000511_PM = ( 268.1 1684.4193549 0. ) BODY2000511_LONG_AXIS = ( 0. ) \begintext Gaspra Old values: Values are unchanged in the 2015 IAU report. Current values: \begindata BODY9511010_POLE_RA = ( 9.47 0. 0. ) BODY9511010_POLE_DEC = ( 26.70 0. 0. ) BODY9511010_PM = ( 83.67 1226.9114850 0. ) BODY9511010_LONG_AXIS = ( 0. ) \begintext Steins Old values are from the 2009 IAU report. body2002867_pole_ra = ( 90. 0. 0. ) body2002867_pole_dec = ( -62. 0. 0. ) body2002867_pm = ( 93.94 1428.852332 0. ) body2002867_long_axis = ( 0. ) Current values: \begindata BODY2002867_POLE_RA = ( 91. 0. 0. ) BODY2002867_POLE_DEC = ( -62. 0. 0. ) BODY2002867_PM = ( 321.76 1428.09917 0. ) BODY2002867_LONG_AXIS = ( 0. ) \begintext Itokawa Old values: Values are unchanged in the 2015 IAU report. Current values: \begindata BODY2025143_POLE_RA = ( 90.53 0. 0. ) BODY2025143_POLE_DEC = ( -66.30 0. 0. ) BODY2025143_PM = ( 000.0 712.143 0. ) BODY2025143_LONG_AXIS = ( 0. ) \begintext 9P/Tempel 1 Old values are from the 2009 IAU report. body1000093_pole_ra = ( 294. 0. 0. ) body1000093_pole_dec = ( 73. 0. 0. ) body1000093_pm = ( 252.63 212.064 0. ) body1000093_long_axis = ( 0. ) Current values: Values are from the 2015 IAU report [1]. Two sets of prime meridian values are given in [1]: one for the epoch of the Deep Impact mission's impactor's collision with the comet, and one for the epoch of the Stardust NExT closest approach. Deep Impact: Epoch: 2005-07-04 05:45:38.4 TDB 2453555.740027 JD TDB . 2 2 2 W = 109.7, W = 211.849 deg/day, d W/dt = 0.024 deg/day Stardust NExT: Epoch: 2011-02-15 04:40:18.6 TDB 2455607.694660 JD TDB . W = 69.2, W = 212.807 deg/day The values of W shown above are the prime meridian angles at the respective epochs. Prime meridian data below are those associated with the epoch of the Stardust NExT closest approach. Pole direction data are the same for both epochs. \begindata BODY1000093_POLE_RA = ( 255. 0. 0. ) BODY1000093_POLE_DEC = ( 64.5 0. 0. ) BODY1000093_PM = ( 69.2 212.807 0. ) BODY1000093_LONG_AXIS = ( 0. ) BODY1000093_CONSTANTS_JED_EPOCH = 2455607.694660 \begintext 19P/Borrelly Old values: body1000005_pole_ra = ( 218.5 0. 0. ) body1000005_pole_dec = ( -12.5 0. 0. ) body1000005_pm = ( 000. 390.0 0. ) body1000005_long_axis = ( 0. ) Current values: The 2015 IAU report does not cite a value for W0, so a complete orientation model based on that source is not available. Data are provided here for backward compatibility with pck00010.tpc. The W0 value was set to zero in that file and so is zero here. \begindata BODY1000005_POLE_RA = ( 218.5 0. 0. ) BODY1000005_POLE_DEC = ( -12.5 0. 0. ) BODY1000005_PM = ( 000. 324.3 0. ) BODY1000005_LONG_AXIS = ( 0. ) \begintext 67P/Churyumov-Gerasimenko Current values: Values are provided for the first time in the 2015 IAU report. The time range associated with the rotation model is 2014 MAR 3 : 2014 SEP 3 The reference epoch of the rotational elements is J2000. \begindata BODY1000012_POLE_RA = ( 69.54 0. 0. ) BODY1000012_POLE_DEC = ( 64.11 0. 0. ) BODY1000012_PM = ( 114.69 696.543884683 0. ) BODY1000012_LONG_AXIS = ( 0. ) \begintext 103P/Hartley 2 Current values: Values are provided for the first time in the 2015 IAU report. The 2015 IAU report provides only right ascension and declination values for body axes at the epoch of the EPOXI closest approach. The Z-axis is the long axis. The report uses the symbols alpha and delta to denote right ascension and declination respectively. Epoch: 2010-11-04 14:00:53.9 TDB JD 2455505.083957 TDB alpha = 285.1 deg. delta = -31.8 deg. X X alpha = 350.4 deg. delta = 34.4 deg. Y Y alpha = 226.1 deg. delta = 39.4 deg. Z Z Radii of Sun and Planets -------------------------------------------------------- Sun Old values: Values are from the 2009 IAU report. body10_radii = ( 696000. 696000. 696000. ) \begindata BODY10_RADII = ( 695700. 695700. 695700. ) \begintext Mercury Old values: Values are from the 2009 IAU report. body199_radii = ( 2439.7 2439.7 2439.7 ) Current values: \begindata BODY199_RADII = ( 2440.53 2440.53 2438.26 ) \begintext Venus Old values: Values are unchanged in the 2015 IAU report. Current values: \begindata BODY299_RADII = ( 6051.8 6051.8 6051.8 ) \begintext Earth Old values: Values are unchanged in the 2015 IAU report. Current values: \begindata BODY399_RADII = ( 6378.1366 6378.1366 6356.7519 ) \begintext Mars Old values: Values are unchanged in the 2015 IAU report. Current values: The 2015 IAU report gives separate values for the north and south polar radii: north: 3373.19 south: 3379.21 The report provides the average of these values as well, which we use as the polar radius for the triaxial model. \begindata BODY499_RADII = ( 3396.19 3396.19 3376.20 ) \begintext Jupiter Old values: Values are unchanged in the 2015 IAU report. Current values: \begindata BODY599_RADII = ( 71492 71492 66854 ) \begintext Saturn Old values: Values are unchanged in the 2015 IAU report. Current values: \begindata BODY699_RADII = ( 60268 60268 54364 ) \begintext Uranus Old values: Values are unchanged in the 2015 IAU report. Current values: \begindata BODY799_RADII = ( 25559 25559 24973 ) \begintext Neptune Old values: Values are unchanged in the 2015 IAU report. Current values: (Values are for the 1 bar pressure level.) \begindata BODY899_RADII = ( 24764 24764 24341 ) \begintext Radii of the Dwarf Planet Pluto -------------------------------------------------------- Pluto Old values: Values are from the 2009 IAU report. body999_radii = ( 1195 1195 1195 ) Current values: \begindata BODY999_RADII = ( 1188.3 1188.3 1188.3 ) \begintext Radii of Satellites -------------------------------------------------------- Moon Old values: Values are unchanged in the 2015 IAU report. Current values: \begindata BODY301_RADII = ( 1737.4 1737.4 1737.4 ) \begintext Satellites of Mars Old values: Values are unchanged in the 2015 IAU report. Current values: \begindata BODY401_RADII = ( 13.0 11.4 9.1 ) BODY402_RADII = ( 7.8 6.0 5.1 ) \begintext Satellites of Jupiter Old values: Values are unchanged in the 2015 IAU report. Current values: Note that for Ganymede and Callisto only mean radii are provided. \begindata BODY501_RADII = ( 1829.4 1819.4 1815.7 ) BODY502_RADII = ( 1562.6 1560.3 1559.5 ) BODY503_RADII = ( 2631.2 2631.2 2631.2 ) BODY504_RADII = ( 2410.3 2410.3 2410.3 ) BODY505_RADII = ( 125 73 64 ) \begintext Only mean radii are available in the 2015 IAU report for bodies 506-513. \begindata BODY506_RADII = ( 85 85 85 ) BODY507_RADII = ( 40 40 40 ) BODY508_RADII = ( 18 18 18 ) BODY509_RADII = ( 14 14 14 ) BODY510_RADII = ( 12 12 12 ) BODY511_RADII = ( 15 15 15 ) BODY512_RADII = ( 10 10 10 ) BODY513_RADII = ( 5 5 5 ) BODY514_RADII = ( 58 49 42 ) BODY515_RADII = ( 10 8 7 ) BODY516_RADII = ( 30 20 17 ) \begintext Satellites of Saturn Old values: Values are from the 2009 IAU report. body601_radii = ( 207.8 196.7 190.6 ) body602_radii = ( 256.6 251.4 248.3 ) body603_radii = ( 538.4 528.3 526.3 ) body604_radii = ( 563.4 561.3 559.6 ) body605_radii = ( 765.0 763.1 762.4 ) body606_radii = ( 2575.15 2574.78 2574.47 ) body607_radii = ( 180.1 133.0 102.7 ) body608_radii = ( 745.7 745.7 712.1 ) body609_radii = ( 109.4 108.5 101.8 ) body610_radii = ( 101.5 92.5 76.3 ) body611_radii = ( 64.9 57.0 53.1 ) body612_radii = ( 21.7 19.1 13.0 ) body613_radii = ( 16.3 11.8 10.0 ) body614_radii = ( 15.1 11.5 7.0 ) body615_radii = ( 20.4 17.7 9.4 ) body616_radii = ( 67.8 39.7 29.7 ) body617_radii = ( 52.0 40.5 32.0 ) body618_radii = ( 17.2 15.7 10.4 ) body632_radii = ( 1.6 1.6 1.6 ) body633_radii = ( 2.9 2.8 2.0 ) body634_radii = ( 1.5 1.2 1.0 ) body635_radii = ( 4.3 4.1 3.2 ) body649_radii = ( 1 1 1 ) Current values: \begindata BODY601_RADII = ( 207.8 196.7 190.6 ) BODY602_RADII = ( 256.6 251.4 248.3 ) BODY603_RADII = ( 538.4 528.3 526.3 ) BODY604_RADII = ( 563.4 561.3 559.6 ) BODY605_RADII = ( 765.0 763.1 762.4 ) BODY606_RADII = ( 2575.15 2574.78 2574.47 ) BODY607_RADII = ( 180.1 133.0 102.7 ) BODY608_RADII = ( 745.7 745.7 712.1 ) BODY609_RADII = ( 109.4 108.5 101.8 ) BODY610_RADII = ( 101.7 93.0 76.3 ) BODY611_RADII = ( 64.9 57.3 53.0 ) BODY612_RADII = ( 22.5 19.6 13.3 ) BODY613_RADII = ( 16.3 11.8 9.8 ) BODY614_RADII = ( 15.3 9.3 6.3 ) BODY615_RADII = ( 20.5 17.8 9.4 ) BODY616_RADII = ( 68.2 41.6 28.2 ) BODY617_RADII = ( 52.2 40.8 31.5 ) BODY618_RADII = ( 17.2 15.4 10.4 ) BODY632_RADII = ( 1.94 1.29 1.21 ) BODY633_RADII = ( 2.88 2.08 1.8 ) BODY634_RADII = ( 1.5 1.2 1.0 ) BODY635_RADII = ( 4.6 4.5 2.8 ) BODY649_RADII = ( 0.5 0.5 0.5 ) BODY653_RADII = ( 0.7 0.25 0.2 ) \begintext Satellites of Uranus Old values: Values are unchanged in the 2015 IAU report. Current values: \begindata BODY701_RADII = ( 581.1 577.9 577.7 ) BODY702_RADII = ( 584.7 584.7 584.7 ) BODY703_RADII = ( 788.9 788.9 788.9 ) BODY704_RADII = ( 761.4 761.4 761.4 ) BODY705_RADII = ( 240.4 234.2 232.9 ) \begintext The 2015 IAU report gives only mean radii for satellites 706--715. \begindata BODY706_RADII = ( 13 13 13 ) BODY707_RADII = ( 15 15 15 ) BODY708_RADII = ( 21 21 21 ) BODY709_RADII = ( 31 31 31 ) BODY710_RADII = ( 27 27 27 ) BODY711_RADII = ( 42 42 42 ) BODY712_RADII = ( 54 54 54 ) BODY713_RADII = ( 27 27 27 ) BODY714_RADII = ( 33 33 33 ) BODY715_RADII = ( 77 77 77 ) \begintext Satellites of Neptune Old values: Values are unchanged in the 2015 IAU report. Current values: The 2015 IAU report gives mean radii only for bodies 801-806. \begindata BODY801_RADII = ( 1352.6 1352.6 1352.6 ) BODY802_RADII = ( 170 170 170 ) BODY803_RADII = ( 29 29 29 ) BODY804_RADII = ( 40 40 40 ) BODY805_RADII = ( 74 74 74 ) BODY806_RADII = ( 79 79 79 ) \begintext The second equatorial radius for Larissa is not given in the 2009 report. The available values are: BODY807_RADII = ( 104 --- 89 ) For use within the SPICE system, we use only the mean radius. \begindata BODY807_RADII = ( 96 96 96 ) BODY808_RADII = ( 218 208 201 ) \begintext Satellites of Pluto Old values: Values are from the 2009 IAU report. BODY901_RADII = ( 605 605 605 ) Current values: \begindata BODY901_RADII = ( 606 606 606 ) \begintext Radii for Selected Comets and Asteroids -------------------------------------------------------- Ceres Old values: Values are from the 2009 IAU report. body2000001_radii = ( 487.3 487.3 454.7 ) Current values: \begindata BODY2000001_RADII = ( 487.3 487.3 446. ) \begintext Vesta Old values: Values are unchanged in the 2015 IAU report. Current values: \begindata BODY2000004_RADII = ( 289. 280. 229. ) \begintext Psyche Current values: Values are provided for the first time in the 2015 IAU report. \begindata BODY2000016_RADII = ( 139.5 116. 94.5 ) \begintext Lutetia Old values: Values are unchanged in the 2015 IAU report. Current values: \begindata BODY2000021_RADII = ( 62.0 50.5 46.5 ) \begintext 52 Europa Current values: Values are provided for the first time in the 2015 IAU report. \begindata BODY2000052_RADII = ( 189.5 165. 124.5 ) \begintext Ida Old values: Values are unchanged in the 2015 IAU report. Current values: \begindata BODY2431010_RADII = ( 26.8 12.0 7.6 ) \begintext Mathilde Old values: Values are unchanged in the 2015 IAU report. Current values: \begindata BODY2000253_RADII = ( 33. 24. 23. ) \begintext Eros Old values: Values are unchanged in the 2015 IAU report. Current values: \begindata BODY2000433_RADII = ( 17.0 5.5 5.5 ) \begintext Davida Old values: Values are unchanged in the 2015 IAU report. Current values: \begindata BODY2000511_RADII = ( 180. 147. 127. ) \begintext Gaspra Old values: Values are unchanged in the 2015 IAU report. Current values: \begindata BODY9511010_RADII = ( 9.1 5.2 4.4 ) \begintext Steins Old values: Values are unchanged in the 2015 IAU report. Current values: \begindata BODY2002867_RADII = ( 3.24 2.73 2.04 ) \begintext Toutatis Old values: Values are unchanged in the 2015 IAU report. Current values: \begindata BODY2004179_RADII = ( 2.13 1.015 0.85 ) \begintext Itokawa Old values: Values are from the 2009 IAU report. Note that the diameters rather than radii were given. body2025143_radii = ( 0.535 0.294 0.209 ) Current values: \begindata BODY2025143_RADII = ( 0.268 0.147 0.104 ) \begintext Kleopatra Old values: Values are from the 2003 report [13]. A shape model was not provided in later reports because, according to [5], the shape had been "modeled from low resolution radar data, and cannot be mapped from those data." body2000216_radii = ( 108.5 47 40.5 ) Current values: No values are provided in the 2015 IAU report. Halley Old values: Values are unchanged in the 2015 IAU report. Current values: \begindata BODY1000036_RADII = ( 8.0 4.0 4.0 ) \begintext 9P/Tempel 1 Old values: The effective radius is unchanged in the 2009 IAU report. Current values: According to [1]: The maximum and minimum radii are not properly the values of the principal semi-axes, they are half the maximum and minimum values of the diameter. Due to the large deviations from a simple ellipsoid, they may not correspond with measurements along the principal axes, or be orthogonal to each other. The radii along the first and second principal axes are given as 3.7 km 2.5 km The value in the data assignment below is the mean radius. \begindata BODY1000093_RADII = ( 3.0 3.0 3.0 ) \begintext 19P/Borrelly Old values: Values are unchanged in the 2015 IAU report. Current values: The first principal axis length is 3.5 km The lengths of the other semi-axes are not provided by [1]. The value in the data assignment below is the mean radius. \begindata BODY1000005_RADII = ( 4.22 4.22 4.22 ) \begintext 81P/Wild 2 Old values: Values are unchanged in the 2015 IAU report. Current values: \begindata BODY1000107_RADII = ( 2.7 1.9 1.5 ) \begintext 67P/Churyumov-Gerasimenko Current values: Values are provided for the first time in the 2015 IAU report. \begindata BODY1000012_RADII = ( 2.40 1.55 1.20 ) \begintext 103P/Hartley 2 The most recent "Report of the IAU Working Group on Cartographic Coordinates and Rotational Elements: 2015" appears to incorrectly list the radii for Comet 103P/Hartley 2 in Table 6. The following text by Brent Archinal, Chair of the Working Group, examines this problem and what radii should likely be used. However, note that this explanation has not yet been officially considered and the proposed changes recommended by the Working Group. Such a process will begin shortly, and a consensus document about any changes may be published on the Working Group website. Clearly from the many figures in various papers (e.g. A'Hearn et al, 2011, Science, 332, 1396; Belton, et al., 2012 Icarus, 222, 595; Thomas, et al. 2013, Icarus, 222, 550), Comet 103P/Hartley 2 has an elongated nucleus, with the long axis being the (reference) spin axis. This is stated/shown e.g., in Figure 3 of the A'Hearn et al. paper. The size is stated in a few places as having a diameter of 0.69 to 2.33 km and a mean radius of 0.58 +/-0.02 km (A'Hearn, et al., Table 1; Thomas et al., Table 1 (but now with a mean radius uncertainty of 0.018 km)). This of course translates to a mean radius of 0.58 km, a minimum radius of 0.345 km (or rounding, 0.34 km), and a maximum radius of 1.165 km (rounding, 1.16 km). I don't really see a clear statement in these papers that these last two numbers can be used for the semi axes, just that they are minimum and maximum values. Apparently though that's been assumed (as it has been for some of the other comets listed in the WG report). There is also no clear statement of what if any difference there is between the first and second semi axis, but only that they are "similar". E.g., Thomas et al. says (Section 3) "This bi-lobed object has near rotational symmetry". That does correspond to what's said in footnote (g) of the WG report. So, I think it is correct that: mean radius = 0.58 km a semi-axis = 0.34 km b semi-axis = 0.34 km (or "~0.34 km") c semi-axis (polar axis) = 1.16 km Due to their uncertain status, these data are included in this file only as comments. To enable SPICE software to access the data, move this assignment BODY1000041_RADII = ( 0.34 0.34 1.16 ) below the \begindata marker below. \begindata \begintext =========================================================================== End of file pck00011_n0066.tpc ===========================================================================