KPL/FK

ExoMars2016 Target Body DSK Surface ID Codes
========================================================================

   This frame kernel contains a set of ExoMars2016 Target Body DSK Surface ID
   Codes for Phobos, Deimos, Mars and the TGO spacecraft.


Version and Date
------------------------------------------------------------------------

   Version 0.0 -- January 4, 2019 -- Marc Costa Sitja, ESAC/ESA

      First version.


References
------------------------------------------------------------------------

   1. ``Frames Required Reading''

   2. ``Kernel Pool Required Reading''

   3. ``DS-Kernel Required Reading''

   4. TGO Frames Kernel.


Contact Information
------------------------------------------------------------------------

   If you have any questions regarding this file contact SPICE support at
   ESAC:

           Marc Costa Sitja
           (+34) 91-8131-457
           mcosta@sciops.esa.int, esa_spice@sciops.esa.int

     or SPICE support at IKI:

             Alexander Abbakumov
             +7 (495) 333-40-13
             aabbakumov@romance.iki.rssi.ru

   or NAIF at JPL:

           Boris Semenov
           +1 (818) 354-8136
           Boris.Semenov@jpl.nasa.gov


Implementation Notes
------------------------------------------------------------------------

  This file is used by the SPICE system as follows: programs that make use
  of this frame kernel must "load" the kernel normally during program
  initialization. Loading the kernel associates the data items with
  their names in a data structure called the "kernel pool".  The SPICELIB
  routine FURNSH loads a kernel into the pool as shown below:

    FORTRAN: (SPICELIB)

      CALL FURNSH ( frame_kernel_name )

    C: (CSPICE)

      furnsh_c ( frame_kernel_name );

    IDL: (ICY)

      cspice_furnsh, frame_kernel_name

    MATLAB: (MICE)

         cspice_furnsh ( 'frame_kernel_name' )

    PYTHON: (SPICEYPY)*

         furnsh( frame_kernel_name )

  In order for a program or routine to extract data from the pool, the
  SPICELIB routines GDPOOL, GIPOOL, and GCPOOL are used.  See [2] for
  more details.

  This file was created and may be updated with a text editor or word
  processor.

  * SPICEPY is a non-official, community developed Python wrapper for the
    NAIF SPICE toolkit. Its development is managed on Github.
    It is available at: https://github.com/AndrewAnnex/SpiceyPy


Definition Section
------------------------------------------------------------------------

   This section contains name to ID mappings for the ExoMars2016 target
   body DSK surfaces. These mappings are supported by all SPICE
   toolkits with integrated DSK capabilities (version N0066 or later).

   Mars Satellite Phobos Surface name/IDs:

          DSK Surface Name          ID    Body ID
      ===========================  =====  =======

      PHOBOS_M157_GAS_V01          14011      401
      PHOBOS_K137_DLR_V01          10041      401


   Name-ID Mapping keywords:

   \begindata

      NAIF_SURFACE_NAME += 'PHOBOS_M157_GAS_V01'
      NAIF_SURFACE_CODE += 14011
      NAIF_SURFACE_BODY += 401

      NAIF_SURFACE_NAME += 'PHOBOS_K137_DLR_V01'
      NAIF_SURFACE_CODE += 10041
      NAIF_SURFACE_BODY += 401

   \begintext


   Mars Satellite Deimos Surface name/IDs:

          DSK Surface Name          ID    Body ID
      ===========================  =====  =======

      DEIMOS_K002_THO_V01          14020      402


   Name-ID Mapping keywords:

   \begindata

      NAIF_SURFACE_NAME += 'DEIMOS_K002_THO_V01'
      NAIF_SURFACE_CODE += 14020
      NAIF_SURFACE_BODY += 402

   \begintext


End of FK file.