Data Set Information
DATA_SET_NAME SMALL BODY SHAPE MODELS V2.1
DATA_SET_ID EAR-A-5-DDR-SHAPE-MODELS-V2.1
NSSDC_DATA_SET_ID GD-11F
DATA_SET_TERSE_DESCRIPTION Optical shape models of 9 planetary moons and asteroids, derived from spacecraft imaging by P. Thomas.
DATA_SET_DESCRIPTION
Data Set Overview
        =================
        This data set contains the Peter Thomas shape models for small
        solar system bodies, as well as image mosaics constructed from
        these models.  These shape models are based on optical data and
        are distinct from the shape models based on radar observations
        which are included in a separate data set, EAR-A-5-DDR-
        RADARSHAPE-MODELS-V1.0. The current version of this data set
        contains the following.
 
        243 Ida:        Shape model, image mosaic, and a list of Galileo
                        SSI images used to construct the image mosaic
 
        951 Gaspra:     Shape model, image mosaic, and a list of Galileo
                        SSI images used to construct the image mosaic
 
        253 Mathilde:   Shape model and a list of NEAR MSI images used
                        to produce the shape model.
 
        4 Vesta:        Shape model and a list of HST images used to
                        produce the shape model.
 
        M1 Phobos:      Shape model, image mosaic and a list of Viking
                        Orbiter images use to construct the image mosaic
 
        M2 Deimos:      Shape model, image mosaic and a list of Viking
                        Orbiter images use to construct the image mosaic
 
        S7 Hyperion:    Shape model, image mosaic and a list of Voyager
                        2 Narrow Angle images use to construct the image
                        mosaic
 
        S10 Janus:      Shape model and list of Voyager 1 and 2 images
                        used to derive the model (image mosaic not yet
                        completed)
 
        S11 Epimetheus: Shape model and list of Voyager 1 and 2 images
                        used to derive the model (image mosaic not yet
                        completed)
 
 
        Parameters
        ==========
        The shape models consist of a grid of body-centered latitude and
        longitude with a diameter listed for each grid point.  Details
        of mapping and production of each model are given in the PDS
        label for the shape model file, and further details are given in
        the relevant published papers.
 
        Davies, M.E., V.K. Abalakin, A. Brahic, M. Bursa, B.H. Chovitz,
        J.H. Lieske, P.K. Seidelmann, A.T. Sinclair, and I.S. Tiuflin
        1992. Report of the IAU/IAG/COSPAR Working Group on Cartographic
        Coordinates and Rotational Elements of the Planets and
        Satellites - 1991.  Celestial Mechanics and Dynamical Astronomy,
        53, no. 4, 377-397. [DAVIESETAL1992]
 
        Simonelli, D.P., P.C. Thomas, B.T. Carcich, and J. Veverka 1993.
        Generation and use of numerical shape models for irregular solar
        system objects.  Icarus, 103, 49-61. [SIMONELLIETAL1993]
 
        Thomas, P.C. 1993.  Gravity, tides, and topography on small
        satellites and asteroids.  Icarus 105, 326-344. [THOMAS1993]
 
        Duxbury, T.C., and J.D. Callahan 1989.  Phobos and Deimos
        control networks.  Icarus 77, 275-286. [DUXBURY&CALLAHAN1989]
 
        Duxbury, T.C., J.D. Callahan, and A.C. Ocampo 1984.  Phobos:
        Close encounter imaging from the Viking Orbiters.  NASA
        reference publication 1109. [DUXBURYETAL1984]
 
        Davies, M.E., T.R. Colvin, M.J.S. Belton, J. Veverka, and P.
        Thomas 1994.  The direction of the north pole and the control
        network of asteroid 951 Gaspra.  Icarus 107, 18-22.
        [DAVIESETAL1994A]
 
        Davies, M.E., T.R. Colvin, M.J.S. Belton, J. Veverka, and P.
        Thomas 1996.  The direction of the north pole and the control
        network of asteroid 243 Ida.  Icarus 120, 33-37.
        [DAVIESETAL1996]
 
        Thomas, P.C., J. Veverka, D. Simonelli, P. Helfenstein, B.
        Carcich, M.J.S.  Belton, M.E. Davies, and C. Chapman 1994.  The
        shape of Gaspra.  Icarus 107, 25-36. [THOMASETAL1994]
 
        Thomas, P.C., M.J.S. Belton, B. Carcich, C. R. Chapman, M.E.
        Davies, R.  Sullivan, and J. Veverka 1996.  The shape of Ida.
        Icarus 120, 20-32. [THOMASETAL1996]
 
        Thomas, P.C., G.J. Black, and P.D. Nicholson 1995.  Hyperion:
        Rotation, shape, and geology from Voyager images.  Icarus 117,
        128-148. [THOMASETAL1995]
 
        Yoder, C.F., S.P. Synnott, and H. Salo 1989.  Orbits and masses
        of Saturn's co-orbiting satellites Janus and Epimetheus.
        Astron. J. 98, 1875-1889. [YODERETAL1989]
 
        Thomas, P. 1989.  The shapes of small satellites.  Icarus 77,
        248-274. [THOMAS1989]
 
        Thomas, P.C., R.P. Binzel, M.J. Gaffey, B.H. Zellner,
        A.D. Storrs, and E. Wells 1997.  Vesta:  Spin pole, size, and
        shape from HST images.  Icarus 128, 88-94.  [THOMASETAL1997]
 
        Thomas, P.C., J. Veverka, J.F. Bell III, B.E. Clark, B. Carcich,
        J. Joseph, M. Robinson, L.A. McFadden, M.C. Malin, C.R. Chapman,
        W. Merline, and S. Murchie 1999.  Mathilde:  Size, shape, and
        geology.  Icarus 140, 17-27.  [THOMASETAL1999]
 
 
        Update History
        ==============
        This data set was first reviewed and archived in 1997.  It is
        now being updated to include two new shape models which have
        become available, those of the asteroids 253 Mathilde and 4
        Vesta.
 
        In February 2002 a critical look was taken at the labels of
        these files in order to fill in information previously left
        blank. The following changes were made:
 
          o  INSTRUMENT and INSTRUMENT_HOST were provided in all cases.
          o  START_TIME and STOP_TIME were provided as accurately as
          they could be determined from data elsewhere in the PDS
          archives. [ Note that the START_TIME and STOP_TIME for the
          entire data set has been left as 'N/A,' since the concept is
          not really relevant to the shape model content as a whole.]
          o  The AXIS_ORDER_TYPE keyword was added to the IMAGE object
          in FITS file PDS labels with a value of 'FIRST ORDER FASTEST'.
          This is the appropriate order for FITS files (but not the PDS
          default).
          o  A few minor typographical errors in description fields were
          corrected.
          o  The 'mathilde.lbl' file, which was inadvertently left
          incomplete and contained several syntactical errors, was
          completed and the format verified.
          o  The file names and TARGET_NAME values corresponding to
          asteroids were changed to the (new) standard format
          _.
DATA_SET_RELEASE_DATE 2000-06-01T00:00:00.000Z
START_TIME 1976-06-22T12:00:00.000Z
STOP_TIME 1997-06-27T11:59:00.000Z
MISSION_NAME SUPPORT ARCHIVES
MISSION_START_DATE 2004-03-22T12:00:00.000Z
MISSION_STOP_DATE N/A (ongoing)
TARGET_NAME 4 VESTA
GASPRA
IDA
MATHILDE
DEIMOS
EPIMETHEUS
HYPERION
JANUS
PHOBOS
TARGET_TYPE ASTEROID
ASTEROID
ASTEROID
ASTEROID
SATELLITE
SATELLITE
SATELLITE
SATELLITE
SATELLITE
INSTRUMENT_HOST_ID GO
HST
NEAR
VG1
VG2
VO1
VO2
INSTRUMENT_NAME IMAGING SCIENCE SUBSYSTEM - NARROW ANGLE
IMAGING SCIENCE SUBSYSTEM - NARROW ANGLE
MULTI-SPECTRAL IMAGER
SOLID STATE IMAGING SYSTEM
VISUAL IMAGING SUBSYSTEM - CAMERA A
VISUAL IMAGING SUBSYSTEM - CAMERA B
WIDE FIELD PLANETARY CAMERA 2
INSTRUMENT_ID ISSN
ISSN
MSI
SSI
VISA
VISB
WFPC2
INSTRUMENT_TYPE CAMERA
CAMERA
CAMERA
CAMERA
CAMERA
CAMERA
CAMERA
NODE_NAME Small Bodies
ARCHIVE_STATUS LOCALLY_ARCHIVED
CONFIDENCE_LEVEL_NOTE
Review
      ======
      This data set underwent external peer review on June 1, 2000.
CITATION_DESCRIPTION TBD
ABSTRACT_TEXT Optical shape models of 10 planetary moons and asteroids, derived from spacecraft imaging by Philip Stooke.
PRODUCER_FULL_NAME CAROL NEESE
SEARCH/ACCESS DATA
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