PDS_VERSION_ID      = PDS3                                                    
LABEL_REVISION_NOTE = "                                                       
  08 Apr 2002, C. Neese:  Begin label revision history.                       
  16 May 2002, C. Neese:  Improve description text.                           
  18 Jan 2003, A.C.Raugh: Lien-resolution editing                             
  "                                                                           
                                                                              
OBJECT     = DATA_SET                                                         
  DATA_SET_ID       = "EAR-A-5-DDR-STOOKE-SHAPE-MODELS-V1.0"                  
  DATA_SET_LOCAL_ID = "STKSHAPE"                                              
                                                                              
  OBJECT     = DATA_SET_INFORMATION                                           
    DATA_SET_NAME                  = "STOOKE SMALL BODY SHAPE MODELS V1.0"    
    DATA_SET_TERSE_DESC            = "Optical shape models of 10 planetary    
       moons and asteroids, derived from spacecraft imaging by Philip         
       Stooke."                                                               
    ARCHIVE_STATUS                 = "LOCALLY_ARCHIVED"                       
    DATA_SET_COLLECTION_MEMBER_FLG = "N"                                      
    DATA_OBJECT_TYPE               = "TABLE"                                  
    START_TIME                     = 1979                                     
    STOP_TIME                      = 1993                                     
    DATA_SET_RELEASE_DATE          = 2002-05-10                               
    PRODUCER_FULL_NAME             = "CAROL NEESE"                            
    OBSERVER_FULL_NAME             = "PHILIP STOOKE"                          
    DATA_SET_UPDATE_PERIOD         = 1.0                                      
    DETAILED_CATALOG_FLAG          = "N"                                      
    DATA_SET_DESC                  = "                                        
                                                                              
      Data Set Overview                                                       
      =================                                                       
      This data set contains the Philip Stooke shape models for small         
      solar system bodies.  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.  Other optical shape models         
      prepared by Peter Thomas are also available in PDS data set             
      EAR-A-5-DDR-SHAPE-MODELS-V2.1.                                          
                                                                              
      The current version of this data set contains shape models for          
      243 Ida, 951 Gaspra, comet Halley, J5 Amalthea, N7 Larissa,             
      N8 Proteus, S10 Janus, S11 Epimetheus, S16 Prometheus, and              
      S17 Pandora.                                                            
                                                                              
      Parameters                                                              
      ==========                                                              
      The shape models consist of a grid of body-centered latitude and        
      longitude with a radius listed for each grid point.  Coordinates        
      are planetocentric, increasing to the west.  West is defined as being   
      to the left when north is up, regardless of the rotation direction      
      of the body.  North is defined as the pole on the north side of the     
      invariant plane of the solar system.  (These are the cartographic       
      coordinate system definitions approved by the IAU's Working Group       
      on Cartographic Coordinates, reported in Seidelman, et al. 2002)        
      [SEIDELMANETAL2002].  Radii are given in kilometers.                    
                                                                              
      Uncertainties are highly variable from place to place, depending        
      on locations of limb profiles used to create the models.  Thus, the     
      data format cannot reflect the accuracy of the radii and there may      
      be more decimal places given than are significant.  An estimate of      
      uncertainties is provided in the data label where available.  A full    
      discussion of the uncertainties of the models is available in the       
      published papers.                                                       
                                                                              
      Further details are given in the relevant published papers.             
                                                                              
      Seidelmann, P.K., Abalakin, V.K., Bursa, M., Davies, M.E.,              
      de Bergh, C., Lieske, J.H., Oberst, J., Simon, J.L., Standish,          
      E.M., Stooke, P.J. and P.C. Thomas.  'Report of the IAU/IAG Working     
      Group on Cartographic Coordinates and Rotational Elements of the        
      planets and satellites: 2000.'  Celestial Mechanics and Dynamical       
      Astronomy, v. 82, 83-100, 2002. [SEIDELMANNETAL2002]                    
                                                                              
      "                                                                       
    CONFIDENCE_LEVEL_NOTE          = "                                        
                                                                              
      P. Stooke notes (especially with respect to the Comet Halley model):    
                                                                              
         Comparison of independent shape models by P. Stooke and              
         P. Thomas for the same bodies (Amalthea, Janus, Epimetheus)          
         suggests that Thomas tends towards models more convex than           
         the likely shapes, and Stooke tends towards models which             
         are too faceted, or which exaggerate the depths of depressions.      
                                                                              
      Review                                                                  
      ======                                                                  
      This data set underwent external peer review on May 10, 2002."          
                                                                              
  END_OBJECT = DATA_SET_INFORMATION                                           
                                                                              
  OBJECT     = DATA_SET_TARGET                                                
    TARGET_NAME = { "1P/HALLEY (1682 Q1)",                                    
                    "S11 EPIMETHEUS",                                         
                    "951 GASPRA",                                             
                    "J5 AMALTHEA",                                            
                    "243 IDA",                                                
                    "S10 JANUS",                                              
                    "N7 LARISSA",                                             
                    "N8 PROTEUS",                                             
                    "S17 PANDORA",                                            
                    "S16 PROMETHEUS" }                                        
  END_OBJECT = DATA_SET_TARGET                                                
                                                                              
  OBJECT     = DATA_SET_HOST                                                  
    INSTRUMENT_HOST_ID = { "VEGA1","VEGA2",                                   
                           "VG1","VG2",                                       
                           "GO",                                              
                           "GIO" }                                            
    INSTRUMENT_ID      = { "TVS",                                             
                           "ISSN",                                            
                           "SSI",                                             
                           "HMC" }                                            
  END_OBJECT = DATA_SET_HOST                                                  
                                                                              
  OBJECT     = DATA_SET_REFERENCE_INFORMATION                                 
    REFERENCE_KEY_ID = { "BELTONETAL1991",                                    
                         "SEIDELMANNETAL2002",                                
                         "SIMONELLIETAL1995",                                 
                         "STOOKE1993A",                                       
                         "STOOKE1993B",                                       
                         "STOOKE1993C",                                       
                         "STOOKE1994A",                                       
                         "STOOKE1994B",                                       
                         "STOOKE1997",                                        
                         "THOMASETAL1994",                                    
                         "THOMASETAL1996" }                                   
  END_OBJECT = DATA_SET_REFERENCE_INFORMATION                                 
                                                                              
END_OBJECT = DATA_SET                                                         
                                                                              
END