Data Set Information
DATA_SET_NAME STOOKE SMALL BODY SHAPE MODELS V1.0
DATA_SET_ID EAR-A-5-DDR-STOOKE-SHAPE-MODELS-V1.0
NSSDC_DATA_SET_ID
DATA_SET_TERSE_DESCRIPTION
DATA_SET_DESCRIPTION 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]
DATA_SET_RELEASE_DATE 2002-05-10T00:00:00.000Z
START_TIME 1979-01-01T12:00:00.000Z
STOP_TIME 1993-01-01T12:00:00.000Z
MISSION_NAME
MISSION_START_DATE
MISSION_STOP_DATE
TARGET_NAME GASPRA
N8 PROTEUS
IDA
JANUS
HALLEY
EPIMETHEUS
TARGET_TYPE ASTEROID
SATELLITE
COMET
INSTRUMENT_HOST_ID VEGA1
GIO
VEGA2
GO
VG1
VG2
INSTRUMENT_NAME SOLID STATE IMAGING SYSTEM
IMAGING SCIENCE SUBSYSTEM - NARROW ANGLE
TELEVISION SYSTEM
HALLEY MULTICOLOUR CAMERA
INSTRUMENT_ID SSI
ISSN
TVS
HMC
INSTRUMENT_TYPE FRAMING CAMERA
CAMERA
NODE_NAME Small Bodies
ARCHIVE_STATUS SUPERSEDED
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.
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
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