The Visual and Infrared Mapping Spectrometer (VIMS) instrument
onboard the Cassini spacecraft observed the system of Saturn,
acquiring spectral cubes in the range 0.4-5.2 microns. This service
focuses on Saturn satellites, and provides access to calibrated and
ancillary data, computed as described here:
https://vims.univ-nantes.fr/info/isis-calibration. It also provides
direct links to a larger web site with previews.
Main characteristics of Solar System planets. Data are included in
the table, which includes non-standard EPN-TAP parameters. Data are
retrieved from Archinal et al 2018 (IAU report 2015,
2018CeMDA.130...22A) [radii] and Cox et al 2000 (Allen's astrophysical
quantities, 2000asqu.book.....C) [masses, heliocentric distances, and
rotation periods].
This service provides access to the spectral library in support of
the CRISM experiment on Mars Reconnaissance Orbiter. This is a
redesigned version of the library once distributed by the PDS
Geosciences node, with data files provided as VOTable (the native
version was available at:
http://pds-geosciences.wustl.edu/mro/mro-m-crism-4-speclib-v1/mrocr_90xx/
Reference: Murchie et al (2007) Compact Reconnaissance Imaging
Spectrometer for Mars (CRISM) on Mars Reconnaissance Orbiter (MRO).
JGR Planets, 112:E05S03
Paris Astronomical Data Centre - Constructor University
Description:
GMap provides planetary geological maps of different Solar System
bodies, developed by an open community, reviewed by scientists. GMap
inherits its data model from Planmap, most of the maps provide
morphological information, some provide stratigraphic or compositional
information too. Each original data packages provided is a collection
of vector, raster, and, in some cases, 3D models. In this EPN-TAP
service, the data records (`granule_uid`) refer to each of the data
files in the whole of GMAP archive, grouped by (`granule_gid`) the
data package --map-- they compose.
HST observations of planets, dwarf planets, and satellites, extracted
from the CADC database catalogue (with daily updates). Data are linked
to the CADC repository, with file names common to all HST archives.
Both calibrated and derived products are included. The main target is
identified. Physical ephemeris and thumbnails are provided when
available. Files and previews are not accessible during the
proprietary period.
Measurements of comet Halley in the spectral channel of IKS on board
the Vega-1 spacecraft. Data are retrieved from the PDS Small Bodies
Node data set (2011 reformatted version) and updated. The data set
consists in 101 tables providing the radiance spectrum of comet Halley
from various distances, plus two composite spectra. For details and
further references, see: Combes M. et al., 1988, The 2.5-12 micron
Spectrum of Comet Halley from the IKS-VEGA Experiment, Icarus, 76,
404-436 [1988Icar...76..404C]
