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PADC TAP Server on voparis-tap-planeto.obspm.fr TAP service
The PADC TAP Server on voparis-tap-planeto.obspm.fr's TAP end point. The Table Access Protocol (TAP) lets you execute queries against our database tables, inspect various metadata, and upload your own data. It is thus the VO's premier way to access public data holdings. Tables exposed through this endpoint include: epn_core from the apis schema, epn_core from the basecom schema, epn_core from the crism_speclib schema, epn_core from the dynastvo schema, epn_core from the exoplanet schema, epn_core from the gmap schema, epn_core from the hst_planeto schema, epn_core from the iks schema, epn_core from the lunar_craters schema, epn_core from the m4ast schema, epn_core from the mars_craters schema, epn_core from the mars_craters_lagain schema, epn_core from the mercury_craters schema, epn_core from the meteor_showers schema, epn_core from the moonsprop schema, epn_core from the pds_speclib schema, epn_core from the planets schema, epn_core from the spectro_asteroids schema, epn_core from the spectro_m_ast schema, epn_core from the spectro_planets schema, epn_core from the spectro_stars schema, epn_core from the spectro_trojans schema, columns, groups, key_columns, keys, schemas, tables from the tap_schema schema, epn_core from the terrestrial_impact_craters schema, epn_core from the titan_profiles schema, epn_core from the usgs_wms schema, epn_core from the venus_craters schema, epn_core from the vims_satellites schema, epn_core from the vir_ros schema, epn_core from the voccdb schema, epn_core from the vros_geocor schema, epn_core from the vvex_db schema, epn_core from the vvex schema.
Abundancy Vertical Profile at Titan with Cassini/CIRS
EPNcore table for temperature, pressure and element abundance profiles in Titan's atmosphere.
Auroral Planetary Imaging and Spectroscopy
EpnCore table for APIS service
CRISM spectral library
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
Cassini VIMS
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.
Characteristics of Planets
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].
DynastVO ephemeris service
This database displays calculated orbital parameters for small bodies
Exoplanet Catalog
Encyclopedia of extrasolar planet
GMAP
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 and satellites
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.
IKS
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]
Lunar craters (demo)
Lunar crater catalogue
M4AST
compiled database for asteroid spectra in the visible and NIR regions
Mars Craters
The Mars Crater Catalog by S.J. Robbins was generated from THEMIS Daytime IR and Viking MDIM 2.1 global mosaics of Mars. Craters were selected using 5 points along the rim. The table is statistically complete to the diameter of ~1.0 km. The table contains morphologic and morphometric data for craters with diameter larger than 3 km. The Prometheus basin has been excluded from the Catalog due to technical issues. Reference: "A New Global Database of Mars Impact Craters ≥1 km: (1) Database Creation, Properties, and Parameters", S.J. Robbins and B.M. Hynek, Journal of Geophysical Research - Planets, v.117. (2012) DOI: 10.1029/2011JE003966
Mercury craters
Mercury crater catalogue
Predictions of stellar occultations by the main planetary satellites
The VOccDB database provides prediction and parameters of stellar occultations by the main planetary satellites. Observations of a stellar occultations help to better determine the size and the shape of the occulting body, as well as its astrometric position at the milli-arcsecond level precision. Only the main moons of giant planets Jupiter, Saturn, Uranus and Neptune are considered in the event prediction database. Predictions are provided over period 2023-2032, up to visual magnitude 12 for the biggest satellites, and magnitude 14 for other satellites. For each stellar occultation event prediction, the database provides circumstances and observational data, date and timing of the occultation, star position and magnitude, excepted duration, etc.
Properties of natural satellites
This service provides the physical and dynamical characteristics of natural satellites in the Solar System: size, mass, rotational properties, magnitude and albedo, orbital elements. These quantities are taken from various publications listed under the bib_reference parameter. These data will be updated as new values are published.
Spectra of asteroids from VizieR
This service provides a compilation of spectra of asteroids in the visible and NIR range. It is composed of various libraries distributed as VizieR catalogues. Reformatted VOtable or fits versions are provided with thumbnails. Ephemeris data are retrieved from Miriade (IMCCE) for the reference date when possible.
Spectra of planets
This service provides a compilation of global spectra of planets and satellites in the visible and NIR range, for quick reference purpose. It is made from various libraries, including the Tohoku-Hiroshima-Nagoya Planet Spectra Library (Lundock et al 2009) and spectra from a USGS web site (R. Clark). Reformatted VOtable versions are provided together with links to the original data.
Stellar spectra
The stellar spectra service is a compilation of several libraries distributed by large observatories, which are intended to calibrate telescopic observations. It currently provides access to two libraries of reference stars distributed by ESO (composite spectra: https://www.eso.org/sci/observing/tools/standards/IR_spectral_library.html) and NASA IRTF (observations from SpeX: http://irtfweb.ifa.hawaii.edu/~spex/IRTF_Spectral_Library/References_files/All.html).
Terrestrial impact craters
Terrestrial Impact Craters
USGS_WMS
Catalogue of USGS Astrogeology WMS Map Layers
VIRTIS Rosetta cometary phase (demo)
Spectroscopy of comet 67P
VIRTIS Rosetta geometry corrected products
Spectroscopy of comet 67P, recalibrated
VIRTIS Venus Express nominal mission
Spectroscopy of Venus
VOEvent meteor shower service
The ephemeris were produced by simulating the ejection of meteoroids from the sunlit hemisphere of cometary nuclei, typically from 0 to 3 au, followed by the propagation of orbits of meteoroids in the Solar System, taking into account the gravity of the Sun, the 8 planets, Pluto, and the Moon, as well as the radiation pressure and the Poynting-Robertson drag. Note that asteroid parent bodies were considered as active (i.e. comet-like bodies) even if they are not active today. The showers are predicted when a planet enters a large enough set of meteoroids, at a distance less than typically 0.01 au. See Vaubaillon J., Colas F., Jorda L. 2005 A new method to predict meteor showers. I. Description of the model, Astronomy and Astrophysics, Volume 439/2 p.751-760, as well as: Vaubaillon J. 2017 A confidence index for forecasting of meteor showers, Planetary and Space Science, Volume 143 p.78-82
Venus craters
Venus crater catalogue