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Start Over Subject solar-system-astronomy Content Level Research
11. Mars Craters Lagain
ID:
ivo://jacobsuni/mars_craters_lagain/q/epn_core
Title:
Mars Craters Lagain
Short Name:
mars_craters_lag
Date:
07 Jun 2023 14:24:39
Publisher:
JacobsUni EPN node
Description:
A catalogue of Mars craters by Lagain et al. (2020), extending the previous catalogue from Robbins and Hynek (2012, DOI:10.1029/2011JE003966). 185 craters were added by Lagain, the object IDs are compatible with the previous work. Reference: "Impact cratering rate consistency test from ages of layered ejecta on Mars", Lagain et al., Planetary and Space Science, v.180. (2020) DOI: 10.1016/j.pss.2019.104755
12. mars_dust
ID:
ivo://lmd.jussieu/mars_dust/q/epn_core
Title:
mars_dust
Date:
19 Apr 2024 00:00:02
Publisher:
Laboratoire Méteorologie Dynamique
Description:
Mars_dust provides a multiannual climatology of Martian airborne dust as measured by various space missions. The retrieved column dust optical depth is mapped for each Martian year and formatted as cubes with time in the 3rd dimension. Two versions are available: irregularly gridded maps, and regular maps produced by kriging. These latter maps are used as column-integrated dust scenarios in the Mars Climate Database (MCD v5). The detailed description of the methodology and dataset can be found in: Montabone et al (2015) Icarus 251, pp. 65-95https://doi.org/10.1016/j.icarus.2014.12.034 ; Montabone et al (2020) JGR-Planets https://doi.org/10.1029/2019JE006111
13. mcd
ID:
ivo://lmd.jussieu/mcd/q/epn_core
Title:
mcd
Date:
28 Jan 2022 00:57:05
Publisher:
Laboratoire Méteorologie Dynamique
Description:
The database contains some outputs of the MCD for all the scenarios available, at different positions of latitude and longitude. These MCD outputs are provided as Votables containing profiles of temperatures, pressures, density and abundances of O2 and O3 for altitudes between 0 and 249.5 km from the surface.
14. MCD
ID:
ivo://lmd.jussieu/mcd/q/collection
Title:
MCD
Date:
26 Aug 2021 09:44:39
Publisher:
Laboratoire Méteorologie Dynamique
Description:
MCD is a database of atmospheric statistics compiled from Global Climate Model (GCM) numerical simulation of Martian atmosphere (<a href=http://www-mars.lmd.jussieu.fr>http://www-mars.lmd.jussieu.fr</a>). The GCM computes in 3D the atmospheric circulation and climate taking into account radiative transfer through the gaseous atmospheres and the dust and ice aerosols, includes a representation of the CO2 ice condensation and sublimation on the ground and in the atmosphere, simulates the water cycle (with modelling of cloud microphysics), the dust multisize particle transport, the atmospheric composition controlled by the photochemistry and the local non-condensible gas enrichment and depletion induced by CO2 condensation and sublimation, and has been extended into the thermosphere and to model ionospheric processes (due to chemistry). The database extends up to exobase (the top of the thermosphere, roughly at 300km in altitude); in addition to statistics on temperature, wind, pressure, radiative fluxes, it provides data such as atmospheric composition (including dust water vapor and ice content) and make use of 'dust and Extreme Ultra Violet (EUV) scenarios' to represent the variation of dust in the atmosphere and solar EUV conditions. User Manual of the service : <a href=http://vo.lmd.jussieu.fr:8080/MCD_VESPA_service_user_manual.pdf>User Manual of the service </a> .
15. Mercury craters
ID:
ivo://padc.obspm.planeto/mercury_craters/q/epn_core
Title:
Mercury craters
Short Name:
mercury_craters.
Date:
16 Jul 2024 13:55:03
Publisher:
Paris Astronomical Data Centre - LESIA
Description:
Mercury crater catalogue
16. Predictions of stellar occultations by the main planetary satellites
ID:
ivo://padc.obspm.planeto/voccdb/q/epn_core
Title:
Predictions of stellar occultations by the main planetary satellites
Short Name:
voccdb.epn_core
Date:
26 Feb 2025 14:03:55
Publisher:
Paris Astronomical Data Centre
Description:
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.
17. PRETHARSIS
ID:
ivo://geops.ipsl/pretharsis/q/epn_core
Title:
PRETHARSIS
Short Name:
pretharsis.epn_c
Date:
17 Jul 2024 15:25:23
Publisher:
IPSL/GEOPS
Description:
"The growth of the Tharsis volcanic complex on Mars during Noachian/Hesperian era induced a reorientation of the spin axis of the planet (true polar wander). This service gives access to a map of Mars topography before Tharsis formation (Early Noachian) and a map of Mars topography before true polar wander (Late Noachian/Early Esperian), from the model described in Bouley, S., Baratoux, D., Matsuyama, I. et al. Late Tharsis formation and implications for early Mars. Nature 531, 344–347 (2016). https://doi.org/10.1038/nature17171 ."
18. SPICAM
ID:
ivo://latmos.ipsl/spicam/q/epn_core
Title:
SPICAM
Short Name:
spicam.epn_core
Date:
02 May 2022 14:11:03
Publisher:
Laboratoire Atmosphères, Milieux, Observations Spatiales
Description:
The database contains profiles of atmospheric CO2 density and temperature derived thereof, and ozone concentration profiles, all derived from the first year(s) of SPICAM UV stellar occultation observations (Forget et al. 2009, Lebonnois et al. 2006). The database also includes the full dataset of four Martian years of aerosol extinction profiles from SPICAM UV solar occultations (Määttänen et al. 2013).
19. Terrestrial impact craters
ID:
ivo://padc.obspm.planeto/terrestrial_impact_craters/q/epn_core
Title:
Terrestrial impact craters
Short Name:
terrestrial_impa
Date:
26 Feb 2025 13:36:59
Publisher:
PADC
Description:
Terrestrial Impact Craters
20. TNOs fluxes measured from space
ID:
ivo://padc.obspm.planeto/tnosarecool/q/epn_core
Title:
TNOs fluxes measured from space
Short Name:
TNOsarecool
Date:
16 Jul 2024 13:55:03
Publisher:
Paris Astronomical Data Centre - LESIA
Description:
This service lists TNO thermal properties as derived mostly from Spitzer and Herschel observations.