- ID:
- ivo://padc.obspm.planeto/hst_planeto/q/epn_core
- Title:
- HST observations of planets and satellites
- Short Name:
- HST Planeto
- Date:
- 07 May 2024 03:01:53
- Publisher:
- Paris Astronomical Data Centre - LESIA
- Description:
- 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.
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2. PRETHARSIS
- ID:
- ivo://geops.ipsl/pretharsis/q/epn_core
- Title:
- PRETHARSIS
- Short Name:
- pretharsis.epn_c
- Date:
- 01 May 2024 01:20:23
- 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, 344â347 (2016). https://doi.org/10.1038/nature17171 ."
3. 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
4. Mars Craters
- ID:
- ivo://padc.obspm.planeto/mars_craters/q/epn_core
- Title:
- Mars Craters
- Short Name:
- mars_craters.epn
- Date:
- 17 Apr 2024 13:17:11
- Publisher:
- Paris Astronomical Data Centre - Constructor University
- Description:
- 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
- ID:
- ivo://padc.obspm.planeto/mars_craters_lagain/q/epn_core
- Title:
- Mars Craters Lagain
- Short Name:
- mars_craters_lag
- Date:
- 17 Apr 2024 13:07:37
- Publisher:
- Paris Astronomical Data Centre - Constructor University
- 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
- ID:
- ivo://bira-iasb/gem_mars/q/epn_core
- Title:
- GEM-Mars GCM profiles
- Short Name:
- gem_mars.epn_cor
- Date:
- 28 Oct 2023 16:50:48
- Publisher:
- Planetary Atmospheres Research Unit - Royal Belgian Institute for Space Aeronomy
- Description:
- Profiles of pressure, temperature and species of the Martian atmosphere simulated with the GEM-Mars general circulation model. See for the main model descritpion Neary, L., et al. 2018. The GEM-Mars general circulation model for Mars: Description and evaluation. Icarus 300, 458-476. https://doi.org/10.1016/j.icarus.2017.09.028. See for the chemistry description Dearden, F. et al., 2019, Mars atmospheric chemistry simulations with the GEM-Mars general circulation model, Icarus, 326, 197-224, https://doi.org/10.1016/j.icarus.2019.02.030.
- ID:
- ivo://bira-iasb/nomad/q/epn_core
- Title:
- Mars atmospheric profiles - From NOMAD/TGO
- Short Name:
- nomad.epn_core
- Date:
- 28 Oct 2023 16:48:34
- Publisher:
- Planetary Atmospheres Research Unit - Royal Belgian Institute for Space Aeronomy
- Description:
- Profiles of pressure, temperature and species of the Martian atmosphere derived from measurements of the NOMAD instrument on board ESA's Trace Gas Orbiter. See paper https://doi.org/10.1007/s11214-018-0517-2
- ID:
- ivo://padc.obspm.planeto/bdip/q/epn_core
- Title:
- Planetary Images Database
- Short Name:
- BDIP
- Date:
- 23 Nov 2022 15:28:18
- Publisher:
- Paris Astronomical Data Centre
- Description:
- Planetary Images Database
- ID:
- ivo://padc.obspm.planeto/bdip/q/observatories
- Title:
- Planetary Images Database
- Short Name:
- bdip.observatori
- Date:
- 23 Nov 2022 15:28:18
- Publisher:
- Paris Astronomical Data Centre
- Description:
- Observatory names
10. 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).