Planetary Atmospheres Research Unit - Royal Belgian Institute for
Space Aeronomy
Description:
Derived data from measurements of the NOMAD instrument on board ESA's
Trace Gas Orbiter. For more info on NOMAD, see Vandaele et al. (2018)
https://doi.org/10.1007/s11214-018-0517-2 Vertical profiles of CO2
density and temperature of the Martian atmosphere: See papers Trompet
et al. (2023a,b) https://doi.org/10.1029/2022JE007277,
https://doi.org/10.1029/2022JE007279. Vertical profiles of H2O
density: see paper Aoki et al. (2022)
https://doi.org/10.1029/2022JE007231. Vertical profiles of O3 density:
see paper Piccialli et al. (2022) https://doi.
org/10.1029/2022EA002429 Vertical profiles of aerosols: see paper
Flimon et al. (in rev.)
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
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
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
2MASS has uniformly scanned the entire sky in three near-infrared bands to detect and characterize point sources brighter than about 1 mJy in each band, with signal-to-noise ratio (SNR) greater than 1.
This collection contains the MAVEN mission events file including
events from the MAVEN Payload Operations Center events database, and
MAVEN science events
