Mercury Mascons for the Cover of JGR Planets
A gravity map of Mercury shows mass concentrations (red) centered on the Caloris basin (center) and the Sobkou region (right limb).
This image appeared on the cover of the December, 2014 issue of Journal of Geophysical Research: Planets. In a lengthy article in the same issue, planetary scientist Erwan Mazarico and his co-authors describe their new and improved gravity map of Mercury, named HgM005. The map is based on a careful analysis of the orbit of the MESSENGER spacecraft. It shows variations in the strength of Mercury's gravity caused by mass concentrations, or mascons — dense lumps of material beneath the surface of the planet. The analysis also led to more accurate values for Mercury's tilt and the length of its day and allowed researchers to find stable near-circular orbits that could be used by future Mercury probes.
Credits
Please give credit for this item to:
NASA's Scientific Visualization Studio
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Data visualizer
- Ernie Wright (USRA)
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Scientist
- Erwan M. Mazarico (Massachusetts Institute of Technology)
Release date
This page was originally published on Friday, February 6, 2015.
This page was last updated on Wednesday, May 3, 2023 at 1:50 PM EDT.
Missions
This page is related to the following missions:Related papers
Mazarico, E., et al. (2015). The gravity field, orientation, and ephemeris of Mercury from MESSENGER observations after three years in orbit. J. Geophys. Res. Planets, 119, 2417–2436, doi:10.1002/2014JE004675.
Mazarico, E., et al. (2015). The gravity field, orientation, and ephemeris of Mercury from MESSENGER observations after three years in orbit. J. Geophys. Res. Planets, 119, 2417–2436, doi:10.1002/2014JE004675.
Datasets used
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Global Mosaic [MESSENGER: MDIS]
ID: 859 -
Global DTM [MESSENGER: MDIS]
ID: 860 -
HgM005 (HgM005 Gravity Map) [MESSENGER]
ID: 861
Note: While we identify the data sets used on this page, we do not store any further details, nor the data sets themselves on our site.