Currently, sci.esa.int is under review and not being updated. For the latest information and news from ESA science missions and scientific results, please visit esa.int. For a comprehensive overview of ESA’s Science Programme and its missions, please refer to science.esa.int. For in-depth technical information aimed at ESA's scientific communities, you may also wish to consult cosmos.esa.int.

Asset Publisher

Back The Surface Composition of Mercury from Ultraviolet-Visible-Infrared Spectroscopy: State of the Art and Future Strategies

The Surface Composition of Mercury from Ultraviolet-Visible-Infrared Spectroscopy: State of the Art and Future Strategies

Start date: 04 Jun 2009
Address: University of Parma, Parma, Italy

More info: http://www.mbc09.unipr.it/

The two successful MESSENGER flybys of Mercury in 2008 and the planned BepiColombo mission challenge the planetary community to develop strategies for an effective and timely interpretation of spectral reflectance and emissivity data in terms of mineral composition and geologic significance for the innermost planet.

Last Update: 1 September 2019
24-Jan-2026 17:38 UT

ShortUrl Portlet

Shortcut URL

https://sci.esa.int/s/wV6Vj7w

Images And Videos

Related Publications

Related Links

See Also

Documentation