Letter

Nature 435, 790-794 (9 June 2005) | doi:10.1038/nature03603; Received 3 February 2005; Accepted 29 March 2005

Discovery of an aurora on Mars

Jean-Loup Bertaux1, François Leblanc1, Olivier Witasse2, Eric Quemerais1, Jean Lilensten3, S. A. Stern4, B. Sandel5 & Oleg Korablev6

  1. Service d'Aéronomie du CNRS/IPSL, BP 3, Verrières-le-Buisson, 91371, France
  2. ESA-ESTEC, Postbus 299, NL 2200AG, Noordwijk, The Netherlands
  3. Laboratoire de Planétologie de Grenoble, CNRS, Université J. Fourier, B.P. 53, 38041, Grenoble, France
  4. Southwest Research Institute, 1050 Walnut Street, Boulder, Colorado 80302, USA
  5. Lunar and Planetary Laboratory, 1541 E. University Boulevard, University of Arizona, Tucson, Arizona 85721, USA
  6. Space Research Institute (IKI), 84/32 Profsoyuznaya, 117810 Moscow, Russia

Correspondence to: Jean-Loup Bertaux1 Correspondence and requests for materials should be addressed to J.-L.B. (Email: bertaux@aerov.jussieu.fr).

In the high-latitude regions of Earth, aurorae are the often-spectacular visual manifestation of the interaction between electrically charged particles (electrons, protons or ions) with the neutral upper atmosphere, as they precipitate along magnetic field lines. More generally, auroral emissions in planetary atmospheres "are those that result from the impact of particles other than photoelectrons" (ref. 1). Auroral activity has been found on all four giant planets possessing a magnetic field (Jupiter2, Saturn3, Uranus4 and Neptune5), as well as on Venus, which has no magnetic field6. On the nightside of Venus, atomic O emissions at 130.4 nm and 135.6 nm appear in bright patches of varying sizes and intensities6, which are believed to be produced by electrons with energy <300 eV (ref. 7). Here we report the discovery of an aurora in the martian atmosphere, using the ultraviolet spectrometer SPICAM on board Mars Express. It corresponds to a distinct type of aurora not seen before in the Solar System: it is unlike aurorae at Earth and the giant planets, which lie at the foot of the intrinsic magnetic field lines near the magnetic poles, and unlike venusian auroras, which are diffuse, sometimes spreading over the entire disk. Instead, the martian aurora is a highly concentrated and localized emission controlled by magnetic field anomalies in the martian crust.

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