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The Planetary X-ray Emission

  • Anil Bhardwaj
Conference paper
Part of the Astrophysics and Space Science Proceedings book series (ASSSP)

Abstract

With the advent of Chandra and XMM-Newton X-ray observatories, several new solar system bodies have been discovered to be an X-ray source at energies below 2 keV: leading to significant advances in the field of planetary X-ray emission and astronomy during the last one decade. Apart from the Sun, the known X-ray emitters now include Venus, Earth, Mars, Jupiter, and Saturn, planetary satellites (Moon, Io, Europa, and Ganymede), all active comets, the Io plasma torus, the rings of Saturn, the exospheres of Earth, Venus and Mars, and the heliosphere. Progress in modeling X-ray emission and laboratory studies of X-ray production have also greatly contributed in enhancing our understanding of X-rays from the solar system bodies. This chapter provides an overview of the planetary X-rays, their production source processes and important characteristics.

Keywords

Solar Wind Solar System Planetary Atmosphere Galilean Satellite Solar System Body 
These keywords were added by machine and not by the authors. This process is experimental and the keywords may be updated as the learning algorithm improves.

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Copyright information

© Springer-Verlag Berlin Heidelberg 2010

Authors and Affiliations

  1. 1.Space Physics LaboratoryVikram Sarabhai Space CentreTrivandrumIndia

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