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R. F. Elsner (NASA MSFC), A. Bhardwaj (NRC-MSFC), R. Gladstone (SwRI), J. H. Waite (U. Mich.), T. Cravens (U. Kansas), P. Ford (MIT), G. Branduardi-Raymont, G. Ramsay (MSSL), B. D. Ramsey (NASA MSFC)
Chandra X-ray Observatory (CXO) and XMM-Newton observations of x-rays from the Jovian system have answered questions that arose from early observations with the Einstein and Rosat X-ray Observatories, but in the process of vastly increasing our knowledge of x-ray emission from Jupiter and its environs they have also raised new questions and point to new opportunities for future studies. We will review recent x-ray results on the Jovian system, from the point of view of the CXO, and discuss various questions that have arisen in the course of our studies. We will discuss prospects for more observations in the immediate future, and how they might address open questions. Finally we will briefly descibe ways in which an imaging x-ray spectrometer in the vicinity of the Jovian system could provide a wealth of data and results concerning Jupiter's x-ray auroral and disk emission, elemental abundance measurements for the Galilean moons, and detailed studies of x-ray emission from the Io Plasma Torus.
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Bulletin of the American Astronomical Society, 37 #3
© 2004. The American Astronomical Soceity.