Please use this identifier to cite or link to this item:
Title: Magnetosphere-ionosphere coupling at Jupiter-like exoplanets with internal plasma sources: implications for detectability of auroral radio emissions
Authors: Nichols, Jonathan D.
First Published: 31-Mar-2011
Publisher: Blackwell Publishing on behalf of the Royal Astronomical Society
Citation: Monthly Notices of the Royal Astronomical Society, 2011, 414 (3), pp. 2125-2138
Abstract: In this paper we provide the first consideration of magnetosphere–ionosphere coupling at Jupiter-like exoplanets with internal plasma sources such as volcanic moons. We estimate the radio power emitted by such systems under the condition of near-rigid corotation throughout the closed magnetosphere, in order to examine the behaviour of the best candidates for detection with next generation radio telescopes. We thus estimate for different stellar X-ray–UV (XUV) luminosity cases the orbital distances within which the ionospheric Pedersen conductance would be high enough to maintain near-rigid corotation, and we then consider the magnitudes of the large-scale magnetosphere-ionosphere currents flowing within the systems, and the resulting radio powers, at such distances. We also examine the effects of two key system parameters, i.e. the planetary angular velocity and the plasma mass outflow rate from sources internal to the magnetosphere. In all XUV luminosity cases studied, a significant number of parameter combinations within an order of magnitude of the jovian values are capable of producing emissions observable beyond 1 pc, in most cases requiring exoplanets orbiting at distances between ∼1 and 50 au, and for the higher XUV luminosity cases these observable distances can reach beyond ∼50 pc for massive, rapidly rotating planets. The implication of these results is that the best candidates for detection of such internally generated radio emissions are rapidly rotating Jupiter-like exoplanets orbiting stars with high XUV luminosity at orbital distances beyond ∼1 au, and searching for such emissions may offer a new method of detection of more distant-orbiting exoplanets.
DOI Link: 10.1111/j.1365-2966.2011.18528.x
ISSN: 0035-8711
eISSN: 1365-2966
Version: Publisher Version
Status: Peer-reviewed
Type: Journal Article
Rights: Copyright © 2011 The Author. Monthly Notices of the Royal Astronomical Society Copyright © 2011 RAS. Deposited with reference to the Journal Exclusive Licence Form, which permits posting of the Blackwell Publishing PDF version of the article on the author's employer's repository six months after publication. The definitive version is available at
Appears in Collections:Published Articles, Dept. of Physics and Astronomy

Files in This Item:
File Description SizeFormat 
j.1365-2966.2011.18528.x[1].pdfPlease select a version963.43 kBAdobe PDFView/Open

Items in LRA are protected by copyright, with all rights reserved, unless otherwise indicated.