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Discovery of the Atomic Iron Tail of Comet MCNaught Using the Heliospheric Imager on STEREO - IOPscience

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Discovery of the Atomic Iron Tail of Comet MCNaught Using the Heliospheric Imager on STEREO

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Published 2007 April 27 © 2007. The American Astronomical Society. All rights reserved. Printed in U.S.A.
, , Citation M. Fulle et al 2007 ApJ 661 L93 DOI 10.1086/518719

1538-4357/661/1/L93

Abstract

In 2007 January, at the heliocentric distance r < 0.3 AUえーゆー, comet McNaught 2006P1 became the brightest comet since C/Ikeya-Seki 1965S1 and was continuously monitored by space-based solar observatories. We provide strong evidence that an archlike tail observed by the Heliospheric Imager aboard the STEREO spacecraft is the first ever detected tail composed of neutral Fe atoms. We obtain an Fe lifetime τたう = (4.1 ± 0.4) × 104 s at r = 0.25 AUえーゆー, in agreement with theoretical predictions of the photoionization lifetime. The expected dust temperature is inconsistent with iron sublimation, suggesting that Fe atoms are coming from troilite evaporation.

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10.1086/518719