First Scattered Light Images of Debris Disks around HD 53143 and HD 139664

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Published 2006 January 19 © 2006. The American Astronomical Society. All rights reserved. Printed in U.S.A.
, , Citation Paul Kalas et al 2006 ApJ 637 L57 DOI 10.1086/500305

1538-4357/637/1/L57

Abstract

We present the first scattered light images of debris disks around a K star (HD 53143) and an F star (HD 139664) using the coronagraphic mode of the Advanced Camera for Surveys (ACS) on board the Hubble Space Telescope (HST). With ages of 0.3-1 Gyr, these are among the oldest optically detected debris disks. HD 53143, viewed ~45° from edge-on, does not show radial variation in disk structure and has a width >55 AU. HD 139664 is seen close to edge-on and has a beltlike morphology with a dust peak 83 AU from the star and a distinct outer boundary at 109 AU. We discuss evidence for significant diversity in the radial architecture of debris disks that appears unconnected to stellar spectral type or age. HD 139664 and possibly the solar system belong in a category of narrow belts 20-30 AU wide. HD 53143 represents a class of wide-disk architecture with a characteristic width >50 AU.

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10.1086/500305