Hubble Space Telescope NICMOS Multiband Photometry of Proteus and Puck

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© 2003. The American Astronomical Society. All rights reserved. Printed in U.S.A.
, , Citation Christophe Dumas et al 2003 AJ 126 1080 DOI 10.1086/375909

1538-3881/126/2/1080

Abstract

We report 1.1–2.4 μm multiband photometry of the small Uranian satellites Puck and Portia and of the small Neptunian satellite Proteus obtained with the Hubble Space Telescope and its near-infrared camera NICMOS. The surface of Puck (and likely Portia) displays an absorption feature matching the 2.0 μm band of water ice. In the case of Proteus, a shallower absorption is detected in the long-wavelength region of the spectrum. Although water ice cannot be entirely ruled out, this feature could also be produced by C–H– or C≡N–bearing material. Future spectroscopic observations at high angular resolution are needed to further investigate the nature of the compounds covering the surface of the small moons of Uranus and Neptune.

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10.1086/375909