The Inhomogeneous Surface of Centaur 32522 Thereus (2001 PT 13 )

  • Licandro J
  • Pinilla-Alonso N
22Citations
Citations of this article
7Readers
Mendeley users who have this article in their library.

Abstract

Eight low-resolution near-infrared spectra (0.8-2.4 μm) of 32522 Thereus were obtained on 2002 August 28 from 0:30 to 5:30 UT, covering more than half of its rotation period, with the 3.56 m Telescopic Nazionale Galileo (TNG) at El Roque de los Muchachos Observatory (ORM, Canary Islands, Spain). All the spectra are red, probably due to a mantle of organic materials resulting from long-term irradiation. During at least 1.5 hr, the spectra clearly present the typical water ice absorption bands at 1.5 and 2.0 μm indicative of an inhomogeneous surface with a major concentration of water ice in part of it. One possible scenario is that a collision destroyed part of the irradiation mantle and moved ice from below to the surface, part of the material being vaporized over the surface by the impact. © 2005. The American Astronomical Society. All rights reserved.

Cite

CITATION STYLE

APA

Licandro, J., & Pinilla-Alonso, N. (2005). The Inhomogeneous Surface of Centaur 32522 Thereus (2001 PT 13 ). The Astrophysical Journal, 630(1), L93–L96. https://doi.org/10.1086/491469

Register to see more suggestions

Mendeley helps you to discover research relevant for your work.

Already have an account?

Save time finding and organizing research with Mendeley

Sign up for free