The High-Albedo Kuiper Belt Object (55565) 2002 AW197

Details The High-Albedo Kuiper Belt Object (55565) 2002 AW197 The High-Albedo Kuiper Belt Object (55565) 2002 AW197

May 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005apj...624l..53c&link_type=abstract

The Astrophysical Journal, Volume 624, Issue 1, pp. L53-L56.

Astronomy and Astrophysics

Astronomy

15

Infrared: Solar System, Kuiper Belt, Minor Planets, Asteroids

Scientific paper

We detected thermal emission from the Kuiper Belt object 2002 AW197 in 2003 December and again in 2004 April using the Multiband Imaging Photometer on the Spitzer Space Telescope. In combination with the absolute visual magnitude, the thermal measurements indicate a geometric albedo of 0.17+/-0.03 and a diameter of 700+/-50 km. The albedo of 2002 AW197 is significantly higher than the 0.04 value typically assumed for trans-Neptunian objects, and consequently the object is smaller than previously thought based on that assumption. Our thermal measurements at two wavelengths (24 and 70 μm) allow us to constrain the surface temperature and thereby place constraints on the thermal inertia. We find that the standard thermal model (STM) is inconsistent with the 24/70 μm color unless we set the beaming parameter η>0.95, indicating that the object has a significant thermal inertia and, therefore, that the STM is inappropriate. The other end-member thermal inertia model is the fast-rotator, or isothermal-latitude, model (ILM). The data are well represented by an ILM with the pole of rotation inclined to the Sun by 45deg+/-10deg. The high albedo is consistent with a surface containing significant amounts of weakly absorbing materials, with ices and/or fine-grained silicates as likely candidates.

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