Albedos of Small Hilda Group Asteroids as Revealed by Spitzer
arXiv:1103.0724 · doi:10.1088/0004-6256/141/6/186
Abstract
We present thermal 24 m observations from the \textit{Spitzer Space Telescope} of 62 Hilda asteroid group members with diameters ranging from 3 to 12 kilometers. Measurements of the thermal emission when combined with reported absolute magnitudes allow us to constrain the albedo and diameter of each object. From our \textit{Spitzer} sample, we find the mean geometric albedo, 0.07 0.05 for small (D 10 km) Hilda group asteroids. This value of is greater than and spans a larger range in albedo space than the mean albedo of large (D 10 km) Hilda group asteroids which is 0.04 0.01. Though this difference may be attributed to space weathering, the small Hilda group population reportedly displays greater taxonomic range from C-, D- and X-type whose albedo distributions are commensurate with the range of determined albedos. We discuss the derived Hilda size-frequency distribution, color-color space, and geometric albedo for our survey sample in the context of the expected migration induced "seeding" of the Hilda asteroid group with outer solar system proto-planetesimals as outlined in the "Nice" formalism.
34 pages, 6 figures. Submitted to Astronomical Journal
References in corpus (9)
- Origin of the Structure of the Kuiper Belt during a Dynamical Instability in the Orbits of Uranus and Neptune
- Thermal inertia of near-Earth asteroids and implications for the magnitude of the Yarkovsky effect
- High Albedos of Low Inclination Classical Kuiper Belt Objects
- Absolute Calibration and Characterization of the Multiband Imaging Photometer for Spitzer. III. An Asteroid-based Calibration of MIPS at 160 microns
- Thermal inertia of main belt asteroids smaller than 100 km from IRAS data
- Rectified Asteroid Albedos and Diameters from IRAS and MSX
- Asteroid families in the first order resonances with Jupiter
- Albedos of Main-Belt Comets 133P/Elst-Pizarro and 176P/LINEAR
- Albedos of Small Jovian Trojans