Epoch 2009 June 18.0 TT = JDT 2455000.5 MPC M 331.00417 (2000.0) P Q n 0.23004263 Peri. 91.25031 +0.99832235 -0.03147896 a 2.6379334 Node 270.55507 +0.00956789 +0.91744867 e 0.6243026 Incl. 2.78557 +0.05710466 +0.39660687 P 4.28 H 15.99 G 0.15 U 1 From 152 observations at 9 oppositions, 1949-2002
Comet 107P (4015) Wilson-Harrington Comet Wilson-Harrington is a periodic comet (formally designated 107P/Wilson-Harrington). Little known about it distinguishes it from other comets, but for the fact that it is also designated an asteroid, 4015 Wilson-Harrington (which, incidentally, is currently the longest asteroid name with 17 characters).
Title: Spitzer observations of the asteroid-comet transition object and potential spacecraft target 107P (4015) Wilson-Harrington Authors: J. Licandro, H. Campins, M. Kelley, Y. Fernandez, M. Delbo, W. T. Reach, O. Groussin, P. L. Lamy, I. Toth, M. F. A'Hearn, J. M. Bauer, S. C. Lowry, A. Fitzsimmons, C. M. Lisse, K. J. Meech, J. Pittichova, C. Snodgrass, H. A. Weaver
Context. Near-Earth asteroid-comet transition object 107P/ (4015) Wilson-Harrington is a possible target of the joint European Space Agency (ESA) and Japanese Aerospace Exploration Agency (JAXA) Marco Polo sample return mission. Physical studies of this object are relevant to this mission, and also to understanding its asteroidal or cometary nature. Aims. Our aim is to obtain significant new constraints on the surface thermal properties of this object. Methods. We present mid-infrared photometry in two filters (16 and 22 microns) obtained with NASA's Spitzer Space Telescope on February 12, 2007, and results from the application of the Near Earth Asteroid Thermal Model (NEATM).We obtained high S/N in two mid-IR bands allowing accurate measurements of its thermal emission. Results. We obtain a well constrained beaming parameter (eta = 1.39 ±0.26) and obtain a diameter and geometric albedo of D = 3.46 ±0.32 km, and pV = 0.059 ±0.011. We also obtain similar results when we apply this best-fitting thermal model to single-band mid-IR photometry reported by Campins et al. (1995), Kraemer et al. (2005) and Reach et al. (2007). Conclusions. The albedo of 4015 Wilson-Harrington is low, consistent with those of comet nuclei and primitive C-, P-, D-type asteroids. We establish a rough lower limit for the thermal inertia of W-H of 60 Jm^-2s^(-0.5)K^-1 when it is at r=1AU, which is slightly over the limit of 30 Jm^-2s^(-0.5)K-1 derived by Groussin et al. (2009) for the thermal inertia of the nucleus of comet 22P/Kopff.