Photometric analysis and disk-resolved thermal modeling of Comet 19P/Borrelly from Deep Space 1 data

To link to full-text access for this article, visit this link: http://dx.doi.org/10.1016/j.icarus.2006.11.015 Byline: Jian-Yang Li (a), Michael F. A'Hearn (a), Lucy A. McFadden (a), Michael J.S. Belton (b) Keywords: Comet Borrelly; Photometry Abstract: Images returned from the Deep Space 1 (DS-1) spacecraft during its encounter with Comet 19P/Borrelly are used to study its disk-integrated and disk-resolved photometry and its thermal properties. A disk-integrated phase function was constructed from a combination of DS-1 images and ground-based observations, giving a geometric albedo of 0.072[+ or -]0.020 and a phase slope of 0.043 magadeg.sup.-1. The shape model of Borrelly [Kirk, R.L., Howington-Kraus, E., Soderblom, L.A., Giese, B., Oberst, J., 2004a. Icarus 167, 54-69] and the ephemerides of DS-1 were used to analyze the disk-resolved photometric data with Hapke's theoretical model. It was found that the surface of Borrelly displays large photometric heterogeneities in its photometric parameters. The single-scattering albedo, w, varies by a factor of 2.5 with an average of 0.057[+ or -]0.009; the asymmetry factor, g, ranges from almost isotropic (-0.1) to strongly backscattering (-0.7) with an average of -0.43[+ or -]0.07; the roughness parameter, I[cedilla], is less than 35[degrees] for most parts of surface but ranges up to 55[degrees] in some areas. Its average is 22[degrees][+ or -]5[degrees]. The observed 1-D temperature profile is modeled well by the standard thermal model (STM) for inactive regions and is found to be consistent with a very low thermal inertia. Water sublimation in the source region of the fan jet is observed to decrease the surface temperature from the STM predictions by 20-40 K. The source areas of two collimated jets could not be determined from either photometric model or thermal model. It is evident that the fan jet activity occurring on Borrelly's surface can be correlated to areas of relatively high albedo, weak backscattering, and high roughness. Author Affiliation: (a) Department of Astronomy, University of Maryland, College Park, MD 20742, USA (b) Belton Space Exploration Initiatives, LLC, 430 S. Randolph Way, Tucson, AZ 85716, USA Article History: Received 14 February 2006; Revised 15 September 2006