A New Analysis of Spitzer Observations of Comet 29P/Schwassmann-Wachmann 1
Charles A. Schambeau, Yanga R. Fernandez, Carey M. Lisse, Nalin, Samarasinha, and Laura M. Woodney

TL;DR
This paper reanalyzes Spitzer observations of comet 29P/Schwassmann-Wachmann 1 using updated data processing, revealing new nucleus measurements and detailed dust composition analysis, improving understanding of this comet's properties.
Contribution
It provides a new analysis with advanced image processing, incorporating previously unobserved data, and offers refined measurements of the comet's nucleus and dust composition.
Findings
Nucleus radius measured at 30.2 km
Infrared beaming parameter of 0.99
Dust mainly composed of amorphous ferromagnesian silicates
Abstract
We present a new analysis of observations of comet 29P/Schwassmann-Wachmann 1 taken on UT 2003 November 21, 23, and 24, similar to a previous investigation of the observations (Stansberry et al. 2004), but using the most recent data pipeline products and intensive image processing techniques. Analysis of images from the IRAC 5.8 & 8.0 m bands and the MIPS 24.0 & 70.0 m bands resulted in photometry measurements of the nucleus after a suite of coma modeling and removal processes were implemented. SW1 was not identified in the 5.8 m image from the previous work so its incorporation into this analysis is entirely new. Using the Near Earth Asteroid Thermal Model (Harris 1998) resulted in a nucleus radius measurement of = 30.2 km and an infrared beaming parameter value of . We also measured an…
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