Evidence of fragmenting dust particles from near-simultaneous optical and near-infrared photometry and polarimetry of comet 73P/Schwassmann-Wachmann 3

Terry Jay Jones, David Stark, Charles E. Woodward, Michael S. Kelley, Ludmilla Kolokolova, Dan Clemens, April Pinnick

Research output: Contribution to journalArticlepeer-review

15 Scopus citations

Abstract

We report imaging polarimetry of segments B and C of the Jupiter-family comet 73P/Schwassmann-Wachmann 3 in the I and H bandpasses at solar phase angles of approximately 35° and 85°. The level of polarization was typical for active comets, but larger than expected for a Jupiter-family comet. The polarimetric color was slightly red (δP/δλ = +1.2 0.4) at a phase angle of 35° and either neutral or slightly blue at a phase angle of 85°. Observations during the closest approach from 2006 May 11-13 achieved a resolution of 35 km at the nucleus. Both segments clearly depart from a 1/ρ surface brightness for the first 50-200 km from the nucleus. Simulations of radiation-driven dust dynamics can reproduce some of the observed coma morphology, but only with a wide distribution of initial dust velocities (at least a factor of 10) for a given grain radius. Grain aggregate breakup and fragmentation are able to reproduce the observed profile perpendicular to the Sun-comet axis, but fit the observations less well along this axis (into the tail). The required fragmentation is significant, with a reduction in the mean grain aggregate size by about a factor of 10. A combination of the two processes could possibly explain the surface brightness profile of the comet.

Original languageEnglish (US)
Pages (from-to)1318-1327
Number of pages10
JournalAstronomical Journal
Volume135
Issue number4
DOIs
StatePublished - Apr 1 2008

Keywords

  • Comets: individual (73P)
  • Techniques: polarimetric

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