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arXiv · 1410.5084

The Main-Belt Comets: The Pan-STARRS1 Perspective

Henry H. Hsieh·Larry Denneau·Richard J. Wainscoat·Norbert Schorghofer·Bryce Bolin·Alan Fitzsimmons·Robert Jedicke·Jan Kleyna·Marco Micheli·Peter Veres·Nicholas Kaiser·Kenneth C. Chambers·William S. Burgett·Heather Flewelling·Klaus W. Hodapp·Eugene A. Magnier·Jeffrey S. Morgan·Paul A. Price·John L. Tonry·Christopher Waters
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Abstract

We analyze 760475 observations of 333026 main-belt objects obtained by the Pan-STARRS1 (PS1) survey telescope between 2012 May 20 and 2013 November 9, a period during which PS1 discovered two main-belt comets, P/2012 T1 (PANSTARRS) and P/2013 R3 (Catalina-PANSTARRS). PS1 comet detection procedures currently consist of the comparison of the point spread functions (PSFs) of moving objects to those of reference stars, and the flagging of objects that show anomalously large radial PSF widths. Based on the number of missed discovery opportunities among comets discovered by other observers, we estimate an upper limit comet discovery efficiency rate of ~70% for PS1. Additional analyses that could improve comet discovery yields in future surveys include linear PSF analysis, modeling of trailed stellar PSFs for comparison to trailed moving object PSFs, searches for azimuthally localized activity, comparison of point-source-optimized photometry to extended-source-optimized photometry, searches for photometric excesses in objects with known absolute magnitudes, and crowd-sourcing. Analysis of PS1 survey statistics indicates an expected fraction of 59 MBCs per 10^6 outer main-belt asteroids, and a 95% confidence upper limit of 96 MBCs per 10^6 outer main-belt asteroids. We note that more sensitive future surveys could detect many more MBCs than estimated here. We find an excess of high eccentricities (0.1 < e < 0.3) among all known MBCs relative to the background asteroid population. Theoretical calculations show that, given these eccentricities, the sublimation rate for a typical MBC is orders of magnitude larger at perihelion than at aphelion, providing a plausible physical explanation for the observed behavior of MBCs peaking in observed activity strength near perihelion.

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Henry H. Hsieh, Larry Denneau, Richard J. Wainscoat, Norbert Schorghofer, Bryce Bolin, Alan Fitzsimmons, Robert Jedicke, Jan Kleyna, Marco Micheli, Peter Veres, Nicholas Kaiser, Kenneth C. Chambers, William S. Burgett, Heather Flewelling, Klaus W. Hodapp, Eugene A. Magnier, Jeffrey S. Morgan, Paul A. Price, John L. Tonry, Christopher Waters. 2014-10-19. The Main-Belt Comets: The Pan-STARRS1 Perspective. https://doi.org/10.1016/j.icarus.2014.10.031

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