Comet C/2011 L4 (PanStarrs): Small nucleus, fast rotator and dust rich comet observed after perihelion
Toni Scarmato

TL;DR
This paper reports detailed observations of comet C/2011 L4 (PanStarrs), revealing a small nucleus, rapid rotation, and dust-rich coma, providing new insights into its physical characteristics after perihelion.
Contribution
It presents the first detailed observational analysis of C/2011 L4's nucleus size, rotation period, and dust production, highlighting its unique physical properties.
Findings
Small nucleus size estimated from observations
Fast rotation period determined
Dust production rate characterized
Abstract
Orbital elements of C2011 L4 (PanStarrs) Oort cloud comet, computed by MPC (Minor Planet Center, Minor Planet Electronic Circular 2012-T08), show that the closest approach to the Sun occurred on 2013 March 10th, at about 0.3 A.U., then about 4,51x10^7 km. Discovered by Richard Wainscoat (Institute for Astronomy, University of Hawaii) on four CCD images taken with the 1.8-m "Pan-STARRS 1" telescope at Haleakala taken on 2011 June 6th. My first observation of the comet was on 2013 March 10th whit the comet visible in the twilight. I did the following visual estimation; Mar. 10.73,-1.0*,5'(T. Scarmato, Calabria, Italy, 7x50 binoculars; altitude 7 deg, tail 1 deg in pa 140 deg), reported to the ICQ (International Comet Quarterly). Easy comet in 7x50 binoculars I started to see C/2011 L4 at 18:35 L.T. when the comet was at about 7{\deg} above the horizon. I saw a tail long about 1,5{\deg} in…
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Taxonomy
TopicsAstro and Planetary Science · Stellar, planetary, and galactic studies · Scientific Research and Discoveries
