Estimating The Dust Particle Size Of Comet Hale Bopp By Studying The Motion Of The Ejecta On September 10 11, 1996

Details Estimating The Dust Particle Size Of Comet Hale Bopp By Studying The Motion Of The Ejecta On September 10 11, 1996 Estimating The Dust Particle Size Of Comet Hale Bopp By Studying The Motion Of The Ejecta On September 10 11, 1996

Apr 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002em%26p...88...61q&link_type=abstract

Earth, Moon, and Planets, v. 88, Issue 2, p. 61-74 (2002).

Astronomy and Astrophysics

Astronomy

Comet Hale-Bopp, Kinematics, Outburst, Comet Hale&Ndash, Bopp

Scientific paper

We report the observation of an outburst of comet Hale Bopp (C/1995 O1) happened on September 10 11, 1996, carried by the 1.56 m telescope of Shanghai Astronomical Observatory. Two ejecta were found in CCD images during the outburst. According to the positions of ejecta, we discuss the motion of the ejecta considering dust particles are subjected to the gravity and the Solar radiation pressure, and conclude that the mean radii of dust grains in the ejecta were about submicron-sized. So the observed X-ray emission are most likely produced by small size particles scattering the Solar X-ray.

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