The activity of comet C/2007 D1 (LINEAR) at 9.7 AU from the Sun

被引:28
作者
Epifani, E. Mazzotta [1 ]
Dall'Ora, M. [1 ]
Di Fabrizio, L. [2 ]
Licandro, J. [3 ,4 ]
Palumbo, P. [5 ]
Colangeli, L. [1 ]
机构
[1] Osserv Astron Capodimonte, INAF, I-80131 Naples, Italy
[2] INAF, Fdn Galileo Galilei, Brena Baja 38712, TF, Spain
[3] Inst Astrofis Canarias, Tenerife 38200, Spain
[4] Univ La Laguna, Dept Astrofis, Tenerife 38205, Spain
[5] Univ Parthenope, Dip Sci Applicate, Ctr Direz Isola C4, I-80143 Naples, Italy
关键词
comets:; individual:; C/2007; D1; (LINEAR); O1; HALE-BOPP; WATER ICE; DUST; GAS; SPECTROSCOPY; PHOTOMETRY; PROGRAM; EARTH;
D O I
10.1051/0004-6361/200913535
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
Aims. We report on the unusual distant activity of the dynamically new comet C/2007 D1 (LINEAR), observed at r(h) = 9.7 AU postperihelion. This comet is particularly interesting because of its quite large perihelion distance (r(q) = 8.8 AU). Methods. We analyse V and R band images taken at the TNG telescope to characterise the dust coma of the comet and investigate its photometry, colours, and dust production. Results. The colour of the dust is redder than the Sun (V - R = 0.505 +/- 0.093 at the photometric aperture of radius 2.2"). The Af rho value is measured to be 1983 +/- 81 cm for an aperture of radius = 2.2 ''. An upper limit to the cometary nucleus radius of a(N) <= 18 km is derived. A dust mass-loss rate of dM(d)/dt = 5.3 x 10(2) kg s(-1) is measured, which implies that C/2007 D1 (LINEAR) is a very active comet despite its quite large perihelion distance.
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页数:5
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