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Comet C/2011 J2 (LINEAR) nucleus splitting: Dynamical and structural analysis.

Authors :
Manzini, Federico
Oldani, Virginio
Hirabayashi, Masatoshi
Behrend, Raoul
Crippa, Roberto
Ochner, Paolo
Pina, José Pablo Navarro
Haver, Roberto
Baransky, Alexander
Bryssinck, Eric
Dan, Andras
De Queiroz, Josè
Frappa, Eric
Lavayssiere, Maylis
Source :
Planetary & Space Science. Jul2016, Vol. 126, p8-23. 16p.
Publication Year :
2016

Abstract

After the discovery of the breakup event of comet C/2011 J2 in August 2014, we followed the primary body and the main fragment B for about 120 days in the context of a wide international collaboration. From the analysis of all published magnitude estimates we calculated the comet׳s absolute magnitude H =10.4, and its photometric index n =1.7. We also calculated a water production of only 110 kg/s at the perihelion. These values are typical of a low-activity, long-period or new comet. Analysis of the motion of fragment B over the observation period showed that the first breakout event likely occurred between 12 July and 30 July 2014. Nucleus B remained persistently visible throughout the 4-month observation period. The projected separation velocity of nucleus B from the parent body was 4.22 m/s at the time of the breakup and 12.7 m/s at the end of the observation period, suggesting that nucleus B was subjected to a constant deceleration a = 6.87 ∙ 10 − 7 m / s 2 . The spin period of the main nucleus was estimated as 4.56 h±0.05 h by photometric analysis. The structural analysis of the comet showed a cohesive strength of the nucleus greater than ~0.9 kPa; assuming a bulk density of 500 kg/m 3 , with a rotation period of 4.56 h the cometary nucleus might have failed structurally, especially if the body was elongated. These results suggest that the nucleus of comet C/2011 J2 has an elongated shape, with a ratio of the semi-minor axis to the semi-major axis β < 0.675 ; the semi-major axis of the pristine nucleus could be larger than 8 km. From this study, we propose that rotational disruption, possibly combined with sublimation pressure, was a reasonable explanation for the breakup event in comet C/2011 J2. [ABSTRACT FROM AUTHOR]

Details

Language :
English
ISSN :
00320633
Volume :
126
Database :
Academic Search Index
Journal :
Planetary & Space Science
Publication Type :
Academic Journal
Accession number :
115413405
Full Text :
https://doi.org/10.1016/j.pss.2016.04.004