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2014-2015 MULTIPLE OUTBURSTS OF 15P/FINLAY

ABSTRACT Multiple outbursts of a Jupiter-family comet (JFC), 15P/Finlay, occurred from late 2014 to early 2015. We conducted an observation of the comet after the first outburst and subsequently witnessed another outburst on 2015 January 15.6-15.7. The gas, consisting mostly of C2 and CN, and dust p...

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Published in:The Astronomical journal 2016-12, Vol.152 (6), p.169
Main Authors: Ishiguro, Masateru, Kuroda, Daisuke, Hanayama, Hidekazu, Kwon, Yuna Grace, Kim, Yoonyoung, Lee, Myung Gyoon, Watanabe, Makoto, Akitaya, Hiroshi, Kawabata, Koji, Itoh, Ryosuke, Nakaoka, Tatsuya, Yoshida, Michitoshi, Imai, Masataka, Sarugaku, Yuki, Yanagisawa, Kenshi, Ohta, Kouji, Kawai, Nobuyuki, Miyaji, Takeshi, Fukushima, Hideo, Honda, Satoshi, Takahashi, Jun, Sato, Mikiya, Vaubaillon, Jeremie J., Watanabe, Jun-ichi
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container_issue 6
container_start_page 169
container_title The Astronomical journal
container_volume 152
creator Ishiguro, Masateru
Kuroda, Daisuke
Hanayama, Hidekazu
Kwon, Yuna Grace
Kim, Yoonyoung
Lee, Myung Gyoon
Watanabe, Makoto
Akitaya, Hiroshi
Kawabata, Koji
Itoh, Ryosuke
Nakaoka, Tatsuya
Yoshida, Michitoshi
Imai, Masataka
Sarugaku, Yuki
Yanagisawa, Kenshi
Ohta, Kouji
Kawai, Nobuyuki
Miyaji, Takeshi
Fukushima, Hideo
Honda, Satoshi
Takahashi, Jun
Sato, Mikiya
Vaubaillon, Jeremie J.
Watanabe, Jun-ichi
description ABSTRACT Multiple outbursts of a Jupiter-family comet (JFC), 15P/Finlay, occurred from late 2014 to early 2015. We conducted an observation of the comet after the first outburst and subsequently witnessed another outburst on 2015 January 15.6-15.7. The gas, consisting mostly of C2 and CN, and dust particles expanded at speeds of 1110 180 m s−1 and 570 40 m s−1 at a heliocentric distance of 1.0 au. We estimated the maximum ratio of solar radiation pressure with respect to the solar gravity βmax = 1.6 0.2, which is consistent with porous dust particles composed of silicates and organics. We found that 108-109 kg of dust particles (assumed to be 0.3 m-1 mm) were ejected through each outburst. Although the total mass is three orders of magnitude smaller than that of the 17P/Holmes event observed in 2007, the kinetic energy per unit mass (104 J kg−1) is equivalent to the estimated values of 17P/Holmes and 332P/2010 V1 (Ikeya-Murakami), suggesting that the outbursts were caused by a similar physical mechanism. From a survey of cometary outbursts on the basis of voluntary reports, we conjecture that 15P/Finlay-class outbursts occur >1.5 times annually and inject dust particles from JFCs and Encke-type comets into interplanetary space at a rate of ∼10 kg s−1 or more.
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subjects ASTROPHYSICS
ASTROPHYSICS, COSMOLOGY AND ASTRONOMY
CARBON NITRIDES
COMETS
comets: individual (15P/Finlay)
COSMIC DUST
GRAVITATION
interplanetary medium
INTERPLANETARY SPACE
INTERSTELLAR SPACE
JUPITER PLANET
KINETIC ENERGY
MASS
METEORITES
meteorites, meteors, meteoroids
METEOROIDS
Physics
POROUS MATERIALS
RADIATION PRESSURE
SILICATES
SOLAR RADIATION
title 2014-2015 MULTIPLE OUTBURSTS OF 15P/FINLAY
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