Multiple Outbursts of Halley-type Comet 12P/Pons–Brooks

We present optical observations of the Halley-type comet 12P/Pons–Brooks (12P) on its approach to perihelion. The comet was active even in the first observations at ∼8 au. Starting at ∼4 au, 12P exhibited an extraordinary series of outbursts, in which the brightness changed by a factor up to 100 and...

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Main Authors: David Jewitt, Jane Luu
Format: Article
Language:English
Published: IOP Publishing 2025-01-01
Series:The Astronomical Journal
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Online Access:https://doi.org/10.3847/1538-3881/add2ff
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author David Jewitt
Jane Luu
author_facet David Jewitt
Jane Luu
author_sort David Jewitt
collection DOAJ
description We present optical observations of the Halley-type comet 12P/Pons–Brooks (12P) on its approach to perihelion. The comet was active even in the first observations at ∼8 au. Starting at ∼4 au, 12P exhibited an extraordinary series of outbursts, in which the brightness changed by a factor up to 100 and the coma morphology transformed under the action of radiation pressure into a distinctive “horned” appearance. Individual outburst dust masses are several ×10 ^9 kg, with kinetic energies ∼10 ^14 J, release times ∼10 ^4 s, and effective power ∼10 ^10 W. These properties are most consistent with, although do not definitively establish, an origin by the crystallization of amorphous water ice with the related release of trapped supervolatile gases. This interpretation is supported by the observation that the specific outburst energy and the specific crystallization energy are comparable (both ∼10 ^5 J kg ^−1 ).
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spelling doaj-art-d01ab96f5c3b4201a392dff383c521eb2025-08-20T03:21:39ZengIOP PublishingThe Astronomical Journal1538-38812025-01-01169633810.3847/1538-3881/add2ffMultiple Outbursts of Halley-type Comet 12P/Pons–BrooksDavid Jewitt0Jane Luu1https://orcid.org/0000-0002-3104-4933Department of Earth, Planetary and Space Sciences, University of California, Los Angeles , Los Angeles, CA 90095-1567, USA ; djewitt@gmail.comCentre for Planetary Habitability (PHAB), Department of Geosciences, University of Oslo , NO-0315 Oslo, NorwayWe present optical observations of the Halley-type comet 12P/Pons–Brooks (12P) on its approach to perihelion. The comet was active even in the first observations at ∼8 au. Starting at ∼4 au, 12P exhibited an extraordinary series of outbursts, in which the brightness changed by a factor up to 100 and the coma morphology transformed under the action of radiation pressure into a distinctive “horned” appearance. Individual outburst dust masses are several ×10 ^9 kg, with kinetic energies ∼10 ^14 J, release times ∼10 ^4 s, and effective power ∼10 ^10 W. These properties are most consistent with, although do not definitively establish, an origin by the crystallization of amorphous water ice with the related release of trapped supervolatile gases. This interpretation is supported by the observation that the specific outburst energy and the specific crystallization energy are comparable (both ∼10 ^5 J kg ^−1 ).https://doi.org/10.3847/1538-3881/add2ffComet interiorsComet nucleiComet volatilesLong period cometsShort period comets
spellingShingle David Jewitt
Jane Luu
Multiple Outbursts of Halley-type Comet 12P/Pons–Brooks
The Astronomical Journal
Comet interiors
Comet nuclei
Comet volatiles
Long period comets
Short period comets
title Multiple Outbursts of Halley-type Comet 12P/Pons–Brooks
title_full Multiple Outbursts of Halley-type Comet 12P/Pons–Brooks
title_fullStr Multiple Outbursts of Halley-type Comet 12P/Pons–Brooks
title_full_unstemmed Multiple Outbursts of Halley-type Comet 12P/Pons–Brooks
title_short Multiple Outbursts of Halley-type Comet 12P/Pons–Brooks
title_sort multiple outbursts of halley type comet 12p pons brooks
topic Comet interiors
Comet nuclei
Comet volatiles
Long period comets
Short period comets
url https://doi.org/10.3847/1538-3881/add2ff
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