Secular Light Curve of 2P/Encke: A Comet Active At Aphelion

We present the secular light curve of comet 2P/Encke in two phase spaces, the log plot, and the time plot. The main conclusions of this work are: a) The comet shows activity at perihelion and aphelion, caused by two different active areas: Source 1, close to the South pole, active at perihelion, and...

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Main Author: Ferrin, Ignacio
Format: Text
Language:unknown
Published: arXiv 2008
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Online Access:https://dx.doi.org/10.48550/arxiv.0806.2161
https://arxiv.org/abs/0806.2161
id ftdatacite:10.48550/arxiv.0806.2161
record_format openpolar
spelling ftdatacite:10.48550/arxiv.0806.2161 2023-05-15T18:23:12+02:00 Secular Light Curve of 2P/Encke: A Comet Active At Aphelion Ferrin, Ignacio 2008 https://dx.doi.org/10.48550/arxiv.0806.2161 https://arxiv.org/abs/0806.2161 unknown arXiv https://dx.doi.org/10.1016/j.icarus.2008.04.012 arXiv.org perpetual, non-exclusive license http://arxiv.org/licenses/nonexclusive-distrib/1.0/ Astrophysics astro-ph FOS Physical sciences article-journal Article ScholarlyArticle Text 2008 ftdatacite https://doi.org/10.48550/arxiv.0806.2161 https://doi.org/10.1016/j.icarus.2008.04.012 2022-04-01T15:18:57Z We present the secular light curve of comet 2P/Encke in two phase spaces, the log plot, and the time plot. The main conclusions of this work are: a) The comet shows activity at perihelion and aphelion, caused by two different active areas: Source 1, close to the South pole, active at perihelion, and Source 2, at the North pole, centered at aphelion. b) More than 18 physical parameters are measured from the secular light curves, many of them new, and are listed in the individual plots of the comet. Specifically we find for Source 1 the location of the turn on and turn off points of activity, RON= -1.63+-0.03 AU, ROFF= +1.49+-0.20 AU, TON= -87+-5 d, TOFF= +94+-15 d, the time lag, LAG(q)= 6+-1 d, the total active time, TACTIVITY= 181+-16 d, and the amplitude of the secular light curve, ASEC(1,1) = 4.8+-0.1 mag. c) From this information the photometric age and the time-age defined in Ferrin (Icarus 178, 493-516, 2005a, and Icarus, 185, 523-543, 2006), can be calculated, and we find P-AGE=97+-8 comet years and T-AGE= 103+-9 comet years (cy). Thus comet 2P/Encke is an old comet entering the methuselah stage (100 cy < age). d) The activity at aphelion (Source 2), extends for TACTIVITY = 815+-30 d and the amplitude of the secular light curve is ASEC (1,Q) = 3.0+-0.2 mag. e) From a new phase diagram an absolute magnitude and phase coefficient for the nucleus are determined, and we find RNUC(1,1,0)= 15.05+-0.14, and betha= 0.066+-0.003. From this data we find a nucleus effective diameter DEFFE = 5.12(+2.5;-1.7) km. These values are not much different from previous determinations but exhibit smaller errors. Additional results appear in the full abstract. : 58 pages, 13 figures, 1 table, set your printer to color Text South pole DataCite Metadata Store (German National Library of Science and Technology) North Pole South Pole
institution Open Polar
collection DataCite Metadata Store (German National Library of Science and Technology)
op_collection_id ftdatacite
language unknown
topic Astrophysics astro-ph
FOS Physical sciences
spellingShingle Astrophysics astro-ph
FOS Physical sciences
Ferrin, Ignacio
Secular Light Curve of 2P/Encke: A Comet Active At Aphelion
topic_facet Astrophysics astro-ph
FOS Physical sciences
description We present the secular light curve of comet 2P/Encke in two phase spaces, the log plot, and the time plot. The main conclusions of this work are: a) The comet shows activity at perihelion and aphelion, caused by two different active areas: Source 1, close to the South pole, active at perihelion, and Source 2, at the North pole, centered at aphelion. b) More than 18 physical parameters are measured from the secular light curves, many of them new, and are listed in the individual plots of the comet. Specifically we find for Source 1 the location of the turn on and turn off points of activity, RON= -1.63+-0.03 AU, ROFF= +1.49+-0.20 AU, TON= -87+-5 d, TOFF= +94+-15 d, the time lag, LAG(q)= 6+-1 d, the total active time, TACTIVITY= 181+-16 d, and the amplitude of the secular light curve, ASEC(1,1) = 4.8+-0.1 mag. c) From this information the photometric age and the time-age defined in Ferrin (Icarus 178, 493-516, 2005a, and Icarus, 185, 523-543, 2006), can be calculated, and we find P-AGE=97+-8 comet years and T-AGE= 103+-9 comet years (cy). Thus comet 2P/Encke is an old comet entering the methuselah stage (100 cy < age). d) The activity at aphelion (Source 2), extends for TACTIVITY = 815+-30 d and the amplitude of the secular light curve is ASEC (1,Q) = 3.0+-0.2 mag. e) From a new phase diagram an absolute magnitude and phase coefficient for the nucleus are determined, and we find RNUC(1,1,0)= 15.05+-0.14, and betha= 0.066+-0.003. From this data we find a nucleus effective diameter DEFFE = 5.12(+2.5;-1.7) km. These values are not much different from previous determinations but exhibit smaller errors. Additional results appear in the full abstract. : 58 pages, 13 figures, 1 table, set your printer to color
format Text
author Ferrin, Ignacio
author_facet Ferrin, Ignacio
author_sort Ferrin, Ignacio
title Secular Light Curve of 2P/Encke: A Comet Active At Aphelion
title_short Secular Light Curve of 2P/Encke: A Comet Active At Aphelion
title_full Secular Light Curve of 2P/Encke: A Comet Active At Aphelion
title_fullStr Secular Light Curve of 2P/Encke: A Comet Active At Aphelion
title_full_unstemmed Secular Light Curve of 2P/Encke: A Comet Active At Aphelion
title_sort secular light curve of 2p/encke: a comet active at aphelion
publisher arXiv
publishDate 2008
url https://dx.doi.org/10.48550/arxiv.0806.2161
https://arxiv.org/abs/0806.2161
geographic North Pole
South Pole
geographic_facet North Pole
South Pole
genre South pole
genre_facet South pole
op_relation https://dx.doi.org/10.1016/j.icarus.2008.04.012
op_rights arXiv.org perpetual, non-exclusive license
http://arxiv.org/licenses/nonexclusive-distrib/1.0/
op_doi https://doi.org/10.48550/arxiv.0806.2161
https://doi.org/10.1016/j.icarus.2008.04.012
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