首页|Understanding the Activity Performance of Comets 38P/Stephan-Oterma,64P/Swift-Gehrels and C/2017 M4(ATLAS)through Broadband Photometric Observations

Understanding the Activity Performance of Comets 38P/Stephan-Oterma,64P/Swift-Gehrels and C/2017 M4(ATLAS)through Broadband Photometric Observations

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In this work,we report observations of three comets:38P/Stephan-Oterma,64P/Swift-Gehrels,and C/2017 M4(ATLAS),conducted with the Nanshan one-meter wide-field telescope in 2018 August and November,and 2019 January.We extracted morphological features through image enhancement techniques and calculated the dust activity parameter,Afρ,along with dust mass loss rates and coma color indices using broadband photometric data.Our morphological analysis uncovered a spectrum of dust characteristics among the observed comets,ranging from a significant twisted structure in comet 38P/Stephan-Oterma's coma to the regular coma envelope surrounding comet 64P/Swift-Gehrels.The Afρ values varied between 148.8±0.3 cm for 64P/Swift-Gehrels and 1118.5±6.2 cm for C/2017 M4(ATLAS)(measured within a reference aperture radius of ρ=6"),indicating a range from moderate to high activity levels.Dust mass loss rates were estimated from 328.1 kg s-1 for comet 64P/Swift-Gehrels to 1395.5 kg s-1 for comet C/2017 M4(ATLAS).The color indices of comets 38P/Stephan-Oterma and C/2017 M4(ATLAS)closely resemble the average colors of active short-period comets and active long-period comets,respectively.In contrast,64P/Swift-Gehrels exhibits a significantly bluer hue than typical Jupiter family comets.

comets:generalcomets:individual(38P/Stephan-Oterma,64P/Swift-Gehrels,C/2017 M4(ATLAS))techniques:photometric

Xuan Zhang、Jin-Zhong Liu、Le-Tian Wang

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Xinjiang Astronomical Observatory,Chinese Academy of Sciences,Urumqi 830011,China

Natural Science Foundation of Xinjiang Uygur Autonomous Region of ChinaTianshan Talent Training Program

2021D01B1122023TSYCCX0101

2024

天文和天体物理学研究
中国科学院国家天文台

天文和天体物理学研究

CSTPCD
影响因子:0.406
ISSN:1674-4527
年,卷(期):2024.24(8)