Analysis of CN Coma Morphology Features of Comet 21P/Giacobini-Zinner
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Lunar and Planetary Laboratory, University of ArizonaIssue Date
2023-02-09
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Institute of PhysicsCitation
Charles Goldberg et al 2023 Planet. Sci. J. 4 28Journal
Planetary Science JournalRights
© 2023. The Author(s). Published by the American Astronomical Society. Original content from this work may be used under the terms of the Creative Commons Attribution 4.0 licence.Collection Information
This item from the UA Faculty Publications collection is made available by the University of Arizona with support from the University of Arizona Libraries. If you have questions, please contact us at repository@u.library.arizona.edu.Abstract
We analyze jet features found in the coma of comet 21P/Giacobini-Zinner (21P/GZ) during its 2018 perihelion passage using narrowband CN photometric imaging in order to determine the comet’s rotational period, and we constrain the CN gas outflow velocity and rotational state through the analysis of azimuthally enhanced morphological features. We find that 21P/GZ has a period of either 7.39 ± 0.01 hr or 10.66 ± 0.01 hr. We measure a lower limit to the outflow velocity for the northern jet of 730 ± 30 m s−1 and for the southern jet of 740 ± 30 m s−1. We analyze the morphologies of the jet features and determine that the northern jet possesses a corkscrew pattern, and we utilize that knowledge to determine a rotational pole position at an R.A. of 169 − 23 + 28 deg and a decl. of 73 − 11 + 5 deg, with an undetermined sense of rotation. © 2023. The Author(s). Published by the American Astronomical Society.Note
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2632-3338Version
Final Published Versionae974a485f413a2113503eed53cd6c53
10.3847/PSJ/acb436
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Except where otherwise noted, this item's license is described as © 2023. The Author(s). Published by the American Astronomical Society. Original content from this work may be used under the terms of the Creative Commons Attribution 4.0 licence.