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dc.contributor.authorArimatsu, Koen
dc.contributor.authorTsumura, Kohjien
dc.contributor.authorUsui, Fumihikoen
dc.contributor.authorWatanabe, Jun-ichien
dc.contributor.alternative有松, 亘ja
dc.contributor.alternative津村, 耕司ja
dc.contributor.alternative臼井, 文彦ja
dc.contributor.alternative渡部, 潤一ja
dc.date.accessioned2022-09-13T09:33:02Z-
dc.date.available2022-09-13T09:33:02Z-
dc.date.issued2022-07-01-
dc.identifier.urihttp://hdl.handle.net/2433/276263-
dc.description木星で超大型の衝突閃光現象を発見 --京大のとある屋上の小さな望遠鏡による大発見--. 京都大学プレスリリース. 2022-09-13.ja
dc.description.abstractWe report the detection of an optical impact flash on Jupiter on 2021 October 15 by a dedicated telescope, Planetary ObservatioN Camera for Optical Transient Surveys, for the first time. Our temporally resolved three-band observations of the flash allowed investigations of its optical energy without the need for approximations on the impact brightness temperature. The kinetic energy of the impactor was equivalent to approximately two megatons of TNT, an order of magnitude greater than that of previously detected flashes on Jupiter and comparable with the Tunguska impact on Earth in 1908. This detection indicates that Tunguska-like impact events on Jupiter occur approximately once per year, two to three orders of magnitude more frequently than terrestrial impacts. The observed flash displayed a single-temperature blackbody spectrum with an effective temperature of approximately 8300 K without clear temporal variation, possibly representing common radiative features of terrestrial Tunguska-class superbolides.en
dc.language.isoeng-
dc.publisherAmerican Astronomical Societyen
dc.rights© 2022. The Author(s). Published by the American Astronomical Society.en
dc.rightsOriginal content from this work may be used under the terms of the Creative Commons Attribution 4.0 licence. Any further distribution of this work must maintain attribution to the author(s) and the title of the work, journal citation and DOI.en
dc.rights.urihttp://creativecommons.org/licenses/by/4.0/-
dc.subjectJupiteren
dc.subjectImpact phenomenaen
dc.subjectTime domain astronomyen
dc.subjectPlanetary atmospheresen
dc.subjectSolar system astronomyen
dc.titleDetection of an extremely large impact flash on Jupiter by high-cadence multiwavelength observationsen
dc.typejournal article-
dc.type.niitypeJournal Article-
dc.identifier.jtitleThe Astrophysical Journal Lettersen
dc.identifier.volume933-
dc.identifier.issue1-
dc.relation.doi10.3847/2041-8213/ac7573-
dc.textversionpublisher-
dc.identifier.artnumL5-
dc.addressThe Hakubi Center/Astronomical Observatory, Graduate School of Science, Kyoto Universityen
dc.addressDepartment of Natural Science, Faculty of Science and Engineering, Tokyo City Universityen
dc.addressInstitute of Space and Astronautical Science (ISAS), Japan Aerospace Exploration Agency (JAXA)en
dc.addressPublic Relations Center, National Astronomical Observatory of Japanen
dc.relation.urlhttps://www.kyoto-u.ac.jp/ja/research-news/2022-09-13-
dcterms.accessRightsopen access-
datacite.awardNumber18K13606-
datacite.awardNumber21H01153-
datacite.awardNumber.urihttps://kaken.nii.ac.jp/grant/KAKENHI-PROJECT-18K13606/-
datacite.awardNumber.urihttps://kaken.nii.ac.jp/grant/KAKENHI-PROJECT-21H01153/-
dc.identifier.pissn2041-8205-
dc.identifier.eissn2041-8213-
jpcoar.funderName日本学術振興会ja
jpcoar.funderName日本学術振興会ja
jpcoar.awardTitleオールト雲の解明ja
jpcoar.awardTitleオールトの雲へ: 小望遠鏡群で拓く太陽系のさいはてja
出現コレクション:学術雑誌掲載論文等

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