Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/7915
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dc.contributor.authorSharma, Kritti-
dc.contributor.authorKelley, Michael S. P-
dc.contributor.authorJoharle, Simran-
dc.contributor.authorKumar, Harsh-
dc.contributor.authorSwain, Vishwajeet-
dc.contributor.authorBhalerao, Varun-
dc.contributor.authorAnupama, G. C-
dc.contributor.authorBarway, Sudhanshu-
dc.date.accessioned2022-01-29T05:23:42Z-
dc.date.available2022-01-29T05:23:42Z-
dc.date.issued2021-12-
dc.identifier.citationResearch Notes of the AAS, Vol. 5, No. 12, 277en_US
dc.identifier.issn2515-5172-
dc.identifier.urihttp://hdl.handle.net/2248/7915-
dc.descriptionOpen accessen_US
dc.description.abstractWe monitored the comet 67P/Churyumov-Gerasimenko close to its perihelion in November 2021 with the GROWTH-India Telescope. We observed two outbursts of this comet on 2021 October 29.940 and November 17.864 UTC, -3.12 days and +15.81 days respectively from the perihelion date. The brightening in the first outburst appears as a compact source, with a radial extent up to 8.″5. The comet brightened by 0.26 ± 0.03 mag in the outburst, with a 27% increase in the effective geometric cross-section and total outburst dust mass of ~5.3 × 105 kg. The second outburst caused a brightening of 0.49 ± 0.08 mag with effective geometric cross-section and total outburst dust mass 2.5 times larger than the first event. These outbursts are up to an order of magnitude larger than the strongest outburst event observed in situ by the Rosetta spacecraft in 2015.en_US
dc.language.isoenen_US
dc.publisherIOP Publishingen_US
dc.relation.urihttps://doi.org/10.3847/2515-5172/ac3ee4-
dc.rights© The Author(s)-
dc.titleOutbursts of Comet 67P/Churyumov-Gerasimenkoen_US
dc.typeArticleen_US
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