Polarization of disintegrating Comet C/2019 Y4 (ATLAS)
ABSTRACT We observe Comet C/2019 Y4 (ATLAS) before and after its disintegration while making polarimetric measurements over a wide range of phase angles. The disintegration event was marked with a dramatic growth of the positive polarization branch that is consistent with a large relative abundance...
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Veröffentlicht in: | Monthly notices of the Royal Astronomical Society 2020-09, Vol.497 (2), p.1536-1542 |
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creator | Zubko, Evgenij Zheltobryukhov, Maxim Chornaya, Ekaterina Kochergin, Anton Videen, Gorden Kornienko, Gennady Kim, Sungsoo S |
description | ABSTRACT
We observe Comet C/2019 Y4 (ATLAS) before and after its disintegration while making polarimetric measurements over a wide range of phase angles. The disintegration event was marked with a dramatic growth of the positive polarization branch that is consistent with a large relative abundance of absorbing material of up to (96.5 ± 3.4) per cent. This polarization spike relaxed as the carbonaceous particles are preferentially swept from the coma due to solar-radiation pressure. The observations suggest that the primordial material stored within comets is extremely rich in carbonaceous material. The pristine cometary material is processed by subsequent solar interactions, forming a refractory crust on the nucleus surface. Polarimetry provides a means of measuring the volume ratio of carbonaceous material, and hence the weathering that has occurred on the comet due to these interactions. The polarimetric response of Comet C/2019 Y4 (ATLAS) appears similar to that of Comet C/1995 O1 (Hale-Bopp), except on few epochs that are similar to that of Comet C/1996 B2 (Hyakutake). |
doi_str_mv | 10.1093/mnras/staa1725 |
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We observe Comet C/2019 Y4 (ATLAS) before and after its disintegration while making polarimetric measurements over a wide range of phase angles. The disintegration event was marked with a dramatic growth of the positive polarization branch that is consistent with a large relative abundance of absorbing material of up to (96.5 ± 3.4) per cent. This polarization spike relaxed as the carbonaceous particles are preferentially swept from the coma due to solar-radiation pressure. The observations suggest that the primordial material stored within comets is extremely rich in carbonaceous material. The pristine cometary material is processed by subsequent solar interactions, forming a refractory crust on the nucleus surface. Polarimetry provides a means of measuring the volume ratio of carbonaceous material, and hence the weathering that has occurred on the comet due to these interactions. The polarimetric response of Comet C/2019 Y4 (ATLAS) appears similar to that of Comet C/1995 O1 (Hale-Bopp), except on few epochs that are similar to that of Comet C/1996 B2 (Hyakutake).</description><identifier>ISSN: 0035-8711</identifier><identifier>EISSN: 1365-2966</identifier><identifier>DOI: 10.1093/mnras/staa1725</identifier><language>eng</language><publisher>Oxford University Press</publisher><ispartof>Monthly notices of the Royal Astronomical Society, 2020-09, Vol.497 (2), p.1536-1542</ispartof><rights>2020 The Author(s) Published by Oxford University Press on behalf of the Royal Astronomical Society 2020</rights><lds50>peer_reviewed</lds50><woscitedreferencessubscribed>false</woscitedreferencessubscribed><citedby>FETCH-LOGICAL-c273t-1ed79a1a8f54017b61fff674a6ec891794e815dd7116c4a63a8a2205fdee97f13</citedby><cites>FETCH-LOGICAL-c273t-1ed79a1a8f54017b61fff674a6ec891794e815dd7116c4a63a8a2205fdee97f13</cites><orcidid>0000-0001-5246-3857 ; 0000-0002-5570-2160 ; 0000-0001-9994-923X</orcidid></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><link.rule.ids>314,776,780,1598,27901,27902</link.rule.ids><linktorsrc>$$Uhttps://dx.doi.org/10.1093/mnras/staa1725$$EView_record_in_Oxford_University_Press$$FView_record_in_$$GOxford_University_Press</linktorsrc></links><search><creatorcontrib>Zubko, Evgenij</creatorcontrib><creatorcontrib>Zheltobryukhov, Maxim</creatorcontrib><creatorcontrib>Chornaya, Ekaterina</creatorcontrib><creatorcontrib>Kochergin, Anton</creatorcontrib><creatorcontrib>Videen, Gorden</creatorcontrib><creatorcontrib>Kornienko, Gennady</creatorcontrib><creatorcontrib>Kim, Sungsoo S</creatorcontrib><title>Polarization of disintegrating Comet C/2019 Y4 (ATLAS)</title><title>Monthly notices of the Royal Astronomical Society</title><description>ABSTRACT
We observe Comet C/2019 Y4 (ATLAS) before and after its disintegration while making polarimetric measurements over a wide range of phase angles. The disintegration event was marked with a dramatic growth of the positive polarization branch that is consistent with a large relative abundance of absorbing material of up to (96.5 ± 3.4) per cent. This polarization spike relaxed as the carbonaceous particles are preferentially swept from the coma due to solar-radiation pressure. The observations suggest that the primordial material stored within comets is extremely rich in carbonaceous material. The pristine cometary material is processed by subsequent solar interactions, forming a refractory crust on the nucleus surface. Polarimetry provides a means of measuring the volume ratio of carbonaceous material, and hence the weathering that has occurred on the comet due to these interactions. The polarimetric response of Comet C/2019 Y4 (ATLAS) appears similar to that of Comet C/1995 O1 (Hale-Bopp), except on few epochs that are similar to that of Comet C/1996 B2 (Hyakutake).</description><issn>0035-8711</issn><issn>1365-2966</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2020</creationdate><recordtype>article</recordtype><recordid>eNqFjz1PwzAYhC0EEqGwMnukQxq_dmzHYxTxJUVqJcrAFL0kdhXUxJUdBvj1BAoz00mnu9M9hFwDWwEzIhvGgDGLEyJoLk9IAkLJlBulTknCmJBpoQHOyUWMb4yxXHCVELXxewz9J069H6l3tOtjP052F2Zn3NHKD3aiVcYZGPqS05tyW5dPy0ty5nAf7dWvLsjz3e22ekjr9f1jVdZpy7WYUrCdNghYOJkz0K8KnHNK56hsWxjQJrcFyK6bf6l2dgUWyDmTrrPWaAdiQVbH3Tb4GIN1zSH0A4aPBljzTd38UDd_1HNheSz498N_2S--yVja</recordid><startdate>20200901</startdate><enddate>20200901</enddate><creator>Zubko, Evgenij</creator><creator>Zheltobryukhov, Maxim</creator><creator>Chornaya, Ekaterina</creator><creator>Kochergin, Anton</creator><creator>Videen, Gorden</creator><creator>Kornienko, Gennady</creator><creator>Kim, Sungsoo S</creator><general>Oxford University Press</general><scope>AAYXX</scope><scope>CITATION</scope><orcidid>https://orcid.org/0000-0001-5246-3857</orcidid><orcidid>https://orcid.org/0000-0002-5570-2160</orcidid><orcidid>https://orcid.org/0000-0001-9994-923X</orcidid></search><sort><creationdate>20200901</creationdate><title>Polarization of disintegrating Comet C/2019 Y4 (ATLAS)</title><author>Zubko, Evgenij ; Zheltobryukhov, Maxim ; Chornaya, Ekaterina ; Kochergin, Anton ; Videen, Gorden ; Kornienko, Gennady ; Kim, Sungsoo S</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-c273t-1ed79a1a8f54017b61fff674a6ec891794e815dd7116c4a63a8a2205fdee97f13</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2020</creationdate><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Zubko, Evgenij</creatorcontrib><creatorcontrib>Zheltobryukhov, Maxim</creatorcontrib><creatorcontrib>Chornaya, Ekaterina</creatorcontrib><creatorcontrib>Kochergin, Anton</creatorcontrib><creatorcontrib>Videen, Gorden</creatorcontrib><creatorcontrib>Kornienko, Gennady</creatorcontrib><creatorcontrib>Kim, Sungsoo S</creatorcontrib><collection>CrossRef</collection><jtitle>Monthly notices of the Royal Astronomical Society</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext_linktorsrc</fulltext></delivery><addata><au>Zubko, Evgenij</au><au>Zheltobryukhov, Maxim</au><au>Chornaya, Ekaterina</au><au>Kochergin, Anton</au><au>Videen, Gorden</au><au>Kornienko, Gennady</au><au>Kim, Sungsoo S</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Polarization of disintegrating Comet C/2019 Y4 (ATLAS)</atitle><jtitle>Monthly notices of the Royal Astronomical Society</jtitle><date>2020-09-01</date><risdate>2020</risdate><volume>497</volume><issue>2</issue><spage>1536</spage><epage>1542</epage><pages>1536-1542</pages><issn>0035-8711</issn><eissn>1365-2966</eissn><abstract>ABSTRACT
We observe Comet C/2019 Y4 (ATLAS) before and after its disintegration while making polarimetric measurements over a wide range of phase angles. The disintegration event was marked with a dramatic growth of the positive polarization branch that is consistent with a large relative abundance of absorbing material of up to (96.5 ± 3.4) per cent. This polarization spike relaxed as the carbonaceous particles are preferentially swept from the coma due to solar-radiation pressure. The observations suggest that the primordial material stored within comets is extremely rich in carbonaceous material. The pristine cometary material is processed by subsequent solar interactions, forming a refractory crust on the nucleus surface. Polarimetry provides a means of measuring the volume ratio of carbonaceous material, and hence the weathering that has occurred on the comet due to these interactions. The polarimetric response of Comet C/2019 Y4 (ATLAS) appears similar to that of Comet C/1995 O1 (Hale-Bopp), except on few epochs that are similar to that of Comet C/1996 B2 (Hyakutake).</abstract><pub>Oxford University Press</pub><doi>10.1093/mnras/staa1725</doi><tpages>7</tpages><orcidid>https://orcid.org/0000-0001-5246-3857</orcidid><orcidid>https://orcid.org/0000-0002-5570-2160</orcidid><orcidid>https://orcid.org/0000-0001-9994-923X</orcidid></addata></record> |
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title | Polarization of disintegrating Comet C/2019 Y4 (ATLAS) |
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