{"title":"6384 kervin:一颗可能的匈牙利双星小行星。","authors":"Brian D Warner, Amadeo Aznar Macías","doi":"","DOIUrl":null,"url":null,"abstract":"<p><p>Analysis of CCD photometric observations in late 2015 of the Hungaria asteroid 6384 Kervin indicates that it may be a binary asteroid with a primary lightcurve of <i>P</i> <sub><i>1</i></sub> = 3.6194 ± 0.0001 h, <i>A</i> <sub><i>1</i></sub> = 0.06 ± 0.01 mag. The secondary lightcurve parameters are <i>P</i> <sub><i>2</i></sub> = 15.94 ± 0.01 h, <i>A</i> <sub><i>2</i></sub> = 0.03 ± 0.01 mag. No mutual events (occultations or eclipses) were observed. However, other indicators give an estimated diameter ratio on the order of <i>Ds/Dp</i> ~ 0.3, possibly greater.</p>","PeriodicalId":75145,"journal":{"name":"The Minor planet bulletin","volume":"43 2","pages":"184-185"},"PeriodicalIF":0.0000,"publicationDate":"2016-04-01","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"https://www.ncbi.nlm.nih.gov/pmc/articles/PMC7243992/pdf/nihms-1570096.pdf","citationCount":"0","resultStr":"{\"title\":\"6384 KERVIN: A POSSIBLE HUNGARIA BINARY ASTEROID.\",\"authors\":\"Brian D Warner, Amadeo Aznar Macías\",\"doi\":\"\",\"DOIUrl\":null,\"url\":null,\"abstract\":\"<p><p>Analysis of CCD photometric observations in late 2015 of the Hungaria asteroid 6384 Kervin indicates that it may be a binary asteroid with a primary lightcurve of <i>P</i> <sub><i>1</i></sub> = 3.6194 ± 0.0001 h, <i>A</i> <sub><i>1</i></sub> = 0.06 ± 0.01 mag. The secondary lightcurve parameters are <i>P</i> <sub><i>2</i></sub> = 15.94 ± 0.01 h, <i>A</i> <sub><i>2</i></sub> = 0.03 ± 0.01 mag. No mutual events (occultations or eclipses) were observed. However, other indicators give an estimated diameter ratio on the order of <i>Ds/Dp</i> ~ 0.3, possibly greater.</p>\",\"PeriodicalId\":75145,\"journal\":{\"name\":\"The Minor planet bulletin\",\"volume\":\"43 2\",\"pages\":\"184-185\"},\"PeriodicalIF\":0.0000,\"publicationDate\":\"2016-04-01\",\"publicationTypes\":\"Journal Article\",\"fieldsOfStudy\":null,\"isOpenAccess\":false,\"openAccessPdf\":\"https://www.ncbi.nlm.nih.gov/pmc/articles/PMC7243992/pdf/nihms-1570096.pdf\",\"citationCount\":\"0\",\"resultStr\":null,\"platform\":\"Semanticscholar\",\"paperid\":null,\"PeriodicalName\":\"The Minor planet bulletin\",\"FirstCategoryId\":\"1085\",\"ListUrlMain\":\"\",\"RegionNum\":0,\"RegionCategory\":null,\"ArticlePicture\":[],\"TitleCN\":null,\"AbstractTextCN\":null,\"PMCID\":null,\"EPubDate\":\"\",\"PubModel\":\"\",\"JCR\":\"\",\"JCRName\":\"\",\"Score\":null,\"Total\":0}","platform":"Semanticscholar","paperid":null,"PeriodicalName":"The Minor planet bulletin","FirstCategoryId":"1085","ListUrlMain":"","RegionNum":0,"RegionCategory":null,"ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"","JCRName":"","Score":null,"Total":0}
Analysis of CCD photometric observations in late 2015 of the Hungaria asteroid 6384 Kervin indicates that it may be a binary asteroid with a primary lightcurve of P1 = 3.6194 ± 0.0001 h, A1 = 0.06 ± 0.01 mag. The secondary lightcurve parameters are P2 = 15.94 ± 0.01 h, A2 = 0.03 ± 0.01 mag. No mutual events (occultations or eclipses) were observed. However, other indicators give an estimated diameter ratio on the order of Ds/Dp ~ 0.3, possibly greater.
求助内容：
应助结果提醒方式：
京公网安备 11010802042870号
