{"title":"用BRITE寻找系外行星","authors":"R. Dvorak, Á. Bazsó","doi":"10.1553/CIA152S166","DOIUrl":null,"url":null,"abstract":"We summarize in this report the possibilities of observing the reflecting light of a close by giant planet. BRITE could do these kind of observations only for very bright stars, but the chances that such a bright star with a close by large planet, a hot Jupiter, exists in the Solar environment are rather small. We discuss our present knowledge of analyzing reflecting light in light curves of stars.","PeriodicalId":151133,"journal":{"name":"Third Coast","volume":null,"pages":null},"PeriodicalIF":0.0000,"publicationDate":"1900-01-01","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"1","resultStr":"{\"title\":\"The search for extrasolar planets with BRITE\",\"authors\":\"R. Dvorak, Á. Bazsó\",\"doi\":\"10.1553/CIA152S166\",\"DOIUrl\":null,\"url\":null,\"abstract\":\"We summarize in this report the possibilities of observing the reflecting light of a close by giant planet. BRITE could do these kind of observations only for very bright stars, but the chances that such a bright star with a close by large planet, a hot Jupiter, exists in the Solar environment are rather small. We discuss our present knowledge of analyzing reflecting light in light curves of stars.\",\"PeriodicalId\":151133,\"journal\":{\"name\":\"Third Coast\",\"volume\":null,\"pages\":null},\"PeriodicalIF\":0.0000,\"publicationDate\":\"1900-01-01\",\"publicationTypes\":\"Journal Article\",\"fieldsOfStudy\":null,\"isOpenAccess\":false,\"openAccessPdf\":\"\",\"citationCount\":\"1\",\"resultStr\":null,\"platform\":\"Semanticscholar\",\"paperid\":null,\"PeriodicalName\":\"Third Coast\",\"FirstCategoryId\":\"1085\",\"ListUrlMain\":\"https://doi.org/10.1553/CIA152S166\",\"RegionNum\":0,\"RegionCategory\":null,\"ArticlePicture\":[],\"TitleCN\":null,\"AbstractTextCN\":null,\"PMCID\":null,\"EPubDate\":\"\",\"PubModel\":\"\",\"JCR\":\"\",\"JCRName\":\"\",\"Score\":null,\"Total\":0}","platform":"Semanticscholar","paperid":null,"PeriodicalName":"Third Coast","FirstCategoryId":"1085","ListUrlMain":"https://doi.org/10.1553/CIA152S166","RegionNum":0,"RegionCategory":null,"ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"","JCRName":"","Score":null,"Total":0}
We summarize in this report the possibilities of observing the reflecting light of a close by giant planet. BRITE could do these kind of observations only for very bright stars, but the chances that such a bright star with a close by large planet, a hot Jupiter, exists in the Solar environment are rather small. We discuss our present knowledge of analyzing reflecting light in light curves of stars.