{"id":34,"date":"2016-11-15T21:39:27","date_gmt":"2016-11-15T21:39:27","guid":{"rendered":"https:\/\/courses.lumenlearning.com\/astronomy\/?post_type=chapter&#038;p=34"},"modified":"2016-11-15T21:39:27","modified_gmt":"2016-11-15T21:39:27","slug":"the-brightest-twenty-stars","status":"publish","type":"chapter","link":"https:\/\/courses.lumenlearning.com\/towson-astronomy\/chapter\/the-brightest-twenty-stars\/","title":{"raw":"The Brightest Twenty Stars","rendered":"The Brightest Twenty Stars"},"content":{"raw":"<body>\n<div data-type=\"document-title\">The Brightest Twenty Stars<\/div>\n<p id=\"fs-id1172467001315\">Note: These are the stars that <em data-effect=\"italics\">appear<\/em> the brightest visually, as seen from our vantage point on Earth. They are not necessarily the stars that are intrinsically the most luminous.<\/p>\n<figure id=\"OSC_Astro_AstroTable_Brightest20_App_J\"><figcaption>The brightest stars typically have names from antiquity. Next to each star\u2019s ancient name, we have added a column with its name in the system originated by Bayer (see the <a href=\"\/contents\/e7866b9e-59bd-4e63-a285-58320ddaf41c#fs-id1165721974313\">Naming Stars<\/a> feature box.) The distances of the more remote stars are estimated from their spectral types and apparent brightnesses and are only approximate. The luminosities for those stars are approximate to the same degree. Right ascension and declination is given for Epoch 2000.0.<\/figcaption><span data-type=\"media\" id=\"fs-id1163976746193\" data-alt=\"A table titled \" the brightest twenty stars with eleven columns and twenty-one rows. first row is a header labels each column: name footnote: typically have names from antiquity. next to star ancient we added column its in system originated by bayer distances of more remote are estimated their spectral types apparent brightnesses only approximate. luminosities for those approximate same degree. type motion: ra dec ascension right given epoch declination second reads canis majoris v third carinae ii fourth kentaurus centauri k iv fifth bootis iii sixth lyrae seventh aurigae g0 eighth orionis i ninth minoris iv-v tenth eridani eleventh twelfth thirteenth aquilae fourteenth crucis b1 fifteenth tauri sixteenth virginis iii-iv b2 seventeenth scorpii b2.5 eighteenth geminorum nineteenth piscis austrini twentieth twenty-first cygni>\n<img src=\"https:\/\/s3-us-west-2.amazonaws.com\/courses-images\/wp-content\/uploads\/sites\/1095\/2016\/11\/03154647\/OSC_Astro_AstroTable_Brightest20_App_J.jpg\" data-media-type=\"image\/jpeg\" alt=\"A table titled \" the brightest twenty stars with eleven columns and twenty-one rows. first row is a header labels each column: name footnote: typically have names from antiquity. next to star ancient we added column its in system originated by bayer distances of more remote are estimated their spectral types apparent brightnesses only approximate. luminosities for those approximate same degree. type motion: ra dec ascension right given epoch declination second reads canis majoris v third carinae ii fourth kentaurus centauri k iv fifth bootis iii sixth lyrae seventh aurigae g0 eighth orionis i ninth minoris iv-v tenth eridani eleventh twelfth thirteenth aquilae fourteenth crucis b1 fifteenth tauri sixteenth virginis iii-iv b2 seventeenth scorpii b2.5 eighteenth geminorum nineteenth piscis austrini twentieth twenty-first cygni><\/span>\n\n<\/figure>\n<\/body>","rendered":"<div data-type=\"document-title\">The Brightest Twenty Stars<\/div>\n<p id=\"fs-id1172467001315\">Note: These are the stars that <em data-effect=\"italics\">appear<\/em> the brightest visually, as seen from our vantage point on Earth. They are not necessarily the stars that are intrinsically the most luminous.<\/p>\n<figure id=\"OSC_Astro_AstroTable_Brightest20_App_J\"><figcaption>The brightest stars typically have names from antiquity. Next to each star\u2019s ancient name, we have added a column with its name in the system originated by Bayer (see the <a href=\"\/contents\/e7866b9e-59bd-4e63-a285-58320ddaf41c#fs-id1165721974313\">Naming Stars<\/a> feature box.) The distances of the more remote stars are estimated from their spectral types and apparent brightnesses and are only approximate. The luminosities for those stars are approximate to the same degree. Right ascension and declination is given for Epoch 2000.0.<\/figcaption><span data-type=\"media\" id=\"fs-id1163976746193\" data-alt=\"A table titled\" is=\"\"><br \/>\n<img decoding=\"async\" src=\"https:\/\/s3-us-west-2.amazonaws.com\/courses-images\/wp-content\/uploads\/sites\/1095\/2016\/11\/03154647\/OSC_Astro_AstroTable_Brightest20_App_J.jpg\" data-media-type=\"image\/jpeg\" alt=\"A table titled\" is=\"\" id=\"\" \/><\/span><\/p>\n<\/figure>\n\n\t\t\t <section class=\"citations-section\" role=\"contentinfo\">\n\t\t\t <h3>Candela Citations<\/h3>\n\t\t\t\t\t <div>\n\t\t\t\t\t\t <div id=\"citation-list-34\">\n\t\t\t\t\t\t\t <div class=\"licensing\"><div class=\"license-attribution-dropdown-subheading\">CC licensed content, Shared previously<\/div><ul class=\"citation-list\"><li>Astronomy. <strong>Provided by<\/strong>: OpenStax CNX. <strong>Located at<\/strong>: <a target=\"_blank\" href=\"http:\/\/cnx.org\/contents\/2e737be8-ea65-48c3-aa0a-9f35b4c6a966@10.1\">http:\/\/cnx.org\/contents\/2e737be8-ea65-48c3-aa0a-9f35b4c6a966@10.1<\/a>. <strong>License<\/strong>: <em><a target=\"_blank\" rel=\"license\" href=\"https:\/\/creativecommons.org\/licenses\/by\/4.0\/\">CC BY: Attribution<\/a><\/em>. <strong>License Terms<\/strong>: Download for free at http:\/\/cnx.org\/contents\/2e737be8-ea65-48c3-aa0a-9f35b4c6a966@10.1.<\/li><\/ul><\/div>\n\t\t\t\t\t\t <\/div>\n\t\t\t\t\t <\/div>\n\t\t\t <\/section>","protected":false},"author":17,"menu_order":10,"template":"","meta":{"_candela_citation":"[{\"type\":\"cc\",\"description\":\"Astronomy\",\"author\":\"\",\"organization\":\"OpenStax CNX\",\"url\":\"http:\/\/cnx.org\/contents\/2e737be8-ea65-48c3-aa0a-9f35b4c6a966@10.1\",\"project\":\"\",\"license\":\"cc-by\",\"license_terms\":\"Download for free at http:\/\/cnx.org\/contents\/2e737be8-ea65-48c3-aa0a-9f35b4c6a966@10.1.\"}]","CANDELA_OUTCOMES_GUID":"","pb_show_title":"on","pb_short_title":"","pb_subtitle":"","pb_authors":[],"pb_section_license":""},"chapter-type":[],"contributor":[],"license":[],"class_list":["post-34","chapter","type-chapter","status-publish","hentry"],"part":18,"_links":{"self":[{"href":"https:\/\/courses.lumenlearning.com\/towson-astronomy\/wp-json\/pressbooks\/v2\/chapters\/34","targetHints":{"allow":["GET"]}}],"collection":[{"href":"https:\/\/courses.lumenlearning.com\/towson-astronomy\/wp-json\/pressbooks\/v2\/chapters"}],"about":[{"href":"https:\/\/courses.lumenlearning.com\/towson-astronomy\/wp-json\/wp\/v2\/types\/chapter"}],"author":[{"embeddable":true,"href":"https:\/\/courses.lumenlearning.com\/towson-astronomy\/wp-json\/wp\/v2\/users\/17"}],"version-history":[{"count":1,"href":"https:\/\/courses.lumenlearning.com\/towson-astronomy\/wp-json\/pressbooks\/v2\/chapters\/34\/revisions"}],"predecessor-version":[{"id":1127,"href":"https:\/\/courses.lumenlearning.com\/towson-astronomy\/wp-json\/pressbooks\/v2\/chapters\/34\/revisions\/1127"}],"part":[{"href":"https:\/\/courses.lumenlearning.com\/towson-astronomy\/wp-json\/pressbooks\/v2\/parts\/18"}],"metadata":[{"href":"https:\/\/courses.lumenlearning.com\/towson-astronomy\/wp-json\/pressbooks\/v2\/chapters\/34\/metadata\/"}],"wp:attachment":[{"href":"https:\/\/courses.lumenlearning.com\/towson-astronomy\/wp-json\/wp\/v2\/media?parent=34"}],"wp:term":[{"taxonomy":"chapter-type","embeddable":true,"href":"https:\/\/courses.lumenlearning.com\/towson-astronomy\/wp-json\/pressbooks\/v2\/chapter-type?post=34"},{"taxonomy":"contributor","embeddable":true,"href":"https:\/\/courses.lumenlearning.com\/towson-astronomy\/wp-json\/wp\/v2\/contributor?post=34"},{"taxonomy":"license","embeddable":true,"href":"https:\/\/courses.lumenlearning.com\/towson-astronomy\/wp-json\/wp\/v2\/license?post=34"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}