{"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":"2017-07-26T18:46:02","modified_gmt":"2017-07-26T18:46:02","slug":"the-brightest-twenty-stars","status":"publish","type":"chapter","link":"https:\/\/courses.lumenlearning.com\/suny-astronomy\/chapter\/the-brightest-twenty-stars\/","title":{"raw":"The Brightest Twenty Stars","rendered":"The Brightest Twenty Stars"},"content":{"raw":"<p id=\"fs-id1172467001315\">Note: These are the stars that <em>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>\r\n\r\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. 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 id=\"fs-id1163976746193\" data-type=\"media\" data-alt=\"A table titled \"> <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\" alt=\"A table titled \" name=\"\" data-media-type=\"image\/jpeg\" \/><\/span><\/figure>","rendered":"<p id=\"fs-id1172467001315\">Note: These are the stars that <em>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. 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 id=\"fs-id1163976746193\" data-type=\"media\" data-alt=\"A table titled\"> <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\" alt=\"A table titled\" data-media-type=\"image\/jpeg\" id=\"\" \/><\/span><\/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\/suny-astronomy\/wp-json\/pressbooks\/v2\/chapters\/34","targetHints":{"allow":["GET"]}}],"collection":[{"href":"https:\/\/courses.lumenlearning.com\/suny-astronomy\/wp-json\/pressbooks\/v2\/chapters"}],"about":[{"href":"https:\/\/courses.lumenlearning.com\/suny-astronomy\/wp-json\/wp\/v2\/types\/chapter"}],"author":[{"embeddable":true,"href":"https:\/\/courses.lumenlearning.com\/suny-astronomy\/wp-json\/wp\/v2\/users\/17"}],"version-history":[{"count":4,"href":"https:\/\/courses.lumenlearning.com\/suny-astronomy\/wp-json\/pressbooks\/v2\/chapters\/34\/revisions"}],"predecessor-version":[{"id":2225,"href":"https:\/\/courses.lumenlearning.com\/suny-astronomy\/wp-json\/pressbooks\/v2\/chapters\/34\/revisions\/2225"}],"part":[{"href":"https:\/\/courses.lumenlearning.com\/suny-astronomy\/wp-json\/pressbooks\/v2\/parts\/18"}],"metadata":[{"href":"https:\/\/courses.lumenlearning.com\/suny-astronomy\/wp-json\/pressbooks\/v2\/chapters\/34\/metadata\/"}],"wp:attachment":[{"href":"https:\/\/courses.lumenlearning.com\/suny-astronomy\/wp-json\/wp\/v2\/media?parent=34"}],"wp:term":[{"taxonomy":"chapter-type","embeddable":true,"href":"https:\/\/courses.lumenlearning.com\/suny-astronomy\/wp-json\/pressbooks\/v2\/chapter-type?post=34"},{"taxonomy":"contributor","embeddable":true,"href":"https:\/\/courses.lumenlearning.com\/suny-astronomy\/wp-json\/wp\/v2\/contributor?post=34"},{"taxonomy":"license","embeddable":true,"href":"https:\/\/courses.lumenlearning.com\/suny-astronomy\/wp-json\/wp\/v2\/license?post=34"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}