{"id":245,"date":"2022-02-11T16:28:57","date_gmt":"2022-02-11T16:28:57","guid":{"rendered":"https:\/\/pressbooks.ccconline.org\/astronomy\/?post_type=chapter&#038;p=245"},"modified":"2022-02-11T16:30:52","modified_gmt":"2022-02-11T16:30:52","slug":"key-terms-2","status":"publish","type":"chapter","link":"https:\/\/pressbooks.ccconline.org\/astronomy\/chapter\/key-terms-2\/","title":{"raw":"Key Terms","rendered":"Key Terms"},"content":{"raw":"<dl id=\"fs-id1168048332291\">\r\n \t<dt id=\"7\">apparent solar time<\/dt>\r\n \t<dd id=\"fs-id1168048481217\">time as measured by the position of the Sun in the sky (the time that would be indicated by a sundial)<\/dd>\r\n<\/dl>\r\n<dl id=\"fs-id1168048623216\">\r\n \t<dt id=\"8\">declination<\/dt>\r\n \t<dd id=\"fs-id1168046348880\">the angular distance north or south of the celestial equator<\/dd>\r\n<\/dl>\r\n<dl id=\"fs-id1168048291103\">\r\n \t<dt id=\"9\">great circle<\/dt>\r\n \t<dd id=\"fs-id1168048374770\">a circle on the surface of a sphere that is the curve of intersection of the sphere with a plane passing through its center<\/dd>\r\n<\/dl>\r\n<dl id=\"fs-id1168048515777\">\r\n \t<dt id=\"80\">International Date Line<\/dt>\r\n \t<dd id=\"fs-id1168048282502\">an arbitrary line on the surface of Earth near longitude 180\u00b0 across which the date changes by one day<\/dd>\r\n<\/dl>\r\n<dl id=\"fs-id1168047141002\">\r\n \t<dt id=\"13\">lunar eclipse<\/dt>\r\n \t<dd id=\"fs-id1168047134019\">an eclipse of the Moon, in which the Moon moves into the shadow of Earth; lunar eclipses can occur only at the time of full moon<\/dd>\r\n<\/dl>\r\n<dl id=\"fs-id1168048449754\">\r\n \t<dt id=\"90\">mean solar time<\/dt>\r\n \t<dd id=\"fs-id1168048511927\">time based on the rotation of Earth; mean solar time passes at a constant rate, unlike apparent solar time<\/dd>\r\n<\/dl>\r\n<dl id=\"fs-id1168048403578\">\r\n \t<dt id=\"10\">meridian<\/dt>\r\n \t<dd id=\"fs-id1168048535627\">a great circle on the terrestrial or celestial sphere that passes through the poles<\/dd>\r\n<\/dl>\r\n<dl id=\"fs-id1168047360264\">\r\n \t<dt id=\"70\">phases of the Moon<\/dt>\r\n \t<dd id=\"fs-id1168047792933\">the different appearance of light and dark on the Moon as seen from Earth during its monthly cycle, from new moon to full moon and back to new moon<\/dd>\r\n<\/dl>\r\n<dl id=\"fs-id1168048320963\">\r\n \t<dt id=\"11\">right ascension<\/dt>\r\n \t<dd id=\"fs-id1168048290756\">the coordinate for measuring the east-west positions of celestial bodies; the angle measured eastward along the celestial equator from the vernal equinox to the hour circle passing through a body<\/dd>\r\n<\/dl>\r\n<dl id=\"fs-id1168046060994\">\r\n \t<dt id=\"100\">sidereal day<\/dt>\r\n \t<dd id=\"fs-id1168048499590\">Earth\u2019s rotation period as defined by the positions of the stars in the sky; the time between successive passages of the same star through the meridian<\/dd>\r\n<\/dl>\r\n<dl id=\"fs-id1168047194530\">\r\n \t<dt id=\"81\">sidereal month<\/dt>\r\n \t<dd id=\"fs-id1168047973882\">the period of the Moon\u2019s revolution about Earth measured with respect to the stars<\/dd>\r\n<\/dl>\r\n<dl id=\"fs-id1168046090564\">\r\n \t<dt id=\"111\">solar day<\/dt>\r\n \t<dd id=\"fs-id1168048594364\">Earth\u2019s rotation period as defined by the position of the Sun in the sky; the time between successive passages of the Sun through the meridian<\/dd>\r\n<\/dl>\r\n<dl id=\"fs-id1168047518349\">\r\n \t<dt id=\"14\">solar eclipse<\/dt>\r\n \t<dd id=\"fs-id1168047542224\">an eclipse of the Sun by the Moon, caused by the passage of the Moon in front of the Sun; solar eclipses can occur only at the time of the new moon<\/dd>\r\n<\/dl>\r\n<dl id=\"fs-id1168047645340\">\r\n \t<dt id=\"91\">solar month<\/dt>\r\n \t<dd id=\"fs-id1168047959915\">the time interval in which the phases repeat\u2014say, from full to full phase<\/dd>\r\n<\/dl>\r\n<dl id=\"fs-id1168047697874\">\r\n \t<dt id=\"101\">synchronous rotation<\/dt>\r\n \t<dd id=\"fs-id1168047647868\">when a body (for example, the Moon) rotates at the same rate that it revolves around another body<\/dd>\r\n<\/dl>\r\n<dl id=\"fs-id1168047221106\">\r\n \t<dt id=\"131\">tides<\/dt>\r\n \t<dd id=\"fs-id1168047201483\">alternate rising and falling of sea level caused by the difference in the strength of the Moon\u2019s gravitational pull on different parts of Earth<\/dd>\r\n<\/dl>\r\n<div class=\"textbox\">This book was adapted from the following: Fraknoi, A., Morrison, D., &amp; Wolff, S. C. (2016). Key Terms. In <i>Astronomy<\/i>. OpenStax. https:\/\/openstax.org\/books\/astronomy\/pages\/4-key-terms under a <a href=\"http:\/\/creativecommons.org\/licenses\/by\/4.0\/\" target=\"_blank\" rel=\"noopener noreferrer\">Creative Commons Attribution License 4.0<\/a><\/div>\r\n<div>Access the entire book for free at <a href=\"https:\/\/openstax.org\/books\/astronomy\/pages\/1-introduction\">https:\/\/openstax.org\/books\/astronomy\/pages\/1-introduction<\/a><\/div>","rendered":"<dl id=\"fs-id1168048332291\">\n<dt id=\"7\">apparent solar time<\/dt>\n<dd id=\"fs-id1168048481217\">time as measured by the position of the Sun in the sky (the time that would be indicated by a sundial)<\/dd>\n<\/dl>\n<dl id=\"fs-id1168048623216\">\n<dt id=\"8\">declination<\/dt>\n<dd id=\"fs-id1168046348880\">the angular distance north or south of the celestial equator<\/dd>\n<\/dl>\n<dl id=\"fs-id1168048291103\">\n<dt id=\"9\">great circle<\/dt>\n<dd id=\"fs-id1168048374770\">a circle on the surface of a sphere that is the curve of intersection of the sphere with a plane passing through its center<\/dd>\n<\/dl>\n<dl id=\"fs-id1168048515777\">\n<dt id=\"80\">International Date Line<\/dt>\n<dd id=\"fs-id1168048282502\">an arbitrary line on the surface of Earth near longitude 180\u00b0 across which the date changes by one day<\/dd>\n<\/dl>\n<dl id=\"fs-id1168047141002\">\n<dt id=\"13\">lunar eclipse<\/dt>\n<dd id=\"fs-id1168047134019\">an eclipse of the Moon, in which the Moon moves into the shadow of Earth; lunar eclipses can occur only at the time of full moon<\/dd>\n<\/dl>\n<dl id=\"fs-id1168048449754\">\n<dt id=\"90\">mean solar time<\/dt>\n<dd id=\"fs-id1168048511927\">time based on the rotation of Earth; mean solar time passes at a constant rate, unlike apparent solar time<\/dd>\n<\/dl>\n<dl id=\"fs-id1168048403578\">\n<dt id=\"10\">meridian<\/dt>\n<dd id=\"fs-id1168048535627\">a great circle on the terrestrial or celestial sphere that passes through the poles<\/dd>\n<\/dl>\n<dl id=\"fs-id1168047360264\">\n<dt id=\"70\">phases of the Moon<\/dt>\n<dd id=\"fs-id1168047792933\">the different appearance of light and dark on the Moon as seen from Earth during its monthly cycle, from new moon to full moon and back to new moon<\/dd>\n<\/dl>\n<dl id=\"fs-id1168048320963\">\n<dt id=\"11\">right ascension<\/dt>\n<dd id=\"fs-id1168048290756\">the coordinate for measuring the east-west positions of celestial bodies; the angle measured eastward along the celestial equator from the vernal equinox to the hour circle passing through a body<\/dd>\n<\/dl>\n<dl id=\"fs-id1168046060994\">\n<dt id=\"100\">sidereal day<\/dt>\n<dd id=\"fs-id1168048499590\">Earth\u2019s rotation period as defined by the positions of the stars in the sky; the time between successive passages of the same star through the meridian<\/dd>\n<\/dl>\n<dl id=\"fs-id1168047194530\">\n<dt id=\"81\">sidereal month<\/dt>\n<dd id=\"fs-id1168047973882\">the period of the Moon\u2019s revolution about Earth measured with respect to the stars<\/dd>\n<\/dl>\n<dl id=\"fs-id1168046090564\">\n<dt id=\"111\">solar day<\/dt>\n<dd id=\"fs-id1168048594364\">Earth\u2019s rotation period as defined by the position of the Sun in the sky; the time between successive passages of the Sun through the meridian<\/dd>\n<\/dl>\n<dl id=\"fs-id1168047518349\">\n<dt id=\"14\">solar eclipse<\/dt>\n<dd id=\"fs-id1168047542224\">an eclipse of the Sun by the Moon, caused by the passage of the Moon in front of the Sun; solar eclipses can occur only at the time of the new moon<\/dd>\n<\/dl>\n<dl id=\"fs-id1168047645340\">\n<dt id=\"91\">solar month<\/dt>\n<dd id=\"fs-id1168047959915\">the time interval in which the phases repeat\u2014say, from full to full phase<\/dd>\n<\/dl>\n<dl id=\"fs-id1168047697874\">\n<dt id=\"101\">synchronous rotation<\/dt>\n<dd id=\"fs-id1168047647868\">when a body (for example, the Moon) rotates at the same rate that it revolves around another body<\/dd>\n<\/dl>\n<dl id=\"fs-id1168047221106\">\n<dt id=\"131\">tides<\/dt>\n<dd id=\"fs-id1168047201483\">alternate rising and falling of sea level caused by the difference in the strength of the Moon\u2019s gravitational pull on different parts of Earth<\/dd>\n<\/dl>\n<div class=\"textbox\">This book was adapted from the following: Fraknoi, A., Morrison, D., &amp; Wolff, S. C. (2016). Key Terms. In <i>Astronomy<\/i>. OpenStax. https:\/\/openstax.org\/books\/astronomy\/pages\/4-key-terms under a <a href=\"http:\/\/creativecommons.org\/licenses\/by\/4.0\/\" target=\"_blank\" rel=\"noopener noreferrer\">Creative Commons Attribution License 4.0<\/a><\/div>\n<div>Access the entire book for free at <a href=\"https:\/\/openstax.org\/books\/astronomy\/pages\/1-introduction\">https:\/\/openstax.org\/books\/astronomy\/pages\/1-introduction<\/a><\/div>\n","protected":false},"author":33,"menu_order":8,"template":"","meta":{"pb_show_title":"on","pb_short_title":"","pb_subtitle":"","pb_authors":[],"pb_section_license":""},"chapter-type":[48],"contributor":[],"license":[],"class_list":["post-245","chapter","type-chapter","status-publish","hentry","chapter-type-numberless"],"part":222,"_links":{"self":[{"href":"https:\/\/pressbooks.ccconline.org\/astronomy\/wp-json\/pressbooks\/v2\/chapters\/245","targetHints":{"allow":["GET"]}}],"collection":[{"href":"https:\/\/pressbooks.ccconline.org\/astronomy\/wp-json\/pressbooks\/v2\/chapters"}],"about":[{"href":"https:\/\/pressbooks.ccconline.org\/astronomy\/wp-json\/wp\/v2\/types\/chapter"}],"author":[{"embeddable":true,"href":"https:\/\/pressbooks.ccconline.org\/astronomy\/wp-json\/wp\/v2\/users\/33"}],"version-history":[{"count":2,"href":"https:\/\/pressbooks.ccconline.org\/astronomy\/wp-json\/pressbooks\/v2\/chapters\/245\/revisions"}],"predecessor-version":[{"id":251,"href":"https:\/\/pressbooks.ccconline.org\/astronomy\/wp-json\/pressbooks\/v2\/chapters\/245\/revisions\/251"}],"part":[{"href":"https:\/\/pressbooks.ccconline.org\/astronomy\/wp-json\/pressbooks\/v2\/parts\/222"}],"metadata":[{"href":"https:\/\/pressbooks.ccconline.org\/astronomy\/wp-json\/pressbooks\/v2\/chapters\/245\/metadata\/"}],"wp:attachment":[{"href":"https:\/\/pressbooks.ccconline.org\/astronomy\/wp-json\/wp\/v2\/media?parent=245"}],"wp:term":[{"taxonomy":"chapter-type","embeddable":true,"href":"https:\/\/pressbooks.ccconline.org\/astronomy\/wp-json\/pressbooks\/v2\/chapter-type?post=245"},{"taxonomy":"contributor","embeddable":true,"href":"https:\/\/pressbooks.ccconline.org\/astronomy\/wp-json\/wp\/v2\/contributor?post=245"},{"taxonomy":"license","embeddable":true,"href":"https:\/\/pressbooks.ccconline.org\/astronomy\/wp-json\/wp\/v2\/license?post=245"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}