{"id":141,"date":"2022-02-07T22:19:07","date_gmt":"2022-02-07T22:19:07","guid":{"rendered":"https:\/\/pressbooks.ccconline.org\/astronomy\/?post_type=chapter&#038;p=141"},"modified":"2022-02-11T15:50:03","modified_gmt":"2022-02-11T15:50:03","slug":"chapter-2-key-terms","status":"publish","type":"chapter","link":"https:\/\/pressbooks.ccconline.org\/astronomy\/chapter\/chapter-2-key-terms\/","title":{"raw":"Chapter 2 Key Terms","rendered":"Chapter 2 Key Terms"},"content":{"raw":"<dl id=\"fs-id1170326396909\">\r\n \t<dt id=\"13\">accelerate<\/dt>\r\n \t<dd id=\"fs-id1170326470898\">to change velocity; to speed up, slow down, or change direction.<\/dd>\r\n<\/dl>\r\n<dl id=\"fs-id1170325095551\">\r\n \t<dt id=\"15\">apparent magnitude<\/dt>\r\n \t<dd id=\"fs-id1170325095556\">a measure of how bright a star looks in the sky; the larger the number, the dimmer the star appears to us<\/dd>\r\n<\/dl>\r\n<dl id=\"fs-id1170326143963\">\r\n \t<dt id=\"5\">astrology<\/dt>\r\n \t<dd id=\"fs-id1170326283014\">the pseudoscience that deals with the supposed influences on human destiny of the configurations and locations in the sky of the Sun, Moon, and planets<\/dd>\r\n<\/dl>\r\n<dl id=\"fs-id1170324970349\">\r\n \t<dt id=\"18\">celestial equator<\/dt>\r\n \t<dd id=\"fs-id1170325093696\">a great circle on the celestial sphere 90\u00b0 from the celestial poles; where the celestial sphere intersects the plane of Earth\u2019s equator<\/dd>\r\n<\/dl>\r\n<dl id=\"fs-id1170325002253\">\r\n \t<dt id=\"19\">celestial poles<\/dt>\r\n \t<dd id=\"fs-id1170325088497\">points about which the celestial sphere appears to rotate; intersections of the celestial sphere with Earth\u2019s polar axis<\/dd>\r\n<\/dl>\r\n<dl id=\"fs-id1170325064102\">\r\n \t<dt id=\"20\">celestial sphere<\/dt>\r\n \t<dd id=\"fs-id1170324987060\">the apparent sphere of the sky; a sphere of large radius centered on the observer; directions of objects in the sky can be denoted by their position on the celestial sphere<\/dd>\r\n<\/dl>\r\n<dl id=\"fs-id1170325032942\">\r\n \t<dt id=\"21\">circumpolar zone<\/dt>\r\n \t<dd id=\"fs-id1170324989580\">those portions of the celestial sphere near the celestial poles that are either always above or always below the horizon<\/dd>\r\n<\/dl>\r\n<dl id=\"fs-id1170325095562\">\r\n \t<dt id=\"16\">cosmology<\/dt>\r\n \t<dd id=\"fs-id1170325095567\">the study of the organization and evolution of the universe<\/dd>\r\n<\/dl>\r\n<dl id=\"fs-id1170324969936\">\r\n \t<dt id=\"22\">ecliptic<\/dt>\r\n \t<dd id=\"fs-id1170325067672\">the apparent annual path of the Sun on the celestial sphere<\/dd>\r\n<\/dl>\r\n<dl id=\"fs-id1170325095571\">\r\n \t<dt id=\"17\">epicycle<\/dt>\r\n \t<dd id=\"fs-id1170325095577\">the circular orbit of a body in the Ptolemaic system, the center of which revolves about another circle (the deferent)<\/dd>\r\n<\/dl>\r\n<dl id=\"fs-id1170325055979\">\r\n \t<dt id=\"23\">geocentric<\/dt>\r\n \t<dd id=\"fs-id1170324968036\">centered on Earth<\/dd>\r\n<\/dl>\r\n<dl id=\"fs-id1170326450350\">\r\n \t<dt id=\"14\">heliocentric<\/dt>\r\n \t<dd id=\"fs-id1170326322884\">centered on the Sun<\/dd>\r\n<\/dl>\r\n<dl id=\"fs-id1170324944293\">\r\n \t<dt id=\"24\">horizon (astronomical)<\/dt>\r\n \t<dd id=\"fs-id1170325093639\">a great circle on the celestial sphere 90\u00b0 from the zenith; more popularly, the circle around us where the dome of the sky meets Earth<\/dd>\r\n<\/dl>\r\n<dl id=\"fs-id1170326165367\">\r\n \t<dt id=\"6\">horoscope<\/dt>\r\n \t<dd id=\"fs-id1170326223008\">a chart used by astrologers that shows the positions along the zodiac and in the sky of the Sun, Moon, and planets at some given instant and as seen from a particular place on Earth\u2014usually corresponding to the time and place of a person\u2019s birth<\/dd>\r\n<\/dl>\r\n<dl id=\"fs-id1170325095582\">\r\n \t<dt id=\"180\">parallax<\/dt>\r\n \t<dd id=\"fs-id1170325062431\">the apparent displacement of a nearby star that results from the motion of Earth around the Sun<\/dd>\r\n<\/dl>\r\n<dl id=\"fs-id1170325049170\">\r\n \t<dt id=\"25\">planet<\/dt>\r\n \t<dd id=\"fs-id1170324989909\">today, any of the larger objects revolving about the Sun or any similar objects that orbit other stars; in ancient times, any object that moved regularly among the fixed stars<\/dd>\r\n<\/dl>\r\n<dl id=\"fs-id1170325016119\">\r\n \t<dt id=\"190\">precession (of Earth)<\/dt>\r\n \t<dd id=\"fs-id1170325069396\">the slow, conical motion of Earth\u2019s axis of rotation caused principally by the gravitational pull of the Moon and Sun on Earth\u2019s equatorial bulge<\/dd>\r\n<\/dl>\r\n<dl id=\"fs-id1170325210121\">\r\n \t<dt id=\"200\">retrograde motion<\/dt>\r\n \t<dd id=\"fs-id1170325210126\">the apparent westward motion of a planet on the celestial sphere or with respect to the stars<\/dd>\r\n<\/dl>\r\n<dl id=\"fs-id1170324920069\">\r\n \t<dt id=\"26\">year<\/dt>\r\n \t<dd id=\"fs-id1170325095723\">the period of revolution of Earth around the Sun<\/dd>\r\n<\/dl>\r\n<dl id=\"fs-id1170324984349\">\r\n \t<dt id=\"27\">zenith<\/dt>\r\n \t<dd id=\"fs-id1170325057193\">the point on the celestial sphere opposite the direction of gravity; point directly above the observer<\/dd>\r\n<\/dl>\r\n<dl id=\"fs-id1170325073502\">\r\n \t<dt id=\"28\">zodiac<\/dt>\r\n \t<dd id=\"fs-id1170325082987\">a belt around the sky about 18\u00b0 wide centered on the ecliptic<\/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\/2-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-id1170326396909\">\n<dt id=\"13\">accelerate<\/dt>\n<dd id=\"fs-id1170326470898\">to change velocity; to speed up, slow down, or change direction.<\/dd>\n<\/dl>\n<dl id=\"fs-id1170325095551\">\n<dt id=\"15\">apparent magnitude<\/dt>\n<dd id=\"fs-id1170325095556\">a measure of how bright a star looks in the sky; the larger the number, the dimmer the star appears to us<\/dd>\n<\/dl>\n<dl id=\"fs-id1170326143963\">\n<dt id=\"5\">astrology<\/dt>\n<dd id=\"fs-id1170326283014\">the pseudoscience that deals with the supposed influences on human destiny of the configurations and locations in the sky of the Sun, Moon, and planets<\/dd>\n<\/dl>\n<dl id=\"fs-id1170324970349\">\n<dt id=\"18\">celestial equator<\/dt>\n<dd id=\"fs-id1170325093696\">a great circle on the celestial sphere 90\u00b0 from the celestial poles; where the celestial sphere intersects the plane of Earth\u2019s equator<\/dd>\n<\/dl>\n<dl id=\"fs-id1170325002253\">\n<dt id=\"19\">celestial poles<\/dt>\n<dd id=\"fs-id1170325088497\">points about which the celestial sphere appears to rotate; intersections of the celestial sphere with Earth\u2019s polar axis<\/dd>\n<\/dl>\n<dl id=\"fs-id1170325064102\">\n<dt id=\"20\">celestial sphere<\/dt>\n<dd id=\"fs-id1170324987060\">the apparent sphere of the sky; a sphere of large radius centered on the observer; directions of objects in the sky can be denoted by their position on the celestial sphere<\/dd>\n<\/dl>\n<dl id=\"fs-id1170325032942\">\n<dt id=\"21\">circumpolar zone<\/dt>\n<dd id=\"fs-id1170324989580\">those portions of the celestial sphere near the celestial poles that are either always above or always below the horizon<\/dd>\n<\/dl>\n<dl id=\"fs-id1170325095562\">\n<dt id=\"16\">cosmology<\/dt>\n<dd id=\"fs-id1170325095567\">the study of the organization and evolution of the universe<\/dd>\n<\/dl>\n<dl id=\"fs-id1170324969936\">\n<dt id=\"22\">ecliptic<\/dt>\n<dd id=\"fs-id1170325067672\">the apparent annual path of the Sun on the celestial sphere<\/dd>\n<\/dl>\n<dl id=\"fs-id1170325095571\">\n<dt id=\"17\">epicycle<\/dt>\n<dd id=\"fs-id1170325095577\">the circular orbit of a body in the Ptolemaic system, the center of which revolves about another circle (the deferent)<\/dd>\n<\/dl>\n<dl id=\"fs-id1170325055979\">\n<dt id=\"23\">geocentric<\/dt>\n<dd id=\"fs-id1170324968036\">centered on Earth<\/dd>\n<\/dl>\n<dl id=\"fs-id1170326450350\">\n<dt id=\"14\">heliocentric<\/dt>\n<dd id=\"fs-id1170326322884\">centered on the Sun<\/dd>\n<\/dl>\n<dl id=\"fs-id1170324944293\">\n<dt id=\"24\">horizon (astronomical)<\/dt>\n<dd id=\"fs-id1170325093639\">a great circle on the celestial sphere 90\u00b0 from the zenith; more popularly, the circle around us where the dome of the sky meets Earth<\/dd>\n<\/dl>\n<dl id=\"fs-id1170326165367\">\n<dt id=\"6\">horoscope<\/dt>\n<dd id=\"fs-id1170326223008\">a chart used by astrologers that shows the positions along the zodiac and in the sky of the Sun, Moon, and planets at some given instant and as seen from a particular place on Earth\u2014usually corresponding to the time and place of a person\u2019s birth<\/dd>\n<\/dl>\n<dl id=\"fs-id1170325095582\">\n<dt id=\"180\">parallax<\/dt>\n<dd id=\"fs-id1170325062431\">the apparent displacement of a nearby star that results from the motion of Earth around the Sun<\/dd>\n<\/dl>\n<dl id=\"fs-id1170325049170\">\n<dt id=\"25\">planet<\/dt>\n<dd id=\"fs-id1170324989909\">today, any of the larger objects revolving about the Sun or any similar objects that orbit other stars; in ancient times, any object that moved regularly among the fixed stars<\/dd>\n<\/dl>\n<dl id=\"fs-id1170325016119\">\n<dt id=\"190\">precession (of Earth)<\/dt>\n<dd id=\"fs-id1170325069396\">the slow, conical motion of Earth\u2019s axis of rotation caused principally by the gravitational pull of the Moon and Sun on Earth\u2019s equatorial bulge<\/dd>\n<\/dl>\n<dl id=\"fs-id1170325210121\">\n<dt id=\"200\">retrograde motion<\/dt>\n<dd id=\"fs-id1170325210126\">the apparent westward motion of a planet on the celestial sphere or with respect to the stars<\/dd>\n<\/dl>\n<dl id=\"fs-id1170324920069\">\n<dt id=\"26\">year<\/dt>\n<dd id=\"fs-id1170325095723\">the period of revolution of Earth around the Sun<\/dd>\n<\/dl>\n<dl id=\"fs-id1170324984349\">\n<dt id=\"27\">zenith<\/dt>\n<dd id=\"fs-id1170325057193\">the point on the celestial sphere opposite the direction of gravity; point directly above the observer<\/dd>\n<\/dl>\n<dl id=\"fs-id1170325073502\">\n<dt id=\"28\">zodiac<\/dt>\n<dd id=\"fs-id1170325082987\">a belt around the sky about 18\u00b0 wide centered on the ecliptic<\/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\/2-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":11,"template":"","meta":{"pb_show_title":"on","pb_short_title":"","pb_subtitle":"","pb_authors":[],"pb_section_license":""},"chapter-type":[48],"contributor":[],"license":[],"class_list":["post-141","chapter","type-chapter","status-publish","hentry","chapter-type-numberless"],"part":98,"_links":{"self":[{"href":"https:\/\/pressbooks.ccconline.org\/astronomy\/wp-json\/pressbooks\/v2\/chapters\/141","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\/141\/revisions"}],"predecessor-version":[{"id":206,"href":"https:\/\/pressbooks.ccconline.org\/astronomy\/wp-json\/pressbooks\/v2\/chapters\/141\/revisions\/206"}],"part":[{"href":"https:\/\/pressbooks.ccconline.org\/astronomy\/wp-json\/pressbooks\/v2\/parts\/98"}],"metadata":[{"href":"https:\/\/pressbooks.ccconline.org\/astronomy\/wp-json\/pressbooks\/v2\/chapters\/141\/metadata\/"}],"wp:attachment":[{"href":"https:\/\/pressbooks.ccconline.org\/astronomy\/wp-json\/wp\/v2\/media?parent=141"}],"wp:term":[{"taxonomy":"chapter-type","embeddable":true,"href":"https:\/\/pressbooks.ccconline.org\/astronomy\/wp-json\/pressbooks\/v2\/chapter-type?post=141"},{"taxonomy":"contributor","embeddable":true,"href":"https:\/\/pressbooks.ccconline.org\/astronomy\/wp-json\/wp\/v2\/contributor?post=141"},{"taxonomy":"license","embeddable":true,"href":"https:\/\/pressbooks.ccconline.org\/astronomy\/wp-json\/wp\/v2\/license?post=141"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}