{"id":303,"date":"2022-02-11T17:15:23","date_gmt":"2022-02-11T17:15:23","guid":{"rendered":"https:\/\/pressbooks.ccconline.org\/astronomy\/?post_type=part&#038;p=303"},"modified":"2022-02-11T17:15:23","modified_gmt":"2022-02-11T17:15:23","slug":"chapter-6-astronomical-instruments","status":"publish","type":"part","link":"https:\/\/pressbooks.ccconline.org\/astronomy\/part\/chapter-6-astronomical-instruments\/","title":{"raw":"Chapter 6 Astronomical Instruments","rendered":"Chapter 6 Astronomical Instruments"},"content":{"raw":"<div>\r\n<div id=\"OSC_Astro_06_00_HubbleST\" class=\"os-figure has-splash\">\r\n<figure class=\"splash\" data-id=\"OSC_Astro_06_00_HubbleST\">\r\n\r\n[caption id=\"\" align=\"aligncenter\" width=\"1312\"]<img id=\"2\" src=\"https:\/\/openstax.org\/apps\/archive\/20210823.155019\/resources\/f6dbd02932efdb827deb9aa8497c7808a33fd1b0\" alt=\"Artist's depiction of the Hubble Space Telescope\" width=\"1312\" height=\"553\" data-media-type=\"image\/jpeg\" \/> <strong>Figure\u00a06.1<\/strong>\u00a0Hubble Space Telescope (HST).\u00a0This artist\u2019s impression shows the Hubble above Earth, with the rectangular solar panels that provide it with power seen to the left and right.[\/caption]<\/figure>\r\n<\/div>\r\n<div class=\"intro-body\">\r\n<div class=\"os-chapter-outline\">\r\n<h3 class=\"os-title\">Chapter Outline<\/h3>\r\n<div class=\"os-chapter-objective\"><span class=\"os-number\">6.1<\/span><span class=\"os-divider\">\u00a0<\/span><span class=\"os-text\" data-type=\"\">Telescopes<\/span><\/div>\r\n<div class=\"os-chapter-objective\"><span class=\"os-number\">6.2<\/span><span class=\"os-divider\">\u00a0<\/span><span class=\"os-text\" data-type=\"\">Telescopes Today<\/span><\/div>\r\n<div class=\"os-chapter-objective\"><span class=\"os-number\">6.3<\/span><span class=\"os-divider\">\u00a0<\/span><span class=\"os-text\" data-type=\"\">Visible-Light Detectors and Instruments<\/span><\/div>\r\n<div class=\"os-chapter-objective\"><span class=\"os-number\">6.4<\/span><span class=\"os-divider\">\u00a0<\/span><span class=\"os-text\" data-type=\"\">Radio Telescopes<\/span><\/div>\r\n<div class=\"os-chapter-objective\"><span class=\"os-number\">6.5<\/span><span class=\"os-divider\">\u00a0<\/span><span class=\"os-text\" data-type=\"\">Observations outside Earth\u2019s Atmosphere<\/span><\/div>\r\n<div class=\"os-chapter-objective\"><span class=\"os-number\">6.6<\/span><span class=\"os-divider\">\u00a0<\/span><span class=\"os-text\" data-type=\"\">The Future of Large Telescopes<\/span><\/div>\r\n<\/div>\r\n<div class=\"intro-text\">\r\n<p id=\"fs-id1167471063116\" class=\" \">If you look at the sky when you are far away from city lights, there seem to be an overwhelming number of stars up there. In reality, only about 9000 stars are visible to the unaided eye (from both hemispheres of our planet). The light from most stars is so weak that by the time it reaches Earth, it cannot be detected by the human eye. How can we learn about the vast majority of objects in the universe that our unaided eyes simply cannot see?<\/p>\r\n<p id=\"fs-id1167470969727\" class=\" \">In this chapter, we describe the tools astronomers use to extend their vision into space. We have learned almost everything we know about the universe from studying electromagnetic radiation, as discussed in the chapter on\u00a0Radiation and Spectra (Chapter 5). In the twentieth century, our exploration of space made it possible to detect electromagnetic radiation at all wavelengths, from gamma rays to radio waves. The different wavelengths carry different kinds of information, and the appearance of any given object often depends on the wavelength at which the observations are made.<\/p>\r\n\r\n<\/div>\r\n<\/div>\r\n<\/div>\r\n<div class=\"textbox\">This book was adapted from the following: Fraknoi, A., Morrison, D., &amp; Wolff, S. C. (2016). Thinking Ahead. In <i>Astronomy<\/i>. OpenStax. https:\/\/openstax.org\/books\/astronomy\/pages\/6-thinking-ahead 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":"<div>\n<div id=\"OSC_Astro_06_00_HubbleST\" class=\"os-figure has-splash\">\n<figure class=\"splash\" data-id=\"OSC_Astro_06_00_HubbleST\">\n<figure style=\"width: 1312px\" class=\"wp-caption aligncenter\"><img loading=\"lazy\" decoding=\"async\" id=\"2\" src=\"https:\/\/openstax.org\/apps\/archive\/20210823.155019\/resources\/f6dbd02932efdb827deb9aa8497c7808a33fd1b0\" alt=\"Artist's depiction of the Hubble Space Telescope\" width=\"1312\" height=\"553\" data-media-type=\"image\/jpeg\" \/><figcaption class=\"wp-caption-text\"><strong>Figure\u00a06.1<\/strong>\u00a0Hubble Space Telescope (HST).\u00a0This artist\u2019s impression shows the Hubble above Earth, with the rectangular solar panels that provide it with power seen to the left and right.<\/figcaption><\/figure>\n<\/figure>\n<\/div>\n<div class=\"intro-body\">\n<div class=\"os-chapter-outline\">\n<h3 class=\"os-title\">Chapter Outline<\/h3>\n<div class=\"os-chapter-objective\"><span class=\"os-number\">6.1<\/span><span class=\"os-divider\">\u00a0<\/span><span class=\"os-text\" data-type=\"\">Telescopes<\/span><\/div>\n<div class=\"os-chapter-objective\"><span class=\"os-number\">6.2<\/span><span class=\"os-divider\">\u00a0<\/span><span class=\"os-text\" data-type=\"\">Telescopes Today<\/span><\/div>\n<div class=\"os-chapter-objective\"><span class=\"os-number\">6.3<\/span><span class=\"os-divider\">\u00a0<\/span><span class=\"os-text\" data-type=\"\">Visible-Light Detectors and Instruments<\/span><\/div>\n<div class=\"os-chapter-objective\"><span class=\"os-number\">6.4<\/span><span class=\"os-divider\">\u00a0<\/span><span class=\"os-text\" data-type=\"\">Radio Telescopes<\/span><\/div>\n<div class=\"os-chapter-objective\"><span class=\"os-number\">6.5<\/span><span class=\"os-divider\">\u00a0<\/span><span class=\"os-text\" data-type=\"\">Observations outside Earth\u2019s Atmosphere<\/span><\/div>\n<div class=\"os-chapter-objective\"><span class=\"os-number\">6.6<\/span><span class=\"os-divider\">\u00a0<\/span><span class=\"os-text\" data-type=\"\">The Future of Large Telescopes<\/span><\/div>\n<\/div>\n<div class=\"intro-text\">\n<p id=\"fs-id1167471063116\" class=\"\">If you look at the sky when you are far away from city lights, there seem to be an overwhelming number of stars up there. In reality, only about 9000 stars are visible to the unaided eye (from both hemispheres of our planet). The light from most stars is so weak that by the time it reaches Earth, it cannot be detected by the human eye. How can we learn about the vast majority of objects in the universe that our unaided eyes simply cannot see?<\/p>\n<p id=\"fs-id1167470969727\" class=\"\">In this chapter, we describe the tools astronomers use to extend their vision into space. We have learned almost everything we know about the universe from studying electromagnetic radiation, as discussed in the chapter on\u00a0Radiation and Spectra (Chapter 5). In the twentieth century, our exploration of space made it possible to detect electromagnetic radiation at all wavelengths, from gamma rays to radio waves. The different wavelengths carry different kinds of information, and the appearance of any given object often depends on the wavelength at which the observations are made.<\/p>\n<\/div>\n<\/div>\n<\/div>\n<div class=\"textbox\">This book was adapted from the following: Fraknoi, A., Morrison, D., &amp; Wolff, S. C. (2016). Thinking Ahead. In <i>Astronomy<\/i>. OpenStax. https:\/\/openstax.org\/books\/astronomy\/pages\/6-thinking-ahead 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},"parent":0,"menu_order":6,"template":"","meta":{"pb_part_invisible":false,"pb_part_invisible_string":""},"contributor":[],"license":[],"class_list":["post-303","part","type-part","status-publish","hentry"],"_links":{"self":[{"href":"https:\/\/pressbooks.ccconline.org\/astronomy\/wp-json\/pressbooks\/v2\/parts\/303","targetHints":{"allow":["GET"]}}],"collection":[{"href":"https:\/\/pressbooks.ccconline.org\/astronomy\/wp-json\/pressbooks\/v2\/parts"}],"about":[{"href":"https:\/\/pressbooks.ccconline.org\/astronomy\/wp-json\/wp\/v2\/types\/part"}],"version-history":[{"count":1,"href":"https:\/\/pressbooks.ccconline.org\/astronomy\/wp-json\/pressbooks\/v2\/parts\/303\/revisions"}],"predecessor-version":[{"id":304,"href":"https:\/\/pressbooks.ccconline.org\/astronomy\/wp-json\/pressbooks\/v2\/parts\/303\/revisions\/304"}],"wp:attachment":[{"href":"https:\/\/pressbooks.ccconline.org\/astronomy\/wp-json\/wp\/v2\/media?parent=303"}],"wp:term":[{"taxonomy":"contributor","embeddable":true,"href":"https:\/\/pressbooks.ccconline.org\/astronomy\/wp-json\/wp\/v2\/contributor?post=303"},{"taxonomy":"license","embeddable":true,"href":"https:\/\/pressbooks.ccconline.org\/astronomy\/wp-json\/wp\/v2\/license?post=303"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}