{"id":47,"date":"2016-11-15T21:35:40","date_gmt":"2016-11-15T21:35:40","guid":{"rendered":"https:\/\/courses.lumenlearning.com\/astronomy\/?post_type=chapter&#038;p=47"},"modified":"2018-01-22T15:29:06","modified_gmt":"2018-01-22T15:29:06","slug":"numbers-in-astronomy","status":"publish","type":"chapter","link":"https:\/\/courses.lumenlearning.com\/suny-geneseo-astronomy\/chapter\/numbers-in-astronomy\/","title":{"raw":"1.4 Numbers in Astronomy","rendered":"1.4 Numbers in Astronomy"},"content":{"raw":"In astronomy we deal with distances on a scale you may never have thought about before, with numbers larger than any you may have encountered. We adopt two approaches that make dealing with astronomical numbers a little bit easier. First, we use a system for writing large and small numbers called <em>scientific notation<\/em> (or sometimes <em>powers-of-ten notation<\/em>). This system is very appealing because it eliminates the many zeros that can seem overwhelming to the reader. In scientific notation, if you want to write a number such as 500,000,000, you express it as 5 \u00d7 10<sup>8<\/sup>. The small raised number after the 10, called an <em>exponent<\/em>, keeps track of the number of places we had to move the decimal point to the left to convert 500,000,000 to 5. If you are encountering this system for the first time or would like a refresher, we suggest you look at <a href=\".\/chapter\/scientific-notation\/\" target=\"_blank\" rel=\"noopener\">Scientific Notation<\/a>\u00a0and Example 1\u00a0for more information. The second way we try to keep numbers simple is to use a consistent set of units\u2014the metric International System of Units, or SI (from the French <em>Syst\u00e8me International d\u2019Unit\u00e9s<\/em>). The metric system is summarized in <a href=\".\/chapter\/units-used-in-science\/\" target=\"_blank\" rel=\"noopener\">Units Used in Science<\/a>\u00a0(see Example 2).\r\n<div class=\"textbox\"><a href=\"https:\/\/www.pbslearningmedia.org\/resource\/muen-math-ee-scientificnotation\/scientific-notation\/\" target=\"_blank\" rel=\"noopener\">Watch this brief PBS animation that explains how scientific notation works and why it\u2019s useful.<\/a><\/div>\r\nA common unit astronomers use to describe distances in the universe is a light-year, which is the distance light travels during one year. Because light always travels at the same speed, and because its speed turns out to be the fastest possible speed in the universe, it makes a good standard for keeping track of distances. You might be confused because a \"light-year\" seems to imply that we are measuring time, but this mix-up of time and distance is common in everyday life as well. For example, when your friend asks where the movie theater is located, you might say \"about 20 minutes from downtown.\"\r\n\r\nSo, how many kilometers are there in a light-year? Light travels at the amazing pace of 3 \u00d7 10<sup>5<\/sup> kilometers per second (km\/s), which makes a light-year 9.46 \u00d7 10<sup>12<\/sup> kilometers. You might think that such a large unit would reach the nearest star easily, but the stars are far more remote than our imaginations might lead us to believe. Even the nearest star is 4.3 light-years away\u2014more than 40 trillion kilometers. Other stars visible to the unaided eye are hundreds to thousands of light-years away (Figure 1).\r\n\r\n[caption id=\"\" align=\"aligncenter\" width=\"500\"]<img class=\"\" src=\"https:\/\/s3-us-west-2.amazonaws.com\/courses-images\/wp-content\/uploads\/sites\/1095\/2016\/11\/03154700\/OSC_Astro_01_04_Nebula.jpg\" alt=\"Photograph of the Orion Nebula. This image is dominated by large areas and bright swirls of glowing gas clouds, crisscrossed by dark bands of dust.\" width=\"500\" height=\"500\" \/> <strong>Figure 1: Orion Nebula.<\/strong> This beautiful cloud of cosmic raw material (gas and dust from which new stars and planets are being made) called the <strong>Orion Nebula<\/strong> is about 1400 light-years away. That\u2019s a distance of roughly 1.34 \u00d7 10<sup>16<\/sup> kilometers\u2014a pretty big number. The gas and dust in this region are illuminated by the intense light from a few extremely energetic adolescent stars. (credit: NASA, ESA, M. Robberto (Space Telescope Science Institute\/ESA) and the Hubble Space Telescope Orion Treasury Project Team)[\/caption]\r\n\r\n<div class=\"textbox examples\">\r\n<h3>Example 1: Scientific Notation<\/h3>\r\nIn 2015, the richest human being on our planet had a net worth of $79.2 billion. Some might say this is an astronomical sum of money. Express this amount in scientific notation.\r\n[reveal-answer q=\"744837\"]Show Solution[\/reveal-answer]\r\n[hidden-answer a=\"744837\"]$79.2 billion can be written $79,200,000,000. Expressed in scientific notation it becomes $7.92 \u00d7 10<sup>10<\/sup>.[\/hidden-answer]\r\n\r\n<\/div>\r\n<div class=\"textbox examples\">\r\n<h3>Example 2: Getting Familiar with a Light-Year<\/h3>\r\nHow many kilometers are there in a light-year?\r\n\r\n[reveal-answer q=\"113669\"]Show Solution[\/reveal-answer]\r\n[hidden-answer a=\"113669\"]\r\n\r\nLight travels 3 \u00d7 10<sup>5<\/sup> km in 1 s. So, let\u2019s calculate how far it goes in a year:\r\n<ul>\r\n \t<li>There are 60 (6 \u00d7 10<sup>1<\/sup>) s in 1 min, and 6 \u00d7 10<sup>1<\/sup> min in 1 h.<\/li>\r\n \t<li>Multiply these together and you find that there are 3.6 \u00d7 10<sup>3<\/sup> s\/h.<\/li>\r\n \t<li>Thus, light covers 3 \u00d7 10<sup>5<\/sup> km\/s \u00d7 3.6 \u00d7 10<sup>3<\/sup> s\/h = 1.08 \u00d7 10<sup>9<\/sup> km\/h.<\/li>\r\n \t<li>There are 24 or 2.4 \u00d7 10<sup>1<\/sup> h in a day, and 365.24 (3.65 \u00d7 10<sup>2<\/sup>) days in 1 y.<\/li>\r\n \t<li>The product of these two numbers is 8.77 \u00d7 10<sup>3<\/sup> h\/y.<\/li>\r\n \t<li>Multiplying this by 1.08 \u00d7 10<sup>9<\/sup> km\/h gives 9.46 \u00d7 10<sup>12<\/sup> km\/light-year.<\/li>\r\n<\/ul>\r\nThat\u2019s almost 10,000,000,000,000 km that light covers in a year. To help you imagine how long this distance is, we\u2019ll mention that a string 1 light-year long could fit around the circumference of Earth 236 million times.\r\n\r\n[\/hidden-answer]\r\n\r\n<\/div>","rendered":"<p>In astronomy we deal with distances on a scale you may never have thought about before, with numbers larger than any you may have encountered. We adopt two approaches that make dealing with astronomical numbers a little bit easier. First, we use a system for writing large and small numbers called <em>scientific notation<\/em> (or sometimes <em>powers-of-ten notation<\/em>). This system is very appealing because it eliminates the many zeros that can seem overwhelming to the reader. In scientific notation, if you want to write a number such as 500,000,000, you express it as 5 \u00d7 10<sup>8<\/sup>. The small raised number after the 10, called an <em>exponent<\/em>, keeps track of the number of places we had to move the decimal point to the left to convert 500,000,000 to 5. If you are encountering this system for the first time or would like a refresher, we suggest you look at <a href=\".\/chapter\/scientific-notation\/\" target=\"_blank\" rel=\"noopener\">Scientific Notation<\/a>\u00a0and Example 1\u00a0for more information. The second way we try to keep numbers simple is to use a consistent set of units\u2014the metric International System of Units, or SI (from the French <em>Syst\u00e8me International d\u2019Unit\u00e9s<\/em>). The metric system is summarized in <a href=\".\/chapter\/units-used-in-science\/\" target=\"_blank\" rel=\"noopener\">Units Used in Science<\/a>\u00a0(see Example 2).<\/p>\n<div class=\"textbox\"><a href=\"https:\/\/www.pbslearningmedia.org\/resource\/muen-math-ee-scientificnotation\/scientific-notation\/\" target=\"_blank\" rel=\"noopener\">Watch this brief PBS animation that explains how scientific notation works and why it\u2019s useful.<\/a><\/div>\n<p>A common unit astronomers use to describe distances in the universe is a light-year, which is the distance light travels during one year. Because light always travels at the same speed, and because its speed turns out to be the fastest possible speed in the universe, it makes a good standard for keeping track of distances. You might be confused because a &#8220;light-year&#8221; seems to imply that we are measuring time, but this mix-up of time and distance is common in everyday life as well. For example, when your friend asks where the movie theater is located, you might say &#8220;about 20 minutes from downtown.&#8221;<\/p>\n<p>So, how many kilometers are there in a light-year? Light travels at the amazing pace of 3 \u00d7 10<sup>5<\/sup> kilometers per second (km\/s), which makes a light-year 9.46 \u00d7 10<sup>12<\/sup> kilometers. You might think that such a large unit would reach the nearest star easily, but the stars are far more remote than our imaginations might lead us to believe. Even the nearest star is 4.3 light-years away\u2014more than 40 trillion kilometers. Other stars visible to the unaided eye are hundreds to thousands of light-years away (Figure 1).<\/p>\n<div style=\"width: 510px\" class=\"wp-caption aligncenter\"><img loading=\"lazy\" decoding=\"async\" class=\"\" src=\"https:\/\/s3-us-west-2.amazonaws.com\/courses-images\/wp-content\/uploads\/sites\/1095\/2016\/11\/03154700\/OSC_Astro_01_04_Nebula.jpg\" alt=\"Photograph of the Orion Nebula. This image is dominated by large areas and bright swirls of glowing gas clouds, crisscrossed by dark bands of dust.\" width=\"500\" height=\"500\" \/><\/p>\n<p class=\"wp-caption-text\"><strong>Figure 1: Orion Nebula.<\/strong> This beautiful cloud of cosmic raw material (gas and dust from which new stars and planets are being made) called the <strong>Orion Nebula<\/strong> is about 1400 light-years away. That\u2019s a distance of roughly 1.34 \u00d7 10<sup>16<\/sup> kilometers\u2014a pretty big number. The gas and dust in this region are illuminated by the intense light from a few extremely energetic adolescent stars. (credit: NASA, ESA, M. Robberto (Space Telescope Science Institute\/ESA) and the Hubble Space Telescope Orion Treasury Project Team)<\/p>\n<\/div>\n<div class=\"textbox examples\">\n<h3>Example 1: Scientific Notation<\/h3>\n<p>In 2015, the richest human being on our planet had a net worth of $79.2 billion. Some might say this is an astronomical sum of money. Express this amount in scientific notation.<\/p>\n<div class=\"qa-wrapper\" style=\"display: block\"><span class=\"show-answer collapsed\" style=\"cursor: pointer\" data-target=\"q744837\">Show Solution<\/span><\/p>\n<div id=\"q744837\" class=\"hidden-answer\" style=\"display: none\">$79.2 billion can be written $79,200,000,000. Expressed in scientific notation it becomes $7.92 \u00d7 10<sup>10<\/sup>.<\/div>\n<\/div>\n<\/div>\n<div class=\"textbox examples\">\n<h3>Example 2: Getting Familiar with a Light-Year<\/h3>\n<p>How many kilometers are there in a light-year?<\/p>\n<div class=\"qa-wrapper\" style=\"display: block\"><span class=\"show-answer collapsed\" style=\"cursor: pointer\" data-target=\"q113669\">Show Solution<\/span><\/p>\n<div id=\"q113669\" class=\"hidden-answer\" style=\"display: none\">\n<p>Light travels 3 \u00d7 10<sup>5<\/sup> km in 1 s. So, let\u2019s calculate how far it goes in a year:<\/p>\n<ul>\n<li>There are 60 (6 \u00d7 10<sup>1<\/sup>) s in 1 min, and 6 \u00d7 10<sup>1<\/sup> min in 1 h.<\/li>\n<li>Multiply these together and you find that there are 3.6 \u00d7 10<sup>3<\/sup> s\/h.<\/li>\n<li>Thus, light covers 3 \u00d7 10<sup>5<\/sup> km\/s \u00d7 3.6 \u00d7 10<sup>3<\/sup> s\/h = 1.08 \u00d7 10<sup>9<\/sup> km\/h.<\/li>\n<li>There are 24 or 2.4 \u00d7 10<sup>1<\/sup> h in a day, and 365.24 (3.65 \u00d7 10<sup>2<\/sup>) days in 1 y.<\/li>\n<li>The product of these two numbers is 8.77 \u00d7 10<sup>3<\/sup> h\/y.<\/li>\n<li>Multiplying this by 1.08 \u00d7 10<sup>9<\/sup> km\/h gives 9.46 \u00d7 10<sup>12<\/sup> km\/light-year.<\/li>\n<\/ul>\n<p>That\u2019s almost 10,000,000,000,000 km that light covers in a year. To help you imagine how long this distance is, we\u2019ll mention that a string 1 light-year long could fit around the circumference of Earth 236 million times.<\/p>\n<\/div>\n<\/div>\n<\/div>\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-47\">\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":5,"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-47","chapter","type-chapter","status-publish","hentry"],"part":38,"_links":{"self":[{"href":"https:\/\/courses.lumenlearning.com\/suny-geneseo-astronomy\/wp-json\/pressbooks\/v2\/chapters\/47","targetHints":{"allow":["GET"]}}],"collection":[{"href":"https:\/\/courses.lumenlearning.com\/suny-geneseo-astronomy\/wp-json\/pressbooks\/v2\/chapters"}],"about":[{"href":"https:\/\/courses.lumenlearning.com\/suny-geneseo-astronomy\/wp-json\/wp\/v2\/types\/chapter"}],"author":[{"embeddable":true,"href":"https:\/\/courses.lumenlearning.com\/suny-geneseo-astronomy\/wp-json\/wp\/v2\/users\/17"}],"version-history":[{"count":4,"href":"https:\/\/courses.lumenlearning.com\/suny-geneseo-astronomy\/wp-json\/pressbooks\/v2\/chapters\/47\/revisions"}],"predecessor-version":[{"id":2258,"href":"https:\/\/courses.lumenlearning.com\/suny-geneseo-astronomy\/wp-json\/pressbooks\/v2\/chapters\/47\/revisions\/2258"}],"part":[{"href":"https:\/\/courses.lumenlearning.com\/suny-geneseo-astronomy\/wp-json\/pressbooks\/v2\/parts\/38"}],"metadata":[{"href":"https:\/\/courses.lumenlearning.com\/suny-geneseo-astronomy\/wp-json\/pressbooks\/v2\/chapters\/47\/metadata\/"}],"wp:attachment":[{"href":"https:\/\/courses.lumenlearning.com\/suny-geneseo-astronomy\/wp-json\/wp\/v2\/media?parent=47"}],"wp:term":[{"taxonomy":"chapter-type","embeddable":true,"href":"https:\/\/courses.lumenlearning.com\/suny-geneseo-astronomy\/wp-json\/pressbooks\/v2\/chapter-type?post=47"},{"taxonomy":"contributor","embeddable":true,"href":"https:\/\/courses.lumenlearning.com\/suny-geneseo-astronomy\/wp-json\/wp\/v2\/contributor?post=47"},{"taxonomy":"license","embeddable":true,"href":"https:\/\/courses.lumenlearning.com\/suny-geneseo-astronomy\/wp-json\/wp\/v2\/license?post=47"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}