{"id":46,"date":"2022-02-07T16:21:36","date_gmt":"2022-02-07T16:21:36","guid":{"rendered":"https:\/\/pressbooks.ccconline.org\/astronomy\/chapter\/1-4numbers-in-astronomy\/"},"modified":"2022-04-21T19:18:27","modified_gmt":"2022-04-21T19:18:27","slug":"1-4numbers-in-astronomy","status":"publish","type":"chapter","link":"https:\/\/pressbooks.ccconline.org\/astronomy\/chapter\/1-4numbers-in-astronomy\/","title":{"raw":"1.4 Numbers in Astronomy","rendered":"1.4 Numbers in Astronomy"},"content":{"raw":"
\r\n

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\u00a0scientific notation<\/em>\u00a0(or sometimes\u00a0powers-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 [latex]5 \\times {10^8}[\/latex].<\/p>\r\n

The small raised number after the 10, called an 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\u00a0Appendix C\u00a0and\u00a0Example 1.1\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\u00a0Syst\u00e8me International d\u2019Unit\u00e9s<\/em>). The metric system is summarized in\u00a0Appendix D\u00a0(see\u00a0Example 1.2).<\/p>\r\n\r\n

\r\n

Link to Learning<\/h3>\r\n<\/header>\r\n
\r\n\r\nWatch this\u00a0brief PBS animation<\/a>\u00a0that explains how scientific notation works and why it\u2019s useful.\r\n\r\n<\/div>\r\n<\/div>\r\n

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 \u201clight-year\u201d 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 \u201cabout 20 minutes from downtown.\u201d<\/p>\r\n

So, how many kilometers are there in a light-year? Light travels at the amazing pace of [latex]3 \\times {10^5}[\/latex]\u00a0kilometers per second (km\/s), which makes a light-year [latex]9.46 \\times {10^{12}}[\/latex]\u00a0kilometers. 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 1.4).<\/p>\r\n\r\n

\r\n
\r\n\r\n[caption id=\"\" align=\"aligncenter\" width=\"487\"]\"Photograph Figure 1.4 Orion Nebula<\/strong>. This beautiful cloud of cosmic raw material (gas and dust from which new stars and planets are being made) called the Orion Nebula is about 1400 light-years away. That\u2019s a distance of roughly 1.34 \u00d7 1016 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
This book was adapted from the following: Fraknoi, A., Morrison, D., & Wolff, S. C. (2016). 1.4 Numbers in Astronomy. In Astronomy<\/i>. OpenStax. https:\/\/openstax.org\/books\/astronomy\/pages\/1-3-the-laws-of-nature under a Creative Commons Attribution License 4.0<\/a><\/div>\r\n
Access the entire book for free at https:\/\/openstax.org\/books\/astronomy\/pages\/1-introduction<\/a><\/div><\/figure>\r\n<\/div>\r\n<\/div>","rendered":"
\n

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\u00a0scientific notation<\/em>\u00a0(or sometimes\u00a0powers-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 [latex]5 \\times {10^8}[\/latex].<\/p>\n

The small raised number after the 10, called an 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\u00a0Appendix C\u00a0and\u00a0Example 1.1\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\u00a0Syst\u00e8me International d\u2019Unit\u00e9s<\/em>). The metric system is summarized in\u00a0Appendix D\u00a0(see\u00a0Example 1.2).<\/p>\n

\n
\n

Link to Learning<\/h3>\n<\/header>\n
\n

Watch this\u00a0brief PBS animation<\/a>\u00a0that explains how scientific notation works and why it\u2019s useful.<\/p>\n<\/div>\n<\/div>\n

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 \u201clight-year\u201d 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 \u201cabout 20 minutes from downtown.\u201d<\/p>\n

So, how many kilometers are there in a light-year? Light travels at the amazing pace of [latex]3 \\times {10^5}[\/latex]\u00a0kilometers per second (km\/s), which makes a light-year [latex]9.46 \\times {10^{12}}[\/latex]\u00a0kilometers. 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 1.4).<\/p>\n

\n
\n
\"Photograph
Figure 1.4 Orion Nebula<\/strong>. This beautiful cloud of cosmic raw material (gas and dust from which new stars and planets are being made) called the Orion Nebula is about 1400 light-years away. That\u2019s a distance of roughly 1.34 \u00d7 1016 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)<\/figcaption><\/figure>\n
This book was adapted from the following: Fraknoi, A., Morrison, D., & Wolff, S. C. (2016). 1.4 Numbers in Astronomy. In Astronomy<\/i>. OpenStax. https:\/\/openstax.org\/books\/astronomy\/pages\/1-3-the-laws-of-nature under a Creative Commons Attribution License 4.0<\/a><\/div>\n
Access the entire book for free at https:\/\/openstax.org\/books\/astronomy\/pages\/1-introduction<\/a><\/div>\n<\/figure>\n<\/div>\n<\/div>\n","protected":false},"author":33,"menu_order":4,"template":"","meta":{"pb_show_title":"on","pb_short_title":"","pb_subtitle":"","pb_authors":[],"pb_section_license":""},"chapter-type":[48],"contributor":[],"license":[],"class_list":["post-46","chapter","type-chapter","status-publish","hentry","chapter-type-numberless"],"part":66,"_links":{"self":[{"href":"https:\/\/pressbooks.ccconline.org\/astronomy\/wp-json\/pressbooks\/v2\/chapters\/46","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":19,"href":"https:\/\/pressbooks.ccconline.org\/astronomy\/wp-json\/pressbooks\/v2\/chapters\/46\/revisions"}],"predecessor-version":[{"id":734,"href":"https:\/\/pressbooks.ccconline.org\/astronomy\/wp-json\/pressbooks\/v2\/chapters\/46\/revisions\/734"}],"part":[{"href":"https:\/\/pressbooks.ccconline.org\/astronomy\/wp-json\/pressbooks\/v2\/parts\/66"}],"metadata":[{"href":"https:\/\/pressbooks.ccconline.org\/astronomy\/wp-json\/pressbooks\/v2\/chapters\/46\/metadata\/"}],"wp:attachment":[{"href":"https:\/\/pressbooks.ccconline.org\/astronomy\/wp-json\/wp\/v2\/media?parent=46"}],"wp:term":[{"taxonomy":"chapter-type","embeddable":true,"href":"https:\/\/pressbooks.ccconline.org\/astronomy\/wp-json\/pressbooks\/v2\/chapter-type?post=46"},{"taxonomy":"contributor","embeddable":true,"href":"https:\/\/pressbooks.ccconline.org\/astronomy\/wp-json\/wp\/v2\/contributor?post=46"},{"taxonomy":"license","embeddable":true,"href":"https:\/\/pressbooks.ccconline.org\/astronomy\/wp-json\/wp\/v2\/license?post=46"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}