{"id":266,"date":"2021-02-03T23:36:36","date_gmt":"2021-02-03T23:36:36","guid":{"rendered":"https:\/\/courses.lumenlearning.com\/calculus1\/?post_type=chapter&#038;p=266"},"modified":"2026-02-06T21:10:42","modified_gmt":"2026-02-06T21:10:42","slug":"putting-it-together-limits","status":"publish","type":"chapter","link":"https:\/\/courses.lumenlearning.com\/calculus1\/chapter\/putting-it-together-limits\/","title":{"raw":"Putting It Together: Limits","rendered":"Putting It Together: Limits"},"content":{"raw":"<div id=\"fs-id1170572624549\" data-type=\"problem\">\r\n<div class=\"os-problem-container \">\r\n<h3>Einstein's Equation<\/h3>\r\n<p id=\"fs-id1170572624574\">At the beginning of the module, we mentioned briefly how Albert Einstein showed that a limit exists to how fast any object can travel. Given Einstein\u2019s equation for the mass of a moving object, what is the value of this bound?<\/p>\r\n\r\n<\/div>\r\n<\/div>\r\nOur starting point is Einstein\u2019s equation for the mass of a moving object,\r\n<p style=\"text-align: center;\">[latex]m=\\dfrac{m_0}{\\sqrt{1-\\frac{v^2}{c^2}}}[\/latex]<\/p>\r\nwhere [latex]m_0[\/latex]\u00a0is the object\u2019s mass at rest, [latex]v[\/latex]\u00a0is its speed, and\u00a0[latex]c[\/latex]\u00a0is the speed of light. To see how the mass changes at high speeds, we can graph the ratio of masses [latex]\\frac{m}{m_0}[\/latex]\u00a0as a function of the ratio of speeds,\u00a0[latex]\\frac{v}{c}[\/latex].\r\n\r\n[caption id=\"attachment_5013\" align=\"aligncenter\" width=\"325\"]<img class=\"wp-image-5013 size-full\" src=\"https:\/\/courses.lumenlearning.com\/calculus1\/wp-content\/uploads\/sites\/5584\/2021\/02\/figure2-23.webp\" alt=\"A graph showing the ratio of masses as a function of the ratio of speed in Einstein\u2019s equation for the mass of a moving object. The x axis is the ratio of the speeds, v\/c. The y axis is the ratio of the masses, m\/m0. The equation of the function is m = m0 \/ sqrt(1 \u2013 v2 \/ c2 ). The graph is only in quadrant 1. It starts at (0,1) and curves up gently until about 0.8, where it increases seemingly exponentially; there is a vertical asymptote at v\/c (or x) = 1.\" width=\"325\" height=\"263\" \/> Figure 2.23 This graph shows the ratio of masses as a function of the ratio of speeds in Einstein\u2019s equation for the mass of a moving object.[\/caption]\r\n\r\nWe can see that as the ratio of speeds approaches 1\u2014that is, as the speed of the object approaches the speed of light\u2014the ratio of masses increases without bound. In other words, the function has a vertical asymptote at [latex]\\frac{v}{c}=1[\/latex]. We can try a few values of this ratio to test this idea.\r\n<table style=\"border-collapse: collapse; width: 99.9999%; height: 48px;\" border=\"1\">\r\n<tbody>\r\n<tr style=\"height: 12px;\">\r\n<td style=\"width: 33.3333%; height: 12px;\">[latex]\\dfrac{v}{c}[\/latex]<\/td>\r\n<td style=\"width: 33.3333%; height: 12px;\">[latex]\\sqrt{1-\\frac{v^2}{c^2}}[\/latex]<\/td>\r\n<td style=\"width: 33.3333%; height: 12px;\">[latex]\\dfrac{m}{m_0}[\/latex]<\/td>\r\n<\/tr>\r\n<tr style=\"height: 12px;\" valign=\"top\">\r\n<td style=\"width: 33.3333%; height: 12px;\" data-align=\"left\">[latex]0.99[\/latex]<\/td>\r\n<td style=\"width: 33.3333%; height: 12px;\" data-align=\"left\">[latex]0.1411[\/latex]<\/td>\r\n<td style=\"width: 33.3333%; height: 12px;\" data-align=\"left\">[latex]7.089[\/latex]<\/td>\r\n<\/tr>\r\n<tr style=\"height: 12px;\" valign=\"top\">\r\n<td style=\"width: 33.3333%; height: 12px;\" data-align=\"left\">[latex]0.999[\/latex]<\/td>\r\n<td style=\"width: 33.3333%; height: 12px;\" data-align=\"left\">[latex]0.0447[\/latex]<\/td>\r\n<td style=\"width: 33.3333%; height: 12px;\" data-align=\"left\">[latex]22.37[\/latex]<\/td>\r\n<\/tr>\r\n<tr style=\"height: 12px;\" valign=\"top\">\r\n<td style=\"width: 33.3333%; height: 12px;\" data-align=\"left\">[latex]0.9999[\/latex]<\/td>\r\n<td style=\"width: 33.3333%; height: 12px;\" data-align=\"left\">[latex]0.0141[\/latex]<\/td>\r\n<td style=\"width: 33.3333%; height: 12px;\" data-align=\"left\">[latex]70.71[\/latex]<\/td>\r\n<\/tr>\r\n<\/tbody>\r\n<\/table>\r\nSo what does this mean?\r\n\r\nAccording to Table 1, if an object with mass [latex]100[\/latex] kg is traveling at [latex]0.9999c[\/latex], its mass becomes [latex]7071[\/latex] kg. Since no object can have an infinite mass, we conclude that no object can travel at or more than the speed of light.","rendered":"<div id=\"fs-id1170572624549\" data-type=\"problem\">\n<div class=\"os-problem-container\">\n<h3>Einstein&#8217;s Equation<\/h3>\n<p id=\"fs-id1170572624574\">At the beginning of the module, we mentioned briefly how Albert Einstein showed that a limit exists to how fast any object can travel. Given Einstein\u2019s equation for the mass of a moving object, what is the value of this bound?<\/p>\n<\/div>\n<\/div>\n<p>Our starting point is Einstein\u2019s equation for the mass of a moving object,<\/p>\n<p style=\"text-align: center;\">[latex]m=\\dfrac{m_0}{\\sqrt{1-\\frac{v^2}{c^2}}}[\/latex]<\/p>\n<p>where [latex]m_0[\/latex]\u00a0is the object\u2019s mass at rest, [latex]v[\/latex]\u00a0is its speed, and\u00a0[latex]c[\/latex]\u00a0is the speed of light. To see how the mass changes at high speeds, we can graph the ratio of masses [latex]\\frac{m}{m_0}[\/latex]\u00a0as a function of the ratio of speeds,\u00a0[latex]\\frac{v}{c}[\/latex].<\/p>\n<div id=\"attachment_5013\" style=\"width: 335px\" class=\"wp-caption aligncenter\"><img loading=\"lazy\" decoding=\"async\" aria-describedby=\"caption-attachment-5013\" class=\"wp-image-5013 size-full\" src=\"https:\/\/courses.lumenlearning.com\/calculus1\/wp-content\/uploads\/sites\/5584\/2021\/02\/figure2-23.webp\" alt=\"A graph showing the ratio of masses as a function of the ratio of speed in Einstein\u2019s equation for the mass of a moving object. The x axis is the ratio of the speeds, v\/c. The y axis is the ratio of the masses, m\/m0. The equation of the function is m = m0 \/ sqrt(1 \u2013 v2 \/ c2 ). The graph is only in quadrant 1. It starts at (0,1) and curves up gently until about 0.8, where it increases seemingly exponentially; there is a vertical asymptote at v\/c (or x) = 1.\" width=\"325\" height=\"263\" srcset=\"https:\/\/courses.lumenlearning.com\/calculus1\/wp-content\/uploads\/sites\/5584\/2021\/02\/figure2-23.webp 325w, https:\/\/courses.lumenlearning.com\/calculus1\/wp-content\/uploads\/sites\/5584\/2021\/02\/figure2-23-300x243.webp 300w, https:\/\/courses.lumenlearning.com\/calculus1\/wp-content\/uploads\/sites\/5584\/2021\/02\/figure2-23-65x53.webp 65w, https:\/\/courses.lumenlearning.com\/calculus1\/wp-content\/uploads\/sites\/5584\/2021\/02\/figure2-23-225x182.webp 225w\" sizes=\"auto, (max-width: 325px) 100vw, 325px\" \/><\/p>\n<p id=\"caption-attachment-5013\" class=\"wp-caption-text\">Figure 2.23 This graph shows the ratio of masses as a function of the ratio of speeds in Einstein\u2019s equation for the mass of a moving object.<\/p>\n<\/div>\n<p>We can see that as the ratio of speeds approaches 1\u2014that is, as the speed of the object approaches the speed of light\u2014the ratio of masses increases without bound. In other words, the function has a vertical asymptote at [latex]\\frac{v}{c}=1[\/latex]. We can try a few values of this ratio to test this idea.<\/p>\n<table style=\"border-collapse: collapse; width: 99.9999%; height: 48px;\">\n<tbody>\n<tr style=\"height: 12px;\">\n<td style=\"width: 33.3333%; height: 12px;\">[latex]\\dfrac{v}{c}[\/latex]<\/td>\n<td style=\"width: 33.3333%; height: 12px;\">[latex]\\sqrt{1-\\frac{v^2}{c^2}}[\/latex]<\/td>\n<td style=\"width: 33.3333%; height: 12px;\">[latex]\\dfrac{m}{m_0}[\/latex]<\/td>\n<\/tr>\n<tr style=\"height: 12px;\" valign=\"top\">\n<td style=\"width: 33.3333%; height: 12px;\" data-align=\"left\">[latex]0.99[\/latex]<\/td>\n<td style=\"width: 33.3333%; height: 12px;\" data-align=\"left\">[latex]0.1411[\/latex]<\/td>\n<td style=\"width: 33.3333%; height: 12px;\" data-align=\"left\">[latex]7.089[\/latex]<\/td>\n<\/tr>\n<tr style=\"height: 12px;\" valign=\"top\">\n<td style=\"width: 33.3333%; height: 12px;\" data-align=\"left\">[latex]0.999[\/latex]<\/td>\n<td style=\"width: 33.3333%; height: 12px;\" data-align=\"left\">[latex]0.0447[\/latex]<\/td>\n<td style=\"width: 33.3333%; height: 12px;\" data-align=\"left\">[latex]22.37[\/latex]<\/td>\n<\/tr>\n<tr style=\"height: 12px;\" valign=\"top\">\n<td style=\"width: 33.3333%; height: 12px;\" data-align=\"left\">[latex]0.9999[\/latex]<\/td>\n<td style=\"width: 33.3333%; height: 12px;\" data-align=\"left\">[latex]0.0141[\/latex]<\/td>\n<td style=\"width: 33.3333%; height: 12px;\" data-align=\"left\">[latex]70.71[\/latex]<\/td>\n<\/tr>\n<\/tbody>\n<\/table>\n<p>So what does this mean?<\/p>\n<p>According to Table 1, if an object with mass [latex]100[\/latex] kg is traveling at [latex]0.9999c[\/latex], its mass becomes [latex]7071[\/latex] kg. Since no object can have an infinite mass, we conclude that no object can travel at or more than the speed of light.<\/p>\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-266\">\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>Calculus Volume 1. <strong>Authored by<\/strong>: Gilbert Strang, Edwin (Jed) Herman. <strong>Provided by<\/strong>: OpenStax. <strong>Located at<\/strong>: <a target=\"_blank\" href=\"https:\/\/openstax.org\/details\/books\/calculus-volume-1\">https:\/\/openstax.org\/details\/books\/calculus-volume-1<\/a>. <strong>License<\/strong>: <em><a target=\"_blank\" rel=\"license\" href=\"https:\/\/creativecommons.org\/licenses\/by-nc-sa\/4.0\/\">CC BY-NC-SA: Attribution-NonCommercial-ShareAlike<\/a><\/em>. <strong>License Terms<\/strong>: Access for free at https:\/\/openstax.org\/books\/calculus-volume-1\/pages\/1-introduction<\/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":17533,"menu_order":24,"template":"","meta":{"_candela_citation":"[{\"type\":\"cc\",\"description\":\"Calculus Volume 1\",\"author\":\"Gilbert Strang, Edwin (Jed) Herman\",\"organization\":\"OpenStax\",\"url\":\"https:\/\/openstax.org\/details\/books\/calculus-volume-1\",\"project\":\"\",\"license\":\"cc-by-nc-sa\",\"license_terms\":\"Access for free at https:\/\/openstax.org\/books\/calculus-volume-1\/pages\/1-introduction\"}]","CANDELA_OUTCOMES_GUID":"","pb_show_title":"on","pb_short_title":"","pb_subtitle":"","pb_authors":[],"pb_section_license":""},"chapter-type":[],"contributor":[],"license":[],"class_list":["post-266","chapter","type-chapter","status-publish","hentry"],"part":28,"_links":{"self":[{"href":"https:\/\/courses.lumenlearning.com\/calculus1\/wp-json\/pressbooks\/v2\/chapters\/266","targetHints":{"allow":["GET"]}}],"collection":[{"href":"https:\/\/courses.lumenlearning.com\/calculus1\/wp-json\/pressbooks\/v2\/chapters"}],"about":[{"href":"https:\/\/courses.lumenlearning.com\/calculus1\/wp-json\/wp\/v2\/types\/chapter"}],"author":[{"embeddable":true,"href":"https:\/\/courses.lumenlearning.com\/calculus1\/wp-json\/wp\/v2\/users\/17533"}],"version-history":[{"count":11,"href":"https:\/\/courses.lumenlearning.com\/calculus1\/wp-json\/pressbooks\/v2\/chapters\/266\/revisions"}],"predecessor-version":[{"id":5014,"href":"https:\/\/courses.lumenlearning.com\/calculus1\/wp-json\/pressbooks\/v2\/chapters\/266\/revisions\/5014"}],"part":[{"href":"https:\/\/courses.lumenlearning.com\/calculus1\/wp-json\/pressbooks\/v2\/parts\/28"}],"metadata":[{"href":"https:\/\/courses.lumenlearning.com\/calculus1\/wp-json\/pressbooks\/v2\/chapters\/266\/metadata\/"}],"wp:attachment":[{"href":"https:\/\/courses.lumenlearning.com\/calculus1\/wp-json\/wp\/v2\/media?parent=266"}],"wp:term":[{"taxonomy":"chapter-type","embeddable":true,"href":"https:\/\/courses.lumenlearning.com\/calculus1\/wp-json\/pressbooks\/v2\/chapter-type?post=266"},{"taxonomy":"contributor","embeddable":true,"href":"https:\/\/courses.lumenlearning.com\/calculus1\/wp-json\/wp\/v2\/contributor?post=266"},{"taxonomy":"license","embeddable":true,"href":"https:\/\/courses.lumenlearning.com\/calculus1\/wp-json\/wp\/v2\/license?post=266"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}