{"id":405,"date":"2022-02-11T20:50:00","date_gmt":"2022-02-11T20:50:00","guid":{"rendered":"https:\/\/pressbooks.ccconline.org\/astronomy\/?post_type=part&#038;p=405"},"modified":"2022-02-11T20:51:49","modified_gmt":"2022-02-11T20:51:49","slug":"chapter-10-earthlike-planets-venus-and-mars","status":"publish","type":"part","link":"https:\/\/pressbooks.ccconline.org\/astronomy\/part\/chapter-10-earthlike-planets-venus-and-mars\/","title":{"raw":"Chapter 10  Earthlike Planets: Venus and Mars","rendered":"Chapter 10  Earthlike Planets: Venus and Mars"},"content":{"raw":"<div id=\"OSC_Astro_10_00_SpiritRov\" class=\"os-figure has-splash\">\r\n<figure class=\"splash\" data-id=\"OSC_Astro_10_00_SpiritRov\">\r\n\r\n[caption id=\"\" align=\"aligncenter\" width=\"1312\"]<img id=\"2\" src=\"https:\/\/openstax.org\/apps\/archive\/20210823.155019\/resources\/05e179071f77f2313c259811f6760f1ed4a210ef\" alt=\"Spirit Rover on Mars. Beginning in the upper right of this photograph, the tracks left by the passage of the Spirit rover are visible on the flat, rock strewn martian terrain. At the bottom, the tracks form a loop where the rover changed direction, and portions of the rover\u2019s body are seen.\" width=\"1312\" height=\"553\" data-media-type=\"image\/jpeg\" \/> <strong>Figure\u00a010.1<\/strong>\u00a0Spirit\u00a0Rover on Mars.\u00a0This May 2004 image shows the tracks made by the Mars Exploration\u00a0Spirit\u00a0rover on the surface of the red planet.\u00a0Spirit\u00a0was active on Mars between 2004 and 2010, twenty times longer than its planners had expected. It \u201cdrove\u201d over 7.73 kilometers in the process of examining the martian landscape. (credit: modification of work by NASA\/JPL\/Cornell)[\/caption]<\/figure>\r\n<div class=\"os-caption-container\"><span style=\"font-family: 'Cormorant Garamond', serif; font-size: 1.602em; word-spacing: normal;\">Chapter Outline<\/span><\/div>\r\n<\/div>\r\n<div class=\"intro-body\">\r\n<div class=\"os-chapter-outline\">\r\n<div class=\"os-chapter-objective\"><span class=\"os-number\">10.1<\/span><span class=\"os-divider\">\u00a0<\/span><span class=\"os-text\" data-type=\"\">The Nearest Planets: An Overview<\/span><\/div>\r\n<div class=\"os-chapter-objective\"><span class=\"os-number\">10.2<\/span><span class=\"os-divider\">\u00a0<\/span><span class=\"os-text\" data-type=\"\">The Geology of Venus<\/span><\/div>\r\n<div class=\"os-chapter-objective\"><span class=\"os-number\">10.3<\/span><span class=\"os-divider\">\u00a0<\/span><span class=\"os-text\" data-type=\"\">The Massive Atmosphere of Venus<\/span><\/div>\r\n<div class=\"os-chapter-objective\"><span class=\"os-number\">10.4<\/span><span class=\"os-divider\">\u00a0<\/span><span class=\"os-text\" data-type=\"\">The Geology of Mars<\/span><\/div>\r\n<div class=\"os-chapter-objective\"><span class=\"os-number\">10.5<\/span><span class=\"os-divider\">\u00a0<\/span><span class=\"os-text\" data-type=\"\">Water and Life on Mars<\/span><\/div>\r\n<div class=\"os-chapter-objective\"><span class=\"os-number\">10.6<\/span><span class=\"os-divider\">\u00a0<\/span><span class=\"os-text\" data-type=\"\">Divergent Planetary Evolution<\/span><\/div>\r\n<\/div>\r\n<div class=\"intro-text\">\r\n<p id=\"fs-id1168048514244\" class=\" \">The Moon and Mercury are geologically dead. In contrast, the larger terrestrial planets\u2014Earth, Venus, and Mars\u2014are more active and interesting worlds. We have already discussed Earth, and we now turn to Venus and Mars. These are the nearest planets and the most accessible to spacecraft. Not surprisingly, the greatest effort in planetary exploration has been devoted to these fascinating worlds. In the chapter, we discuss some of the results of more than four decades of scientific exploration of Mars and Venus. Mars is exceptionally interesting, with evidence that points to habitable conditions in the past. Even today, we are discovering things about Mars that make it the most likely place where humans might set up a habitat in the future. However, our robot explorers have clearly shown that neither Venus nor Mars has conditions similar to Earth. How did it happen that these three neighboring terrestrial planets have diverged so dramatically in their evolution?<\/p>\r\n\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\/10-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 id=\"OSC_Astro_10_00_SpiritRov\" class=\"os-figure has-splash\">\n<figure class=\"splash\" data-id=\"OSC_Astro_10_00_SpiritRov\">\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\/05e179071f77f2313c259811f6760f1ed4a210ef\" alt=\"Spirit Rover on Mars. Beginning in the upper right of this photograph, the tracks left by the passage of the Spirit rover are visible on the flat, rock strewn martian terrain. At the bottom, the tracks form a loop where the rover changed direction, and portions of the rover\u2019s body are seen.\" width=\"1312\" height=\"553\" data-media-type=\"image\/jpeg\" \/><figcaption class=\"wp-caption-text\"><strong>Figure\u00a010.1<\/strong>\u00a0Spirit\u00a0Rover on Mars.\u00a0This May 2004 image shows the tracks made by the Mars Exploration\u00a0Spirit\u00a0rover on the surface of the red planet.\u00a0Spirit\u00a0was active on Mars between 2004 and 2010, twenty times longer than its planners had expected. It \u201cdrove\u201d over 7.73 kilometers in the process of examining the martian landscape. (credit: modification of work by NASA\/JPL\/Cornell)<\/figcaption><\/figure>\n<\/figure>\n<div class=\"os-caption-container\"><span style=\"font-family: 'Cormorant Garamond', serif; font-size: 1.602em; word-spacing: normal;\">Chapter Outline<\/span><\/div>\n<\/div>\n<div class=\"intro-body\">\n<div class=\"os-chapter-outline\">\n<div class=\"os-chapter-objective\"><span class=\"os-number\">10.1<\/span><span class=\"os-divider\">\u00a0<\/span><span class=\"os-text\" data-type=\"\">The Nearest Planets: An Overview<\/span><\/div>\n<div class=\"os-chapter-objective\"><span class=\"os-number\">10.2<\/span><span class=\"os-divider\">\u00a0<\/span><span class=\"os-text\" data-type=\"\">The Geology of Venus<\/span><\/div>\n<div class=\"os-chapter-objective\"><span class=\"os-number\">10.3<\/span><span class=\"os-divider\">\u00a0<\/span><span class=\"os-text\" data-type=\"\">The Massive Atmosphere of Venus<\/span><\/div>\n<div class=\"os-chapter-objective\"><span class=\"os-number\">10.4<\/span><span class=\"os-divider\">\u00a0<\/span><span class=\"os-text\" data-type=\"\">The Geology of Mars<\/span><\/div>\n<div class=\"os-chapter-objective\"><span class=\"os-number\">10.5<\/span><span class=\"os-divider\">\u00a0<\/span><span class=\"os-text\" data-type=\"\">Water and Life on Mars<\/span><\/div>\n<div class=\"os-chapter-objective\"><span class=\"os-number\">10.6<\/span><span class=\"os-divider\">\u00a0<\/span><span class=\"os-text\" data-type=\"\">Divergent Planetary Evolution<\/span><\/div>\n<\/div>\n<div class=\"intro-text\">\n<p id=\"fs-id1168048514244\" class=\"\">The Moon and Mercury are geologically dead. In contrast, the larger terrestrial planets\u2014Earth, Venus, and Mars\u2014are more active and interesting worlds. We have already discussed Earth, and we now turn to Venus and Mars. These are the nearest planets and the most accessible to spacecraft. Not surprisingly, the greatest effort in planetary exploration has been devoted to these fascinating worlds. In the chapter, we discuss some of the results of more than four decades of scientific exploration of Mars and Venus. Mars is exceptionally interesting, with evidence that points to habitable conditions in the past. Even today, we are discovering things about Mars that make it the most likely place where humans might set up a habitat in the future. However, our robot explorers have clearly shown that neither Venus nor Mars has conditions similar to Earth. How did it happen that these three neighboring terrestrial planets have diverged so dramatically in their evolution?<\/p>\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\/10-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":10,"template":"","meta":{"pb_part_invisible":false,"pb_part_invisible_string":""},"contributor":[],"license":[],"class_list":["post-405","part","type-part","status-publish","hentry"],"_links":{"self":[{"href":"https:\/\/pressbooks.ccconline.org\/astronomy\/wp-json\/pressbooks\/v2\/parts\/405","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":3,"href":"https:\/\/pressbooks.ccconline.org\/astronomy\/wp-json\/pressbooks\/v2\/parts\/405\/revisions"}],"predecessor-version":[{"id":408,"href":"https:\/\/pressbooks.ccconline.org\/astronomy\/wp-json\/pressbooks\/v2\/parts\/405\/revisions\/408"}],"wp:attachment":[{"href":"https:\/\/pressbooks.ccconline.org\/astronomy\/wp-json\/wp\/v2\/media?parent=405"}],"wp:term":[{"taxonomy":"contributor","embeddable":true,"href":"https:\/\/pressbooks.ccconline.org\/astronomy\/wp-json\/wp\/v2\/contributor?post=405"},{"taxonomy":"license","embeddable":true,"href":"https:\/\/pressbooks.ccconline.org\/astronomy\/wp-json\/wp\/v2\/license?post=405"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}