{"id":753044,"date":"2025-01-15T18:12:10","date_gmt":"2025-01-15T12:42:10","guid":{"rendered":"https:\/\/infinitylearn.com\/surge\/?p=753044"},"modified":"2025-01-22T15:22:12","modified_gmt":"2025-01-22T09:52:12","slug":"gravitation-mcq-class-11-physics","status":"publish","type":"post","link":"https:\/\/infinitylearn.com\/surge\/mcqs\/class-11-physics-gravitation\/","title":{"rendered":"Gravitation MCQ Class 11 Physics"},"content":{"rendered":"<div id=\"ez-toc-container\" class=\"ez-toc-v2_0_37 counter-hierarchy ez-toc-counter ez-toc-grey ez-toc-container-direction\">\n<div class=\"ez-toc-title-container\">\n<p class=\"ez-toc-title\">Table of Contents<\/p>\n<span class=\"ez-toc-title-toggle\"><a href=\"#\" class=\"ez-toc-pull-right ez-toc-btn ez-toc-btn-xs ez-toc-btn-default ez-toc-toggle\" style=\"display: none;\"><label for=\"item\" aria-label=\"Table of Content\"><span style=\"display: flex;align-items: center;width: 35px;height: 30px;justify-content: center;\"><svg style=\"fill: #999;color:#999\" xmlns=\"http:\/\/www.w3.org\/2000\/svg\" class=\"list-377408\" width=\"20px\" height=\"20px\" viewBox=\"0 0 24 24\" fill=\"none\"><path d=\"M6 6H4v2h2V6zm14 0H8v2h12V6zM4 11h2v2H4v-2zm16 0H8v2h12v-2zM4 16h2v2H4v-2zm16 0H8v2h12v-2z\" fill=\"currentColor\"><\/path><\/svg><svg style=\"fill: #999;color:#999\" class=\"arrow-unsorted-368013\" xmlns=\"http:\/\/www.w3.org\/2000\/svg\" width=\"10px\" height=\"10px\" viewBox=\"0 0 24 24\" version=\"1.2\" baseProfile=\"tiny\"><path d=\"M18.2 9.3l-6.2-6.3-6.2 6.3c-.2.2-.3.4-.3.7s.1.5.3.7c.2.2.4.3.7.3h11c.3 0 .5-.1.7-.3.2-.2.3-.5.3-.7s-.1-.5-.3-.7zM5.8 14.7l6.2 6.3 6.2-6.3c.2-.2.3-.5.3-.7s-.1-.5-.3-.7c-.2-.2-.4-.3-.7-.3h-11c-.3 0-.5.1-.7.3-.2.2-.3.5-.3.7s.1.5.3.7z\"\/><\/svg><\/span><\/label><input type=\"checkbox\" id=\"item\"><\/a><\/span><\/div>\n<nav><ul class='ez-toc-list ez-toc-list-level-1' style='display:block'><li class='ez-toc-page-1 ez-toc-heading-level-2'><a class=\"ez-toc-link ez-toc-heading-1\" href=\"https:\/\/infinitylearn.com\/surge\/mcqs\/class-11-physics-gravitation\/#Class_11_Physics_Gravitation_Overview\" title=\"Class 11 Physics Gravitation Overview\">Class 11 Physics Gravitation Overview<\/a><\/li><li class='ez-toc-page-1 ez-toc-heading-level-2'><a class=\"ez-toc-link ez-toc-heading-2\" href=\"https:\/\/infinitylearn.com\/surge\/mcqs\/class-11-physics-gravitation\/#Class_11_Physics_Gravitation_MCQ_with_Answers\" title=\"Class 11 Physics Gravitation MCQ with Answers\">Class 11 Physics Gravitation MCQ with Answers<\/a><\/li><li class='ez-toc-page-1 ez-toc-heading-level-2'><a class=\"ez-toc-link ez-toc-heading-3\" href=\"https:\/\/infinitylearn.com\/surge\/mcqs\/class-11-physics-gravitation\/#FAQs_on_Gravitation_MCQ_Class_11_Physics\" title=\"FAQs on Gravitation MCQ Class 11 Physics\">FAQs on Gravitation MCQ Class 11 Physics<\/a><ul class='ez-toc-list-level-3'><li class='ez-toc-heading-level-3'><a class=\"ez-toc-link ez-toc-heading-4\" href=\"https:\/\/infinitylearn.com\/surge\/mcqs\/class-11-physics-gravitation\/#What_is_Newtons_law_of_universal_gravitation\" title=\"What is Newton&#039;s law of universal gravitation?\">What is Newton&#039;s law of universal gravitation?<\/a><\/li><li class='ez-toc-page-1 ez-toc-heading-level-3'><a class=\"ez-toc-link ez-toc-heading-5\" href=\"https:\/\/infinitylearn.com\/surge\/mcqs\/class-11-physics-gravitation\/#What_is_the_significance_of_Keplers_laws_in_gravitation\" title=\"What is the significance of Kepler\u2019s laws in gravitation?\">What is the significance of Kepler\u2019s laws in gravitation?<\/a><\/li><li class='ez-toc-page-1 ez-toc-heading-level-3'><a class=\"ez-toc-link ez-toc-heading-6\" href=\"https:\/\/infinitylearn.com\/surge\/mcqs\/class-11-physics-gravitation\/#How_does_gravity_affect_satellites_in_orbit\" title=\"How does gravity affect satellites in orbit?\">How does gravity affect satellites in orbit?<\/a><\/li><\/ul><\/li><\/ul><\/nav><\/div>\n<p>Understanding the concept of <strong>gravitation in Class 11 Physics<\/strong> is crucial for building a strong foundation in physics. Chapter 8, Gravitation, deals with key ideas such as Newton&#8217;s law of gravitation, gravitational force, and acceleration due to gravity, which are often tested through Gravitation MCQ. Whether you&#8217;re preparing for CBSE exams or competitive exams, these MCQs on gravitation lass 11 Physics help reinforce concepts such as the law of gravitation, gravitational potential energy, and real-world applications.<\/p>\n<p>Practicing <strong>mcq questions on gravitation for class 11 with solutions<\/strong> enhances your understanding of how forces act on objects, gravitational fields, and the concept of mass and weight. For quick revision, students can also refer to <strong>Gravitation mcq class 11 physics pdf<\/strong> for detailed solutions and practice.<\/p>\n<p>Common topics in these quizzes include gravitational force, universal law of gravitation, acceleration due to gravity, and related objective questions. These <strong>Class 11 Physics chapter 8 MCQs<\/strong> challenge your understanding of concepts like weightlessness, orbital motion, and escape velocity.<\/p>\n<p>Whether you are attempting a <strong>gravitation MCQ quiz<\/strong> or solving physics MCQs on gravitational concepts, these questions offer an excellent way to test your knowledge. Prepare effectively with this content and master gravitation with ease!<\/p>\n<h2><span class=\"ez-toc-section\" id=\"Class_11_Physics_Gravitation_Overview\"><\/span>Class 11 Physics Gravitation Overview<span class=\"ez-toc-section-end\"><\/span><\/h2>\n<div class=\"flex max-w-full flex-col flex-grow\">\n<div class=\"min-h-8 text-message flex w-full flex-col items-end gap-2 whitespace-normal break-words text-start [.text-message+&amp;]:mt-5\" dir=\"auto\" data-message-author-role=\"assistant\" data-message-id=\"c551796c-6b75-44b6-9b15-a65d28361e09\" data-message-model-slug=\"gpt-4o-mini\">\n<div class=\"flex w-full flex-col gap-1 empty:hidden first:pt-[3px]\">\n<div class=\"markdown prose w-full break-words dark:prose-invert light\">\n<p>Chapter 8 of Class 11 Physics, titled <em>Gravitation<\/em>, introduces students to the fundamental forces of nature, with a focus on gravity. This chapter helps learners understand the concept of gravitational force, which governs the motion of celestial bodies and objects on Earth.<\/p>\n<p>Key topics covered in Class 11 Physics Gravitation<\/p>\n<ol>\n<li><strong>Newton\u2019s Law of Gravitation<\/strong>: This law states that every mass exerts an attractive force on every other mass, proportional to the product of their masses and inversely proportional to the square of the distance between them.<\/li>\n<li><strong>Gravitational Constant (G)<\/strong>: Students will learn about the universal gravitational constant, its value, and its significance in the calculation of gravitational force.<\/li>\n<li><strong>Gravitational Field<\/strong>: The concept of gravitational field intensity and the field due to various objects like point masses, spheres, and uniform mass distributions is discussed. This section also explains how gravitational fields are related to gravitational force.<\/li>\n<li><strong>Gravitational Potential Energy<\/strong>: This refers to the energy possessed by an object due to its position in a gravitational field. The chapter explores the gravitational potential energy for an object at a height above the Earth\u2019s surface and how it changes with distance.<\/li>\n<li><strong>Escape Velocity and Orbital Motion<\/strong>: This part explains the velocity needed for an object to escape Earth&#8217;s gravitational pull (escape velocity) and the concepts of satellites, orbital velocity, and the difference between circular and elliptical orbits.<\/li>\n<li><strong>Kepler\u2019s Laws of Planetary Motion<\/strong>: These laws describe the motion of planets in elliptical orbits around the Sun and explain how the gravitational force between the Sun and planets governs their orbits.<\/li>\n<\/ol>\n<p>The chapter concludes with practical applications of gravitational principles, including the motion of planets, satellite trajectories, and the effects of gravity on Earth&#8217;s shape and tides.<\/p>\n<p>This chapter provides the foundation for understanding not only the Earth\u2019s gravitational pull but also how it influences astronomical bodies and space exploration.<\/p>\n<\/div>\n<\/div>\n<\/div>\n<\/div>\n<div id=\"cta4\" class=\"banner-card\" data-id=\"cta1\" data-redirection-url=\"https:\/\/student.infinitylearn.com\/dashboard?isFromExternalApp=true&amp;pageName=masterclasses\" data-source-campaign=\"WP Masterclass banner\">\n<h2><span class=\"ez-toc-section\" id=\"Class_11_Physics_Gravitation_MCQ_with_Answers\"><\/span>Class 11 Physics Gravitation MCQ with Answers<span class=\"ez-toc-section-end\"><\/span><\/h2>\n<p>These multiple-choice questions (MCQs) are designed based on the latest CBSE syllabus and NCERT curriculum. Solving them will help you gain a deeper understanding of the chapter and prepare for the final exam. The correct answers and explanations are provided below each question.<\/p>\n<p><strong>1. Newton\u2019s law of universal gravitation force is given by:<\/strong><\/p>\n<ol style=\"list-style-type: lower-alpha;\">\n<li>F = Gm\u2081m\u2082 \/ r\u2074<\/li>\n<li>F = Gm\u2081m\u2082 \/ r\u00b2<\/li>\n<li>F = G(m\u2081 + m\u2082) \/ r\u00b2<\/li>\n<li>F = G(m\u2081 &#8211; m\u2082) \/ r\u00b2<\/li>\n<\/ol>\n<p><strong>Answer:<\/strong> b. F = Gm\u2081m\u2082 \/ r\u00b2<\/p>\n<p><strong>Explanation:<\/strong> According to Newton\u2019s law of universal gravitation, the gravitational force (F) between two masses (m\u2081 and m\u2082) is directly proportional to the product of their masses and inversely proportional to the square of the distance (r) between them. Hence, the correct formula is <strong>F = Gm\u2081m\u2082 \/ r\u00b2<\/strong>.<\/p>\n<p><strong>2. Which law describes the orbits of planets around the sun?<\/strong><\/p>\n<ol style=\"list-style-type: lower-alpha;\">\n<li>Newton\u2019s law<\/li>\n<li>Faraday\u2019s law<\/li>\n<li>Kepler\u2019s law<\/li>\n<li>Kirchhoff\u2019s Law<\/li>\n<\/ol>\n<p><strong>Answer:<\/strong> b. Kepler\u2019s law<\/p>\n<p><strong>Explanation:<\/strong> Kepler&#8217;s laws describe the motion of planets in elliptical orbits around the Sun. These laws help us understand planetary movements and the relationship between a planet&#8217;s distance from the Sun and its orbital period.<\/p>\n<p><strong>3. The sum of kinetic and potential energy is when a missile is launched with a velocity less than the escape velocity.<\/strong><\/p>\n<ol style=\"list-style-type: lower-alpha;\">\n<li>0<\/li>\n<li>Negative<\/li>\n<li>Positive<\/li>\n<li>None of these options<\/li>\n<\/ol>\n<p><strong>Answer:<\/strong> b. Negative<\/p>\n<p><strong>Explanation:<\/strong> When a missile is launched with a velocity less than the escape velocity, its total mechanical energy (the sum of kinetic and potential energy) is negative. This means the missile does not have enough energy to escape Earth&#8217;s gravity.<\/p>\n<p><strong>4. If the distance between the Earth and the Sun doubles, what would be the duration of the year?<\/strong><\/p>\n<ol style=\"list-style-type: lower-alpha;\">\n<li>365 days<\/li>\n<li>366 days<\/li>\n<li>730 days<\/li>\n<li>1032 days<\/li>\n<\/ol>\n<p><strong>Answer:<\/strong> d. 1032 days<\/p>\n<p><strong>Explanation:<\/strong> According to Kepler&#8217;s third law, the square of the orbital period (T) is directly proportional to the cube of the semi-major axis (a). If the distance between Earth and the Sun doubles, the orbital period (T) will increase by a factor of 8, making the year approximately 1032 days long.<\/p>\n<p><strong>5. What would be the maximum height reached by the body if the body is projected vertically from the surface of the earth of radius R with a velocity equal to half of the escape velocity?<\/strong><\/p>\n<ol style=\"list-style-type: lower-alpha;\">\n<li>2 + R<\/li>\n<li>R<\/li>\n<li>R\/2<\/li>\n<li>R\/3 (Correct Answer)<\/li>\n<\/ol>\n<p><strong>Answer:<\/strong> d. R\/3<\/p>\n<p><strong>Explanation:<\/strong> If a body is projected with half the escape velocity, it will reach a height equal to one-third of Earth&#8217;s radius (R\/3). This is because the escape velocity is the minimum velocity required to overcome Earth&#8217;s gravity, and half of this velocity results in reaching a fraction of the Earth&#8217;s radius.<\/p>\n<p><strong>6. In a manned satellite, people experience no gravity, and this phenomenon is known as:<\/strong><\/p>\n<ol style=\"list-style-type: lower-alpha;\">\n<li>Gravity-weight<\/li>\n<li>Gravitational weight<\/li>\n<li>Weightlessness<\/li>\n<li>Less-weight gravity<\/li>\n<\/ol>\n<p><strong>Answer:<\/strong> c. Weightlessness<\/p>\n<p><strong>Explanation:<\/strong> Weightlessness occurs when objects are in free fall, such as in orbit. In orbit, the satellite and everything inside it are falling towards Earth at the same rate, so the occupants feel weightless.<\/p>\n<p><strong>7. Dimensional formula for gravitational intensity is:<\/strong><\/p>\n<ol style=\"list-style-type: lower-alpha;\">\n<li>[L T\u00b2]<\/li>\n<li>[L T\u207b\u00b2]<\/li>\n<li>[L T]<\/li>\n<li>[L T\u207b\u2074]<\/li>\n<\/ol>\n<p><strong>Answer:<\/strong> b. [L T\u207b\u00b2]\n<p><strong>Explanation:<\/strong> Gravitational intensity is defined as the force per unit mass. Its dimensional formula is [L T\u207b\u00b2], where L represents length and T represents time. This formula is derived from the equation for gravitational force.<\/p>\n<p><strong>8. Gravitational force on a particle inside a spherical shell is:<\/strong><\/p>\n<ol style=\"list-style-type: lower-alpha;\">\n<li>1<\/li>\n<li>-1<\/li>\n<li>0<\/li>\n<li>None of the option<\/li>\n<\/ol>\n<p><strong>Answer:<\/strong>  c. 0<\/p>\n<p><strong>Explanation:<\/strong> According to the shell theorem, the net gravitational force on a particle inside a uniform spherical shell is zero. This means that no matter where you are inside the shell, the forces from the shell cancel each other out.<\/p>\n<p><strong>9. The satellite having the same time period of revolution as that of the Earth is called:<\/strong><\/p>\n<ol style=\"list-style-type: lower-alpha;\">\n<li>Stationary satellite<\/li>\n<li>Geostationary satellite<\/li>\n<li>Gravitational satellite<\/li>\n<li>Geo satellite<\/li>\n<\/ol>\n<p><strong>Answer:<\/strong>  b. Geostationary satellite<\/p>\n<p><strong>Explanation:<\/strong> A geostationary satellite has the same orbital period as Earth (24 hours) and orbits above the equator. It remains stationary relative to a specific point on Earth&#8217;s surface, making it ideal for communication and weather monitoring.<\/p>\n<p><strong>10. State true or false: The gravitational force is a conservative force.<\/strong><\/p>\n<ol style=\"list-style-type: lower-alpha;\">\n<li>True<\/li>\n<li>False<\/li>\n<\/ol>\n<p><strong>Answer:<\/strong>  a. True<\/p>\n<p><strong>Explanation:<\/strong> The gravitational force is a conservative force, meaning that the work done by gravity on an object depends only on the initial and final positions of the object, not on the path taken.<\/p>\n<h2><span class=\"ez-toc-section\" id=\"FAQs_on_Gravitation_MCQ_Class_11_Physics\"><\/span>FAQs on Gravitation MCQ Class 11 Physics<span class=\"ez-toc-section-end\"><\/span><\/h2>\n\t\t<section class=\"sc_fs_faq sc_card \">\n\t\t\t<div>\n\t\t\t\t<h3><span class=\"ez-toc-section\" id=\"What_is_Newtons_law_of_universal_gravitation\"><\/span>What is Newton&#039;s law of universal gravitation?<span class=\"ez-toc-section-end\"><\/span><\/h3>\t\t\t\t<div>\n\t\t\t\t\t\t\t\t\t\t<p>\n\t\t\t\t\t\tNewton's law of universal gravitation states that every mass exerts an attractive force on every other mass, which is directly proportional to the product of their masses and inversely proportional to the square of the distance between their centers. The formula is F = Gm\u2081m\u2082 \/ r\u00b2, where G is the gravitational constant, m\u2081 and m\u2082 are the masses of the objects, and r is the distance between them.\t\t\t\t\t<\/p>\n\t\t\t\t<\/div>\n\t\t\t<\/div>\n\t\t<\/section>\n\t\t\t\t<section class=\"sc_fs_faq sc_card \">\n\t\t\t<div>\n\t\t\t\t<h3><span class=\"ez-toc-section\" id=\"What_is_the_significance_of_Keplers_laws_in_gravitation\"><\/span>What is the significance of Kepler\u2019s laws in gravitation?<span class=\"ez-toc-section-end\"><\/span><\/h3>\t\t\t\t<div>\n\t\t\t\t\t\t\t\t\t\t<p>\n\t\t\t\t\t\tKepler's laws describe the motion of planets around the Sun. They are important for understanding how planets move in elliptical orbits, how the orbital period is related to the distance from the Sun, and how the speed of a planet changes along its orbit. Kepler's laws form the foundation for understanding orbital mechanics and the behavior of celestial bodies in space.\t\t\t\t\t<\/p>\n\t\t\t\t<\/div>\n\t\t\t<\/div>\n\t\t<\/section>\n\t\t\t\t<section class=\"sc_fs_faq sc_card \">\n\t\t\t<div>\n\t\t\t\t<h3><span class=\"ez-toc-section\" id=\"How_does_gravity_affect_satellites_in_orbit\"><\/span>How does gravity affect satellites in orbit?<span class=\"ez-toc-section-end\"><\/span><\/h3>\t\t\t\t<div>\n\t\t\t\t\t\t\t\t\t\t<p>\n\t\t\t\t\t\tGravity keeps satellites in orbit by continuously pulling them toward the Earth, preventing them from flying off into space. For a satellite to stay in a stable orbit, it needs to travel at a specific speed. This balance between the satellite\u2019s forward motion and the gravitational pull of the Earth creates a circular or elliptical orbit.\t\t\t\t\t<\/p>\n\t\t\t\t<\/div>\n\t\t\t<\/div>\n\t\t<\/section>\n\t\t\n<script type=\"application\/ld+json\">\n\t{\n\t\t\"@context\": \"https:\/\/schema.org\",\n\t\t\"@type\": \"FAQPage\",\n\t\t\"mainEntity\": [\n\t\t\t\t\t{\n\t\t\t\t\"@type\": \"Question\",\n\t\t\t\t\"name\": \"What is Newton's law of universal gravitation?\",\n\t\t\t\t\"acceptedAnswer\": {\n\t\t\t\t\t\"@type\": \"Answer\",\n\t\t\t\t\t\"text\": \"Newton's law of universal gravitation states that every mass exerts an attractive force on every other mass, which is directly proportional to the product of their masses and inversely proportional to the square of the distance between their centers. The formula is F = Gm\u2081m\u2082 \/ r\u00b2, where G is the gravitational constant, m\u2081 and m\u2082 are the masses of the objects, and r is the distance between them.\"\n\t\t\t\t\t\t\t\t\t}\n\t\t\t}\n\t\t\t,\t\t\t\t{\n\t\t\t\t\"@type\": \"Question\",\n\t\t\t\t\"name\": \"What is the significance of Kepler\u2019s laws in gravitation?\",\n\t\t\t\t\"acceptedAnswer\": {\n\t\t\t\t\t\"@type\": \"Answer\",\n\t\t\t\t\t\"text\": \"Kepler's laws describe the motion of planets around the Sun. They are important for understanding how planets move in elliptical orbits, how the orbital period is related to the distance from the Sun, and how the speed of a planet changes along its orbit. Kepler's laws form the foundation for understanding orbital mechanics and the behavior of celestial bodies in space.\"\n\t\t\t\t\t\t\t\t\t}\n\t\t\t}\n\t\t\t,\t\t\t\t{\n\t\t\t\t\"@type\": \"Question\",\n\t\t\t\t\"name\": \"How does gravity affect satellites in orbit?\",\n\t\t\t\t\"acceptedAnswer\": {\n\t\t\t\t\t\"@type\": \"Answer\",\n\t\t\t\t\t\"text\": \"Gravity keeps satellites in orbit by continuously pulling them toward the Earth, preventing them from flying off into space. For a satellite to stay in a stable orbit, it needs to travel at a specific speed. This balance between the satellite\u2019s forward motion and the gravitational pull of the Earth creates a circular or elliptical orbit.\"\n\t\t\t\t\t\t\t\t\t}\n\t\t\t}\n\t\t\t\t\t\t]\n\t}\n<\/script>\n\n<\/div>\n","protected":false},"excerpt":{"rendered":"<p>Understanding the concept of gravitation in Class 11 Physics is crucial for building a strong foundation in physics. Chapter 8, [&hellip;]<\/p>\n","protected":false},"author":53,"featured_media":0,"comment_status":"closed","ping_status":"open","sticky":false,"template":"","format":"standard","meta":{"_yoast_wpseo_focuskw":"Gravitation MCQ","_yoast_wpseo_title":"Gravitation MCQ Question with Answers Class 11 Physics","_yoast_wpseo_metadesc":"Master the fundamentals of gravitation with our MCQs for Class 11 Physics. Enhance your understanding and prepare effectively for exams","custom_permalink":"mcqs\/class-11-physics-gravitation\/"},"categories":[11038],"tags":[],"table_tags":[],"acf":[],"yoast_head":"<!-- This site is optimized with the Yoast SEO plugin v17.9 - https:\/\/yoast.com\/wordpress\/plugins\/seo\/ -->\n<title>Gravitation MCQ Question with Answers Class 11 Physics<\/title>\n<meta name=\"description\" content=\"Master the fundamentals of gravitation with our MCQs for Class 11 Physics. 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