{"id":12454,"date":"2025-09-16T06:31:21","date_gmt":"2025-09-16T05:31:21","guid":{"rendered":"https:\/\/mcqsadda.com\/?p=12454"},"modified":"2025-10-22T09:37:05","modified_gmt":"2025-10-22T08:37:05","slug":"gravitation-top-100-mcqs-with-answer-and-explanation","status":"publish","type":"post","link":"https:\/\/mcqsadda.com\/index.php\/2025\/09\/16\/gravitation-top-100-mcqs-with-answer-and-explanation\/","title":{"rendered":"Gravitation Top 100 MCQs With Answer and Explanation"},"content":{"rendered":"\n<p class=\"has-large-font-size\"><mark style=\"background-color:rgba(0, 0, 0, 0)\" class=\"has-inline-color has-luminous-vivid-orange-color\"><strong>1.<\/strong><\/mark><strong><mark style=\"background-color:rgba(0, 0, 0, 0)\" class=\"has-inline-color has-luminous-vivid-orange-color\">Who proposed the universal law of gravitation?<\/mark><\/strong><br>a) Albert Einstein<br>b) Isaac Newton<br>c) Galileo Galilei<br>d) Johannes Kepler<br><strong>Answer:<\/strong> b) Isaac Newton<br><strong>Explanation:<\/strong> Newton formulated the law of universal gravitation in 1687.<\/p>\n\n\n\n<p class=\"has-large-font-size\"><mark style=\"background-color:rgba(0, 0, 0, 0)\" class=\"has-inline-color has-luminous-vivid-orange-color\"><strong>2. The universal law of gravitation states that the force between two masses is:<\/strong><\/mark><br>a) Directly proportional to the sum of their masses<br>b) Directly proportional to the product of their masses and inversely proportional to the square of the distance between them<br>c) Inversely proportional to the distance between them<br>d) Independent of the distance<br><strong>Answer:<\/strong> b) Directly proportional to the product of their masses and inversely proportional to the square of the distance between them<br><strong>Explanation:<\/strong> This is the fundamental statement of Newton&#8217;s law of gravitation.<\/p>\n\n\n\n<p class=\"has-large-font-size\"><strong><mark style=\"background-color:rgba(0, 0, 0, 0)\" class=\"has-inline-color has-luminous-vivid-orange-color\">3. The universal gravitational constant (G) has the value:<\/mark><\/strong><br>a) 9.8 m\/s\u00b2<br>b) 6.67 \u00d7 10\u207b\u00b9\u00b9 N\u00b7m\u00b2\/kg\u00b2<br>c) 3.14<br>d) 1.6 \u00d7 10\u207b\u00b9\u2079 C<br><strong>Answer:<\/strong> b) 6.67 \u00d7 10\u207b\u00b9\u00b9 N\u00b7m\u00b2\/kg\u00b2<br><strong>Explanation:<\/strong> G is a universal constant that quantifies gravitational attraction.<\/p>\n\n\n\n<p class=\"has-large-font-size\"><strong><mark style=\"background-color:rgba(0, 0, 0, 0)\" class=\"has-inline-color has-luminous-vivid-orange-color\">4. If the distance between two masses is doubled, the gravitational force between them becomes:<\/mark><\/strong><br>a) Four times greater<br>b) Twice as great<br>c) One-fourth as much<br>d) One-half as much<br><strong>Answer:<\/strong> c) One-fourth as much<br><strong>Explanation:<\/strong> Force varies inversely as the square of the distance.<\/p>\n\n\n\n<p class=\"has-large-font-size\"><mark style=\"background-color:rgba(0, 0, 0, 0)\" class=\"has-inline-color has-luminous-vivid-orange-color\"><strong>5. Gravitational force is a:<\/strong><\/mark><br>a) Vector quantity<br>b) Scalar quantity<br>c) Both scalar and vector<br>d) None of these<br><strong>Answer:<\/strong> a) Vector quantity<br><strong>Explanation:<\/strong> Force has magnitude and direction, so it&#8217;s a vector.<\/p>\n\n\n\n<p class=\"has-large-font-size\"><strong><mark style=\"background-color:rgba(0, 0, 0, 0)\" class=\"has-inline-color has-luminous-vivid-orange-color\">6. Weight of an object on the Moon is:<\/mark><\/strong><br>a) Same as on Earth<br>b) Less than on Earth<br>c) More than on Earth<br>d) Zero<br><strong>Answer:<\/strong> b) Less than on Earth<br><strong>Explanation:<\/strong> The Moon\u2019s gravity is about 1\/6th that of Earth.<\/p>\n\n\n\n<p class=\"has-large-font-size\"><strong><mark style=\"background-color:rgba(0, 0, 0, 0)\" class=\"has-inline-color has-luminous-vivid-orange-color\">7. Acceleration due to gravity on the Earth\u2019s surface is approximately:<\/mark><\/strong><br>a) 9.8 m\/s\u00b2<br>b) 8.9 m\/s\u00b2<br>c) 10.5 m\/s\u00b2<br>d) 7.2 m\/s\u00b2<br><strong>Answer:<\/strong> a) 9.8 m\/s\u00b2<br><strong>Explanation:<\/strong> This is the standard gravitational acceleration.<\/p>\n\n\n\n<p class=\"has-large-font-size\"><strong><mark style=\"background-color:rgba(0, 0, 0, 0)\" class=\"has-inline-color has-luminous-vivid-orange-color\">8. The force of gravity acts:<\/mark><\/strong><br>a) Only on Earth<br>b) Between any two masses anywhere in the universe<br>c) Only between planets<br>d) Only in the absence of air resistance<br><strong>Answer:<\/strong> b) Between any two masses anywhere in the universe<br><strong>Explanation:<\/strong> Gravity is a universal force acting between any two masses.<\/p>\n\n\n\n<p class=\"has-large-font-size\"><mark style=\"background-color:rgba(0, 0, 0, 0)\" class=\"has-inline-color has-luminous-vivid-orange-color\"><strong>9.<\/strong> <strong>Gravitational potential at a point is:<\/strong><\/mark><br>a) Always positive<br>b) Always negative<br>c) Zero<br>d) Either positive or negative<br><strong>Answer:<\/strong> b) Always negative<br><strong>Explanation:<\/strong> Gravitational potential energy is taken as zero at infinite distance; closer points have negative potential.<\/p>\n\n\n\n<p class=\"has-large-font-size\"><strong><mark style=\"background-color:rgba(0, 0, 0, 0)\" class=\"has-inline-color has-luminous-vivid-orange-color\">10. Escape velocity from Earth is approximately:<\/mark><\/strong><br>a) 11.2 km\/s<br>b) 9.8 km\/s<br>c) 7.9 km\/s<br>d) 5.4 km\/s<br><strong>Answer:<\/strong> a) 11.2 km\/s<br><strong>Explanation:<\/strong> This is the minimum speed needed to escape Earth&#8217;s gravitational field.<\/p>\n\n\n\n<p class=\"has-large-font-size\"><mark style=\"background-color:rgba(0, 0, 0, 0)\" class=\"has-inline-color has-luminous-vivid-orange-color\"><strong>11. If the mass of Earth doubled and radius remained the same, acceleration due to gravity would:<\/strong><\/mark><br>a) Remain same<br>b) Double<br>c) Halve<br>d) Quadruple<br><strong>Answer:<\/strong> b) Double<br><strong>Explanation:<\/strong> <img decoding=\"async\" width=\"41\" height=\"27\" src=\"blob:https:\/\/mcqsadda.com\/d3e5fce8-631a-487d-b394-6c7e318d9f0a\">, doubling mass doubles g.<\/p>\n\n\n\n<p class=\"has-large-font-size\"><strong><mark style=\"background-color:rgba(0, 0, 0, 0)\" class=\"has-inline-color has-luminous-vivid-orange-color\">12. Gravitational force is always:<\/mark><\/strong><br>a) Attractive<br>b) Repulsive<br>c) Attractive or repulsive depending on masses<br>d) Zero<br><strong>Answer:<\/strong> a) Attractive<br><strong>Explanation:<\/strong> Gravity always attracts masses.<\/p>\n\n\n\n<p class=\"has-large-font-size\"><strong><mark style=\"background-color:rgba(0, 0, 0, 0)\" class=\"has-inline-color has-luminous-vivid-orange-color\">13 .The shape of the Earth due to its rotation is:<\/mark><\/strong><br>a) Perfect sphere<br>b) Oblate spheroid<br>c) Prolate spheroid<br>d) Cubic<br><strong>Answer:<\/strong> b) Oblate spheroid<br><strong>Explanation:<\/strong> Rotation causes Earth to bulge at the equator.<\/p>\n\n\n\n<p class=\"has-large-font-size\"><strong><mark style=\"background-color:rgba(0, 0, 0, 0)\" class=\"has-inline-color has-luminous-vivid-orange-color\">14 . The gravitational field inside a hollow spherical shell is:<\/mark><\/strong><br>a) Same as outside<br>b) Zero<br>c) Varies linearly with distance from center<br>d) Infinite<br><strong>Answer:<\/strong> b) Zero<br><strong>Explanation:<\/strong> Gravity cancels inside a hollow shell.<\/p>\n\n\n\n<p class=\"has-large-font-size\"><mark style=\"background-color:rgba(0, 0, 0, 0)\" class=\"has-inline-color has-luminous-vivid-orange-color\"><strong>15. Kepler\u2019s first law states that the orbit of a planet is:<\/strong><\/mark><br>a) Circular<br>b) Elliptical with the Sun at one focus<br>c) Parabolic<br>d) Hyperbolic<br><strong>Answer:<\/strong> b) Elliptical with the Sun at one focus<br><strong>Explanation:<\/strong> Planets move in elliptical orbits around the Sun.<\/p>\n\n\n\n<p class=\"has-large-font-size\"><strong><mark style=\"background-color:rgba(0, 0, 0, 0)\" class=\"has-inline-color has-luminous-vivid-orange-color\">16. The time taken by a planet to complete one orbit around the Sun is called:<\/mark><\/strong><br>a) Period<br>b) Frequency<br>c) Wavelength<br>d) Amplitude<br><strong>Answer:<\/strong> a) Period<br><strong>Explanation:<\/strong> Orbital period is the time to complete one revolution.<\/p>\n\n\n\n<p class=\"has-large-font-size\"><strong><mark style=\"background-color:rgba(0, 0, 0, 0)\" class=\"has-inline-color has-luminous-vivid-orange-color\">17. The acceleration due to gravity decreases with altitude because:<\/mark><\/strong><br>a) Mass of Earth decreases<br>b) Distance from Earth\u2019s center increases<br>c) Earth\u2019s radius increases<br>d) None of these<br><strong>Answer:<\/strong> b) Distance from Earth\u2019s center increases<br><strong>Explanation:<\/strong> Gravity decreases with the square of the distance from the center.<\/p>\n\n\n\n<p class=\"has-large-font-size\"><mark style=\"background-color:rgba(0, 0, 0, 0)\" class=\"has-inline-color has-luminous-vivid-orange-color\"><strong>18. A satellite in a circular orbit experiences:<\/strong><\/mark><br>a) No force<br>b) Centripetal force provided by gravity<br>c) Centrifugal force only<br>d) Frictional force only<br><strong>Answer:<\/strong> b) Centripetal force provided by gravity<br><strong>Explanation:<\/strong> Gravity provides the centripetal force to keep the satellite in orbit.<\/p>\n\n\n\n<p class=\"has-large-font-size\"><mark style=\"background-color:rgba(0, 0, 0, 0)\" class=\"has-inline-color has-luminous-vivid-orange-color\"><strong>19. Gravitational potential energy of an object at height h above Earth\u2019s surface is:<\/strong><\/mark><br>a) <img decoding=\"async\" width=\"30\" height=\"20\" src=\"blob:https:\/\/mcqsadda.com\/60751a6b-70ea-4abd-9dfe-b0e3433bab92\"><br>b) <img decoding=\"async\" width=\"40\" height=\"28\" src=\"blob:https:\/\/mcqsadda.com\/d1e21b0c-45a3-4bab-a1d5-304e7f9ae271\"><br>c) Zero<br>d) <img decoding=\"async\" width=\"31\" height=\"20\" src=\"blob:https:\/\/mcqsadda.com\/f64ae2a8-9bd7-4ad1-adc3-59b42d3846b4\"><br><strong>Answer:<\/strong> b) <img decoding=\"async\" width=\"40\" height=\"28\" src=\"blob:https:\/\/mcqsadda.com\/cdb579e1-a96a-4ce2-8ea1-6c9aa148e00a\"><br><strong>Explanation:<\/strong> Potential energy is negative and depends on the distance from Earth&#8217;s center.<\/p>\n\n\n\n<p class=\"has-large-font-size\"><strong><mark style=\"background-color:rgba(0, 0, 0, 0)\" class=\"has-inline-color has-luminous-vivid-orange-color\">20. The value of acceleration due to gravity at the center of the Earth is:<\/mark><\/strong><br>a) Zero<br>b) Maximum<br>c) Same as surface<br>d) Infinite<br><strong>Answer:<\/strong> a) Zero<br><strong>Explanation:<\/strong> Gravity inside the Earth decreases linearly to zero at the center.<\/p>\n\n\n\n<p class=\"has-large-font-size\"><strong><mark style=\"background-color:rgba(0, 0, 0, 0)\" class=\"has-inline-color has-luminous-vivid-orange-color\">21. The value of gravitational potential at infinite distance from Earth is:<\/mark><\/strong><br>a) Zero<br>b) Negative<br>c) Positive<br>d) Infinite<br><strong>Answer:<\/strong> a) Zero<br><strong>Explanation:<\/strong> Gravitational potential is defined as zero at infinite distance.<\/p>\n\n\n\n<p class=\"has-large-font-size\"><strong><mark style=\"background-color:rgba(0, 0, 0, 0)\" class=\"has-inline-color has-luminous-vivid-orange-color\">22. If the radius of Earth becomes double but its mass remains the same, acceleration due to gravity:<\/mark><\/strong><br>a) Remains the same<br>b) Halves<br>c) Becomes one-fourth<br>d) Doubles<br><strong>Answer:<\/strong> c) Becomes one-fourth<br><strong>Explanation:<\/strong> <img decoding=\"async\" width=\"41\" height=\"27\" src=\"blob:https:\/\/mcqsadda.com\/2d821872-1be3-445e-a654-4e649534cb5f\">, doubling radius reduces gravity by 4 times.<\/p>\n\n\n\n<p class=\"has-large-font-size\"><strong><mark style=\"background-color:rgba(0, 0, 0, 0)\" class=\"has-inline-color has-luminous-vivid-orange-color\">23. The time period of a simple pendulum depends on:<\/mark><\/strong><br>a) Mass of bob<br>b) Length of the pendulum<br>c) Amplitude of oscillation<br>d) Gravitational acceleration<br><strong>Answer:<\/strong> b) Length of the pendulum and d) Gravitational acceleration<br><strong>Explanation:<\/strong> <img decoding=\"async\" width=\"64\" height=\"38\" src=\"blob:https:\/\/mcqsadda.com\/3e5dee88-ff1d-45d6-a5ca-db2a33875da6\">, mass and amplitude (small) do not affect T.<\/p>\n\n\n\n<p class=\"has-large-font-size\"><mark style=\"background-color:rgba(0, 0, 0, 0)\" class=\"has-inline-color has-luminous-vivid-orange-color\"><strong>24. What is the value of escape velocity from Moon compared to Earth?<\/strong><\/mark><br>a) Same<br>b) Greater<br>c) Less<br>d) Zero<br><strong>Answer:<\/strong> c) Less<br><strong>Explanation:<\/strong> Escape velocity depends on mass and radius; Moon has less mass and radius.<\/p>\n\n\n\n<p class=\"has-large-font-size\"><strong><mark style=\"background-color:rgba(0, 0, 0, 0)\" class=\"has-inline-color has-luminous-vivid-orange-color\">25. The geostationary satellite orbits at:<\/mark><\/strong><br>a) 100 km above Earth<br>b) 36000 km above Earth<br>c) 2000 km above Earth<br>d) 500 km above Earth<br><strong>Answer:<\/strong> b) 36000 km above Earth<br><strong>Explanation:<\/strong> This altitude allows the satellite to match Earth\u2019s rotation period.<\/p>\n\n\n\n<p class=\"has-large-font-size\"><strong><mark style=\"background-color:rgba(0, 0, 0, 0)\" class=\"has-inline-color has-luminous-vivid-orange-color\">26. Which of the following affects the gravitational force between two objects?<\/mark><\/strong><br>a) Mass of objects<br>b) Distance between objects<br>c) Medium between objects<br>d) Both a and b<br><strong>Answer:<\/strong> d) Both a and b<br><strong>Explanation:<\/strong> Force depends on mass and distance, not on the medium.<\/p>\n\n\n\n<p class=\"has-large-font-size\"><strong><mark style=\"background-color:rgba(0, 0, 0, 0)\" class=\"has-inline-color has-luminous-vivid-orange-color\">27. Gravitational force inside Earth varies with:<\/mark><\/strong><br>a) Inverse square of radius<br>b) Linearly with radius<br>c) Constant<br>d) Inverse radius<br><strong>Answer:<\/strong> b) Linearly with radius<br><strong>Explanation:<\/strong> Inside Earth, gravity decreases linearly towards the center.<\/p>\n\n\n\n<p class=\"has-large-font-size\"><strong><mark style=\"background-color:rgba(0, 0, 0, 0)\" class=\"has-inline-color has-luminous-vivid-orange-color\">28. If a planet has twice the radius and twice the mass of Earth, acceleration due to gravity on its surface is:<\/mark><\/strong><br>a) Same as Earth<br>b) Twice of Earth<br>c) Half of Earth<br>d) Four times Earth<br><strong>Answer:<\/strong> a) Same as Earth<br><strong>Explanation:<\/strong> <img decoding=\"async\" width=\"186\" height=\"30\" src=\"blob:https:\/\/mcqsadda.com\/093bd962-9449-41ee-94f8-606d9fa21293\">\u2014 Corrected: Actually half of Earth\u2019s gravity, so answer is c) Half of Earth. Sorry!<br><strong>Correction:<\/strong> Answer: c) Half of Earth<\/p>\n\n\n\n<p class=\"has-large-font-size\"><strong><mark style=\"background-color:rgba(0, 0, 0, 0)\" class=\"has-inline-color has-luminous-vivid-orange-color\">29.The period of revolution of a satellite depends on:<\/mark><\/strong><br>a) Its mass<br>b) Radius of orbit<br>c) Mass of Earth<br>d) Both b and c<br><strong>Answer:<\/strong> d) Both b and c<br><strong>Explanation:<\/strong> Period depends on orbit radius and Earth\u2019s mass, not satellite mass.<\/p>\n\n\n\n<p class=\"has-large-font-size\"><strong><mark style=\"background-color:rgba(0, 0, 0, 0)\" class=\"has-inline-color has-luminous-vivid-orange-color\">30.Which quantity remains constant for a satellite moving in an elliptical orbit?<\/mark><\/strong><br>a) Kinetic energy<br>b) Angular momentum<br>c) Potential energy<br>d) Speed<br><strong>Answer:<\/strong> b) Angular momentum<br><strong>Explanation:<\/strong> Angular momentum is conserved in central force motion.<\/p>\n\n\n\n<p class=\"has-large-font-size\"><strong><mark style=\"background-color:rgba(0, 0, 0, 0)\" class=\"has-inline-color has-luminous-vivid-orange-color\">31. Weightlessness in space is due to:<\/mark><\/strong><br>a) Absence of gravity<br>b) Free fall of the spacecraft<br>c) No air resistance<br>d) None of these<br><strong>Answer:<\/strong> b) Free fall of the spacecraft<br><strong>Explanation:<\/strong> Astronauts experience weightlessness due to continuous free fall.<\/p>\n\n\n\n<p class=\"has-large-font-size\"><strong><mark style=\"background-color:rgba(0, 0, 0, 0)\" class=\"has-inline-color has-luminous-vivid-orange-color\">32. If the gravitational force between two objects is F, and the distance between them is halved, the new force is:<\/mark><\/strong><br>a) <img decoding=\"async\" width=\"7\" height=\"27\" src=\"blob:https:\/\/mcqsadda.com\/4bdc6098-a626-41ab-bff6-5b80dcb611f0\"><br>b) <img decoding=\"async\" width=\"18\" height=\"20\" src=\"blob:https:\/\/mcqsadda.com\/131ebc93-4edf-436e-ada0-c6b4fe9e1647\"><br>c) <img decoding=\"async\" width=\"7\" height=\"27\" src=\"blob:https:\/\/mcqsadda.com\/923e39e5-325e-458a-8cb1-2bb8379aa859\"><br>d) <img decoding=\"async\" width=\"18\" height=\"20\" src=\"blob:https:\/\/mcqsadda.com\/5b60a04b-769b-4fdc-8f8c-f5cc693c8746\"><br><strong>Answer:<\/strong> b) <img decoding=\"async\" width=\"18\" height=\"20\" src=\"blob:https:\/\/mcqsadda.com\/33e72438-50b7-462f-9cbb-124622289b37\"><br><strong>Explanation:<\/strong> Force varies inversely with the square of distance.<\/p>\n\n\n\n<p class=\"has-large-font-size\"><strong><mark style=\"background-color:rgba(0, 0, 0, 0)\" class=\"has-inline-color has-luminous-vivid-orange-color\">33. The formula for gravitational potential energy between two masses is:<\/mark><\/strong><br>a) <img decoding=\"async\" width=\"40\" height=\"28\" src=\"blob:https:\/\/mcqsadda.com\/66cec9f8-c02c-4605-8440-9a3b29196757\"><br>b) <img decoding=\"async\" width=\"27\" height=\"28\" src=\"blob:https:\/\/mcqsadda.com\/a65d2833-38b3-4f6c-8bfb-660a4a640c9c\"><br>c) <img decoding=\"async\" width=\"27\" height=\"28\" src=\"blob:https:\/\/mcqsadda.com\/98a29598-0879-4404-b9c4-8c28038f24ec\"><br>d) <img decoding=\"async\" width=\"37\" height=\"27\" src=\"blob:https:\/\/mcqsadda.com\/7fbb5aff-3643-4b4e-91b0-f5280835feb1\"><br><strong>Answer:<\/strong> a) <img decoding=\"async\" width=\"40\" height=\"28\" src=\"blob:https:\/\/mcqsadda.com\/1887cc5e-99fc-4ce6-8370-af48bb8091b9\"><br><strong>Explanation:<\/strong> Gravitational potential energy is negative and inversely proportional to distance.<\/p>\n\n\n\n<p class=\"has-large-font-size\"><strong><mark style=\"background-color:rgba(0, 0, 0, 0)\" class=\"has-inline-color has-luminous-vivid-orange-color\">34. The value of G is determined by:<\/mark><\/strong><br>a) Cavendish experiment<br>b) Newton\u2019s laws<br>c) Kepler\u2019s laws<br>d) Galileo\u2019s experiment<br><strong>Answer:<\/strong> a) Cavendish experiment<br><strong>Explanation:<\/strong> Cavendish measured G using torsion balance.<\/p>\n\n\n\n<p class=\"has-large-font-size\"><strong><mark style=\"background-color:rgba(0, 0, 0, 0)\" class=\"has-inline-color has-luminous-vivid-orange-color\">35. If a satellite\u2019s orbital speed increases, the radius of its orbit:<\/mark><\/strong><br>a) Increases<br>b) Decreases<br>c) Remains same<br>d) Becomes zero<br><strong>Answer:<\/strong> b) Decreases<br><strong>Explanation:<\/strong> Higher speed corresponds to a lower orbit radius for a circular orbit.<\/p>\n\n\n\n<p class=\"has-large-font-size\"><strong><mark style=\"background-color:rgba(0, 0, 0, 0)\" class=\"has-inline-color has-luminous-vivid-orange-color\">36. The acceleration due to gravity on a planet depends on:<\/mark><\/strong><br>a) Mass of the planet only<br>b) Radius of the planet only<br>c) Both mass and radius of the planet<br>d) Neither mass nor radius<br><strong>Answer:<\/strong> c) Both mass and radius of the planet<br><strong>Explanation:<\/strong> <img decoding=\"async\" width=\"45\" height=\"28\" src=\"blob:https:\/\/mcqsadda.com\/d6cd52fd-e771-40c1-a217-bb92957ff87a\">.<\/p>\n\n\n\n<p class=\"has-large-font-size\"><strong><mark style=\"background-color:rgba(0, 0, 0, 0)\" class=\"has-inline-color has-luminous-vivid-orange-color\">37. The law of gravitation is valid:<\/mark><\/strong><br>a) Only near Earth\u2019s surface<br>b) Only for planets<br>c) Universally, for any two masses<br>d) Only in vacuum<br><strong>Answer:<\/strong> c) Universally, for any two masses<br><strong>Explanation:<\/strong> It is a universal law valid everywhere.<\/p>\n\n\n\n<p class=\"has-large-font-size\"><strong><mark style=\"background-color:rgba(0, 0, 0, 0)\" class=\"has-inline-color has-luminous-vivid-orange-color\">38. The velocity required for a satellite to remain in orbit close to Earth\u2019s surface is called:<\/mark><\/strong><br>a) Escape velocity<br>b) Orbital velocity<br>c) Terminal velocity<br>d) Critical velocity<br><strong>Answer:<\/strong> b) Orbital velocity<br><strong>Explanation:<\/strong> Orbital velocity allows satellite to orbit Earth.<\/p>\n\n\n\n<p class=\"has-large-font-size\"><strong><mark style=\"background-color:rgba(0, 0, 0, 0)\" class=\"has-inline-color has-luminous-vivid-orange-color\">39. Kepler\u2019s second law states that:<br><\/mark><\/strong>a) Planets move in elliptical orbits<br>b) Equal areas are swept in equal times<br>c) Square of time period proportional to cube of radius<br>d) None of these<br><strong>Answer:<\/strong> b) Equal areas are swept in equal times<br><strong>Explanation:<\/strong> This implies conservation of angular momentum.<\/p>\n\n\n\n<p class=\"has-large-font-size\"><strong><mark style=\"background-color:rgba(0, 0, 0, 0)\" class=\"has-inline-color has-luminous-vivid-orange-color\">40. The gravitational force between two objects separated by 1 m is 10 N. If their separation becomes 3 m, the force will be:<\/mark><\/strong><br>a) <img decoding=\"async\" width=\"12\" height=\"28\" src=\"blob:https:\/\/mcqsadda.com\/e1d7570d-949c-40bb-9acc-2f852186ee87\">N<br>b) <img decoding=\"async\" width=\"12\" height=\"28\" src=\"blob:https:\/\/mcqsadda.com\/b2acec16-4276-4631-8e00-fadfe947a42d\">N<br>c) 30 N<br>d) 90 N<br><strong>Answer:<\/strong> a) <img decoding=\"async\" width=\"12\" height=\"28\" src=\"blob:https:\/\/mcqsadda.com\/c857076e-3d54-401b-b57f-0e5789cc7e41\">N<br><strong>Explanation:<\/strong> Force scales as <img decoding=\"async\" width=\"12\" height=\"27\" src=\"blob:https:\/\/mcqsadda.com\/9f799372-1a61-4bf5-b3be-4504e124a908\">, so <img decoding=\"async\" width=\"105\" height=\"30\" src=\"blob:https:\/\/mcqsadda.com\/c63162ea-fc97-4f44-a0f0-a82e33ce0b2b\">N.<\/p>\n\n\n\n<ol start=\"21\" class=\"wp-block-list\">\n<li><\/li>\n<\/ol>\n\n\n\n<p class=\"has-large-font-size\"><strong><mark style=\"background-color:rgba(0, 0, 0, 0)\" class=\"has-inline-color has-luminous-vivid-orange-color\">41. The value of gravitational acceleration inside Earth at a distance r from center is proportional to:<\/mark><\/strong><br>a) <img decoding=\"async\" width=\"14\" height=\"20\" src=\"blob:https:\/\/mcqsadda.com\/6a55d46d-cad1-4468-86cc-fe75c26eccc5\"><br>b) <img decoding=\"async\" width=\"7\" height=\"20\" src=\"blob:https:\/\/mcqsadda.com\/345027f9-4fca-480a-8e19-3cf5ebf2b808\"><br>c) <img decoding=\"async\" width=\"6\" height=\"27\" src=\"blob:https:\/\/mcqsadda.com\/d6b9b350-feb4-4978-bd3b-66150835daa4\"><br>d) <img decoding=\"async\" width=\"12\" height=\"27\" src=\"blob:https:\/\/mcqsadda.com\/2b2e9f64-e475-4533-a94c-65383ab5172c\"><br><strong>Answer:<\/strong> b) <img decoding=\"async\" width=\"7\" height=\"20\" src=\"blob:https:\/\/mcqsadda.com\/a9864e9b-c1ce-4d1c-964a-66a0f938d83e\"><br><strong>Explanation:<\/strong> Inside Earth, <img decoding=\"async\" width=\"9\" height=\"20\" src=\"blob:https:\/\/mcqsadda.com\/bd702572-15e3-49f3-b3fc-c36078a07d77\">varies linearly with distance from the center.<\/p>\n\n\n\n<p class=\"has-large-font-size\"><strong><mark style=\"background-color:rgba(0, 0, 0, 0)\" class=\"has-inline-color has-luminous-vivid-orange-color\">42. The gravitational force between Earth and a body of mass m is mg, where g is:<\/mark><\/strong><br>a) The same everywhere on Earth<br>b) The gravitational acceleration at Earth\u2019s surface<br>c) Independent of height<br>d) Varies with mass m<br><strong>Answer:<\/strong> b) The gravitational acceleration at Earth\u2019s surface<br><strong>Explanation:<\/strong> <img decoding=\"async\" width=\"9\" height=\"20\" src=\"blob:https:\/\/mcqsadda.com\/e038849e-c0bf-4b86-b3a9-a1e8d5bddb6f\">is acceleration due to gravity at Earth&#8217;s surface, so <img decoding=\"async\" width=\"50\" height=\"20\" src=\"blob:https:\/\/mcqsadda.com\/e0220e7c-28ed-4216-aeaa-ab5f0ae01f5f\">.<\/p>\n\n\n\n<p class=\"has-large-font-size\"><strong><mark style=\"background-color:rgba(0, 0, 0, 0)\" class=\"has-inline-color has-luminous-vivid-orange-color\">43. The gravitational potential energy of a satellite orbiting Earth is:<\/mark><\/strong><br>a) Zero<br>b) Positive<br>c) Negative<br>d) Infinity<br><strong>Answer:<\/strong> c) Negative<br><strong>Explanation:<\/strong> Potential energy in gravitational field is negative relative to zero at infinite distance.<\/p>\n\n\n\n<p class=\"has-large-font-size\"><strong><mark style=\"background-color:rgba(0, 0, 0, 0)\" class=\"has-inline-color has-luminous-vivid-orange-color\">44. The radius of geostationary orbit is about:<\/mark><\/strong><br>a) 6400 km<br>b) 42160 km<br>c) 35786 km<br>d) 10000 km<br><strong>Answer:<\/strong> c) 35786 km<br><strong>Explanation:<\/strong> Geostationary satellites orbit at about 36,000 km from Earth\u2019s surface (~42,160 km from Earth\u2019s center).<\/p>\n\n\n\n<p class=\"has-large-font-size\"><strong><mark style=\"background-color:rgba(0, 0, 0, 0)\" class=\"has-inline-color has-luminous-vivid-orange-color\">45. The acceleration due to gravity on the surface of a planet is <img decoding=\"async\" width=\"9\" height=\"20\" src=\"blob:https:\/\/mcqsadda.com\/7a5b38c9-ba2c-4d5f-8a9e-164be7275039\">. What is the acceleration at a height h above the surface?<\/mark><\/strong><br>a) <img decoding=\"async\" width=\"50\" height=\"28\" src=\"blob:https:\/\/mcqsadda.com\/c2ff3c01-17e8-4e5f-8d3b-ec056d2f661e\"><br>b) <img decoding=\"async\" width=\"50\" height=\"28\" src=\"blob:https:\/\/mcqsadda.com\/286bff4a-4eb0-422b-b974-023bf7f847e5\"><br>c) <img decoding=\"async\" width=\"43\" height=\"28\" src=\"blob:https:\/\/mcqsadda.com\/04580d04-452d-4819-998a-0abe665dfb2a\"><br>d) <img decoding=\"async\" width=\"43\" height=\"28\" src=\"blob:https:\/\/mcqsadda.com\/893ff808-7637-429a-b0e6-db288f62c271\"><br><strong>Answer:<\/strong> a) <img decoding=\"async\" width=\"50\" height=\"28\" src=\"blob:https:\/\/mcqsadda.com\/569effea-65ab-4557-a45f-b9fc41820bf2\"><br><strong>Explanation:<\/strong> Gravity decreases with square of the distance from the center.<\/p>\n\n\n\n<p class=\"has-large-font-size\"><strong><mark style=\"background-color:rgba(0, 0, 0, 0)\" class=\"has-inline-color has-luminous-vivid-orange-color\">46. If a planet\u2019s radius decreases but its mass remains constant, its surface gravity:<\/mark><\/strong><br>a) Increases<br>b) Decreases<br>c) Remains same<br>d) Zero<br><strong>Answer:<\/strong> a) Increases<br><strong>Explanation:<\/strong> <img decoding=\"async\" width=\"41\" height=\"27\" src=\"blob:https:\/\/mcqsadda.com\/1eedb728-a20b-455c-a8a5-78c7bad7380f\">, so reducing <img decoding=\"async\" width=\"10\" height=\"20\" src=\"blob:https:\/\/mcqsadda.com\/dbb8211c-6175-45b6-883f-023b0152ec5a\">increases <img decoding=\"async\" width=\"9\" height=\"20\" src=\"blob:https:\/\/mcqsadda.com\/cb392731-01f9-4a7a-9027-2d33f4cdd1f1\">.<\/p>\n\n\n\n<p class=\"has-large-font-size\"><strong><mark style=\"background-color:rgba(0, 0, 0, 0)\" class=\"has-inline-color has-luminous-vivid-orange-color\">47. The value of <img decoding=\"async\" width=\"10\" height=\"20\" src=\"blob:https:\/\/mcqsadda.com\/398f1a06-46c5-47c8-9d02-386f8e49b4ff\">can be experimentally determined using:<\/mark><\/strong><br>a) Newton\u2019s cradle<br>b) Torsion balance<br>c) Pendulum<br>d) Barometer<br><strong>Answer:<\/strong> b) Torsion balance<br><strong>Explanation:<\/strong> Cavendish used torsion balance to measure <img decoding=\"async\" width=\"10\" height=\"20\" src=\"blob:https:\/\/mcqsadda.com\/4996c7e9-83b6-41cd-947a-1a40cb880f01\">.<\/p>\n\n\n\n<p class=\"has-large-font-size\"><strong><mark style=\"background-color:rgba(0, 0, 0, 0)\" class=\"has-inline-color has-luminous-vivid-orange-color\">48. Which of the following does NOT affect the orbital speed of a satellite?<\/mark><\/strong><br>a) Mass of satellite<br>b) Mass of Earth<br>c) Radius of orbit<br>d) Gravitational constant<br><strong>Answer:<\/strong> a) Mass of satellite<br><strong>Explanation:<\/strong> Orbital speed depends on <img decoding=\"async\" width=\"22\" height=\"20\" src=\"blob:https:\/\/mcqsadda.com\/42f4ffd3-5ead-4777-bbaa-3e5a8e9058d1\">and radius, independent of satellite\u2019s mass.<\/p>\n\n\n\n<p class=\"has-large-font-size\"><strong><mark style=\"background-color:rgba(0, 0, 0, 0)\" class=\"has-inline-color has-luminous-vivid-orange-color\">49. If Earth\u2019s mass doubles and radius doubles, acceleration due to gravity becomes:<\/mark><\/strong><br>a) Same<br>b) Double<br>c) Half<br>d) Quarter<br><strong>Answer:<\/strong> c) Half<br><strong>Explanation:<\/strong> <img decoding=\"async\" width=\"163\" height=\"30\" src=\"blob:https:\/\/mcqsadda.com\/61810187-b916-4f1f-99af-bf1ab4ff64d2\">.<\/p>\n\n\n\n<p class=\"has-large-font-size\"><strong><mark style=\"background-color:rgba(0, 0, 0, 0)\" class=\"has-inline-color has-luminous-vivid-orange-color\">50. The escape velocity is independent of:<\/mark><\/strong><br>a) Mass of the planet<br>b) Radius of the planet<br>c) Mass of the escaping object<br>d) Gravitational constant<br><strong>Answer:<\/strong> c) Mass of the escaping object<br><strong>Explanation:<\/strong> Escape velocity depends only on planet\u2019s mass and radius.<\/p>\n\n\n\n<p class=\"has-large-font-size\"><strong><mark style=\"background-color:rgba(0, 0, 0, 0)\" class=\"has-inline-color has-luminous-vivid-orange-color\">51. Kepler\u2019s third law is mathematically expressed as:<\/mark><\/strong><br>a) <img decoding=\"async\" width=\"51\" height=\"20\" src=\"blob:https:\/\/mcqsadda.com\/fdc3b15c-02ee-43b1-8f3d-1d06bdd932d5\"><br>b) <img decoding=\"async\" width=\"44\" height=\"20\" src=\"blob:https:\/\/mcqsadda.com\/4c4d4e2e-fc30-45fd-802d-773f7fbd5e78\"><br>c) <img decoding=\"async\" width=\"51\" height=\"20\" src=\"blob:https:\/\/mcqsadda.com\/c6aa6dab-92c2-4dfd-8eee-4c120af5d013\"><br>d) <img decoding=\"async\" width=\"51\" height=\"20\" src=\"blob:https:\/\/mcqsadda.com\/c205bbd9-986f-430e-bf84-0d1f57d72023\"><br><strong>Answer:<\/strong> a) <img decoding=\"async\" width=\"51\" height=\"20\" src=\"blob:https:\/\/mcqsadda.com\/b9c5483d-a8b2-4067-a59c-8d7f0f98b2ea\"><br><strong>Explanation:<\/strong> Square of orbital period proportional to cube of orbital radius.<\/p>\n\n\n\n<p class=\"has-large-font-size\"><strong><mark style=\"background-color:rgba(0, 0, 0, 0)\" class=\"has-inline-color has-luminous-vivid-orange-color\">52. A satellite moving in an elliptical orbit has:<\/mark><\/strong><br>a) Constant speed<br>b) Variable speed<br>c) Constant kinetic energy<br>d) None of the above<br><strong>Answer:<\/strong> b) Variable speed<br><strong>Explanation:<\/strong> Speed changes due to conservation of angular momentum.<\/p>\n\n\n\n<p class=\"has-large-font-size\"><strong><mark style=\"background-color:rgba(0, 0, 0, 0)\" class=\"has-inline-color has-luminous-vivid-orange-color\">53. What happens to gravitational potential energy when the distance between two masses increases?<\/mark><\/strong><br>a) Increases<br>b) Decreases<br>c) Remains constant<br>d) Becomes zero<br><strong>Answer:<\/strong> a) Increases (becomes less negative)<br><strong>Explanation:<\/strong> Gravitational potential energy increases (towards zero) as separation increases.<\/p>\n\n\n\n<p class=\"has-large-font-size\"><strong><mark style=\"background-color:rgba(0, 0, 0, 0)\" class=\"has-inline-color has-luminous-vivid-orange-color\">54. The acceleration due to gravity is zero at:<\/mark><\/strong><br>a) Earth\u2019s surface<br>b) Earth\u2019s center<br>c) Infinite distance from Earth<br>d) Both b and c<br><strong>Answer:<\/strong> d) Both b and c<br><strong>Explanation:<\/strong> Gravity is zero at Earth\u2019s center and infinitely far away.<\/p>\n\n\n\n<p class=\"has-large-font-size\"><strong><mark style=\"background-color:rgba(0, 0, 0, 0)\" class=\"has-inline-color has-luminous-vivid-orange-color\">55. The gravitational force between two identical spheres each of mass m and radius r when placed in contact is:<\/mark><\/strong><br>a) <img decoding=\"async\" width=\"23\" height=\"30\" src=\"blob:https:\/\/mcqsadda.com\/40e344c4-d17e-4a5c-b92f-691663d8099f\"><br>b) <img decoding=\"async\" width=\"27\" height=\"32\" src=\"blob:https:\/\/mcqsadda.com\/183b0a0e-e0e7-4081-8dc6-b1bcb53e9766\"><br>c) <img decoding=\"async\" width=\"23\" height=\"30\" src=\"blob:https:\/\/mcqsadda.com\/01815985-04c8-4e47-8382-8b126789258d\"><br>d) Zero<br><strong>Answer:<\/strong> b) <img decoding=\"async\" width=\"27\" height=\"32\" src=\"blob:https:\/\/mcqsadda.com\/a48f1a86-4adf-400a-8fbb-7b7b2016b8fc\"><br><strong>Explanation:<\/strong> Distance between centers = 2r when spheres are in contact.<\/p>\n\n\n\n<p class=\"has-large-font-size\"><strong><mark style=\"background-color:rgba(0, 0, 0, 0)\" class=\"has-inline-color has-luminous-vivid-orange-color\">56. Weight of an object is maximum at:<\/mark><\/strong><br>a) Equator<br>b) Poles<br>c) Anywhere on Earth<br>d) At the center of Earth<br><strong>Answer:<\/strong> b) Poles<br><strong>Explanation:<\/strong> Earth\u2019s rotation reduces effective gravity at equator.<\/p>\n\n\n\n<p class=\"has-large-font-size\"><strong><mark style=\"background-color:rgba(0, 0, 0, 0)\" class=\"has-inline-color has-luminous-vivid-orange-color\">57. Gravitational force between two bodies is 16 N. If their masses are doubled and distance is doubled, the force becomes:<\/mark><\/strong><br>a) 16 N<br>b) 8 N<br>c) 32 N<br>d) 4 N<br><strong>Answer:<\/strong> b) 8 N<br><strong>Explanation:<\/strong> <img decoding=\"async\" width=\"57\" height=\"27\" src=\"blob:https:\/\/mcqsadda.com\/8cbf1f0b-364d-42e0-a832-88e644280e98\">, new force = <img decoding=\"async\" width=\"125\" height=\"31\" src=\"blob:https:\/\/mcqsadda.com\/ad8244f8-7c52-4c29-a5a9-1796dd7580fc\">. Actually the force remains 16 N, correction here.<br><strong>Correction:<\/strong> New force = 16 N<\/p>\n\n\n\n<p class=\"has-large-font-size\"><strong><mark style=\"background-color:rgba(0, 0, 0, 0)\" class=\"has-inline-color has-luminous-vivid-orange-color\">58. What is the work done by gravitational force on a satellite in a circular orbit?<\/mark><\/strong><br>a) Zero<br>b) Positive<br>c) Negative<br>d) Infinite<br><strong>Answer:<\/strong> a) Zero<br><strong>Explanation:<\/strong> Force is perpendicular to displacement in circular motion.<\/p>\n\n\n\n<p class=\"has-large-font-size\"><strong><mark style=\"background-color:rgba(0, 0, 0, 0)\" class=\"has-inline-color has-luminous-vivid-orange-color\">59. The velocity of satellite in low Earth orbit is approximately:<\/mark><\/strong><br>a) 7.8 km\/s<br>b) 11.2 km\/s<br>c) 3.5 km\/s<br>d) 5 km\/s<br><strong>Answer:<\/strong> a) 7.8 km\/s<br><strong>Explanation:<\/strong> Orbital speed near Earth surface is ~7.8 km\/s.<\/p>\n\n\n\n<p class=\"has-large-font-size\"><strong><mark style=\"background-color:rgba(0, 0, 0, 0)\" class=\"has-inline-color has-luminous-vivid-orange-color\">60. Potential at surface of Earth is:<\/mark><\/strong><br>a) <img decoding=\"async\" width=\"30\" height=\"28\" src=\"blob:https:\/\/mcqsadda.com\/8c6c889b-34d3-467a-913e-f987a01abf9e\"><br>b) <img decoding=\"async\" width=\"17\" height=\"28\" src=\"blob:https:\/\/mcqsadda.com\/87b3b94e-053c-4ca2-b195-d025931d925e\"><br>c) Zero<br>d) Infinite<br><strong>Answer:<\/strong> a) <img decoding=\"async\" width=\"30\" height=\"28\" src=\"blob:https:\/\/mcqsadda.com\/c735d41d-f190-4ce5-a4f7-0109cc8c1eea\"><br><strong>Explanation:<\/strong> Gravitational potential is negative and depends on radius.<\/p>\n\n\n\n<p class=\"has-large-font-size\"><strong><mark style=\"background-color:rgba(0, 0, 0, 0)\" class=\"has-inline-color has-luminous-vivid-orange-color\">61. If the Earth were suddenly shrunk to half its radius without changing its mass, the acceleration due to gravity on its surface would:<\/mark><\/strong><br>a) Remain same<br>b) Double<br>c) Quadruple<br>d) Halve<br><strong>Answer:<\/strong> c) Quadruple<br><strong>Explanation:<\/strong> <img decoding=\"async\" width=\"41\" height=\"27\" src=\"blob:https:\/\/mcqsadda.com\/920318bb-275d-4803-8e7d-d0fe983b98ca\">, halving <img decoding=\"async\" width=\"10\" height=\"20\" src=\"blob:https:\/\/mcqsadda.com\/f617c4bb-f298-43e3-a878-c9ef267fe98e\">increases <img decoding=\"async\" width=\"9\" height=\"20\" src=\"blob:https:\/\/mcqsadda.com\/29587787-5aaf-41a6-a601-d1118d1fb04d\">by factor of 4.<\/p>\n\n\n\n<p class=\"has-large-font-size\"><strong><mark style=\"background-color:rgba(0, 0, 0, 0)\" class=\"has-inline-color has-luminous-vivid-orange-color\">62. In gravitational interaction, the force on the two masses is:<\/mark><\/strong><br>a) Different in magnitude and direction<br>b) Equal in magnitude and opposite in direction<br>c) Equal in magnitude and same direction<br>d) Zero<br><strong>Answer:<\/strong> b) Equal in magnitude and opposite in direction<br><strong>Explanation:<\/strong> Newton\u2019s third law states action and reaction forces are equal and opposite.<\/p>\n\n\n\n<p class=\"has-large-font-size\"><strong><mark style=\"background-color:rgba(0, 0, 0, 0)\" class=\"has-inline-color has-luminous-vivid-orange-color\">63. The time period of satellite orbiting Earth depends on:<\/mark><\/strong><br>a) Satellite\u2019s mass only<br>b) Radius of orbit only<br>c) Both satellite\u2019s mass and radius<br>d) Neither<br><strong>Answer:<\/strong> b) Radius of orbit only<br><strong>Explanation:<\/strong> <img decoding=\"async\" width=\"73\" height=\"38\" src=\"blob:https:\/\/mcqsadda.com\/64e085db-36aa-4793-81f0-8ca0c63ff5ea\">, independent of satellite mass.<\/p>\n\n\n\n<p class=\"has-large-font-size\"><strong><mark style=\"background-color:rgba(0, 0, 0, 0)\" class=\"has-inline-color has-luminous-vivid-orange-color\">64. Gravitational force is a:<\/mark><\/strong><br>a) Contact force<br>b) Non-contact force<br>c) Both<br>d) None<br><strong>Answer:<\/strong> b) Non-contact force<br><strong>Explanation:<\/strong> Gravity acts at a distance without physical contact.<\/p>\n\n\n\n<p class=\"has-large-font-size\"><mark style=\"background-color:rgba(0, 0, 0, 0)\" class=\"has-inline-color has-luminous-vivid-orange-color\"><strong>65. Escape velocity is independent of:<\/strong><\/mark><br>a) Radius of planet<br>b) Mass of planet<br>c) Mass of escaping body<br>d) Gravitational constant<br><strong>Answer:<\/strong> c) Mass of escaping body<br><strong>Explanation:<\/strong> Escape velocity formula doesn\u2019t include the object\u2019s mass.<\/p>\n\n\n\n<p class=\"has-large-font-size\"><strong><mark style=\"background-color:rgba(0, 0, 0, 0)\" class=\"has-inline-color has-luminous-vivid-orange-color\">66. If the gravitational constant G were to increase, the acceleration due to gravity on Earth\u2019s surface would:<\/mark><\/strong><br>a) Increase<br>b) Decrease<br>c) Remain same<br>d) Become zero<br><strong>Answer:<\/strong> a) Increase<br><strong>Explanation:<\/strong> <img decoding=\"async\" width=\"45\" height=\"28\" src=\"blob:https:\/\/mcqsadda.com\/6f71c094-abb7-45f7-8793-f91343de0bb5\">, so increasing G increases g.<\/p>\n\n\n\n<p class=\"has-large-font-size\"><strong><mark style=\"background-color:rgba(0, 0, 0, 0)\" class=\"has-inline-color has-luminous-vivid-orange-color\">67. A satellite in a circular orbit is:<\/mark><\/strong><br>a) Accelerating<br>b) Moving with constant speed and no acceleration<br>c) Moving with uniform velocity<br>d) At rest<br><strong>Answer:<\/strong> a) Accelerating<br><strong>Explanation:<\/strong> Acceleration is centripetal, directed towards Earth\u2019s center.<\/p>\n\n\n\n<p class=\"has-large-font-size\"><strong><mark style=\"background-color:rgba(0, 0, 0, 0)\" class=\"has-inline-color has-luminous-vivid-orange-color\">68. The energy of a satellite in orbit is:<\/mark><\/strong><br>a) Kinetic energy only<br>b) Potential energy only<br>c) Sum of kinetic and potential energy<br>d) Zero<br><strong>Answer:<\/strong> c) Sum of kinetic and potential energy<br><strong>Explanation:<\/strong> Total mechanical energy = KE + PE.<\/p>\n\n\n\n<p class=\"has-large-font-size\"><strong><mark style=\"background-color:rgba(0, 0, 0, 0)\" class=\"has-inline-color has-luminous-vivid-orange-color\">69. The net gravitational force on a mass inside a hollow spherical shell is:<\/mark><\/strong><br>a) Same as outside<br>b) Zero<br>c) Infinite<br>d) Equal to shell\u2019s mass<br><strong>Answer:<\/strong> b) Zero<br><strong>Explanation:<\/strong> Inside a hollow shell, gravitational forces cancel out.<\/p>\n\n\n\n<p class=\"has-large-font-size\"><mark style=\"background-color:rgba(0, 0, 0, 0)\" class=\"has-inline-color has-luminous-vivid-orange-color\"><strong>70. The gravitational force between two objects depends on:<\/strong><\/mark><br>a) Product of their masses<br>b) Square of distance between them<br>c) Sum of their masses<br>d) Difference of their masses<br><strong>Answer:<\/strong> a) Product of their masses<br><strong>Explanation:<\/strong> Newton\u2019s law: <img decoding=\"async\" width=\"59\" height=\"26\" src=\"blob:https:\/\/mcqsadda.com\/161d71a8-d4c3-4f15-884b-b717acd060f4\">.<\/p>\n\n\n\n<p class=\"has-large-font-size\"><strong><mark style=\"background-color:rgba(0, 0, 0, 0)\" class=\"has-inline-color has-luminous-vivid-orange-color\">71. If a satellite moves to an orbit with twice the radius, its orbital period becomes:<\/mark><\/strong><br>a) Twice<br>b) Four times<br>c) <img decoding=\"async\" width=\"26\" height=\"22\" src=\"blob:https:\/\/mcqsadda.com\/f636620f-fef8-450a-8287-8a7f80fdb81e\">times<br>d) <img decoding=\"async\" width=\"18\" height=\"22\" src=\"blob:https:\/\/mcqsadda.com\/8d6c337f-aea5-4ce9-8dc8-fd7f61535dad\">times<br><strong>Answer:<\/strong> d) <img decoding=\"async\" width=\"18\" height=\"22\" src=\"blob:https:\/\/mcqsadda.com\/8151e78e-3d5d-453b-b969-3659625df9d0\">times<br><strong>Explanation:<\/strong> <img decoding=\"async\" width=\"53\" height=\"21\" src=\"blob:https:\/\/mcqsadda.com\/7f3bfbbe-fdc5-49e7-95c3-3ba175857edf\">, so <img decoding=\"async\" width=\"163\" height=\"22\" src=\"blob:https:\/\/mcqsadda.com\/ada852ce-d174-4d38-93f5-1b2aa4c0bae0\">.<\/p>\n\n\n\n<p class=\"has-large-font-size\"><strong><mark style=\"background-color:rgba(0, 0, 0, 0)\" class=\"has-inline-color has-luminous-vivid-orange-color\">72. The minimum velocity needed to keep a satellite in orbit close to Earth\u2019s surface is:<\/mark><\/strong><br>a) Escape velocity<br>b) Orbital velocity<br>c) Terminal velocity<br>d) Sound velocity<br><strong>Answer:<\/strong> b) Orbital velocity<br><strong>Explanation:<\/strong> Orbital velocity allows the satellite to stay in orbit.<\/p>\n\n\n\n<p class=\"has-large-font-size\"><strong><mark style=\"background-color:rgba(0, 0, 0, 0)\" class=\"has-inline-color has-luminous-vivid-orange-color\">73. Gravitational potential energy is zero at:<\/mark><\/strong><br>a) Earth\u2019s surface<br>b) Infinity<br>c) Center of Earth<br>d) Moon\u2019s surface<br><strong>Answer:<\/strong> b) Infinity<br><strong>Explanation:<\/strong> Conventionally, potential energy is zero at infinite distance.<\/p>\n\n\n\n<p class=\"has-large-font-size\"><strong><mark style=\"background-color:rgba(0, 0, 0, 0)\" class=\"has-inline-color has-luminous-vivid-orange-color\">74. Acceleration due to gravity on the surface of the Moon is about:<\/mark><\/strong><br>a) 1.62 m\/s\u00b2<br>b) 9.8 m\/s\u00b2<br>c) 3.7 m\/s\u00b2<br>d) 0 m\/s\u00b2<br><strong>Answer:<\/strong> a) 1.62 m\/s\u00b2<br><strong>Explanation:<\/strong> Moon\u2019s gravity is about 1\/6th of Earth\u2019s.<\/p>\n\n\n\n<p class=\"has-large-font-size\"><strong><mark style=\"background-color:rgba(0, 0, 0, 0)\" class=\"has-inline-color has-luminous-vivid-orange-color\">75. Which law states the relation between force and acceleration?<\/mark><\/strong><br>a) Newton\u2019s first law<br>b) Newton\u2019s second law<br>c) Newton\u2019s third law<br>d) Kepler\u2019s first law<br><strong>Answer:<\/strong> b) Newton\u2019s second law<br><strong>Explanation:<\/strong> <img decoding=\"async\" width=\"49\" height=\"20\" src=\"blob:https:\/\/mcqsadda.com\/f3202841-7498-43f7-9160-9ca1e1c6973f\">.<\/p>\n\n\n\n<p class=\"has-large-font-size\"><mark style=\"background-color:rgba(0, 0, 0, 0)\" class=\"has-inline-color has-luminous-vivid-orange-color\"><strong>76. The work done by gravity on a freely falling body is:<\/strong><\/mark><br>a) Zero<br>b) Negative<br>c) Positive<br>d) Infinite<br><strong>Answer:<\/strong> c) Positive<br><strong>Explanation:<\/strong> Gravity does work to increase the body\u2019s kinetic energy.<\/p>\n\n\n\n<p class=\"has-large-font-size\"><strong><mark style=\"background-color:rgba(0, 0, 0, 0)\" class=\"has-inline-color has-luminous-vivid-orange-color\">77. A geostationary satellite revolves around Earth in:<\/mark><\/strong><br>a) 12 hours<br>b) 24 hours<br>c) 1 hour<br>d) 365 days<br><strong>Answer:<\/strong> b) 24 hours<br><strong>Explanation:<\/strong> It matches Earth\u2019s rotation period.<\/p>\n\n\n\n<p class=\"has-large-font-size\"><strong><mark style=\"background-color:rgba(0, 0, 0, 0)\" class=\"has-inline-color has-luminous-vivid-orange-color\">78. The gravitational potential due to a point mass M at distance r is:<\/mark><\/strong><br>a) <img decoding=\"async\" width=\"17\" height=\"28\" src=\"blob:https:\/\/mcqsadda.com\/01f01304-dbb5-4013-b217-b0a5ce73e8f6\"><br>b) <img decoding=\"async\" width=\"30\" height=\"28\" src=\"blob:https:\/\/mcqsadda.com\/bfc4b600-9724-418a-b3b0-09e82be10db9\"><br>c) <img decoding=\"async\" width=\"17\" height=\"28\" src=\"blob:https:\/\/mcqsadda.com\/2be6f3ab-a8d1-426b-b848-165c8cae3599\"><br>d) <img decoding=\"async\" width=\"30\" height=\"28\" src=\"blob:https:\/\/mcqsadda.com\/87ab8f00-2be5-41a7-ab0c-ff82def8399d\"><br><strong>Answer:<\/strong> b) <img decoding=\"async\" width=\"30\" height=\"28\" src=\"blob:https:\/\/mcqsadda.com\/d8e6e4b8-1696-46e0-af42-75acdbed3a51\"><br><strong>Explanation:<\/strong> Potential is negative and inversely proportional to r.<\/p>\n\n\n\n<p class=\"has-large-font-size\"><strong><mark style=\"background-color:rgba(0, 0, 0, 0)\" class=\"has-inline-color has-luminous-vivid-orange-color\">79. When a body moves from Earth\u2019s surface to infinity, its gravitational potential energy:<\/mark><\/strong><br>a) Increases<br>b) Decreases<br>c) Remains constant<br>d) Becomes negative<br><strong>Answer:<\/strong> a) Increases<br><strong>Explanation:<\/strong> Potential energy increases from negative to zero at infinity.<\/p>\n\n\n\n<p class=\"has-large-font-size\"><strong><mark style=\"background-color:rgba(0, 0, 0, 0)\" class=\"has-inline-color has-luminous-vivid-orange-color\">80. The magnitude of gravitational force between two objects is:<\/mark><\/strong><br>a) Proportional to the distance between them<br>b) Proportional to the square of the distance between them<br>c) Inversely proportional to the distance between them<br>d) Inversely proportional to the square of the distance between them<br><strong>Answer:<\/strong> d) Inversely proportional to the square of the distance between them<br><strong>Explanation:<\/strong> According to Newton\u2019s law.<\/p>\n\n\n\n<p class=\"has-large-font-size\"><strong><mark style=\"background-color:rgba(0, 0, 0, 0)\" class=\"has-inline-color has-luminous-vivid-orange-color\">81. The force that keeps the planets in orbit around the Sun is:<\/mark><\/strong><br>\u00a0\u00a0\u00a0\u00a0\u00a0 a) Electromagnetic force<br>\u00a0\u00a0\u00a0\u00a0\u00a0 b) Nuclear force<br>\u00a0\u00a0\u00a0\u00a0\u00a0\u00a0c) Gravitational force<br>\u00a0\u00a0\u00a0\u00a0\u00a0\u00a0d) Frictional force<br><strong>\u00a0\u00a0\u00a0\u00a0\u00a0\u00a0\u00a0Answer:<\/strong> c) Gravitational force<br><strong>\u00a0\u00a0\u00a0\u00a0\u00a0\u00a0\u00a0Explanation:<\/strong> Gravity provides the centripetal force.<\/p>\n\n\n\n<p class=\"has-large-font-size\"><strong><mark style=\"background-color:rgba(0, 0, 0, 0)\" class=\"has-inline-color has-luminous-vivid-orange-color\">82. The gravitational force inside a solid sphere at a distance r from the center is:<\/mark><\/strong><br>a) Zero<br>b) <img decoding=\"async\" width=\"26\" height=\"27\" src=\"blob:https:\/\/mcqsadda.com\/18671b98-36f1-45d3-97d5-d3f781f2b0bb\"><br>c) <img decoding=\"async\" width=\"22\" height=\"20\" src=\"blob:https:\/\/mcqsadda.com\/d626e29f-9ec2-4b5f-9e55-242c223f6333\"><br>d) Constant<br><strong>Answer:<\/strong> c) <img decoding=\"async\" width=\"22\" height=\"20\" src=\"blob:https:\/\/mcqsadda.com\/be438670-1b4e-4d12-a929-b8cb941f2948\"><br><strong>Explanation:<\/strong> Gravity varies linearly inside the sphere.82. <\/p>\n\n\n\n<p class=\"has-large-font-size\"><strong><mark style=\"background-color:rgba(0, 0, 0, 0)\" class=\"has-inline-color has-luminous-vivid-orange-color\">83. Escape velocity from Earth is proportional to:<\/mark><\/strong><br>a) <img decoding=\"async\" width=\"22\" height=\"22\" src=\"blob:https:\/\/mcqsadda.com\/da8b2217-f2af-4aae-b968-286f4338aa54\"><br>b) <img decoding=\"async\" width=\"17\" height=\"28\" src=\"blob:https:\/\/mcqsadda.com\/1f68a625-407d-4e56-81bf-bcfa75677432\"><br>c) <img decoding=\"async\" width=\"13\" height=\"20\" src=\"blob:https:\/\/mcqsadda.com\/183df1b1-1d25-47dd-bcc5-ad7c15d624bd\"><br>d) <img decoding=\"async\" width=\"10\" height=\"27\" src=\"blob:https:\/\/mcqsadda.com\/f2728bba-3cf0-4e68-a83f-be13a15b55fb\"><br><strong>Answer:<\/strong> a) <img decoding=\"async\" width=\"22\" height=\"22\" src=\"blob:https:\/\/mcqsadda.com\/0de89e11-4113-406c-ad3f-ba34186e7acb\"><br><strong>Explanation:<\/strong> <img decoding=\"async\" width=\"67\" height=\"38\" src=\"blob:https:\/\/mcqsadda.com\/98fec616-7926-42c3-9660-21f763a473f1\">.<\/p>\n\n\n\n<p class=\"has-large-font-size\"><strong><mark style=\"background-color:rgba(0, 0, 0, 0)\" class=\"has-inline-color has-luminous-vivid-orange-color\">84. A satellite moving with speed less than orbital velocity:<\/mark><\/strong><br>a) Escapes Earth<br>b) Falls to Earth<br>c) Remains in orbit<br>d) Moves away infinitely<br><strong>Answer:<\/strong> b) Falls to Earth<br><strong>Explanation:<\/strong> Insufficient speed to maintain orbit.<\/p>\n\n\n\n<p class=\"has-large-font-size\"><strong><mark style=\"background-color:rgba(0, 0, 0, 0)\" class=\"has-inline-color has-luminous-vivid-orange-color\">85. The point at which gravitational potential energy is minimum is:<\/mark><\/strong><br>a) At Earth\u2019s surface<br>b) At infinity<br>c) At center of Earth<br>d) On Moon\u2019s surface<br><strong>Answer:<\/strong> c) At center of Earth<br><strong>Explanation:<\/strong> Potential energy is most negative at the center.<\/p>\n\n\n\n<p class=\"has-large-font-size\"><strong><mark style=\"background-color:rgba(0, 0, 0, 0)\" class=\"has-inline-color has-luminous-vivid-orange-color\">86. The weight of an object is less on the Moon because:<\/mark><\/strong><br>a) Moon\u2019s radius is smaller<br>b) Moon\u2019s mass is smaller<br>c) Moon\u2019s gravitational acceleration is smaller<br>d) All of the above<br><strong>Answer:<\/strong> d) All of the above<br><strong>Explanation:<\/strong> All contribute to lower gravity on the Moon.<\/p>\n\n\n\n<p class=\"has-large-font-size\"><strong><mark style=\"background-color:rgba(0, 0, 0, 0)\" class=\"has-inline-color has-luminous-vivid-orange-color\">87. The acceleration due to gravity on Mars is:<\/mark><\/strong><br>a) Less than Earth<br>b) Greater than Earth<br>c) Equal to Earth<br>d) Zero<br><strong>Answer:<\/strong> a) Less than Earth<br><strong>Explanation:<\/strong> Mars has lower mass and size than Earth.<\/p>\n\n\n\n<p class=\"has-large-font-size\"><mark style=\"background-color:rgba(0, 0, 0, 0)\" class=\"has-inline-color has-luminous-vivid-orange-color\"><strong>88. What is the SI unit of gravitational potential?<\/strong><\/mark><br>a) Joule<br>b) Joule per kilogram (J\/kg)<br>c) Newton<br>d) Newton-meter<br><strong>Answer:<\/strong> b) Joule per kilogram (J\/kg)<br><strong>Explanation:<\/strong> Potential energy per unit mass.<\/p>\n\n\n\n<p class=\"has-large-font-size\"><strong><mark style=\"background-color:rgba(0, 0, 0, 0)\" class=\"has-inline-color has-luminous-vivid-orange-color\">89. The energy required to move a unit mass from Earth\u2019s surface to infinity is called:<\/mark><\/strong><br>a) Kinetic energy<br>b) Escape energy<br>c) Gravitational potential energy<br>d) Mechanical energy<br><strong>Answer:<\/strong> b) Escape energy<br><strong>Explanation:<\/strong> Escape energy needed to break free from Earth\u2019s gravity.<\/p>\n\n\n\n<p class=\"has-large-font-size\"><mark style=\"background-color:rgba(0, 0, 0, 0)\" class=\"has-inline-color has-luminous-vivid-orange-color\"><strong>90.<\/strong> <strong>For a satellite in circular orbit, total energy is:<\/strong><\/mark><br>a) Positive<br>b) Negative<br>c) Zero<br>d) Infinite<br><strong>Answer:<\/strong> b) Negative<br><strong>Explanation:<\/strong> Total mechanical energy is negative in bound orbit.<\/p>\n\n\n\n<p class=\"has-large-font-size\"><strong><mark style=\"background-color:rgba(0, 0, 0, 0)\" class=\"has-inline-color has-luminous-vivid-orange-color\">91. Which of the following quantities is a scalar?<\/mark><\/strong><br>a) Gravitational force<br>b) Gravitational potential<br>c) Acceleration due to gravity<br>d) Velocity of satellite<br><strong>Answer:<\/strong> b) Gravitational potential<br><strong>Explanation:<\/strong> Potential is scalar; force and acceleration are vectors.<\/p>\n\n\n\n<p class=\"has-large-font-size\"><strong><mark style=\"background-color:rgba(0, 0, 0, 0)\" class=\"has-inline-color has-luminous-vivid-orange-color\">92. When a body moves from Earth\u2019s surface to a height equal to Earth\u2019s radius, the acceleration due to gravity becomes:<\/mark><\/strong><br>a) <img decoding=\"async\" width=\"7\" height=\"26\" src=\"blob:https:\/\/mcqsadda.com\/fd328ead-9593-4038-885d-669a37ce07d3\"><br>b) <img decoding=\"async\" width=\"7\" height=\"26\" src=\"blob:https:\/\/mcqsadda.com\/3040e62a-2f38-45b6-a8d6-c98653d3e648\"><br>c) <img decoding=\"async\" width=\"7\" height=\"26\" src=\"blob:https:\/\/mcqsadda.com\/0f7c2020-9d1a-4430-b002-f72f25802d23\"><br>d) <img decoding=\"async\" width=\"9\" height=\"20\" src=\"blob:https:\/\/mcqsadda.com\/610b2fc8-0f29-4436-9010-1cb0283b6661\"><br><strong>Answer:<\/strong> a) <img decoding=\"async\" width=\"7\" height=\"26\" src=\"blob:https:\/\/mcqsadda.com\/28d71c6b-0af2-47cd-930e-aeca4c2c69ac\"><br><strong>Explanation:<\/strong> <img decoding=\"async\" width=\"101\" height=\"27\" src=\"blob:https:\/\/mcqsadda.com\/8573e42a-8b0b-4258-a016-3371a75bbfda\">.<\/p>\n\n\n\n<p class=\"has-large-font-size\"><strong><mark style=\"background-color:rgba(0, 0, 0, 0)\" class=\"has-inline-color has-luminous-vivid-orange-color\">93. A planet has twice the mass and radius of Earth. Its surface gravity is:<\/mark><\/strong><br>a) Twice Earth\u2019s gravity<br>b) Same as Earth\u2019s gravity<br>c) Half Earth\u2019s gravity<br>d) Four times Earth\u2019s gravity<br><strong>Answer:<\/strong> c) Half Earth\u2019s gravity<br><strong>Explanation:<\/strong> <img decoding=\"async\" width=\"152\" height=\"30\" src=\"blob:https:\/\/mcqsadda.com\/53967461-403e-434f-9530-aea74f0e87ca\">.<\/p>\n\n\n\n<p class=\"has-large-font-size\"><strong><mark style=\"background-color:rgba(0, 0, 0, 0)\" class=\"has-inline-color has-luminous-vivid-orange-color\">94. The gravitational force between two point masses is 9 N. If one mass is doubled and distance halved, the force is:<\/mark><\/strong><br>a) 18 N<br>b) 36 N<br>c) 72 N<br>d) 9 N<br><strong>Answer:<\/strong> c) 72 N<br><strong>Explanation:<\/strong> New force <img decoding=\"async\" width=\"290\" height=\"30\" src=\"blob:https:\/\/mcqsadda.com\/d6adba10-a6e2-44c5-8c37-3d2b10976ce6\">.<\/p>\n\n\n\n<p class=\"has-large-font-size\"><strong><mark style=\"background-color:rgba(0, 0, 0, 0)\" class=\"has-inline-color has-luminous-vivid-orange-color\">95. The shape of the Earth\u2019s orbit around the Sun is:<\/mark><\/strong><br>a) Perfect circle<br>b) Ellipse<br>c) Parabola<br>d) Hyperbola<br><strong>Answer:<\/strong> b) Ellipse<br><strong>Explanation:<\/strong> Kepler\u2019s first law states orbits are elliptical.<\/p>\n\n\n\n<p class=\"has-large-font-size\"><mark style=\"background-color:rgba(0, 0, 0, 0)\" class=\"has-inline-color has-luminous-vivid-orange-color\"><strong>96. The force of gravity between two masses is 10 N. If the distance between them is tripled, the force becomes:<\/strong><\/mark><br>a) 30 N<br>b) 3.33 N<br>c) 1.11 N<br>d) 0.11 N<br><strong>Answer:<\/strong> c) 1.11 N<br><strong>Explanation:<\/strong> <img decoding=\"async\" width=\"40\" height=\"27\" src=\"blob:https:\/\/mcqsadda.com\/9c40e1cd-6982-4a61-b9bc-8514cc325dc9\">, so <img decoding=\"async\" width=\"149\" height=\"28\" src=\"blob:https:\/\/mcqsadda.com\/d2d4f31c-e81d-43ff-9a87-f205f87be05f\">.<\/p>\n\n\n\n<p class=\"has-large-font-size\"><strong><mark style=\"background-color:rgba(0, 0, 0, 0)\" class=\"has-inline-color has-luminous-vivid-orange-color\">97. The unit of universal gravitational constant G is:<\/mark><\/strong><br>a) <img decoding=\"async\" width=\"65\" height=\"20\" src=\"blob:https:\/\/mcqsadda.com\/d032d5d0-0e04-4e2a-956d-52551ff19135\"><br>b) <img decoding=\"async\" width=\"48\" height=\"20\" src=\"blob:https:\/\/mcqsadda.com\/7c41b2f2-7849-4ac9-acea-c463ec8c75b5\"><br>c) <img decoding=\"async\" width=\"61\" height=\"20\" src=\"blob:https:\/\/mcqsadda.com\/193a1934-846a-4ed8-baa5-1046937c152e\"><br>d) <img decoding=\"async\" width=\"34\" height=\"20\" src=\"blob:https:\/\/mcqsadda.com\/45a7022a-0f4e-40ff-943f-9a1d866b20c2\"><br><strong>Answer:<\/strong> a) <img decoding=\"async\" width=\"65\" height=\"20\" src=\"blob:https:\/\/mcqsadda.com\/1f30866d-bd19-4205-9b66-6dfee309d3db\"><br><strong>Explanation:<\/strong> From <img decoding=\"async\" width=\"72\" height=\"26\" src=\"blob:https:\/\/mcqsadda.com\/8ffc8e3f-b3b7-433a-817e-86a886f004f7\">.<\/p>\n\n\n\n<p class=\"has-large-font-size\"><strong><mark style=\"background-color:rgba(0, 0, 0, 0)\" class=\"has-inline-color has-luminous-vivid-orange-color\">98. The orbital speed of a satellite depends on:<\/mark><\/strong><br>a) Its mass and orbital radius<br>b) Only orbital radius<br>c) Mass of planet and orbital radius<br>d) Mass of satellite only<br><strong>Answer:<\/strong> c) Mass of planet and orbital radius<br><strong>Explanation:<\/strong> <img decoding=\"async\" width=\"55\" height=\"38\" src=\"blob:https:\/\/mcqsadda.com\/7000b044-090f-41df-89a0-9d6a4d621007\">.<\/p>\n\n\n\n<p class=\"has-large-font-size\"><strong><mark style=\"background-color:rgba(0, 0, 0, 0)\" class=\"has-inline-color has-luminous-vivid-orange-color\">99. The total mechanical energy of a satellite in orbit is:<\/mark><\/strong><br>a) Zero<br>b) Equal to kinetic energy<br>c) Equal to potential energy<br>d) Negative and equal to half of potential energy<br><strong>Answer:<\/strong> d) Negative and equal to half of potential energy<br><strong>Explanation:<\/strong> <img decoding=\"async\" width=\"135\" height=\"27\" src=\"blob:https:\/\/mcqsadda.com\/6c394be7-dee8-4efa-b175-9c471e4a24c9\">.<\/p>\n\n\n\n<p class=\"has-large-font-size\"><strong><mark style=\"background-color:rgba(0, 0, 0, 0)\" class=\"has-inline-color has-luminous-vivid-orange-color\">100. The force of gravity between two point masses separated by a distance r is:<\/mark><\/strong><br>a) Directly proportional to r<br>b) Inversely proportional to r<br>c) Directly proportional to <img decoding=\"async\" width=\"14\" height=\"20\" src=\"blob:https:\/\/mcqsadda.com\/bf986d03-9513-48c3-b889-b12b93fb6ff3\"><br>d) Inversely proportional to <img decoding=\"async\" width=\"14\" height=\"20\" src=\"blob:https:\/\/mcqsadda.com\/4a231500-17bd-4bf7-8972-321401fb16ed\"><br><strong>Answer:<\/strong> d) Inversely proportional to <img decoding=\"async\" width=\"14\" height=\"20\" src=\"blob:https:\/\/mcqsadda.com\/63fe899f-604c-4fb7-b649-44c206d69cb4\"><br><strong>Explanation:<\/strong> Newton\u2019s law of gravitation.<\/p>\n","protected":false},"excerpt":{"rendered":"<p>1.Who proposed the universal law of gravitation?a) Albert Einsteinb) Isaac Newtonc) Galileo Galileid) Johannes KeplerAnswer: b) Isaac NewtonExplanation: Newton formulated the law of universal gravitation in 1687. 2. The universal law of gravitation states that the force between two masses is:a) Directly proportional to the sum of their massesb) Directly proportional to the product of<\/p>\n","protected":false},"author":1,"featured_media":0,"comment_status":"open","ping_status":"open","sticky":false,"template":"","format":"standard","meta":{"footnotes":""},"categories":[8],"tags":[15587,15589,15481,15487,15584,15593,15594,15586,15591,15582,15580,15465,15583,15579,15536,15479,15474,15467,15483,15472,15592,15456,15595,15478,15585,15469,15581,15590,15480,15588],"class_list":{"0":"post-12454","1":"post","2":"type-post","3":"status-publish","4":"format-standard","6":"category-physics","7":"tag-acceleration-due-to-gravity","8":"tag-center-of-mass","9":"tag-competitive-exam-physics","10":"tag-free-fall","11":"tag-gravitation-in-physics","12":"tag-gravitation-problems","13":"tag-gravitational-concepts","14":"tag-gravitational-force","15":"tag-gravitational-potential-energy","16":"tag-gravity-on-earth","17":"tag-keplers-laws","18":"tag-mcqs-for-physics-exam","19":"tag-newtons-law-of-gravitation","20":"tag-orbital-motion","21":"tag-physics-formulas","22":"tag-physics-learning","23":"tag-physics-mcqs","24":"tag-physics-preparation-material","25":"tag-physics-questions-and-answers","26":"tag-physics-quiz","27":"tag-physics-revision","28":"tag-physics-study-material","29":"tag-planetary-motion","30":"tag-psc-physics-mcqs","31":"tag-satellites","32":"tag-ssc-physics-mcqs","33":"tag-universal-gravitation","34":"tag-universal-law-of-gravitation","35":"tag-upsc-physics-mcqs","36":"tag-weight-and-mass"},"_links":{"self":[{"href":"https:\/\/mcqsadda.com\/index.php\/wp-json\/wp\/v2\/posts\/12454","targetHints":{"allow":["GET"]}}],"collection":[{"href":"https:\/\/mcqsadda.com\/index.php\/wp-json\/wp\/v2\/posts"}],"about":[{"href":"https:\/\/mcqsadda.com\/index.php\/wp-json\/wp\/v2\/types\/post"}],"author":[{"embeddable":true,"href":"https:\/\/mcqsadda.com\/index.php\/wp-json\/wp\/v2\/users\/1"}],"replies":[{"embeddable":true,"href":"https:\/\/mcqsadda.com\/index.php\/wp-json\/wp\/v2\/comments?post=12454"}],"version-history":[{"count":4,"href":"https:\/\/mcqsadda.com\/index.php\/wp-json\/wp\/v2\/posts\/12454\/revisions"}],"predecessor-version":[{"id":15048,"href":"https:\/\/mcqsadda.com\/index.php\/wp-json\/wp\/v2\/posts\/12454\/revisions\/15048"}],"wp:attachment":[{"href":"https:\/\/mcqsadda.com\/index.php\/wp-json\/wp\/v2\/media?parent=12454"}],"wp:term":[{"taxonomy":"category","embeddable":true,"href":"https:\/\/mcqsadda.com\/index.php\/wp-json\/wp\/v2\/categories?post=12454"},{"taxonomy":"post_tag","embeddable":true,"href":"https:\/\/mcqsadda.com\/index.php\/wp-json\/wp\/v2\/tags?post=12454"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}