14 Questions
सर आइसक न्यूटन ने कौन-कौन से गुण का वर्णन किया?
द्रव्यमान
गुरुत्वाकर्षण के किस नियम में आपसी प्रोपोर्शनलिटी का उल्लेख है?
न्यूटन का पहला नियम
सूर्य से पृथ्वी की दूरी का वर्गक मुकाबला कैसे होता है?
प्रतिकूल
केपलर के प्राणी मोशन के नियमों से संबंधित, सभी ग्रहों की मांसपेशी सक्रियता परिभाषित होती है:
तीसरा नियम
केप्लर का दूसरा नियम क्या कहता है?
प्लानेट की गति पर समय का प्रति समय कितना प्रतिशत प्रतिबिम्बित होता है
कौनसा केप्लर का पहला नियम है?
सूरज के आसपास ग्रह गोलाकार मार्ग में प्रदक्षिण चलते हैं
केप्लर का तीसरा नियम क्या कहता है?
प्लानेट के औसत आकारिक दूरी का वर्ग
कौनसे महा-शास्रीय समझौतों ने हमारे संचार के समझने का मूल होने का मुकाम प्रदान किया?
केप्लर के 3rd and Newton's Law of Universal Gravitation
किस नियम के अनुसार दो वस्तुओं के बीच गुरुत्वाकर्षण शक्ति को न्यूटन का एक सामान्य नियम प्रदान करता है?
ग्रेविटेशनल फ़ोर्स
गुरुत्वाकर्षणीय क्षेत्र की परिभाषा के अनुसार, गुरुत्व कौन से शक्तियों पर प्रभुत्वित होता है?
नाभिकीय-संबंधी शक्तियों
किस मापनीकी देने से पता किया जा सकता है कि किसी पदार्थ का गुरुत्वाकर्षण क्षेत्र में कैसा व्यवहार होगा?
संपीड़क
गुरुत्वाकर्षणीय पोटेंशल ऊर्जा का मान किससे प्राप्त किया जा सकता है?
समीकरण
किसे 'सूर्यकों पर संप्रेषित' के नियमों की 'कीपलेर' ने खोजा?
महान ग्रह
'$$F = G rac{m_1m_2}{r^2}$$' में, $$G$$ को क्या कहा है?
$$F$$
Study Notes
Physics of Gravitation
Gravitation is a fundamental force in physics that attracts objects towards each other. It plays a crucial role in understanding the motion of celestial bodies, such as planets and moons, as well as the behavior of objects on Earth. In this article, we will explore the key concepts related to gravitation, including Newton's law of universal gravitation, gravitational force, gravitational field, gravitational potential energy, and Kepler's laws of planetary motion.
Newton's Law of Universal Gravitation
Newton's law of universal gravitation, introduced by Sir Isaac Newton, states that every particle attracts every other particle in the universe with a force that is proportional to the product of their masses and inversely proportional to the square of the distance separating them. Mathematically, this is represented as:
$$F = G \frac{m_1m_2}{r^2}$$
where:
- $$F$$ is the gravitational force acting between two objects
- $$G$$ is the gravitational constant, approximately equal to $$6.67 \times 10^{-11} , \text{N \cdot m}^2/\text{kg}^2$$
- $$m_1$$ and $$m_2$$ are the masses of the objects
- $$r$$ is the distance between the centers of their masses
Gravitational Force
Gravitational force is the force that attracts objects towards each other due to gravity. It is a result of the gravitational interaction between two objects, which cannot be observed directly. The gravitational force between two objects can be calculated using Newton's law of universal gravitation, as mentioned above.
Gravitational Field
A gravitational field is the region in space where gravity dominates over other forces, such as electromagnetic forces. The gravitational field is a fundamental aspect of the physics of gravitation, as it determines the behavior of objects in its vicinity. The gravitational force in a gravitational field can be determined by calculating the gravitational potential energy of an object in the field.
Gravitational Potential Energy
Gravitational potential energy is the energy stored in an object due to its gravitational interaction with other objects. It is a measure of the work required to move an object from a gravitational field to an area devoid of gravity. The gravitational potential energy can be calculated using the gravitational force and the distance between the objects.
Kepler's Laws of Planetary Motion
Kepler's laws of planetary motion, discovered by Johannes Kepler, describe the orbits of planets around the Sun. These laws provide a simple mathematical description of the orbital motions of celestial bodies and are a fundamental aspect of astrophysics. The three main laws of Kepler are:
- Kepler's First Law: All planets orbit the Sun in elliptical orbits, with the Sun at one focus of the ellipse.
- Kepler's Second Law: The orbital period of a planet is proportional to the square of its average orbital distance from the Sun.
- Kepler's Third Law: The square of the period of revolution of any planet is proportional to the cube of its average orbital distance from the Sun.
These laws, along with Newton's law of universal gravitation, form the foundation of our understanding of the motion of celestial bodies and the forces that govern their interactions. By studying gravitation and its effects on the motion of objects in space, scientists have been able to make accurate predictions about the behavior of planets, moons, and other celestial bodies, as well as the orbits of spacecraft and other man-made objects in space.
Explore the fundamental concepts of gravitation in physics, including Newton's law of universal gravitation, gravitational force, gravitational field, gravitational potential energy, and Kepler's laws of planetary motion. Understand the principles governing the attraction of celestial bodies, the calculation of gravitational force, and the behavior of objects in gravitational fields.
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