المechanics of the Solar System
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Questions and Answers

ما هو شكل مدار الكواكب ตามاً لكيبلر؟

  • مدارات بيضوية (correct)
  • مدارات دائرية
  • مدارات ثلاثية الأبعاد
  • مدارات مربع الشكل
  • ما هي قوة الجذب التي تربط بين الكواكب والشمس؟

  • قوة تكرارية
  • قوة جاذبية (correct)
  • قوة طاردة
  • قوة كهرومغناطيسية
  • ما هو القانون الذي)yربط بين فترة دوران الكوكب ومداره؟

  • قانون مدار الرنين (correct)
  • قانون التوافق
  • قانون المحاور المماثلة
  • قانون التوازن
  • ما هو معادلة قوة الجذب؟

    <p>F = G × (m1 × m2) / r</p> Signup and view all the answers

    ما هو مجال الجذب؟

    <p>مجال الجذب هو منطقة حول جسم متراكز حيث يمكنك الشعور بقوة الجذب</p> Signup and view all the answers

    ما هو علاقة قوة الجذب bìnhاً بالمسافة بين الكتلين؟

    <p>قوة الجذب تقل مع زيادة المسافة بين الكتلين</p> Signup and view all the answers

    Study Notes

    Motion of Planets and Gravity

    Kepler's Laws of Planetary Motion

    • Law of Elliptical Orbits: Planets orbit the sun in elliptical paths, with the sun at one of the focal points.
    • Law of Equal Areas: The line connecting the planet to the sun sweeps out equal areas in equal times.
    • Law of Harmonies: The square of a planet's orbital period is proportional to the cube of its semi-major axis.

    Newton's Law of Universal Gravitation

    • Gravity: A force of attraction between two objects, proportional to the product of their masses and inversely proportional to the square of the distance between them.
    • Universal Gravitation: Gravity is a universal force, affecting all objects with mass, from the falling of objects on Earth to the motion of planets in our solar system.

    Gravitational Force

    • Gravitational Force Equation: F = G * (m1 * m2) / r^2, where G is the gravitational constant, m1 and m2 are the masses, and r is the distance between them.
    • Gravity and Orbital Motion: Gravity is the force that keeps planets in orbit around the sun, and moons in orbit around their parent planets.

    Gravitational Fields

    • Gravitational Field: A region around a massive object where the gravitational force can be detected.
    • Gravitational Field Strength: The strength of the gravitational field depends on the mass of the object and the distance from the object.

    Escape Velocity

    • Escape Velocity: The minimum speed an object needs to escape the gravitational pull of a planet or moon.
    • Escape Velocity Equation: v = √(2 * G * M / r), where G is the gravitational constant, M is the mass of the planet or moon, and r is the radius of the planet or moon.

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    Description

    etest your understanding of the motion of planets and gravity, including Kepler's laws, Newton's law of universal gravitation, gravitational force, gravitational fields, and escape velocity.

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