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  • Calculating the Sun's Mass: A Gravitational Physics Exercise
    Here's how to calculate the mass of the Sun using the orbital data of Earth and compare it to the actual value.

    Understanding the Concepts

    * Newton's Law of Universal Gravitation: This law states that every particle of matter in the universe attracts every other particle with a force that is proportional to the product of their masses and inversely proportional to the square of the distance between their centers. Mathematically:

    F = G * (m1 * m2) / r^2

    Where:

    * F is the force of gravity

    * G is the gravitational constant (6.674 x 10^-11 m^3 kg^-1 s^-2)

    * m1 and m2 are the masses of the two objects

    * r is the distance between their centers

    * Centripetal Force: An object moving in a circular path experiences a force towards the center of the circle. This force is called the centripetal force. It's given by:

    Fc = (m * v^2) / r

    Where:

    * m is the mass of the object

    * v is the orbital velocity of the object

    * r is the radius of the orbit

    * Orbital Period: The time it takes an object to complete one orbit around another object.

    Calculations

    1. Earth's Orbital Data:

    * Orbital radius (r): 1.496 x 10^11 m (average distance between Earth and Sun)

    * Orbital period (T): 365.25 days = 3.156 x 10^7 seconds

    2. Earth's Orbital Velocity:

    * v = 2πr / T

    * v = 2 * π * (1.496 x 10^11 m) / (3.156 x 10^7 s)

    * v ≈ 29,783 m/s

    3. Equating Forces:

    * The force of gravity between the Sun and Earth is what keeps Earth in its orbit. Therefore, the gravitational force (F) equals the centripetal force (Fc).

    * G * (M_sun * m_earth) / r^2 = (m_earth * v^2) / r

    4. Solving for the Sun's Mass (M_sun):

    * M_sun = (v^2 * r) / G

    * M_sun = ((29,783 m/s)^2 * 1.496 x 10^11 m) / (6.674 x 10^-11 m^3 kg^-1 s^-2)

    * M_sun ≈ 1.989 x 10^30 kg

    Comparison to Actual Mass

    The actual mass of the Sun is approximately 1.989 x 10^30 kg.

    Result:

    The mass of the Sun calculated using Earth's orbital data is remarkably close to the actual value. This validates Newton's law of universal gravitation and highlights its importance in understanding celestial mechanics.

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