Kepler's 3 Planetary Laws
1. Elliptical orbits with Sun at focus. 2. Equal areas in equal time (areal velocity dA/dt = L/2m = constant). 3. T² ∝ a³.
Grade 11th · Physics · Gravitation
Complete formula reference, variable dimensions, numerical step-by-step problem-solving templates, and sample calculations. covering Gravitation, Kepler's Laws & Escape Velocity (Advanced Competitive & Board Prep) for Class 11th Physics.
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1. Elliptical orbits with Sun at focus. 2. Equal areas in equal time (areal velocity dA/dt = L/2m = constant). 3. T² ∝ a³.
Escape velocity ve = √(2GM/R) is minimum launch speed to break free from gravitational field without further propulsion.
Detailed educational reference for Gravitation, Kepler's Laws & Escape Velocity (Advanced Competitive & Board Prep). Designed for Class 11th students preparing for board exams and competitive entrance tests.
Always state the governing principle or formula first, write given values with standard SI units, substitute clearly, and highlight the final numerical answer with units in a box for full step marking.
Watch for unit prefixes (cm to m, minutes to seconds, g to kg, degrees to radians). In coordinate and ray optics problems, double-check Cartesian sign conventions before computing.
Test your understanding and perform instant calculations with these free online utilities.
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Orbital period T = 24 hours, parked at ~35,786 km above equator, orbiting West to East.