Tidal Force Calculator

Calculate the tidal force exerted by a massive body. Enter the masses, radius, and distance between centers.

Tidal Force Calculator

Please enter valid positive numbers for all parameters.

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About the Tidal Force Calculator

The Tidal Force Calculator computes the differential gravitational force exerted by a massive body on another body, causing tidal effects. This tool is designed for astronomers, astrophysicists, and students studying celestial mechanics.

Tidal Force: The gravitational force difference across a body due to a nearby massive object, responsible for phenomena like ocean tides, tidal heating, and Roche limit disruptions.

Use this calculator to determine the tidal force for a given system of celestial bodies.

  • Features:
    • Calculates tidal force (\( F_t \)).
    • Inputs include masses (\( M \), \( m \)), radius (\( r \)), and distance (\( d \)).
    • Keypad includes digits (0–9) and decimal point (.).
    • Displays step-by-step calculations in LaTeX format.
    • Clear and backspace functionality, with a "Copy" button for results.
    • Uses MathJax for professional rendering of mathematical expressions.
  • Practical Applications: Useful in studying tidal interactions, satellite stability, and planetary geology.
  • How to Use:
    • Enter mass of the massive body (\( M \), in Solar masses).
    • Enter mass of the affected body (\( m \), in Earth masses).
    • Enter radius of the affected body (\( r \), in kilometers).
    • Enter distance between centers (\( d \), in AU).
    • Use the keypad to input digits and decimal points.
    • Click "Calculate" to compute the tidal force.
    • Use "Clear" to reset or "⌫" to delete the last character.
    • Use "Copy" to copy the results and steps.
    • Share or embed the calculator using the action buttons.
  • Helpful Tips:
    • All inputs must be positive numbers.
    • Typical values: \( M \) (0.1–2 Solar masses), \( m \) (0.001–100 Earth masses), \( r \) (1000–10000 km), \( d \) (0.001–100 AU).
    • Earth mass ≈ 5.972 × 10²⁴ kg, Solar mass ≈ 1.989 × 10³⁰ kg, 1 AU ≈ 1.496 × 10⁸ km.
    • The formula assumes point masses; for extended bodies, results are approximate.
    • Ensure \( d \) is greater than the sum of the bodies' radii to avoid overlap.
  • Examples:
    • Example 1: Moon's tidal force on Earth:
      • Inputs: \( M = 0.0000123 \) Solar masses (Moon), \( m = 1.0 \) Earth mass, \( r = 6371 \) km, \( d = 0.00257 \) AU
      • Steps:
        • Convert units: \( M = 7.342 × 10^{22} \) kg, \( m = 5.972 × 10^{24} \) kg, \( d = 3.844 × 10^5 \) km
        • Numerator: \( 2 G M m r \)
        • Denominator: \( d^3 \)
        • Tidal force: \( F_t = \\frac{2 G M m r}{d^3} \)
      • Result: \( F_t \approx 1.1 × 10^{17} \) N
    • Example 2: Sun's tidal force on Earth:
      • Inputs: \( M = 1.0 \) Solar mass, \( m = 1.0 \) Earth mass, \( r = 6371 \) km, \( d = 1.0 \) AU
      • Steps: Similar calculations.
      • Result: Computed tidal force.

Analyze tidal effects with this interactive calculator. Share or embed it on your site!

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