Tidal Force Calculator
Calculate the tidal force exerted by a massive body. Enter the masses, radius, and distance between centers.
Tidal Force Calculator
Results
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.
- Example 1: Moon's tidal force on Earth:
Analyze tidal effects with this interactive calculator. Share or embed it on your site!