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Escape Velocity & Orbital Speed Calculator

Escape velocity is the minimum speed an unpropelled ballistic body must attain to permanently break free from a gravitational field.

Mass of the celestial body (Earth: 5.972e24 kg, Moon: 7.342e22 kg).

Distance from the center of mass in meters.

Calculated Result
11.19 km/s

Escape Velocity (v_esc)

Escape Velocity

11.19 km/s

Circular Orbital Speed

7.91 km/s

Escape Speed (mph)

25,022 mph

Local Gravity

9.82 m/s²

Calculation Breakdown

  1. Parabolic Escape Velocity Equationv_esc = √((2 × G × M) / r) = 11,186.0 m/s (40.27 km/s)vesc=2GMrv_{\text{esc}} = \sqrt{\frac{2GM}{r}}
  2. Circular Orbital Speed (First Cosmic Velocity)v_orb = 7,909.7 m/s (7.91 km/s)vorb=GMr=vesc2v_{\text{orb}} = \sqrt{\frac{GM}{r}} = \frac{v_{\text{esc}}}{\sqrt{2}}
  3. Local Gravitational Field Strengthg = 9.82 m/s² (1.00 g Earth equivalent)g=GMr2g = \frac{GM}{r^2}

Escape Velocities of Solar System Bodies (km/s)

Interactive visualization based on your current inputs

Velocity (km/s)
0.015304560MoonMarsVenusEarthJupiterCelestial BodyEscape Velocity (km/s)

What Is the Escape Velocity & Orbital Speed Calculator?

Escape velocity represents the speed at which kinetic energy equals the negative gravitational potential energy of a central mass.

How Does the Escape Velocity & Orbital Speed Calculator Work?

As a projectile flies outward, gravity continually decelerates it. At escape velocity, its speed approaches zero as distance approaches infinity.

Escape Velocity & Orbital Speed Calculator Formula & Variables

The core mathematical equation utilized by this calculator is expressed as:

v_{\text{esc}} = \sqrt{\frac{2GM}{r}}, \quad v_{\text{orb}} = \sqrt{\frac{GM}{r}}

Equating kinetic energy to gravitational potential energy reveals that escape velocity is exactly √2 (≈1.414) times circular orbital speed.

How to Use the Escape Velocity & Orbital Speed Calculator

  1. Enter the mass of the planet or star in kilograms.
  2. Enter the radius from the gravitational center in meters.

Step-by-Step Example Calculation

Earth Surface Escape Speed

Input Values:

mass:5.972e24
radius:6.371e6
Worked Steps: From Earth surface, circular orbital speed is ~7.91 km/s (First Cosmic Velocity) and escape speed is ~11.18 km/s (Second Cosmic Velocity).

Understanding Your Result

Escape Velocity: Required parabolic speed to reach interstellar space without extra propulsion.

Orbital Speed: Steady speed required to maintain a stable circular orbit at this radius.

Factors That Affect the Result

  • Planetary Mass: Denser, more massive bodies have dramatically higher escape velocities.
  • Orbital Altitude: Escape velocity decreases as altitude increases (1/√r).

When Should You Use This Calculator?

  • Rocket delta-v budget planning, interplanetary trajectory analysis, and planetary science.

Assumptions & Limitations

  • Neglects atmospheric drag (which necessitates higher initial launch speeds in real rocketry).

Frequently Asked Questions

Calculation Accuracy & Reference Note

Standard two-body Newtonian orbital mechanics formulation.

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