The Formula
- G: Gravitational Constant
- M: Mass of Central Body
- r: Distance from center
Orbital Speed - Perform scientific calculations with precision and accuracy.
Orbital speed is the speed at which an object revolves around the barycenter of a system, usually a massive central body. It is the speed required for an object to maintain a stable orbit, balancing the gravitational pull of the central body with the object's inertia.
Understanding orbital speed is fundamental to space exploration, satellite deployment, and celestial mechanics. It explains why satellites stay in orbit without falling back to Earth and how planets maintain their paths around stars.
Our Orbital Speed Calculator helps you determine the orbital speed of a satellite or planet given the mass of the central body and the orbital radius. This tool is invaluable for students, astronomers, and aerospace engineers.
The mass of the larger object around which another object is orbiting (e.g., Earth, Sun).
The distance from the center of the central body to the orbiting object. For circular orbits, this is constant.
A fundamental physical constant that quantifies the strength of gravitational attraction between masses.
Typically measured in meters per second (m/s) or kilometers per second (km/s).
The user enters the mass of the central body (e.g., Earth, Sun).
The user enters the distance from the center of the central body to the orbiting object.
The calculator applies the formula: v_orbital = √(GM/r), where 'G' is the gravitational constant, 'M' is the mass of the central body, and 'r' is the orbital radius.
Satellites in LEO (e.g., ISS) orbit at high speeds (approx. 7.8 km/s) and complete an orbit in about 90 minutes.
Satellites in GEO orbit at a specific altitude (approx. 35,786 km) and speed (approx. 3.07 km/s) to match Earth's rotation.
The speed required to completely break free from a celestial body's gravitational pull, higher than orbital speed.
Orbital speed is not constant in elliptical orbits; it is faster when closer to the central body and slower when farther away.
Orbital speed is the scalar magnitude of how fast an object is moving in orbit. Orbital velocity is a vector quantity that includes both the speed and the direction of the object's motion in orbit.
No, for a given central body and orbital radius, the orbital speed is independent of the mass of the orbiting object. This is why a small satellite and a large space station can orbit at the same speed at the same altitude.
Objects in lower orbits are closer to the central body, experiencing a stronger gravitational pull. To maintain a stable orbit and prevent falling, they must move faster to generate the necessary centrifugal force to balance gravity.
No. This calculator is a tool to assist with calculations. A solid understanding of the underlying principles of gravity, celestial mechanics, and orbital dynamics is essential for correctly applying the concepts of orbital speed and interpreting the results.
Use our Orbital Speed Calculator to quickly and accurately determine the speed required for stable orbits around celestial bodies.
Master the dynamics of space travel.
Follow these steps to get accurate results with the orbital speed.
Fill in the required input fields above. Units can be changed where available.
Press the calculate button to compute results instantly in your browser.
View the computed outputs and use related calculators for deeper analysis.
Explore these related calculators to help you make informed decisions:
Acceleration - Perform scientific calculations with precision and accuracy.
Angular Acceleration - Perform scientific calculations with precision and accuracy.
Angular Impulse - Perform scientific calculations with precision and accuracy.
Angular Impulse Momentum - Perform scientific calculations with precision and accuracy.
Angular Momentum - Perform scientific calculations with precision and accuracy.
Angular Velocity - Perform scientific calculations with precision and accuracy.
Calculate your Body Mass Index
Estimate monthly mortgage payments
Calculate percentages easily
Calculate loan payments and interest
Calculate daily calorie needs
Calculate compound interest growth
Calculate the velocity required to maintain a stable circular orbit around Planets or Stars.
Orbital velocity is the speed an object must travel to maintain a stable orbit around a massive body. It balances the object's inertia (which wants to fly off straight) with the gravitational pull (which pulls it inward).
The orbital speed does not depend on the mass of the satellite (as long as the satellite is much smaller than the central body).
This is why a tiny satellite and the massive ISS orbit Earth at roughly the same speed at the same altitude!