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Orbital and escape speeds

The second speed is √2 times the first.

How it is calculated

The radius used is a mean radius, and the atmosphere does not drag. A real orbit sits above the surface, so circular speed there is lower.

v1 = √(GM / R), v2 = v1 × √2

Where the numbers come from

  • Body

Example

Earth's first cosmic speed is about 7,91 km/s.

Questions

Why not exactly 7,9?

It depends on the GM and radius that are used. Here Earth’s GM is 3,986004418×10¹⁴ m³/s² and the radius is 6 371 km.

A satellite in a 400 km orbit?

This screen’s formula will not take the larger radius for you: R is built into the body.

The Sun?

It is not on the list. Weight on the planets has its own calculator. These are different tasks.