Second Cosmic Velocity Calculator

Enter the mass and the distance from the center. You get the minimum escape speed. Earth at r = 6371 km is 11.19 km/s, which is v₁√2 at v₁ = 7.91 km/s.

Circular orbit: first cosmic velocity (v₂ = v₁√2). Field: g = GM/r². Circular path: a = v²/r. Force: F = GMm/r².

Inputs

Result

Constant G (N·m²/kg², optional), Mass M (kg) and Distance r (m). The result shows up here.

How it works

v₂ v₂ = √(2GM / r) = v₁√2
Escape speed: the path becomes a hyperbola and the body leaves the gravity well.

Second cosmic velocity is the threshold where mechanical energy stops being negative. From ½mv² − GMm/r ≥ 0 you get v₂ = √(2GM/r). That is exactly v₁√2, because v₁ = √(GM/r). √2 ≈ 1.414, so escape is 41% faster than the circle.

At Earth’s surface, the same M and r as for v₁: 5.972×10²⁴ kg and 6.371×10⁶ m. 2GM/r = 1.251×10⁸, the square root is 11186 m/s, or 11.19 km/s. School 11.2 km/s is a rounding. The path at exactly v₂ is a parabola.

Higher up the threshold falls. On LEO r = 6.771×10⁶ m, v₂ ≈ 10.85 km/s. At geosynchronous r ≈ 4.216×10⁷ m you get about 4.35 km/s. A launch from Earth still has to climb through the atmosphere and the well on the way.

Projectile mass cancels. The formula skips direction: it gives a magnitude. A real launch uses Earth’s rotation and avoids thick air. Below v₂ the body comes back on an ellipse or falls, unless it has thrust.

M and r must be positive. Empty G = 6.67430×10⁻¹¹. The result note reminds you that v₂ = v₁√2 and also prints v₁ for the same inputs. The result is in m/s.

Moon at the surface: v₂ ≈ 2.38 km/s. Mars about 5.03 km/s. From the Sun-Earth scale (r = 1 au) solar escape is around 42 km/s. The circular speed v₁ is a separate page.

How to use

  1. Leave G empty, or type the constant from the problem.
  2. Type M in kilograms, for example 5.972e24.
  3. Type r from the center in meters, for example 6371000.
  4. Click Calculate. Earth and 6371 km give 11.19 km/s. Check that this is 7.91 × √2.
  5. The circle itself is next door as v₁ = √(GM/r). Here you stay with escape.

Formula

v2 = √(2GM / r)

Link to circular orbit: v2 = v1√2 with v1 = √(GM/r).

Letters in v₂ = √(2GM/r)

Escape threshold: v₂ = √(2GM/r) = v₁√2. The same M and r that gave 7.91 km/s now give 11.19 km/s, school 11.2.

v₂
Minimum escape speed. 2GM/r = 1.251×10⁸, square root 11186 m/s, or 11.19 km/s.
G
Again 6.67430×10⁻¹¹ if you leave it blank. The 2 under the root is what separates v₂ from circular v₁.
M
Mass 5.972×10²⁴ kg. √2 ≈ 1.414, so escape is 41% faster than 7.91 km/s.
r
Distance from the center, 6.371×10⁶ m at the surface. That is the escape start, not the ISS radius with v₁ = 7.67 km/s.

Real-life examples

Example 1

v₂ ≈ 11.2 km/s.

Example 2

r ≈ 6771000 m.

Example 3

M ≈ 7.35e+22 kg, r ≈ 1737000 m.

Example 4

M ≈ 6.39e+23 kg, r ≈ 3390000 m.

Example 5

r = 12742000 m.

Example 6

r ≈ 42164000 m.

Example 7

escape from the Sun-Earth system (scale).

Example 8

M ≈ 1.9e+27 kg, r ≈ 69911000 m.

Example 9

G = 6.67e-11, Earth surface.

Example 10

r = 6800000 m.

Ways to use this calculator

  • A quick v₂ for Earth and other bodies.
  • A check of v₂ = v₁√2 on the same M and r.

Frequently asked questions

How much v₂ for Earth at r = 6371 km?

11186 m/s, or 11.19 km/s. School work often writes 11.2 km/s.

Why is v₂ = v₁√2?

Because v₁² = GM/r and v₂² = 2GM/r. The ratio is √2 ≈ 1.414. From 7.91 km/s you get 11.19 km/s.

How is escape different from orbit?

v₁ holds a circle (negative energy). v₂ lets you leave to infinity (zero energy). Above v₂ the path is a hyperbola.

Does v₂ depend on projectile mass?

No. The test mass cancels, as it does for v₁ and for g.

How much v₂ on LEO, r = 6771 km?

About 10.85 km/s. The farther you start, the lower the threshold.

Does direction matter?

The formula gives a magnitude. A real launch uses Earth’s rotation and the atmosphere.

What v₂ does the Moon have?

About 2.38 km/s at r ≈ 1737 km. Mars at the surface is about 5.03 km/s.

What path do you get at exactly v₂?

A parabola, zero energy. Above: hyperbola. Below: a bound orbit or a fall.

Can I change G?

Yes. Type G or leave it empty for 6.67430×10⁻¹¹. Escape speed still uses √(2GM/r).

Where do I compute the circle itself?

On the first cosmic velocity page. Same M and r, no 2 under the square root.

Knowledge sources

The formula is the school one. Units follow SI; NIST SP 330 and BIPM define the measures, not your result.

Page updated in 2026.