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Habitable zone and planet temperature calculator

Estimate the inner and outer edges of a star's habitable zone from its luminosity, or its radius and temperature, and the equilibrium temperature of a planet at a given distance.

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Star described by

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Results

Inner edge of the habitable zone

0.953 AU

Outer edge of the habitable zone

1.374 AU

Planet's equilibrium temperature
-18 °C
Inside the habitable zone
Equilibrium temperature in °F
-1 °F
Star luminosity (Sun = 1)
1

The habitable zone

The habitable zone, sometimes called the “Goldilocks zone”, is the range of distances from a star where a rocky planet with an Earth-like atmosphere could keep liquid water on its surface. Too close, water boils away in a runaway greenhouse; too far, it freezes.

How it is estimated

The boundaries scale with the square root of the star’s luminosity L (in units of the Sun’s):

  • inner edge ≈ √(L ÷ 1.1) AU;
  • outer edge ≈ √(L ÷ 0.53) AU.

These are conservative limits, close to those of Kasting and Kopparapu’s climate models. More optimistic limits, based on early Venus and early Mars, stretch the zone to roughly 0.75 to 1.8 AU for the Sun.

If you know the star’s radius R and temperature T instead, its luminosity is L = R² × (T ÷ 5,772 K)⁴.

Example: the Sun

For L = 1:

  • inner edge ≈ 0.95 AU;
  • outer edge ≈ 1.37 AU.

Earth, at 1 AU, sits inside. Venus (0.72 AU) is too close and Mars (1.52 AU) just outside the conservative zone.

Equilibrium temperature

A planet’s equilibrium temperature, the temperature it would have without a greenhouse effect, is:

T_eq ≈ 278.6 K × L^(1/4) ÷ √d × (1 − albedo)^(1/4)

For Earth, with an albedo of 0.3, T_eq ≈ 255 K, about −18 °C (−1 °F). The actual average surface temperature, about 15 °C (59 °F), is higher thanks to the greenhouse effect.

Other stars

Star type Luminosity Habitable zone
Red dwarf (M) such as Proxima Centauri 0.0016 about 0.04 to 0.05 AU
Orange dwarf (K) 0.3 about 0.5 to 0.75 AU
Sun (G2) 1 about 0.95 to 1.37 AU
Hotter F star 3 about 1.6 to 2.4 AU

Planets in the habitable zones of red dwarfs orbit so close that they are likely tidally locked and exposed to strong flares, which may make them less hospitable than the simple distance suggests.

Beyond the habitable zone

Habitable zone status is only a first filter. A planet’s mass, atmosphere, magnetic field, water content and the star’s activity all matter. Ocean worlds under ice, like Jupiter’s moon Europa, show that liquid water can also exist far outside the classic zone.

Frequently asked questions

What is the habitable zone?

It is the range of distances from a star where a rocky planet with a suitable atmosphere could keep liquid water on its surface.

How does star luminosity set the boundaries?

The flux falls with the square of distance, so the zone edges scale with the square root of luminosity. A star 4 times brighter pushes the zone 2 times farther out.

What is the equilibrium temperature?

It is the temperature a planet would have from starlight alone, given its albedo, with no greenhouse effect. Earth's is about −18 °C, while its real average is about 15 °C.

Are the limits exact?

No. The inner and outer edges depend on climate models and on the planet's atmosphere. The calculator uses flux limits of 1.1 and 0.53 times Earth's, close to the classic Kasting estimates; newer models such as Kopparapu's put the outer edge farther out.

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Results are estimates provided for information purposes. They do not replace professional advice.