Distance to Horizon Calculator

Calculate how far you can see to the horizon from any height above Earth or other celestial bodies

Calculate Distance to Horizon

Height of the observer above the surface

Select the celestial body or use custom radius

Distance to Horizon Results

4.72
Kilometers
2.93
Miles
4722
Meters
2.55
Nautical Miles

Formula used: d = √((r + h)² - r²)

Celestial body: Earth (radius: 6371 km)

Observer height: 1.75 m above surface

Horizon Analysis

On Earth, from a height of 1.75 m, you can see 4.72 km to the horizon.
To see 10 km to the horizon on Earth, you would need to be 357099.6 m high.
To see 50 km to the horizon on Earth, you would need to be 799.75 km high.

Example Calculation

Person on Earth's Surface

Observer height: 1.75 m (average human height)

Earth's radius: 6,371,008 m

Distance to horizon: √((6,371,008 + 1.75)² - 6,371,008²)

Result: 4.72 km

Calculation Steps

1. Add radius and height: r + h = 6,371,008 + 1.75 = 6,371,009.75 m

2. Square both terms: (r + h)² = 40,589,648,319,550.06 m²

3. Square radius: r² = 40,589,734,320,064 m²

4. Subtract and take square root: √(40,589,648,319,550.06 - 40,589,734,320,064) = 4,722 m

Final result: 4.72 km

Celestial Body Radii

Earth:6,371 km
Moon:1,738 km
Mars:3,390 km
Jupiter:69,911 km
Saturn:58,232 km
Venus:6,052 km

Horizon Physics Facts

The horizon is closer on smaller celestial bodies

Height increases horizon distance exponentially

Formula assumes perfect sphere and no obstacles

Atmospheric refraction can extend visible horizon

Based on Pythagorean theorem geometry

Understanding Distance to Horizon

What is the Horizon?

The horizon is the apparent division between the sky and the ground as viewed from an observer near the surface of a spherical celestial body. It represents the farthest point you can see before the curvature of the planet blocks your view.

Why Calculate Horizon Distance?

  • Navigation and maritime applications
  • Astronomy and planetary observations
  • Understanding Earth's curvature
  • Aviation and radar applications

Formula Explanation

d = √((r + h)² - r²)

  • d: Distance to horizon (meters)
  • r: Radius of celestial body (meters)
  • h: Height of observer above surface (meters)

Geometric Principle: The formula derives from the Pythagorean theorem applied to a right triangle formed by the center of the sphere, the observer's position, and the horizon point.

Key Factors Affecting Horizon Distance

Observer Height

Higher observation points dramatically increase horizon distance. Doubling height increases horizon distance by approximately √2 (1.41 times).

Planetary Size

Larger planets have more distant horizons. Jupiter's horizon is about 3× farther than Earth's for the same observer height.

Atmospheric Effects

Real-world factors like atmospheric refraction can extend the visible horizon beyond the geometric calculation by about 6%.