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Horizon Distance Calculator — Distance to the Horizon

Determine how far away the horizon is based on observer eye altitude above sea level. Accounts for standard terrestrial atmospheric refraction (k = 0.17) and Earth curvature.

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Horizon Calculation
Exact Geodetic· Calculated coordinates

Horizon Distance: 3.14 Miles (5.06 km)

Observer eye level: 5.7 feet · Dip angle: 2.5 arcmin · Refraction-adjusted (k=0.13)

Observer Height Presets:
Observer Eye Elevation:feet
Sea Level (0 feet)500 feet1,000 feet2,000 feet
Refracted Distance (True)

3.14 statute mi

Standard atmospheric bending (+7.4%)

Nautical Range

2.73 nmi

Standard marine navigation unit

Geometric (Vacuum)

2.92 mi

Theoretical straight-line tangent

Horizon Dip Angle

2.5′ (0.042°)

Depression angle below true level

Two-Point Line of Sight Calculator (Can A See B?)

How to use the horizon distance calculator

  1. 1Enter your eye height

    Type your height above the ground or sea, in feet or meters.

  2. 2Compute the horizon

    The distance to the horizon is calculated for Earth's curvature, with and without standard atmospheric refraction.

  3. 3Check a distant target

    Read the horizon distance in miles, km and nautical miles, and add a target height to see if it is visible.

How Far Away Is the Horizon?

When gazing across an open ocean or vast flat plain, the line where the sky appears to meet the Earth is defined as the horizon. In classical physics and geodetic surveying, there is a fundamental distinction between the theoretical geometric horizon and the actual apparent (optical) horizon:

  • Geometric Horizon: The theoretical tangent line drawn from the observer's eyeball to the smooth geometric sphere or ellipsoid of the Earth, completely ignoring the presence of an atmosphere. In a vacuum, light travels in absolute straight lines, and the geometric horizon marks the absolute limit of visibility.
  • Apparent (Optical) Horizon: The true boundary perceived by human eyes and optical sensors. Because Earth is enveloped in an atmosphere with varying density, light rays bend as they travel through air, pushing the visible horizon roughly 7% to 8% farther than pure geometry would dictate.
  • Radar Horizon: At radio and microwave frequencies used by marine radar and air traffic control, atmospheric refraction is even stronger, extending the radar horizon approximately 15% beyond the geometric horizon (modeled using the 4/3 effective Earth radius rule).

How Refraction Lets You See Farther

Earth's atmosphere is densest at sea level and thins exponentially with altitude. According to Snell's Law of refraction, light travels slightly slower in denser air (where the refractive index n ≈ 1.000293) than in rarefied upper air.

As light rays travel nearly horizontal across the surface, they pass through layers of decreasing refractive index. The upper edge of the wavefront moves marginally faster than the bottom edge, causing the light path to curve gently downward toward the Earth's center of gravity.

Under International Standard Atmosphere (ISA) conditions (temperature of 15°C, pressure of 1013.25 hPa, and a standard temperature lapse rate of -6.5°C per kilometer), this bending can be mathematically modeled by expanding the apparent radius of the Earth by a factor k ≈ 7/6 ≈ 1.167 (or in radar geodesy, k = 4/3 ≈ 1.333). This downward curvature allows observers to “see around” a portion of the globe's physical curve.

How Far Can You See a Tall Object?

A common navigational question is not merely how far an observer can see the sea surface, but whether an elevated observer can spot an elevated target—such as a lighthouse keeper spotting the masthead of an approaching ship, or two microwave transmission towers communicating across a valley.

When both the observer and target have elevation above the surface, the total line-of-sight distance is the sum of their individual horizon distances:

Mutual Line-of-Sight Principle

Let h₁ be the observer's eye height and h₂ be the height of the distant object (e.g., the lantern gallery of a lighthouse). The maximum distance at which the light remains visible above the horizon before dipping below Earth's curvature is:

d_total = d(h₁) + d(h₂) ≈ 3.86 × (√h₁ + √h₂) km

For example, an observer with eye height 2 meters (√2 ≈ 1.41) looking for a 50-meter lighthouse (√50 ≈ 7.07) can detect the light at a distance of 3.86 × (1.41 + 7.07) ≈ 32.7 kilometers (20.3 miles), long after the lighthouse base has dipped below the horizon.

Horizon Distance Formula and Calculation

The exact geometric distance d along the line of sight from eye height h to the tangent point on a sphere of radius R follows directly from the Pythagorean theorem:

GOVERNING MATHEMATICAL EQUATIONd_geom = √(2Rh + h²) ≈ √(2Rh), d_refract = √(2 · kR · h) ≈ 3.86 · √h (meters) km
VARIABLE DEFINITIONS & CONSTANTS
d_geom:Geometric tangent line-of-sight distance in a vacuum (kilometers)
d_refract:Optical horizon distance accounting for downward terrestrial refraction (kilometers)
R:Mean Earth radius (6,371.008 km)
h:Observer elevation / eye height above sea level (meters)
k:Atmospheric refraction scale factor under standard atmosphere (7/6 ≈ 1.167)
WORKED BENCHMARK: COASTAL CLIFF EDGE (BEACHY HEAD, UK)
Observer Eye Height (h) = 100.0 meters (328.1 feet)Mean Earth Radius (R) = 6,371,008 metersAtmospheric Factor (k) = 1.167 (Effective Radius R' = 7,434,966 m)
  1. Geometric Tangent = √(2 * 6,371,008 * 100 + 100²) = √(1,274,201,600 + 10,000) = 35,696 meters
  2. Geometric Horizon = 35.70 km (22.18 miles)
  3. Refracted Tangent = √(2 * 7,434,966 * 100) = √(1,486,993,200) = 38,561 meters
  4. Refracted Optical Horizon = 38.56 km (23.96 miles)
  5. Refraction Horizon Bonus = 38.56 - 35.70 = +2.86 km (+8.0% visibility extension)
Computed Result:Geometric Horizon: 35.7 km | Refracted Optical Horizon: 38.6 km (24.0 mi)

An observer standing atop the 100m cliff sees sea-level objects out to 38.6 km. If looking at a ship mast extending 25 meters above water, the mast remains visible out to 57.9 km.

Horizon Distance by Height (Table)

Reference this benchmark table comparing geometric versus optical horizon distances across key real-world observation platforms, from beachgoers to cruising jet airliners:

Observer Elevation Benchmarks, Geometric Tangents, and Optical Horizon Distances

Calculated using mean Earth radius R = 6,371 km with standard atmospheric refraction coefficient.

Observation PlatformEye Height (m)Eye Height (ft)Geometric HorizonOptical Horizon (km)Optical Horizon (mi)
Beach Shoreline (Seated)1.0 m3.3 ft3.57 km3.86 km2.40 mi
Standing Adult (Eye Level)1.7 m5.6 ft4.65 km5.03 km3.13 mi
Lifeguard Tower / Small Yacht Deck4.0 m13.1 ft7.14 km7.72 km4.80 mi
Sailing Ship Crow's Nest25.0 m82.0 ft17.85 km19.30 km11.99 mi
White Cliffs of Dover Edge110.0 m360.9 ft37.44 km40.48 km25.15 mi
Burj Khalifa Observation Deck555.0 m1,820.9 ft84.10 km90.93 km56.50 mi
Commercial Airliner Cruising (FL350)10,668 m35,000 ft368.9 km398.8 km247.8 mi
Mount Everest Summit8,848 m29,029 ft335.8 km363.0 km225.6 mi

Accuracy and Limitations: Mirages and Waves

Real-world atmospheric optics deviate significantly from textbook standard conditions under specific meteorological regimes:

  • Superior Mirages & Looming: When warm air flows over very cold ocean water (a strong temperature inversion), the vertical density gradient steepens drastically. Light rays curve more sharply than the Earth's curvature itself, causing islands and ships located dozens of miles beyond the normal horizon to appear floating in mid-air (looming).
  • Fata Morgana: Complex alternating layers of warm and cold air create atmospheric acoustic/optical ducts that compress, stretch, and invert objects into fantastical castles and towering walls on polar and maritime horizons.
  • Inferior Mirages: On hot summer pavement or sun-baked desert sand, superheated surface air is less dense than the cooler air above it. Light rays bend upward away from the ground, creating the illusion of reflective water pools on the horizon.
  • Sea State & Swell Shadow: In maritime navigation, significant wave heights of 3 to 6 meters routinely block direct line-of-sight to the true geometric horizon for small watercraft, reducing practical visibility well below theoretical limits.
Maritime & Navigation Operational Guidance
  • Calculations reflect Standard Atmospheric conditions; actual horizon distance can vary by ±15% or more during intense maritime temperature inversions.
  • For nautical radar navigation, calculate the radar horizon using the 4/3 Earth radius constant (factor 4.12 × √h_meters) rather than optical 3.86.
  • To determine if a distant light or mountain peak is visible, always compute mutual line-of-sight: d_total = 3.86 × (√h_eye + √h_target).

Complementary Elevation & Distance Geodetic Engines

Calculate terrain heights, direct path distances, and antipodal positions:

Quick facts about the horizon distance calculator

FactValueNotes
Geometric Horizond ≈ √(2 · R · h)Pure geometric line-of-sight
Refraction Correctionk = 0.17 Standard AtmosphereExtends visual horizon by ~8%
Sea-Level BaselineMean Earth Radius R = 6,371 kmWGS84 spherical approximation
PRECISION & EXCEPTIONS

Edge cases and exceptions

Atmospheric Inversions & Mirages

Strong temperature inversions (cold air over warm water) can cause superior mirages (looming), extending visible sightlines far beyond standard refraction.

FIELD APPLICATIONS

The horizon distance calculator: worked examples

1

Beach Horizon Distance

Scenario: A person standing at the ocean edge with eye height of 6 feet (1.83 m).

Outcome: Geometric horizon is 2.98 miles away; standard atmospheric refraction extends visible horizon to 3.23 miles.

2

Burj Khalifa Observation Deck

Scenario: Looking out from 555 meters (1,820 feet) above ground.

Outcome: Visual horizon extends to approximately 57 miles (92 kilometers).

FREQUENTLY ASKED QUESTIONS

Frequently asked questions about the horizon distance calculator

How far is the horizon from eye level?

For an average adult standing at sea level (eye height around 5.7 feet / 1.75 m), the horizon is approximately 3.1 miles (5.0 km) away.

What is the formula for distance to the horizon?

On a sphere, d ≈ √(2Rh), where R is Earth's radius and h is the observer's height. In practice, d (miles) ≈ 1.22 × √(height in feet).

How far is the horizon from a mountain or a tall building?

From 1,000 feet the geometric horizon is about 39 miles away. From the top of a 2,717-foot skyscraper like the Burj Khalifa it is more than 60 miles.

What is atmospheric refraction?

The atmosphere bends light slightly around Earth's curvature, making the horizon appear about 8 percent farther than the geometric calculation. The tool applies a standard refraction coefficient.

How far can I see a ship or lighthouse?

Add the horizon distances for the observer and the target. A 6 ft observer and a 100 ft lighthouse can see each other up to about 15 miles away in clear air.

Does the calculation work for aircraft?

Yes. At 35,000 feet the horizon is roughly 230 miles away.

Why can I not see far on a hazy day?

The geometric limit is the maximum. Haze, mirages and obstacles such as hills reduce practical visibility.

Is the ground curved by 8 inches per mile squared?

That popular rule, 8 inches times the miles squared, is a close approximation of the drop below a tangent line for short distances. It is not accurate beyond a few miles.

How does this relate to line-of-sight radio?

Radio horizon is slightly longer than the optical horizon because of refraction. Include antenna heights at both ends.

Can I enter meters?

Yes. Choose feet or meters, and the result shows miles, kilometers and nautical miles.

Keep exploring

Data & Cartographic Authority: Spherical Earth geometry · Calculated in your browser from the data you enter

Written and maintained by . Content updated October 30, 2026; data last verified September 19, 2026. See our editorial policy, methodology, or report an error.