Great Circle — Shortest Path on a Sphere
Compute the geodesic distance between two points on a sphere, plus initial/final bearings and midpoint. Essential for aviation, maritime navigation, and GPS.
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Great circle = geodesic = shortest surface path Flight paths follow great circles—they appear curved on flat maps Initial bearing ≠ final bearing except along equator or meridian Earth mean radius ~6371 km gives ~0.5% typical error Works for any sphere—Mars, Moon, or custom radius
Ready to run the numbers?
Why: Great circles define the shortest path between two points on a sphere. Flight paths, shipping routes, and GPS calculations all use spherical geometry. Understanding geodesics is fundamental to navigation and geospatial applications.
How: Enter latitude and longitude for two points, plus the sphere radius (6371 km for Earth). The calculator uses the Spherical Law of Cosines for the central angle, then multiplies by radius for distance. Bearings and midpoint use standard spherical trigonometry formulas.
Run the calculator when you are ready.
Great Circle — Shortest Path on a Sphere
Distance, bearings, and midpoint between two points. Essential for navigation.
🌍 Sample Routes — Click to Load
Coordinates & Radius
Point 1
Point 2
Visualization
Property Radar
Property Comparison
Property Breakdown
📐 Calculation Breakdown
For educational and informational purposes only. Verify with a qualified professional.
🧮 Fascinating Math Facts
Flight paths follow great circles—routes appear curved on flat maps
— Aviation
Earth mean radius ~6371 km; equatorial and polar radii differ slightly
— Geodesy
Initial bearing ≠ final bearing except when traveling along equator or meridian
— Navigation
Haversine formula is an alternative, more stable for small distances
— Spherical Geometry
📋 Key Takeaways
- • Great circle = shortest path on a sphere (geodesic)
- • Distance d = R × Δσ (radius × central angle in radians)
- • Uses Spherical Law of Cosines for central angle
- • Bearings measured from North (0°=N, 90°=E)
💡 Did You Know?
📖 How It Works
Central Angle
Δσ = arccos(sin φ₁ sin φ₂ + cos φ₁ cos φ₂ cos Δλ) — Spherical Law of Cosines.
Distance
d = R × Δσ (radians). Same unit as radius.
Bearings & Midpoint
Initial/final bearings from atan2 formulas. Midpoint via spherical interpolation.
🎯 Expert Tips
Decimal Degrees
Use decimal degrees (e.g. 40.71) not DMS. North/East positive.
Radius Units
Distance output uses same unit as radius (km, mi, nmi).
Other Spheres
Use Mars radius (~3390 km), Moon (~1737 km) for other bodies.
Accuracy
Earth is oblate; mean radius gives ~0.5% error for most routes.
⚖️ Comparison
| Method | Use Case |
|---|---|
| Spherical Law of Cosines | General, used here |
| Haversine | Small distances, numeric stability |
| Vincenty | Ellipsoid (WGS84), highest accuracy |
❓ FAQ
Great circle vs straight line?
Great circle is shortest path on surface. Straight line through Earth is shorter but not a surface path.
Why do flight paths look curved?
Flat maps distort. Great circles project as curves on Mercator.
Does point order matter?
No. Distance is same. Bearings swap (init↔final).
Other planets?
Yes. Enter coordinates and that body's radius.
How accurate is this?
Spherical model: ~0.5% error. For survey-grade use ellipsoid (Vincenty).
What is central angle?
Angle at sphere center between the two points. d = R × Δσ.
📊 Stats
📚 Sources
⚠️ Disclaimer: Uses spherical Earth. For geodetic accuracy use WGS84 ellipsoid models.
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