Instant · Precise · Universal
32 units available
7 categories total
To international knots: × 1.00064. To km/h: × 1.853. To m/s: × 0.5148.
1 UK knot ≈ 1.853184 km/h = 0.5148 m/s. Slightly faster than the international knot (1.852 km/h).
For example, 1 Knot (UK) (kt (UK)) = 0.00004596190476 Cosmic Velocity - Second (v₂).
| Knot (UK) (kt (UK)) | Cosmic Velocity - Second (v₂) |
|---|---|
| 0.1 | 0.000004596190476 |
| 0.5 | 0.00002298095238 |
| 1 | 0.00004596190476 |
| 2 | 0.00009192380952 |
| 5 | 0.0002298095238 |
| 10 | 0.0004596190476 |
| 25 | 0.001149047619 |
| 50 | 0.002298095238 |
| 100 | 0.004596190476 |
| 500 | 0.02298095238 |
| 1000 | 0.04596190476 |
The UK knot is a historical variation of the knot based on the British nautical mile (6,080 feet) rather than the international nautical mile (6,076.12 feet).
1 UK knot ≈ 1.853184 km/h = 0.5148 m/s. Slightly faster than the international knot (1.852 km/h).
To international knots: × 1.00064. To km/h: × 1.853. To m/s: × 0.5148.
None in modern use. Only relevant for interpreting historical British naval records.
The difference between UK and international knots is only 0.064% — barely noticeable but important for precise navigation.
Assuming all old British ship logs use the same knot as today — they don't, but the difference is tiny.
Historical only. Effectively identical to modern knot. Only matters for historical maritime research.
The second cosmic velocity (Earth's escape velocity) is approximately 11,200 m/s (11.2 km/s), the minimum speed to escape Earth's gravity completely.
v₂ = √(2GM/r) = √2 × v₁ ≈ 11.2 km/s. Exactly √2 times the first cosmic velocity.
To km/h: × 3,600. To mph: × 25,000. 11.2 km/s = 40,320 km/h = 25,053 mph.
Moon missions, Mars missions, deep space probes (Voyager, New Horizons), and any mission leaving Earth's gravity well.
Apollo missions: ~11.2 km/s. Voyager probes: exceeded v₂ to leave solar system. New Horizons: launched at record 16.26 km/s (fastest ever from Earth).
Thinking you need this speed everywhere — you only need it at launch. In space, much less Δv is needed.
~11 km/s to escape Earth. √2 × orbital velocity. Remember: orbit ≈ 8 km/s, escape ≈ 11 km/s.



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