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42.1 km/s

Solar escape at 1 AU

Calculated

Escape speed from the Sun’s gravity at Earth’s distance. √(2GM☉/1 AU) ≈ 42.1 km/s.

To leave the Sun from where Earth is, you need about 42.1 kilometres a second. Not a rounded light-year. A vis-viva number. Earth’s own orbital speed is about 29.8. The extra is the door out.

NASA / JPL

Printed 42s

A proton count. A catalogue seat. A scan. A model boundary. A patch that draws 4 and II. A joke a JPL scientist made in public. Different kinds. NASA printed them. That does not make them one Answer.

The metal

Sky and distance

  • M42Orion Nebula

    Catalogue seat. NASA’s Cosmic Hearth is Maya reception.

  • C42Caldwell 42

    Another catalogue. NGC 7006. Not a measured forty-two.

  • ≈42 AUKuiper collisions

    Stern 1995. A modeled boundary, not Albion’s distance.

  • 42.1 km/sSolar escapehere

    Vis-viva at 1 AU. Family 4.2, not 42.00.

Missions and tools

What it supports

v = √(2GM☉/r) at r = 1 AU. IAU solar GM 1.3271244×10²⁰ m³ s⁻². AU 1.495978707×10¹¹ m. Result 42.12 km/s, commonly printed 42.1. The third cosmic speed relative to the Sun at Earth’s orbit.

What it does not

Not 42.00 exactly. Not Earth’s surface escape 11.2. Not a light-year. 41.9 or 42.3 would still be physics. The hundredths follow the constants.

Calculation

√(2 × 1.3271244×10²⁰ / 1.495978707×10¹¹) = 4.212×10⁴ m/s ≈ 42.1 km/s.

Vis-viva escape at 1 AU. Constants, not a hunt for 42.

ExactnessApproximate

Form4.2

Unitkm/s

Strengthhard

Hung16 September 2026

Source

IAU · GM☉ and the astronomical unit

Owner

THE 42 INDEX