Instant · Precise · Universal
32 units available
6 categories total
To convert AU to km: multiply by 149,597,870.7. To convert AU to light-years: divide by 63,241.
1 AU = 149,597,870,700 m ≈ 149.598 Gm ≈ 499 light-seconds ≈ 8.317 light-minutes.
For example, 1 Astronomical Unit (AU) = 23533.69514 Earth's Polar Radius (R⊕ (polar)).
| Astronomical Unit (AU) | Earth's Polar Radius (R⊕ (polar)) |
|---|---|
| 0.1 | 2353.369514 |
| 0.5 | 11766.84757 |
| 1 | 23533.69514 |
| 2 | 47067.39028 |
| 5 | 117668.4757 |
| 10 | 235336.9514 |
| 25 | 588342.3785 |
| 50 | 1176684.757 |
| 100 | 2353369.514 |
| 500 | 11766847.57 |
| 1000 | 23533695.14 |
The astronomical unit is a unit of length approximating the mean Earth-Sun distance, defined as exactly 149,597,870,700 meters.
1 AU = 149,597,870,700 m ≈ 149.598 Gm ≈ 499 light-seconds ≈ 8.317 light-minutes.
To convert AU to km: multiply by 149,597,870.7. To convert AU to light-years: divide by 63,241.
Spacecraft mission planning, expressing planetary orbit sizes, and solar system scale models.
Light takes about 8 minutes and 20 seconds to travel 1 AU. Mars is about 1.52 AU from the Sun, Jupiter about 5.2 AU.
Thinking the AU is the exact Earth-Sun distance — Earth's actual distance varies from ~147 to ~152 Gm over the year due to orbital eccentricity.
AU makes the solar system manageable: Mercury ≈ 0.39 AU, Venus ≈ 0.72, Earth = 1, Mars ≈ 1.52, Jupiter ≈ 5.2, Saturn ≈ 9.5.
The Earth's polar radius is the distance from Earth's center to either pole, approximately 6,356.752 km.
R⊕(polar) = 6,356,752.3 m. It is about 21.385 km shorter than the equatorial radius.
To convert Earth polar radii to meters: multiply by 6,356,752.3.
Geodetic calculations, gravity modeling, and precise cartography near the poles.
At the poles, you are about 21 km closer to Earth's center than at the equator — you weigh very slightly more!
Approximating Earth as a perfect sphere — the difference between equatorial and polar radii matters for precision applications.
Earth's shape (oblate spheroid) is like a slightly squished ball — wider at the equator, flatter at the poles.



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