Axial Tilt of Uranus
| Value | 1.7064084 rad |
| Status | Conventional / typical value |
| Source | NASA NSSDC Planetary Fact Sheet, Uranus (obliquity to orbit) |
| Categories | Astronomicalsolar-systemplanets |
| microarcsecond | 351,972,000,000 μas |
| milliarcsecond | 351,972,000 mas |
| microradian | 1,706,408.4 μrad |
| arcsecond | 351,972 ″ |
| arcminute | 5,866.2 ′ |
| mil (NATO) | 1,738.1333 mil |
| milliradian | 1,706.4084 mrad |
| gradian | 108.63333 gon |
| degree | 97.769999 ° |
| compass point | 8.6906666 point |
| hour angle | 6.518 h |
| radian | 1.7064084 rad |
| quadrant | 1.0863333 quad |
| revolution | 0.27158333 rev |
Learning zone
Every other planet spins more or less upright as it orbits; Uranus lies on its side. At 97.77° the axis points past the perpendicular, so the planet effectively rolls around the Sun, offering first one pole, then its equator, then the other pole to the light across its 84-year orbit. The moons and rings share the tilt exactly, orbiting in the equatorial plane like a bullseye when a pole faces Earth — which is the central clue: whatever tipped Uranus happened early, before or during the assembly of its satellite system.
The standing explanation is one or more giant impacts by Earth-sized bodies in the young solar system, though a slower alternative — a resonance that pumped the tilt while a massive early moon was later lost — remains alive. Strangest of all, the extreme geometry barely shows in the climate: sluggish heat transport smooths the 42-year polar days and nights into temperature differences of only a few kelvin.