How the Sky Turns · 7 of 8
Why the Sky Moves
Why isn’t your sky tonight the same as someone else’s?
Rotation, latitude and precession — the three reasons the sky you see tonight is not the sky someone else sees.
You’ll be able to say why the sky turns, why your latitude tilts it, and why the pole drifts over millennia.
Before this: Finding the North Star (6 min), The Southern Cross (6 min)
Where and which night
Working out when this is best placed from where you are…
Where
Kept for this guide only, until you change it here — your map settings, and every other guide, stay as they are.
Print, play outside or present
Scan with a phone's camera, or open
Sources
- HYG stellar database v4.2 — star positions and magnitudes
- IERS Conventions (2010), ch. 5 — the sidereal day, 23h 56m 04.0905s of mean solar time
- Capitaine, Wallace & Chapront, A&A 412, 567 (2003) — IAU 2006 precession, 25,772-year cycle
- Meeus, Astronomical Algorithms, 2nd ed. (1998), ch. 13 and 21 — horizon transforms and precession
With a keyboard, focus the sky, aim it with the up and down arrow keys, and press Enter to drop the pin at the centre of the view; or press Show me.