Interactive astronomy lab

If Earth keeps moving, how can we point to the same galaxy?

Move through time and watch how RA / Dec stays fixed while the direction and altitude in your local sky change.

How to explore

Press play or drag the timeline, then orbit the 3D dome to see how direction and altitude work together.

View from London

3D coordinate overlay · M31

The fixed RA / Dec grid is projected onto your changing local Alt / Az sky.

Above the horizon
RA
Dec
Azimuth
Altitude
Cyan solid = local Alt / Az gridViolet dashed = celestial RA / Dec gridGold RA + pink Dec = fixed address

Right Ascension · Fixed

00h 42m 44s

Declination · Fixed

+41° 16′

Azimuth · Direction

42.9°

North-east

Altitude · Height

16.5°

Above the horizon

Simulated time

17 Oct 2026, 15:00 UTC

Play time to watch the violet celestial grid turn against the cyan horizon grid while RA / Dec stays unchanged.

Space coordinates · RA / Dec

Stays fixed

Right Ascension

00h 42m 44s

Declination

+41° 16′

Think of this as an address on the sky map. It uses a reference frame based on very distant objects, so it does not rotate with the ground beneath us.

Local sky coordinates · Alt / Az

Keeps changing

Azimuth

42.9°

Altitude

16.5°

These coordinates tell a telescope which direction to face and how high to tilt right now, so they must be recalculated for the observer's location and time.

A simple way to remember it

1 · Start with a fixed address

Choose a galaxy by its RA / Dec.

2 · Add Earth context

Use the date, time, and observer location.

3 · Point the telescope

Convert the result to Azimuth / Altitude.

One more thing: The light we see comes from the past. M31 is about 2.5 million light-years away, so we see it as it was roughly 2.5 million years ago—not as a live image of this moment.