The Moving Sky: How Star Charts Map a Curved Sky

The Moving Sky Above Our Head

Every star chart begins with the impossible task of fitting the curved dome of the sky onto flat paper. Our night sky has no edges, no corners, no single place to be cut open, so there is no solution that does not distort one part or another. The trouble isn’t the sky’s size, it’s its curvature: a curved surface and a flat sheet simply cannot be matched without something giving way.

However, for thousands of years, people have found ways around this issue. This hub is about those ways. Our resources examine the star chart projection that flattens the dome with the least possible distortion, explain stellar coordinate systems, and explore how early cultures used the night sky as a calendar. To see the trade-off for yourself, drag the sphere in the projection explorer and watch how the math decides where each star lands.

The Wandering North Star

Watch the wanders of the North Star through epochs of time.

The North Star

Why the Stars Aren’t Where Your Ancestors Saw Them. The North Star won’t always be north. Earth wobbles and skies turn.

Sidereal vs. Tropical

Two valid ways to fix a star’s position, one tied to the seasons and one to the stars, and the slowly widening gap between them.

Lahiri Ayanamsa

Modern Indian astronomy needed one exact number to separate the two zodiacs. This is how it was chosen.

Wandering Planets

The five wandering lights the ancients tracked by eye, and how to find tonight’s planets in your own sky.

✦  Astronomy Picture of the Day  ✦

NGC 2442: Galaxy in Volans

April 1, 2023
© Nicolas Rolland
Distorted galaxy NGC 2442 can be found in the southern constellation of the flying fish, (Piscis) Volans. Located about 50 million light-years away, the galaxy's two spiral arms extending from a pronounced central bar give it a hook-shaped appearance in this deep colorful image, with spiky foreground stars scattered across the telescopic field of view. The image also reveals the distant galaxy's obscuring dust lanes, young blue star clusters and reddish star forming regions surrounding a core of yellowish light from an older population of stars. But the star forming regions seem more concentrated along the drawn-out (upper right) spiral arm. The distorted structure is likely the result of an ancient close encounter with the smaller galaxy seen near the top left of the frame. The two interacting galaxies are separated by about 150,000 light-years at the estimated distance of NGC 2442.