The Moving Sky: How Star Charts Map a Curved Sky

The moving sky above our head

Above our heads, the dark skies slowly change in appearance. We might think they are eternal and still because the cycle is not apparent to the eye, but in truth they move in an unending rhythm. What we see is not what our great-grandparents saw, and it is definitely not what the ancients saw. Like a top, Earth wobbles on its axis, completing an entire great cycle every 26,000 years. That wobble affects our view of the sky. The wobble is so slow we cannot feel it, but it is wide enough that the pole star changes. Polaris is our pole star now, but for the Egyptians who built the pyramids it was Thuban, and Vega will come after Polaris.

This is why there are two addresses for the stars. Fix your coordinates to the seasons and you get one set. Fix them to the stars themselves and you get another. The gap between them grows by a degree every 72 years. On this page we look at how the poles have wandered, why the zodiac no longer matches the constellations behind it, and how the planets wander against a background that is itself in motion.

The Wandering North Star

Watch the wanderings 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 selected

Wandering Planets

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

โœฆ  Astronomy Picture of the Day  โœฆ

EUVE Sky Map

January 31, 2002
Credit: EUVE Project, NASA
See this entry on NASA's APOD โ†’
The stars beyond the Sun and the distant galaxies should be undetectable at extreme ultraviolet wavelengths . At least that was the conventional wisdom when it was first realized that the space between the stars is filled with hydrogen , a strong absorber of extreme ultraviolet light. But this idea was seriously questioned as it became apparent that interstellar hydrogen was patchy in its distribution and the quest to explore the extreme ultraviolet sky culminated in 1992 with the launch of the EUVE (Extreme UltraViolet Explorer) spacecraft. An all-sky map, based on the satellite's first six months of operation, appears above showing brightness variations in the EUV sky in false color (north is up). EUVE's scanning by orbit gives the picture a striped look while other instrument artifacts are seen as crosses and data gaps are dark. Multiple images of the Moon combine to form the short, bright dashed lines wandering along the middle of the picture. The belt stars of the familiar constellation Orion are fairly easy to make out left of picture center. EUVE's science operations ceased in 2001 but it ultimately detected nearly 1,000 celestial objects, including over three dozen outside our own galaxy. EUVE's voyage of discovery is now complete, and the spacecraft re-entered the Earth's atmosphere yesterday at approximately 11:15 p.m. EST.