The antumbra is the part of a shadow beyond the tip of the umbra, where the blocking body looks smaller than the light behind it. When the Moon is too far away for its umbra to reach Earth, the antumbra touches down instead, and people inside it see an annular eclipse: a ring of sunlight around the Moon.
Understanding Antumbra
Why the umbra sometimes ends in space
The Moon's umbra averages about 374,000 km long, while the Moon's distance from Earth's surface swings between roughly 350,000 and 400,000 km over its orbit. When the Moon is far away, the tip of the umbra ends before it reaches the ground and Earth sits in the antumbra instead. The umbra falls short a little more often than it reaches, which is why annular eclipses slightly outnumber total ones: about a third of all solar eclipses are annular and about a quarter are total.
Annular eclipses on Orbital Radar
The next two times the Moon's antumbra touches down, each with its own page, path and local times:
| Date | Path of annularity | Longest annularity | Sun hidden |
|---|---|---|---|
| 6 February 2027 | Southern Chile, Argentina (Mar del Plata), the South Atlantic, West Africa (Abidjan, Accra, Lagos) | 7 min 51 s | 86% |
| 26 January 2028 | Galápagos, Ecuador, Peru, Brazil, then Portugal and southern Spain at sunset | 10 min 27 s | 85% |
Total, annular or hybrid: one shadow, different distances
The three kinds of central solar eclipse are the same alignment seen with the Moon at different distances. If the umbra reaches Earth, the path is total. If it falls short, only the antumbra arrives and the path is annular. If the tip reaches the ground only around the middle of the path, where Earth's curved surface is a few thousand kilometres nearer the Moon, the eclipse is total there and annular at the ends: a hybrid eclipse. The drawing above shows the total and annular cases side by side.