Annular Solar Eclipse of February 6, 2027

This eclipse has passed. The next one on our calendar: Penumbral Lunar Eclipse of February 20, 2027.
Type
Annular solar eclipse
Peak (UTC)
February 6, 2027, 15:59 UTC
Greatest eclipse
31.3°S, 48.5°W
Sun covered
Up to 86% at greatest eclipse
Ring at the deepest point
about 7 min 45 s
Saros series
131

The ring of fire crosses southern Chile and Argentina, then the South Atlantic, ending near the coast of West Africa at sunset. A partial eclipse covers most of South America, the Antarctic Peninsula and parts of West Africa.

Where the ring goes

The antumbra makes landfall on the Pacific coast of Chile, crosses Patagonia into Argentina, then runs the length of the South Atlantic; the ring is visible from the ocean for most of the track before it ends near the Gulf of Guinea around local sunset.

For an interactive map of the track, and your own distance from the center line, open our Eclipse Explorer.

Timeline at the point of greatest eclipse

These contact times apply at the single point where the eclipse is deepest; along the rest of the track they shift by minutes to hours. The location panel below computes them for your own coordinates.

StageTime
Partial eclipse begins14:11 UTC
Ring begins15:55 UTC
Greatest eclipse15:59 UTC
Ring ends16:03 UTC
Partial eclipse ends17:39 UTC

Central durations here are computed at the point of greatest eclipse with the engine's standard solar and lunar radii; published limb-corrected path maxima can differ by a few seconds.

What you will see from your location

Enter a location (or use your device's) and we compute your local contact times, how much of the Sun is covered, and the Sun's altitude, all in your browser.

No location set yet. Your coordinates never leave your device.

What an annular solar eclipse is

In an annular eclipse the Moon passes squarely in front of the Sun but sits too far from Earth to cover it completely, leaving a brilliant ring of Sun, the famous ring of fire, around the Moon's silhouette. Because some direct sunlight always remains, the sky never darkens the way it does in a total eclipse, and eye protection is required from start to finish.

Eye safety is not optional

Looking at the Sun without proper protection damages the retina painlessly and permanently. For every partial phase of a solar eclipse, and for the whole of an annular eclipse, you need eclipse glasses that meet the ISO 12312-2 standard, or a pinhole projector, or a solar filter fitted to the FRONT of any binoculars or telescope. Sunglasses, smoked glass, exposed film and stacked filters are not safe, no matter how dark.

The single exception: during the minutes of totality in a total solar eclipse, when the Moon completely covers the Sun, it is safe and unforgettable to look with the naked eye. The instant the first sliver of Sun returns, the glasses go back on.

Frequently asked questions

When is the annular solar eclipse of February 2027?

Greatest eclipse comes on February 6, 2027 at 15:59 UTC. What you see, and when, depends on where you stand; use the location panel on this page for your own local timeline.

Where will the February 2027 solar eclipse be visible?

The ring of fire crosses southern Chile and Argentina, then the South Atlantic, ending near the coast of West Africa at sunset. A partial eclipse covers most of South America, the Antarctic Peninsula and parts of West Africa.

Do I need eclipse glasses for this eclipse?

Yes, for the entire eclipse. Even at maximum, a blinding ring of Sun remains visible, so there is never a safe moment to look without ISO 12312-2 eclipse glasses or a projection method.

What is a Saros series?

Eclipses repeat in families called Saros series: 6,585.3 days (about 18 years 11 days) after any eclipse, the Sun, Moon and lunar nodes return to nearly the same geometry and produce a near-copy shifted a third of the way around Earth. This eclipse belongs to Saros series 131. Our Saros cycle profile explains the whole mechanism.

Keep exploring: the Eclipse Explorer for any date and location, our Saros cycle profile for why eclipses repeat, and how eclipses work from first principles.