Annular Solar Eclipse of February 6, 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 open our Eclipse Explorer, or take the Eclipse Control Center, which gives your distance and bearing to the nearest stretch of the path over land, your own contact times to the second, and a live view of the shadow crossing Earth.
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.
| Stage | Time |
|---|---|
| Partial eclipse begins | 14:11 UTC |
| Ring begins | 15:55 UTC |
| Greatest eclipse | 15:59 UTC |
| Ring ends | 16:03 UTC |
| Partial eclipse ends | 17:39 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.
Never miss an eclipse
Every upcoming solar and lunar eclipse in a free feed your calendar app refreshes on its own, computed by the same engine as this page.
Calendar feeds: subscribe (webcal) · download the .ics · all feeds and setup
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 Control Center for a live console on this eclipse as it happens, the Eclipse Explorer for any date and location, our Saros cycle profile for why eclipses repeat, its longer partners the inex and the exeligmos that together sort every eclipse into families, the eclipse year of 346 days that sets the rhythm of eclipse seasons, and how eclipses work from first principles.
Other eclipses on the calendar
Every eclipse below is engine-verified against the same catalog, so the times are directly comparable.
Total Solar Eclipse of August 12, 2026
Total solar eclipse, Saros series 126. Kept for the record.
Partial Lunar Eclipse of August 28, 2026
Partial lunar eclipse, Saros series 138. Kept for the record.
Penumbral Lunar Eclipse of February 20, 2027
Penumbral lunar eclipse, Saros series 143.
Penumbral Lunar Eclipse of July 18, 2027
Penumbral lunar eclipse, Saros series 110.
Eclipse Control Center
Watch this one happen: your own contact times and countdown, the shadow crossing Earth, and a go or no-go verdict for where you are standing.
Eclipse Explorer
The next eclipse visible from any location you name, with local contact times, plus a walk along a Saros series.
The Saros Cycle
Why an eclipse repeats a near-copy of itself every 18 years 11 days, and why the copy lands a third of the way around the world.