February 17 annular solar eclipse: Timing and visibility

The Moon will cover 96% of the Sun during the event.
PUBLISHED FEB 12, 2026
Annular eclipse photographed at sunset in eastern New Mexico. (Representative Image Source: Kevin Baird)
Annular eclipse photographed at sunset in eastern New Mexico. (Representative Image Source: Kevin Baird)

On Tuesday, February 17, 2026, an annular solar eclipse, popularly known as a “ring of fire,” will be visible from Earth, but only to observers stationed in Antarctica. This type of eclipse happens when the Moon passes directly in front of the Sun but appears too small to fully cover it, creating a brilliant glowing ring around its silhouette. 

This graphic demonstrates the juxtaposition of the Moon with the Sun necessary to produce a partial or complete solar eclipse. (Image Source: ESO/M. Kornmesser
This graphic demonstrates the juxtaposition of the Moon with the Sun necessary to produce a partial or complete solar eclipse. (Representative Image Source: ESO/M. Kornmesser)

Where is it visible and when?

The event is projected to begin peaking at 7:12 a.m. EST (1212 GMT), with annularity visible over Antarctica’s icy expanses for just 1 minute and 52 seconds. For most terrestrial inhabitants, therefore, visibility of the ring is not possible, unless they live in scientific stations like the French-Italian Concordia on the Dome C site and Russia’s Mirny on the Davis Sea coast. While the full ring will remain exclusive to the polar ice cap regions highlighted above, a partial solar eclipse ranging from 12% to 20% will extend visibility to skywatchers elsewhere along the southern tips of South America and southern Africa. Per EarthSky, the partial eclipse will begin at 9:56 GMT (4:56 a.m. EST). No matter where people are observing the eclipse from, they will have to wear eclipse-appropriate glasses.

Photograph of an annular solar eclipse that occurred on October 14, 2023. The photograph was taken from Fillmore, Utah, USA. (Representative Cover Image Source: Getty Images: Rebecca Harding)
Photograph of an annular solar eclipse that occurred on October 14, 2023. The photograph was taken in Fillmore, Utah, USA. (Representative Image Source: Getty Images | Rebecca Harding)

Although the Moon will cover about 96% of the Sun during the eclipse, the infrared and ultraviolet radiation from the Sun can still cause permanent damage to observers' eyes. The protection ensures that it doesn't happen. Space.com recommends dedicated solar binoculars like the Lunt SUNoculars and Celestron Eclipsmart for those who intend to get a closer look at solar eclipses. 

A stock image of a total solar eclipse and Monument Valley at sunrise in Utah, USA. (Image Source: Getty | Diane Miller)
A stock image of a total solar eclipse and Monument Valley at sunrise in Utah, USA. (Representative Image Source: Getty | Diane Miller)

As defined by NASA, an event called Greatest Eclipse marks the moment when the moon’s shadow axis comes closest to Earth’s center, making it a key reference point for the entire eclipse and a simple way to compare eclipses. Greatest Duration, on the other hand, marks the specific moment along the central path where the annular ring phase reaches its longest length, which can differ from Greatest Eclipse due to the motion of the Moon's shadow with respect to the curvature of Earth's surface and to the Equator. 

Schematic diagram showing the shadow path for the annular eclipse on February 17, 2026. (Representative Image Source: F. Espenak, NASA's GSFC)
Schematic diagram showing the shadow path for the annular eclipse on February 17, 2026. (Representative Image Source: F. Espenak, NASA's GSFC)

For reference, these key timings and positional information from the data made available by NASA for the February 17, 2026, annular eclipse are as follows:

Greatest Eclipse at 12:11:54.1 UTC (64°43.0’S, 086°45.2’E), with Sun altitude 12.3°, path width 616.6 km, and central duration 02m 19.6s.

Greatest Duration at 11:48:16 UTC (71°57’S, 136°39’E), with Sun altitude 0.0° near horizon, path width 766.1 km, and central duration 02m 20.9s.

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