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Next Solar & Lunar Eclipse Visibility Explorer

Interactive astronomical trajectory explorer for upcoming solar and lunar eclipses, totality paths, and visibility zones.

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Annular Solar Eclipse of February 6, 2027
Annular Solar
2027-02-067m 51sSouth America
Penumbral Lunar Eclipse of February 20, 2027
Penumbral Lunar
2027-02-204h 12mAmericas
Total Solar Eclipse of August 2, 2027 ('Eclipse of the Century')
Total Solar
2027-08-026m 23sSouthern Europe
Penumbral Lunar Eclipse of August 17, 2027
Penumbral Lunar
2027-08-173h 39mPacific Ocean
Annular Solar Eclipse of January 26, 2028
Annular Solar
2028-01-2610m 27sNorth America
Total Solar Eclipse of July 22, 2028
Total Solar
2028-07-225m 10sAustralasia
Total Lunar Eclipse of December 31, 2028 (New Year's Blood Moon)
Total Lunar
2028-12-311h 11m (Totality)Europe
Total Lunar Eclipse of June 26, 2029
Total Lunar
2029-06-261h 42m (Totality)Americas
Annular Solar Eclipse of June 1, 2030
Annular Solar
2030-06-015m 21sEurope
Total Solar Eclipse of November 25, 2030
Total Solar
2030-11-253m 44sSouthern Africa
Partial Lunar Eclipse of August 28, 2026
ArchivedPartial Lunar
2026-08-283h 18m (Umbral)North America
Total Solar Eclipse of August 12, 2026
ArchivedTotal Solar
2026-08-122m 18sEurope
Active Dataset: 2026–2030 EphemerisAuto-Sorted Chronology
Annular Solar
Saros 131

Annular Solar Eclipse of February 6, 2027

A spectacular 'Ring of Fire' annular eclipse slicing through southern South America before traversing the Atlantic into western equatorial Africa.

Astronomical Calendar HorizonSaturday, February 6, 2027
161days until eclipse maximum
Peak Totality7m 51s
Magnitude0.9281
Gamma Val-0.8516
Central Path of Totality / Maximum Obscuration
  • Chile (Patagonia)
  • Argentina
  • Uruguay
  • Cote d'Ivoire
  • Ghana
  • Nigeria
  • Benin
Broader Continental Visibility Zones
South AmericaWest AfricaAntarcticaAtlantic Ocean
Observational Safety & Optical Protocol

Continuous eye protection (ISO 12312-2) required at ALL times; the Moon does not fully cover the Sun, forming a brilliant 'Ring of Fire'.

Solar and Lunar Eclipse Mechanics: Orbital Syzygy and Shadow Geometry

An eclipse is an astronomical event occurring when three celestial bodies—the Sun, Earth, and Moon—align in a straight line, a configuration known mathematically as syzygy. Because the Moon's orbital plane around Earth is tilted by approximately 5.14 degrees relative to Earth's ecliptic plane around the Sun, eclipses do not happen every month. They occur exclusively during eclipse seasons (approximately every 173.3 days), when the Moon crosses the ecliptic nodes during either a New Moon (Solar Eclipse) or Full Moon (Lunar Eclipse).

Classification I

Total Solar Eclipse

Occurs when the Moon is at perigee, completely obstructing the solar photosphere and unveiling the delicate solar corona in total midday darkness.

Classification II

Annular Solar Eclipse

Takes place when the Moon is near apogee. Its apparent diameter is smaller than the Sun, creating a radiant "Ring of Fire" or antumbra cone.

Classification III

Total Lunar (Blood Moon)

Earth passes directly between the Sun and Full Moon. Refracted atmospheric sunlight bathes the submerged lunar surface in rich coppery crimson hues.

Global Eclipse Ephemeris Matrix: 2026 – 2030 Schedule

The table below details confirmed astronomical ephemeris data for upcoming solar and lunar eclipses, including duration of totality, magnitude index, Saros series identifiers, and primary geographic visibility corridors.

Calendar DateEclipse TypeSaros / GammaMax DurationPrimary Path of Central Totality / Visibility
2026-08-12Total SolarSaros 126 (0.898)2m 18sGreenland, Western Iceland (Reykjavik), Northern & Eastern Spain (Bilbao, Zaragoza, Valencia, Palma)
2026-08-28Partial LunarSaros 138 (-0.496)3h 18m (Umbral)North & South America, Pacific Ocean, Australasia, Eastern Asia (93% disk immersion)
2027-02-06Annular SolarSaros 131 (-0.852)7m 51sPatagonian Chile, Argentina, Uruguay, Cote d'Ivoire, Ghana, Nigeria, Benin
2027-08-02Total Solar (Century Eclipse)Saros 136 (0.142)6m 23sSouthern Spain (Cadiz, Malaga), Gibraltar, Morocco, Algeria, Tunisia, Libya, Egypt (Luxor), Saudi Arabia
2028-01-26Annular SolarSaros 141 (-0.390)10m 27sEcuador, Peru, Colombia, Brazil, French Guiana, Portugal, Spain (Sunset Ring of Fire)
2028-07-22Total SolarSaros 146 (-0.425)5m 10sAustralia (Kimberley, Sydney Harbour, NSW), New Zealand (South Island, Dunedin, Queenstown)
2028-12-31Total Lunar (NYE Blood Moon)Saros 135 (-0.326)1h 11m (Totality)Europe, Africa, Asia, Australasia, Northwest North America (Midnight Lunar Totality)

Certified Safety Protocols & Astrophotography Best Practices

Observing solar phenomena requires strict adherence to international optical standards to prevent irreversible retinal damage known as solar retinopathy.

ISO 12312-2 Standard Solar Filters

Always ensure your solar eclipse glasses are manufactured to the ISO 12312-2 safety standard. Inspect the lenses for punctures, scratches, or separation before use. Regular sunglasses and polarization filters provide zero protection against harmful infrared wavelengths.

Sensor & Lens Protection

When photographing a solar eclipse with DSLRs, mirrorless bodies, or telephoto lenses, place a certified front-element solar filter over the outer optic. Never look through an unshielded optical viewfinder, as the concentrated focal beam will instantaneously cause severe eye injury.

Frequently Asked Questions (FAQ)

What is the difference between a total, annular, and partial solar eclipse?

A total solar eclipse occurs when the Moon is close enough to Earth (perigee) that its apparent disk completely covers the Sun, exposing the solar corona. An annular solar eclipse happens when the Moon is farther away (apogee), appearing slightly smaller than the Sun and leaving a glowing "Ring of Fire" around its silhouette. A partial solar eclipse occurs when the Sun, Moon, and Earth are not in perfect alignment, causing only a fraction of the solar disk to be obscured.

Why does the Moon turn reddish-orange during a total lunar eclipse?

During a total lunar eclipse (commonly called a Blood Moon), Earth completely blocks direct sunlight from reaching the lunar surface. However, sunlight passes through Earth's atmosphere, which scatters shorter blue wavelengths and refracts longer red and orange wavelengths into Earth's shadow cone (the umbra). This filtered atmospheric light reflects off the lunar surface, projecting all of Earth's simultaneous sunrises and sunsets onto the Moon.

What are the essential eye safety rules for observing solar eclipses?

You must NEVER look directly at the uneclipsed, partially eclipsed, or annular Sun without certified ISO 12312-2 compliant solar eclipse glasses or dedicated solar telescope filters. Standard sunglasses, polarized lenses, smoked glass, or unverified dark plastics do NOT block hazardous infrared and ultraviolet radiation. The only time direct unassisted viewing is safe is during the brief period of 100% totality in a total solar eclipse, immediately ceasing as soon as the diamond ring effect reappears.

What is a Saros Series in eclipse mechanics?

A Saros cycle is an astronomical periodicity of approximately 18 years, 11 days, and 8 hours (6,585.3 days) that governs the recurrence of eclipses. Eclipses belonging to the same Saros series share nearly identical orbital geometries, lunar distances, and durations, though Earth's rotation shifts each successive eclipse trajectory approximately 120 degrees westward.

When is the next major total solar eclipse visible from Europe?

The next major total solar eclipse across continental Europe occurs on August 12, 2026, traversing western Iceland and northern Spain. This is followed shortly by the August 2, 2027 "Eclipse of the Century" across southern Spain, Gibraltar, Morocco, and Egypt.

Do I need special protective filters to view a lunar eclipse?

No. Lunar eclipses are 100% safe to view directly with the naked eye, standard binoculars, or optical telescopes. Unlike the Sun, the Moon only reflects dim, refracted sunlight and emits no dangerous levels of radiation.

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