
When day briefly becomes night and a ring of fire crowns the Moon.
Greatest eclipse in 2024: 8 April 2024 at 18:17 UTC. Times for 2026 and 2027 vary along the path. Rows in orange are still to come.
As you scroll through this section, imagine standing inside the path of totality. The light dims, temperatures drop, and bright stars and planets appear in the middle of the day while the Sun becomes a crowned ring of fire.
The Moon slowly bites into the Sun’s disk. Crescent sunlight casts strange, overlapping shadows on the ground known as eclipse crescents.
For just a few minutes, day becomes night. A black silhouette of the Moon is surrounded by the Sun’s ethereal corona or a blazing annular ring.
The Sun re-emerges from behind the Moon. Birds resume singing, temperatures climb, and the sky brightens as quickly as it darkened.
A solar eclipse occurs when the Moon passes directly between the Sun and Earth, casting a moving shadow on our planet. Along the narrow path where the Moon’s darkest shadow – the umbra – falls, observers can experience totality: the Sun’s bright disk is completely covered.
Slight changes in distance create different eclipse types. When the Moon appears large enough in the sky, it can fully block the Sun (a total eclipse). When it appears slightly smaller, a thin ring of sunlight remains – an annular “ring of fire” eclipse.
For a few breathtaking minutes, the architecture of the solar system becomes visible to the naked eye.
A solar eclipse happens when the Moon passes directly between the Sun and Earth, casting its shadow onto Earth’s surface.
Because the Sun is about 400 times farther away and 400 times larger than the Moon, they appear the same size in our sky. Only a precise alignment creates an eclipse.
The darkest central shadow (umbra) creates totality. The penumbra produces partial eclipses. When the Moon is slightly farther away, its smaller disk leaves a bright ring called the antumbra.
During an annular eclipse, a blazing ‘ring of fire’ surrounds the Moon. During totality the Sun’s outer atmosphere—the corona—becomes visible as a ghostly halo.
A solar eclipse happens when the Moon moves directly between the Sun and Earth, blocking some or all of the Sun's light. From Earth, the Sun appears partially or completely covered for a short period of time.
A 'ring of fire' is an annular solar eclipse. It happens when the Moon is slightly farther from Earth and appears too small to cover the entire Sun, leaving a bright ring of sunlight around the Moon's silhouette.
You should never look directly at the Sun without proper eye protection, even during most of an eclipse. Only during the brief phase of totality in a total solar eclipse is it safe to look with the naked eye. For all other phases you must use certified eclipse glasses or solar filters.
Totality typically lasts only a few minutes at any given location. The longest possible totality is around 7 minutes, but most modern eclipses deliver 1–4 minutes of totality along the narrow path where the Moon’s umbra crosses Earth.
Solar eclipses require a precise alignment of the Sun, Moon, and Earth. Eclipses do happen multiple times per year somewhere on Earth, but the path of totality is very narrow—often just a few hundred kilometers wide—so any single location sees a total solar eclipse only every few decades.

The sudden contrast between deep shadow and searing sunlight has inspired silhouettes with sharp cut-outs, molten metallics, and shadow-play tailoring – pieces that feel like wearing the moment the Sun’s corona ignites around the Moon.
Use the Moontians Live Moon Tracker to follow the Moon’s position and prepare for future eclipses.
“Daylight written in gold and shadow.”