The total lunar eclipse of March 2026, known as Lua of solar energy through the Earth’s atmosphere. The event will be visible in regions of eastern Ásia, Austrália, Oceania, Pacífico and América of Norte, with better conditions in the west of América of
Astronomers predict the total phase to last about 58 minutes, with the full eclipse spanning more than five hours. The maximum will occur around 11:33 UTC, when Lua will be completely immersed in the Earth’s umbra. Observadores in different time zones will see the phenomenon at varying local times, such as in the early morning hours on the west coast of Estados Unidos or at night in Austrália.
Eclipse phases and main times
The eclipse begins with the penumbral phase, when the outer shadow of Terra touches Lua, followed by the partial phase, in which the dark shadow advances. Totality begins when Lua is entirely in the umbra, reaching its peak at the moment of greatest coverage. Depois, the phases are reversed until the end of the event.
The umbral magnitude reaches approximately 1.15, indicating that Lua will be covered beyond its full diameter by the central shadow. Binóculos or telescopes improve viewing of details on the lunar surface during the reddish coloration.
Visibility by regions of the world
At América of Norte, the eclipse appears in the early morning hours of March 3, with Lua low on the western horizon in many locations. Observadores on the west coast, as in Califórnia, will see complete totality, while on the east coast the phenomenon may be partial or interrupted by sunrise.
East Asia, Austrália and Nova Zelândia will have favorable night vision, with Lua high in the sky during the main phases. No Pacífico central, the event takes place throughout the night. Partes of América Central and south west of América of Sul capture partial or total phases on the horizon.
Africa, Europa and much of western Ásia will not have visibility as Lua will be below the horizon during the eclipse. Condições clear weather is essential for observation in any location.
Why does Lua turn red
During totality, direct sunlight is blocked, but rays pass through Earth’s atmosphere and are filtered, allowing red and orange hues to reach Lua. Esse effect occurs because blue wavelengths disperse more, leaving red ones dominant.
The phenomenon receives the popular name of Lua from Sangue due to its characteristic appearance. The color varies depending on atmospheric conditions, such as dust or volcanic clouds, which can intensify or change the reddish tone.
Detailed duration of steps
The penumbral phase lasts about 338 minutes in total, the partial phase lasts about 207 minutes and the total phase lasts exactly 58 minutes and 19 seconds. The entire eclipse spans more than five and a half hours, from initial contact to final.
The maximum occurs at the point of greatest immersion, with Lua exhibiting the most intense coloration. Após the peak, the shadow of Terra gradually retreats until Lua returns to normality.
Recommended observation
Anyone with clear skies can observe the eclipse with the naked eye, without the need for eye protection. Aparelhos optics like binoculars reveal red-tinged lunar craters and seas. Fotografias require a tripod and long exposures to capture the faint glow.
The event coincides with the Lua Cheia of March, called Lua of the Minhocas in North American traditions. Astrônomos encourage observation in places with low light pollution for better contrast.
Last total eclipse for years
This total lunar eclipse represents the last visible over wide regions of the planet until the New Year’s eclipse of 2028-2029. Após March 2026, there will be no other total by that date, making the phenomenon particularly anticipated by astronomy enthusiasts.
Regions with full visibility plan public viewing events depending on weather conditions. The Sol-Earth-Moon alignment occurs at the descending node of the lunar orbit, guaranteeing the conditions for the total eclipse.
The March 2026 total lunar eclipse offers a unique opportunity for global observation in selected areas, highlighting astronomical phenomena accessible without specialized equipment.