Why does the Moon turn red during a total eclipse?

Because Earth’s atmosphere filters and bends the Sun’s light: the blue tones scatter away, the reds pass through and faintly light the Moon at the heart of the shadow. It’s the same phenomenon that reddens our sunsets.

Will the March 3, 2026 eclipse be visible from Western Europe?

No. At the moment of totality it’s half past twelve in Paris: the Moon is below the horizon and the Sun is high in the sky. You’d need to be on the Pacific side, in East Asia, in Oceania or in the Americas, or to follow a live stream.

Do you need glasses to watch a lunar eclipse?

No, no protection is needed: the Moon only reflects a very dimmed light. Naked eye, binoculars or a telescope, anything goes, unlike solar eclipses, which demand certified filters.

Moon calendar · eclipses

The lunar eclipse of March 3, 2026 fifty-nine minutes of a red Moon.

On March 3, 2026, the full Moon passes through Earth’s shadow: a total lunar eclipse, with 59 minutes of totality around the peak at 11:34 UTC. The Moon turns red over the Pacific, which has the best seat in the house; East Asia, Australia and the Americas catch it too, each in their own way. From Western Europe there’s nothing to see this time: it’s broad daylight and the Moon sits below the horizon. It stands at 13° of Virgo.

The essentials

Date: March 3, 2026
Type: total lunar (magnitude 1.15)
Peak: 11:34 UTC, i.e. 12:34 in Paris
Totality: from 11:04 to 12:03 UTC, i.e. 59 minutes
Visibility: Pacific, East Asia, Australia, New Zealand, the Americas; not visible from Western Europe or the rest of Europe
Sign occupied: Moon at 13° of Virgo, Sun in Pisces

What happens that day?

A total lunar eclipse is Earth slipping precisely between the Sun and the full Moon. Our planet casts a cone of shadow out into space, and the Moon crosses it from edge to edge. It doesn’t vanish, though: Earth’s atmosphere bends the Sun’s light and lets only its red and coppery tones slip through. What you’d see on the Moon then is the glow of every sunrise and sunset on Earth, projected all at once.

The March 3 sequence unfolds across nearly six hours: the Moon enters the penumbra at 8:44 UTC, makes first contact with the full shadow at 9:50, holds totality from 11:04 to 12:03, leaves the shadow at 13:17, and the show ends around 14:23. At the peak, the Moon sinks deep enough into the shadow (magnitude 1.15) to blush a frank red.

Where and how to watch it, region by region?

The Pacific takes center stage. Hawaii sees the whole eclipse in the middle of the night, high in the sky: the perfect seat. New Zealand and eastern Australia follow it in the evening; in Sydney, the peak falls around 22:34 local time, with the Moon well risen.

In East Asia, Japan, Korea and eastern China watch totality early in the evening, the Moon still close to the eastern horizon: in Tokyo, the peak arrives around 20:34. Over in the Americas, it’s the night of March 2 to 3: Alaska and the West Coast see all of it (peak around 03:34 in Los Angeles); the further east you go, the earlier the Moon sets, and the Atlantic coast watches it sink into the shadow just above the western horizon, right before dawn.

Europe and Africa are out of luck: at 12:34 in Paris, the Moon is below the horizon and the sky is in full daylight. Wherever it is visible, no precautions are needed: a lunar eclipse is safe to watch with the naked eye, and a simple pair of binoculars is enough to make the coppery tones spectacular.

What astrology reads into it

This eclipsed full Moon stands in Virgo, facing the Sun in Pisces: the axis the lunar nodes have held since 2025, and which this run of eclipses travels one last time before tipping toward Leo and Aquarius in the summer of 2026. Tradition reads a lunar eclipse as a full Moon turned up: what was ripening quietly arrives all at once in full light.

Virgo speaks of sorting, of the concrete, of the care given to ordinary things; Pisces, of rest, of trust, of what we agree not to control. A closing on this axis invites you to look at what, between high standards and letting go, is asking to find its right measure. The eclipse decides nothing for you: for the length of one red hour, it lights up what was already there.

And the next one?

The following eclipse season arrives in August 2026, and it’s the headline event of the decade for our continent: the total solar eclipse of August 12, visible from Iceland and northern Spain, partial and spectacular from Western Europe. It will be followed by a partial lunar eclipse on August 28, visible this time from Western Europe, in the small hours of the morning.

Frequently asked questions

Why does the Moon turn red during a total eclipse?: Because Earth’s atmosphere filters and bends the Sun’s light: the blue tones scatter away, the reds pass through and faintly light the Moon at the heart of the shadow. It’s the same phenomenon that reddens our sunsets.
Will the March 3, 2026 eclipse be visible from Western Europe?: No. At the moment of totality it’s half past twelve in Paris: the Moon is below the horizon and the Sun is high in the sky. You’d need to be on the Pacific side, in East Asia, in Oceania or in the Americas, or to follow a live stream.
Do you need glasses to watch a lunar eclipse?: No, no protection is needed: the Moon only reflects a very dimmed light. Naked eye, binoculars or a telescope, anything goes, unlike solar eclipses, which demand certified filters.