The dawn of March 3th 2026 It has in store one of those celestial spectacles that anyone can enjoy simply by looking up. For several hours, the full moon will enter the shadow of our planet and, in the right areas of the globe, will appear tinged with a striking coppery red colorIt is the classic total lunar eclipse that many know as Blood Moon.
Although Europe and Spain will be left out of the direct visibility areaThe event will be a global phenomenon: millions of people in the Americas, Asia, Oceania, and the Pacific will be able to watch live as the lunar disk first darkens and then turns a deep reddish hue. For those in Europe, the online broadcasts And interactive resources will be the best way to not miss a single detail of what is happening above their heads, even if the Moon is below the horizon.
What is a total lunar eclipse and why does the Moon turn red?
A lunar eclipse happens when The Earth aligns between the Sun and the Moon, casting its shadow on the satellite. This configuration can only occur in full moon phasewhen the lunar disk is fully illuminated, as if there were no eclipse. In the case of March 2026, the alignment will be so precise that the Moon will completely cross the Earth's umbra, the darkest part of the shadow, resulting in a total eclipse.
The process unfolds in very well-defined stages: first the Moon enters the penumbrawhere the darkening is almost imperceptible; then the central shadow begins to "bite" the disc and the partial eclipseFinally, the satellite is completely immersed in the umbra, a moment we call totality. It is then that its brightness plummets and it adopts its characteristic appearance. reddish or orange tone.
That color is not due to any esoteric mystery, but to the way in which Earth's atmosphere filters sunlightThe sun's rays that graze the edge of the Earth are slightly bent and pass through a thick layer of air, which preferentially scatters blue wavelengths and allows mainly red and orange ones to pass through. This filtered light is what reaches the lunar surface and tints it coppery, as if all the sunrises and sunsets of the planet They will be projected simultaneously onto the Moon.
Hence the talk of “Red Moon” or “Blood Moon”: both expressions ultimately describe the same physical situation. The intensity of the color will vary depending on the amount of dust, clouds, or aerosols in the atmosphere; after large volcanic eruptions, for example, eclipses can appear especially dark and reddish.
Dates, times and duration of the eclipse of March 3, 2026
The March 2026 eclipse will take place between the night of the 2nd and the early morning of the 3rd depending on the region, but All phases are calculated in Universal Time (UTC) to allow for easy comparison. The entire event will last approximately 5 39 hours and minutes, from entering the twilight until the final exit from the Earth's shadow.
The key moments of the phenomenon, expressed in UTC/GMT, are as follows, with information provided by agencies such as NASA and specialized services:
| Time (UTC) | Phase of the eclipse | What happens on the Moon |
|---|---|---|
| 08:44 | Penumbral beginning | The lunar disk enters the twilight; the darkening is very subtle. |
| 09:50 | Partial start | The umbra begins to cover the Moon and a clearly darker area can be seen. |
| 11:04 | Beginning of totality | The Moon is completely immersed in the dark shadow of the Earth. |
| 11:33 | Maximum of the eclipse | The satellite is located in the deepest part of the umbra; the red color is usually more intense. |
| 12:03 | End of all | The moon begins to leave the shadow and the reddish tone becomes lighter. |
| 13:17 | End of the partial phase | The dark shadow completely abandons the lunar disk. |
| 14:23 | End of the penumbral eclipse | Any trace of shading disappears; the Moon regains its usual brightness. |
La The entire sequence lasts approximately 58 minutes. (from 11:04 to 12:03 UTC), and the maximum, when the Moon is most centered within the shadow, coincides with the 11: 33 UTCIt is during this interval that the Moon will show its most intense hue, provided that the weather conditions are favorable in each region.
It's worth remembering that the exact date on the calendar changes depending on the time zone: in much of America, the full sun will be visible in the early hours of the March 3.While in places like New Zealand the moment of maximum eclipse will fall in the early hours of the morning. March 4..
Where will the total lunar eclipse be visible?
In a lunar eclipse there is no narrow band like in solar eclipses: anyone who has the Moon above the horizon During the event, you may be able to observe it, at least in part. However, not all regions will see the same thing. The combination of time zones and moonrise/moonset determines whether you will see the entire eclipse, only a partial eclipse, or nothing at all.
According to visibility forecasts, the geographical distribution of the 2026 Blood Moon will be approximately as follows:
- Fully visibleeastern areas of Asia, the east of Australiapractically all New Zealand, much of the Pacific Ocean and large areas of western North America and Central AmericaIn these regions, it will be possible to follow the complete eclipse or, at the very least, the entire red phase with the Moon at a good altitude.
- Partial or incomplete visibility: central and eastern regions of U.S. and Canada, as well as a good part of South America and sectors of Central AsiaThey will see the eclipse with the Moon low on the horizon, either rising or setting. In many cases, a deep partial phase will be visible, and in the best scenarios in the far west of South America, a few minutes of a red Moon very close to the horizon.
- Eclipse not visible: located on Europe y Africa, including Iberian PeninsulaThe Moon will remain below the horizon throughout the entire phenomenon. Although the event also affects these areas in orbital terms, there will be no way to see it directly from European soil.
In terms of population, it is estimated that around 2.500 million people They live within the area where totality will be visible, according to estimates based on NASA data. This makes the March 3, 2026 eclipse a global astronomical event.
For those who reside outside that area —in the case of Spain or the rest of Europe— the only realistic option to follow him will be to resort to live broadcasts There are already interactive simulators that show the Moon and its passage through the shadow from different points on the planet.
Visibility across large regions of the planet
The scene varies considerably from region to region. Although the core of the phenomenon is the same for everyone, local times, the moon's altitude, and ambient light all influence the actual viewing experience.
En North AmericaFor example, the Pacific coast—the western United States, western Canada, and northwestern Mexico—will have a particularly favorable position. There, it will be possible to contemplate the full eclipse sequence with the Moon relatively high, from the penumbral beginning to the end of the partial phase, passing through a totality well situated in the night sky.
In the central regions of the continent, such as certain areas of the interior of the United States and much of Mexico, the Blood Moon will also be visible, although not always from the beginning of twilight. What's important for the public is that the The red phase will be clearly visibleeven if the start or end of the event occurs with the Moon already close to the horizon.
At the eastern North America and in sectors of the Caribbean and Central America, the entirety will take place with the Moon very low and about to set. This means that the viewing window will be shorter: in some places the reddish Moon will be visible for a few minutes before it finally disappears, while dawn begins to clear the sky.
En South AmericaThe eclipse will arrive late, near dawn. The best conditions will be in the western edge of the continentwhere the Moon will set while passing through the deepest phases of the eclipse. In cities near the Pacific coast, part of the totality may be visible with the Moon almost touching the western horizon, provided the sky is clear and there are no obstructions.
Visibility in Asia, Australia and the Pacific
On the opposite side of the planet, Eastern Asia And the Pacific region will experience the eclipse at more convenient times, coinciding with the late afternoon and evening. This time frame will favor both direct observation and the organization of outreach activities.
At the far east of AsiaIn areas including parts of the Russian Far East and eastern Japan, the Moon will be above the horizon throughout the entire process. In these regions, the disk will be seen gradually entering shadow, reaching its maximum, and then returning to its normal brightness, all under good ambient darkness.
En Eastern China, Korea, and the rest of JapanThe Moon will rise when the eclipse is already underway, appearing on the horizon with part of its disk obscured and gradually gaining altitude as totality approaches. For many enthusiasts, this will be one of the most photogenic sights. a reddish moon rising over the landscape.
The situation is also favorable in Australia and New ZealandIn eastern Australia and in virtually all of New Zealand, it will be possible to follow the full eclipse from beginning to endwith totality well into the night. Western regions of Australia, however, will miss the beginning of the phenomenon because it occurs before moonrise, although they will be able to see the most interesting part, with the moon already eclipsed shortly after sunrise.
El Pacific Ocean Purely due to geometry, it wins the "jackpot": in many islands of the central Pacific, the Moon will be high and the sky dark throughout the red phase. This circumstance makes them ideal locations for capturing images of the eclipse with a sky full of stars, something more difficult when the Moon is low or dawn is approaching.
What will happen in Europe and in Spain?
For those looking at the map from Europe The news isn't particularly cheerful: during this eclipse, the Moon will remain below the horizon throughout the entire event. In other words, the The total lunar eclipse of March 3, 2026 will not be visible from Spainneither from the rest of the European continent, nor from practically any region of Africa.
In astronomical terms, this doesn't mean the Moon doesn't pass through Earth's shadow "over" Europa; it does, but below the local horizon, during daylight hours or before moonrise. From the observer's point of view, the result is simple: There will be nothing to see in the sky.
There remains the option, however, of going to live broadcasts Visualization tools are already available. Specialized platforms and observatories regularly gather images from various locations around the world, allowing users to follow the evolution of the eclipse with high-sensitivity cameras and expert commentary—something especially useful for educational centers, amateur associations, or anyone curious to better understand what is happening.
In addition, various astronomy portals offer interactive simulators These resources show the appearance of the Moon from any point on the planet and at any phase of the eclipse. They offer a convenient way to "experience" the event from Europe, even if the sky above us is completely detached from the spectacle.
Chronology and indicative schedules by time zones
To get an idea of when the red phase will occur in different parts of the world, it is helpful to translate the totality window—of 11:04 to 12:03 UTC— to the most common local time zones. Always keep in mind that this data is for guidance only and that you should check the specifics of each area (time changes, summer time, etc.).
En North AmericaThe approximate local times for the entire event would be:
- Pacific Time (UTC−8): between 03:04 and 04:03 in the morning of March 3.
- Mountain Time (UTC−7): from 04:04 to 05:03.
- Central Time (UTC−6): from 05:04 to 06:03.
- Eastern Time (UTC−5): from 06:04 to 07:03.
En South AmericaTaking as a reference the standard time zones without daylight saving time:
- UTC−5 (Colombia, Peru, Ecuador): from 06:04 to 07:03, with dawn very close and the Moon descending towards the western horizon.
- UTC−4 (Venezuela and part of the Caribbean): from 07:04 to 08:03.
- UTC−3 (Chile, Argentina, Uruguay in standard time): from 08:04 to 09:03, in many cases with a sky so clear that only a partial stretch will be visible before moonset.
En Australia and New ZealandThe entire event will occur during the afternoon or evening hours, with approximate values like these:
- Western Australia (AWST): around 19:04-20:03.
- Eastern Australia (AEST/AEDT, according to summer time): in the 21:00-23:00 time slot, depending on the specific region.
- New Zealand (NZDT): between 00:04 and 01:03 on March 4.
In much of Eastern AsiaThe hours of totality will be approximately between 18:00 and 21:00Depending on the country and its official time zone, during those periods the Moon will already be well positioned in the night sky or rising rapidly from the eastern horizon.
How to safely observe the total lunar eclipse
One of the advantages of lunar eclipses is that they are sure to observe with the naked eyeUnlike solar eclipses, there is no risk to your eyesight from looking directly at the Moon, even during its darkest phase. No filters or special glasses are needed.
To fully enjoy the event, however, it's advisable to take some basic precautions. The first is to keep an eye on the Weather forecastIf clouds dominate the sky, the eclipse may be completely obscured. The second is to find a location with as little light pollution as possible and with clear horizon in the direction the Moon will be (in many areas of America, towards the west, very low during totality).
Sophisticated equipment isn't needed to appreciate the Blood Moon, although a simple pair of binoculars They can make all the difference. With them, the lunar rim features—craters, seas, and mountain ranges—are more clearly visible as the shadow moves, as well as the subtle color variations during the red phase.
Those with a small telescope will be able to observe finer details: the contrast between lighter and darker areas within the eclipsed disk, the transition between penumbra and umbra, or the changes in tone as the Moon approaches the maximum of the eclipse and then moves away.
Besides the Moon, the eclipse itself offers a curious opportunity: as the lunar brightness is so diminished during totality, The neighboring stars and constellations become more visible than a normal full moon. In this case, the satellite will be located in the constellation of Leo, near the well-known star Regulus and the "sickle" shape formed by several stars in that area of the sky.
Practical tips for photographing the Blood Moon
Capturing an eclipse with a camera, even a mobile phone, is one of the most widespread hobbies among those who follow these events. The main challenge is that The brightness of the moon changes a lot Throughout the eclipse: it goes from being very bright during the full phase to being a relatively faint object during totality.
If using a DSLR or mirrorless camera, it is recommended to mount the equipment on a stable tripodDuring partial phases, short exposure times will suffice, but during totality the Moon darkens so much that longer exposure times are usually needed. longer exposures or increase the ISO sensitivity to avoid underexposed photos.
A moderate telephoto lens—around 200-600mm in full-frame format—allows you to fill a good portion of the frame with the lunar disk and highlight its color nuances. As you approach totality, it's advisable to adjust the exposure time and ISO, trying different combinations until you find the right balance. detail and noise acceptable.
A mobile phone can also be used to document the event, especially the partial phases and the appearance of the reddish moon on the horizon. In this case, it's key. support the device On a firm surface or using a small tripod, reduce the exposure to avoid the disc appearing "burned out" and use the zoom sparingly, because digital magnification often degrades the image.
For those who want to add a more creative touch to the matter, a good idea is to include landscape elements In the photograph: buildings, mountains, antennas, or trees that appear in silhouette against the Moon. In areas where totality occurs with the satellite very low, it is possible to frame scenes in which the red Moon is superimposed on a very recognizable urban or natural horizon.
An event within a year full of astronomical phenomena
The total lunar eclipse of March 3rd is part of a A particularly active year for sky observationAlong with other solar and lunar eclipses and a full moon that, according to the calendar, is traditionally called the "Worm Moon" in the Northern Hemisphere. This name refers to the period of thawing when earthworms and other organisms begin to reappear on the soil surface.
In 2026, in addition to this eclipse, other notable phenomena will occur, such as a partial lunar eclipse at the end of August and various striking encounters of the Moon with bright stars and planets. Around the date of the March eclipse, for example, the satellite will pass close to Regulus, the main star of Leo, and days later a spectacular conjunction of Venus and Saturn in the evening sky.
These coincidences make the first half of the year a great time to get started in astronomical observation at a relaxed pace, without the need for long journeys or expensive equipment. For those living in Europe, the fact that they won't be able to directly see the Blood Moon on March 3rd doesn't prevent them from taking advantage of the rest of the celestial calendar.
For reference, after the total eclipse in March there will not be another Blood Moon for almost three years: the next total lunar eclipse It will arrive at the turn of the year. December 31, 2028 to January 1, 2029visible then from large areas of Europe, Africa, and other regions. Before that, in August 2026, there will be a partial lunar eclipse, less striking but also interesting for observing the dynamics of the Earth's shadow on the satellite.
Although each year's astronomical calendars include numerous meteor showers, conjunctions, and other events, a total lunar eclipse still holds a special place. It combines a certain rarity—it doesn't occur every year in the same regions—with the advantage of being a event accessible to all types of audiences, safe and easy to understand from a physical point of view.
With all this, the total lunar eclipse of March 3, 2026, is shaping up to be one of the great astronomical events of the year: a night in which the Moon gives up its usual appearance to show, for less than an hour, the reddish reflection of our own atmosphere on its surface, while millions of people, spread across half the world, follow live the slow advance of the Earth's shadow.
