ECLIPSE 2027

The Longest Eclipse of the 21st Century

On August 2, 2027, the skies will once again host an unforgettable celestial event—a total solar eclipse that will blanket the skies over southern Spain, North Africa, and the Middle East in darkness. What makes this astronomical phenomenon truly remarkable is the extraordinary length of its totality, set to be the longest total solar eclipse of the remaining 21st century.

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A Unique Event for Southern Spain and North Africa

While this eclipse will be visible in several regions, southern Spain—especially its coastal areas—will take center stage for witnessing the totality. The experience will extend to Spanish territories outside the peninsula, such as Ceuta and Melilla, offering views of this phenomenon on both sides of the Strait of Gibraltar.

Exceptional Duration: Up to 6 Minutes of Totality

The 2027 eclipse will be renowned for its impressive duration, with totality lasting up to 6 minutes and 23 seconds in Egypt. In southern Spain, locations like Tarifa, Ceuta, and Melilla will experience over 4 and a half minutes of totality, providing an extended and immersive viewing experience.

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Privileged Cities Within the Totality Band

Cities like Málaga and Cádiz will enjoy a significant share of totality. Málaga will experience approximately 2 minutes, while Cádiz will enjoy nearly 3 minutes—ample time to appreciate the visual and emotional impact of this awe-inspiring phenomenon.

  • Back-to-Back Eclipses: 2026 and 2027

Remarkably, this eclipse follows just one year after the Great Spanish Eclipse of 2026, solidifying Spain as a premier destination for astronomy enthusiasts. While the 2026 eclipse’s path of totality spanned much of Spain, the 2027 eclipse will focus on the southern regions of the peninsula.

Southern Spain: The Perfect Eclipse Viewing Spot

Although the central line of the eclipse will not cross Spanish territory, the southern coast will offer spectacular views, with over 4 minutes of totality at many points. Summer weather conditions in the region are typically ideal, with high probabilities of clear skies ensuring unobstructed observation.

A Rare Event Until 2053

The total solar eclipse of 2027 will be one of the final opportunities to witness totality in Europe until 2053. Once again, Spain will be the only European country privileged to host this celestial magic. This phenomenon is more than just a visual spectacle—it’s an opportunity to ponder the vastness of the cosmos and our place within it. Prepare to witness one of the longest eclipses of this century from the sunlit shores of southern Spain.

Meteorology

The 2027 lunar shadow first greets the Earth over the sub-tropical mid Atlantic in a region of moderately cloudy skies well to the north of the hurricane-breeding zone off western Africa. The umbral path misses the islands of Porto Santo and Madeira by a meagre 70 km on its eastward trek, choosing instead to make landfall in Spain and Morocco six minutes later. For the next 4,000 km, it skips along the Mediterranean shore, gradually turning to a southeast heading.  The turn to more southerly latitudes comes with increasing amounts of cloud, but, except in the mountains of Arabia, most of that intrudes after the path heads out across the Indian Ocean, toward its ending near the remote atoll of Diego Garcia.

Few eclipses come with a guarantee of cloud-free skies, but, in parts, the path of the 2027 total across North Africa comes very close (Figure 1). A large part of the eclipse track skirts the north side of the Sahara Desert and August climatology along the shadow path borrows its character from that great sand sea. It’s hot, it’s dry, it’s sunny, and it’s dusty.

Figure 1: A low-resolution map of satellite-derived cloud cover across the eclipse track. Eclipse track: Xavier Jubier. Data: NASA.

An eclipse thrives on that kind of climatology. Some parts of the eclipse track—over Libya and western Egypt—have seen no August cloud on eclipse day whatsoever in the past 23 years. And even though Spain and Northwest Africa have their cloudy days, but it’s not common and eclipse-day chances are still among the best.

Most of this good weather comes courtesy of the Azores (or Bermuda) high over the mid-Atlantic that extends a ridge of higher pressures along the track. It’s not until the shadow reaches Egypt that the anticyclone gives way to lower pressures, but these are lows generated by the heating of the land and don’t share the cloud-making character of their more traditional counterparts. Instead, cloud along the track usually follows the wind flow: winds off of the land tend to bring dry weather, while flows of off the Mediterranean or the Red Sea bring clouds. High-level winds bring larger weather systems with larger cloud shields. When terrain is added to the mix, high elevations are where clouds go when all else is dry. After the shadow leaves the African continent for the Arabian Peninsula, sunshine prospects begin to weaken, but even here there are clear-sky refuges that will tempt the most fastidious eclipse chaser.

Figure 4’s graph, which shows the satellite-derived cloud cover along the centerline and the north and south limits, provides a more detailed look at cloud cover along the track. In some cases, eclipse travellers will be better off to deviate off of the centerline to the north or south to take advantage of better cloud prospects.

Spain, Gibraltar and Morocco

This total eclipse is the first of two in this small part of the world; an annular eclipse will follow in just five months, in January 2028. For this 2027 event, the umbral shadow passes primarily over the Alboran Sea (Figure 2), but along the way, touches coastal Andalusia, the autonomous Spanish cities of Ceuta and Melila in North Africa, northern Morocco, and the British territory of Gibraltar.

Figure 2: Topographic map of the Alboran Sea and surrounding area along the eclipse track. Eclipse track: Xavier Jubier. Data: NASA.

The region has a dry sub-tropical climate moderated by the influences of a cold Atlantic Ocean and a warm Mediterranean Sea alongside a rough mountain terrain that abuts the Mediterranean coast. Even tiny Gibraltar has its 426-metre “Rock” to loom over the entrance to the Strait. Wind is an important component of the weather in this area, almost exclusively blowing from either the east (Levanter) or the west (Poniente) across the Alboran Sea and the Gulf of Cadiz. The Levanter (Levante in Spanish) tends to be the more persistent, sometimes blowing steadily for days and even weeks, particularly in the summer months. The two winds make the Strait and the Gulf of Cadiz prime spots for kite boarding and wind surfing.

Figure 3: Early afternoon cloud fraction along the eclipse track extracted from observations made by the Aqua polar-orbiting satellite between 2004 and 2023. Eclipse track: Xavier Jubier. Data: NASA.

In Figure 3, a map of cloud fraction (or percent monthly cloud if multiplied) derived from two decades of satellite observation shows that the waters of the Alboran Sea and the Strait of Gibraltar are cloudier than any other region along the African portion of the track. Fed by inflowing Atlantic currents, the cool surface waters of the Alboran Sea create a stable, surface-based temperature inversion during a Levanter. Air beneath the inversion often (but not always) turns to fog, stratus, and haze as it is cooled from below. This low cloud is thickest in the morning and evening, but seldom penetrates more than a few kilometres inland and usually much less. In the summer months, the Levanter is generally a moderate breeze and its impact on the weather is muted. Because much of the Strait cloudiness forms at a low level in the atmosphere, it is quick to erode as temperatures rise during the day, though that may be too late for an eclipse that occurs at mid-morning. More detail about the cloud climatology is provided in the graph of cloudiness along the centerline and both limits (Figure 4). In this graph, you can determine the value of going off of the centre line in search of a better climatology. Land-based sites are significantly more promising than those over or near water (compare the overwater centreline between Ceuta and Oran with terrestrial paths of both the north and south limits). High terrain also provides less favourable weather prospects: Cloud cover climbs about 8 percent as the south limit crosses the Rif Mountains in Morocco, and nearly 14 percent on the south limit across the Tel Atlas Range between Sebdou and Djelfa in Algeria.

Figure 4: A graph of August cloud fraction derived from the same dataset as in Figure 3. Station names are placed on the traces according to their location with respect to that part of the track. In general, maximum cloud amounts are associated with an over-water passage or higher terrain. Data: NASA.

In Gibraltar, the Levanter is responsible for a streaming flag of cloudiness that frequently flies from the upper slopes of the Rock of Gibraltar, typically when the wind blows between 15 and 40 km/h. This monolithic limestone rock lifts the Levanter wind and condenses its moisture into a long, flowing cloud banner that stretches downwind from the peak. The size and persistence of this iconic banner depends on the strength of the wind, the amount and depth of the moisture, and the stability of the air and can take on many engaging forms, all hanging unmoving from the peak. Eclipse observers should pay close attention to the wind forecast and position themselves off to the side of the peak if the Levanter is active but it could also present an attractive photo opportunity. The eclipse lies in an easterly direction (095°) at relatively low altitude (38°) from Gibraltar. Because the banner is stationary, it is easily avoided or, if you want, engaged.

Table 1: Climate data for selected sites in Spain, Gibraltar, and Morocco.

The opposing wind, the Poniente, is a dry westerly or northwesterly wind that brings good visibility in the summer months – enough to see the coast of Africa from Tarifa. It’s not as frequent as the Levanter and generally a bit weaker. Outside the Strait, at Cádiz, the Poniente is a cool and humid flow that moderates the high temperatures of summer. East or west wind, cloud cover is very low across inland Spain during the summer dry season, averaging 15-20 percent everywhere beneath the shadow path between Cadiz and Málaga. Rainfall amounts to only a few millimetres in August (Table 1).

Figure 5: Terra satellite image of the cloud cover on August 2, 2022. Note the packing of cloud against the coast of Morocco. Image: NASA.

Topography along both coasts of the Alboran Sea also has a significant regional influence on cloudiness. The western end of the Alboran Sea is constrained by the Sierra de las Nieves on the Spanish side and by the Rif Mountains of Morocco on the south. While the terrain on the Spanish side has only a small influence on cloudiness, that on the Moroccan side has a dramatic impact. The coastline of Morocco forms a scooped or basin shape, capturing the easterly Levanter as it impacts the coast (Figure 5). The stratus cloud and the rare weather systems that move over the Alboran Sea occasionally pack up against this coast, pressing cloud against the Rif Mountains, which the cloud is unable to cross. The average August cloud amount reaches nearly 50 percent east of Ceuta in Figure 3. Sunshine observations at Melila average only 61 percent of the maximum possible, well below the 75 to 80 percent at many other locations along the track (Table 1). Cloud piles up against the Rif Mountains impacts the cities of Ceuta, Martil, and Tetouan, significantly reducinf the frequency of sunny hours at Melila and Al Hoceima in Table 1. In Spain, the terrain is most likely to produce convective cloud in the afternoon, sometimes in concert with weak summer cold fronts that sweep across the region and extend into inland Africa. On the Atlantic side of the Strait, and along the ocean-facing coasts of Spain and Morocco, cloud cover changes its character. The flow out of the Strait sometimes creates a “streamer” of cloud that may turn and hug the coast for a short distance to the north or south, but these are uncommon. More frequently, marine clouds or fog moves onto the Atlantic coast of Morocco, though it doesn’t penetrate far inland. Morning convective clouds buildups are common on the mountains and may turn into severe thunderstorms in the afternoon, but this should not be a major problem in the morning when the shadow passes. In spite of the impact of terrain and water, most cloudiness that affects North Africa is not local in origin. There is a moderate amount of mid and high-level cloud that arrives with weather systems that are familiar to Europeans and North Americans. Cold fronts from the Atlantic and Spain occasionally sweep southward across the eclipse track bringing bands of broken cloud from Morocco to Tunisia. The sub-tropical jet stream usually lies across Spain in August, but often dips southward to carry mid- and high-level cloud through the region. Saharan lows bring hot, dusty weather northward while small Mediterranean lows spread cloud and precipitation along the coasts and onto the shadow path. Thunderstorms frequently form on the mountains on either coast and spread cirrus and mid-level cloud downwind though, fortunately, are creatures of the afternoon and the eclipse is in the morning. Overall, however, such systems are infrequent and sunny weather dominates. Most of these larger weather systems will affect the early part of the eclipse track, from Tangier to Sfax, after which the coastline dips sharply southward and the track turns to the southeast, away from the temperate-zone storms and into the desert climatology.

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