No, the world will not go dark this weekend. Rumors about a lengthy total solar eclipse may have been circulating online, but the so-called “eclipse of the century” isn’t for another two years.
A total solar eclipse lasting up to 6 minutes and 23 seconds, at its peak, is expected to occur on Aug. 2, 2027, according to NASA. The total solar eclipse, in which the moon moves perfectly between the sun and Earth and casts a shadow on Earth, will be one of the longest in several decades.
For a time comparison, the total solar eclipse that occured on April 8, 2024, lasted 4 minutes and 28 seconds at its peak. The solar eclipse of 1991, however, lasted 6 minutes and 53 seconds. Space.com reports the Aug. 2, 2027 eclipse will be the longest eclipse totality until 2114.
The eclipse will be visible in parts of Africa, Europe and the Middle East. Unfortunately for American skywatchers, the vast majority of the U.S. won’t have a view of it.
The Aug. 2, 2027 solar eclipse isn’t actually the next total solar eclipse though. That one, on Aug. 12, 2026, will be visible in Greenland, Iceland, Spain, Russia and parts of Portugal, according to NASA.
Here’s what to know about the solar eclipse on Aug. 2, 2027.
Where will the solar eclipse on Aug. 2, 2027 be visible?
The solar eclipse’s path of totality will cross over parts of Africa, Europe and the Middle East, according to National Eclipse and NASA.
Parts of the following countries are within the path of totality.
Spain
Morocco
Algeria
Tunisia
Gibraltar
Libya
Sudan
Egypt
Saudi Arabia
Yemen
Somalia
Other countries in Africa, Europe and the Middle East will have a partial view of the eclipse.
Will the Aug. 2, 2027 solar eclipse be visible in the US?
A partial solar eclipse will be visible in parts of Maine between 5:14 and 5:19 a.m. ET on Aug. 2, 2027, according to Time and Date.
Greta Cross is a national trending reporter at USA TODAY. Story idea? Email her at gcross@usatoday.com.
This article originally appeared on USA TODAY: Total solar eclipse on Aug. 2, 2027 will be special. Here’s why.
