The sun is about to pull another disappearing act across North America, turning day into night during a total solar eclipse.
The peak spectacle on April 8 will last up to 4 minutes, 28 seconds in the path of total darkness — twice as long as the total solar eclipse that dimmed U.S. skies in 2017.
This eclipse will take a different and more populated route, entering over Mexico’s Pacific coast, dashing up through Texas and Oklahoma, and crisscrossing the Midwest, mid-Atlantic and New England, before exiting over eastern Canada into the Atlantic.
An estimated 44 million people live inside the 115-mile-wide (185-kilometer-wide) path of totality stretching from Mazatlán, Mexico to Newfoundland; about 32 million of them are in the U.S., guaranteeing jammed roads for the must-see celestial sensation.
The eclipse will allow many to share in the “wonder of the universe without going very far,” said NASA’s eclipse program manager Kelly Korreck.
Here’s what to know about April’s extravaganza and how to prepare:
What happens during the total solar eclipse?
The moon will line up perfectly between the Earth and the sun, blotting out the sunlight. It will slice a diagonal line from the southwest to the northeast across North America, briefly plunging communities along the track into darkness.
On April 8, a total solar eclipse will cross North America. It will be the last one visible from the contiguous United States until 2044. Here’s what viewers should expect to see during each stage of the eclipse. (Feb. 16) (AP video: Christine Nguyen)
Fifteen U.S. states will get a piece of the action, albeit two of them — Tennessee and Michigan — just barely.
Among the cities smack dab in the action: Dallas; Little Rock, Arkansas; Indianapolis, Cleveland; Buffalo, New York; and Montreal — making for the continent’s biggest eclipse crowd.
Don’t fret if you don’t have front-row seats. Practically everyone on the continent can catch at least a partial eclipse. The farther from the path of totality, the smaller the moon’s bite will be out of the sun. In Seattle and Portland, Oregon, about as far away as you can get in the continental U.S., one-third of the sun will be swallowed.
Why is totality longer?
By a cosmic stroke of luck, the moon will make the month’s closest approach to Earth the day before the total solar eclipse. That puts the moon just 223,000 miles (360,000 kilometers) away on eclipse day.
The moon will appear slightly bigger in the sky thanks to that proximity, resulting in an especially long period of sun-blocked darkness.
What’s more, the Earth and moon will be 93 million miles (150 million kilometers) from the sun that day, the average distance.
When a closer moon pairs up with a more distant sun, totality can last as long as an astounding 7 1/2 minutes. The last time the world saw more than seven minutes of totality was in 1973 over Africa. That won’t happen again until 2150 over the Pacific.
