On Aug. 21, the moon’s shadow will roll across the U.S., as tens of millions of Americans witness a total solar eclipse.
The great American eclipse
Why do total eclipses occur?
Occasionally, the moon’s elliptical orbit carries it directly between the sun and Earth, placing all three celestial objects in complete alignment. The moon’s shadow then falls across Earth’s surface, ultimately appearing to blot out the sun entirely. The phenomenon isn’t especially rare, occurring somewhere on Earth every 18 months or so. But from any single given spot, a total solar eclipse is observable only once in 375 years. This one will be the first anywhere in the U.S. since 1979, and the first since 1918 to be visible from coast to coast. It will also be the first solar eclipse to be seen only on American soil since 1776. “The path of totality will cross through a whopping 14 states,” says astrophysicist Ethan Siegel. “More than 12 million people will get to experience totality without ever leaving their homes.”
What will eclipse gazers see?
It’s a gradual process, beginning with first contact—“when the sun and moon ‘touch,’” explains NASA heliophysicist Mitzi Adams. “This leads to the partial phase, when it looks like someone is taking increasingly large bites from the sun. Next is the actual eclipse itself, when the sun is totally covered by the moon.” All that is visible then is the solar corona, the sun’s gaseous halo, which peeks out from the blackness. Totality lasts from a few seconds to just over two minutes, depending on where you view it. The sun’s brightness in the totality falls by a factor of 1 million, temperatures plummet by as much as 20 degrees, and winds fall still. “Some animals react,” Adams says. “Cows may start walking toward the barn. Crickets start chirping.” Indeed, the sheer strangeness of eclipses has inspired fascination—and fear—since ancient times.
For centuries, people saw eclipses as omens, perhaps as harbingers of Doomsday. “When anything extraordinary happens in nature it stimulates a discussion about instability in the universe,” says astronomer Anthony Aveni. In Indian mythology, it was believed eclipses occur because the Hindu demon Rahu continually chased the sun and occasionally swallowed it up. The Babylonians, one of the first civilizations to study the cosmos, believed eclipses heralded the death of their king; by the 8th century B.C. they had devised mathematical formulas that predicted them. (To “fool” an impending eclipse, they’d dress someone up—usually a condemned man—as a substitute monarch.) Greek historian Herodotus credits the philosopher Thales with accurately predicting the solar eclipse of May 28, 585 B.C. “People realized there were patterns,” says astronomer Tyler Nordgren. “If it is a dragon eating the sun, then evidently the dragon works on a timetable.”
What’s the timing of this eclipse?
Beginning at 10:16 a.m. in Government Point, Ore., the eclipse will follow a 67-mile-wide path from Oregon through Idaho, Wyoming, Nebraska, Kansas, Iowa, Missouri, Illinois, Kentucky, Indiana, Tennessee, North Carolina, Georgia, and South Carolina—ending near Charleston at 2:48 p.m. Some 75 million people live within a 200-mile drive of the totality path, and large crowds are expected to gather in towns and cities along the route, snarling traffic and straining infrastructure and emergency responders. To prepare, communities are coordinating with government, law enforcement, and food vendors, and ferrying in portable cellphone towers. Glendo, Wyo.—population 200—set up an airstrip viewing area to accommodate some 20,000 visitors. Eclipse watchers are advised to bring their own food and water and take appropriate safety precautions (see box). “The biggest shortage on the day will probably be port-a-potties,” predicts geographer Michael Zeiler.
Will scientists learn anything from the eclipse?
They usually do. For example, reduced glare during the total eclipse of 1919 enabled British astronomers Arthur Eddington and Frank Watson Dyson to observe the extent to which solar gravity bends starlight—confirming a key prediction of Einstein’s general theory of relativity. This year, in a project dubbed EclipseMob, astronomers across the country will use special radio receivers to study the ionosphere, an atmospheric region between 46 and 621 miles above Earth ionized by solar and cosmic radiation. Day-to-night ionospheric fluctuations can disrupt radio waves and communications systems. (Ion reduction after sundown is one reason AM stations come through better at night.)
Are there other projects?
In Citizen CATE (Continental-America Telescope Eclipse), astronomers from coast to coast plan to splice film footage into the longest-ever movie of a total solar eclipse—about 90 minutes’ running time. Their primary goal is to analyze the solar corona. Normally almost invisible, the corona is revealed in striking detail during an eclipse. It’s a turbulent region, with temperatures up to 3.5 million degrees Fahrenheit, swirling solar winds, and coronal mass ejections—scorching ionized particles that fly toward Earth, pummeling our atmosphere and sparking the aurora borealis. These ejections pose threats to astronauts, satellites, and ground-based technology, and generate powerful currents that can short out power stations, potentially imperiling the grid. CATE researchers have meticulously synchronized their specialized cameras; there’s no chance for retakes until the next total eclipse in the U.S. in 2024. “You have to be ready when totality starts,” says astronomer Matt Penn, “because you can’t stop the moon.”