Getting ready for the solar eclipse | Science News for Students

Getting ready for the solar eclipse

On August 21, the moon’s shadow will race from Oregon to South Carolina
Apr 27, 2017 — 7:10 am EST

On August 21, a solar eclipse will be viewable across the United States. Those who want to take a look will need eye protection, though. Looking directly at a solar eclipse without such protection can damage the eyes.


Eeriness creeps in. Colors change and shadows sharpen. The last minutes before a total eclipse of the sun triggers a primal reaction, says astronomer Jay Pasachoff.

“You don’t know what’s going on,” says Pasachoff. “But you know something is wrong.”

Millions of people will encounter this reaction on August 21, 2017. That’s when a total eclipse of the sun will sweep across the continental United States. This will be the first eclipse to grace the country since 1979. And it will be the first since 1918 to bring a total, if temporary, blackout coast-to-coast. Its path will be roughly 120 kilometers (75 miles) wide. Created by the moon’s shadow, this so-called totality will pass through 12 states, from Oregon to South Carolina.

Researchers and the public alike have been gearing up to make the most of this rare spectacle. After all, U.S. communities won’t get another chance until 2024.

Story continues below map.

eclipse path
On August 21, a solar eclipse will race across the United States.
Wolfgang Strickling/Wikimedia Commons (CC-BY-SA 2.5)

The mystery of the eclipse

A solar eclipse occurs when the moon passes between the sun and our planet, casting its shadow on Earth. For someone sitting on Earth viewing the eclipse (with some kind of eye protection), it appears that the moon nearly blots out the sun. A total solar eclipse occurs about once every 18 months.

Eclipse enthusiasts will travel from all over the world to experience up to nearly three minutes of midday twilight and glimpse the sun’s corona (Koh-ROH-nah). The outer layer of the sun, it is an intensely hot, ionized gas, or plasma. During a total eclipse, this seldom-seen halo of light will frame the blacked-out sun.

eclipse corona
During a solar eclipse, the moon blocks out the sun. That allows people to see the sun’s corona (as visible in this picture from a 1999 eclipse).
Luc Viatour/Wikipedia Commons, (CC-BY-SA-3.0)

At its sight, “People cheer and people cry,” Pasachoff says of Williams College in Williamstown, Mass. And he should know. He’s already witnessed 33 total solar eclipses and 30 partial ones.

People like him will often have to travel to the far ends of the Earth to experience an eclipse. That’s because eclipses that pass over densely populated portions of the planet are fairly rare. This explains why the 2017 event is so special. Millions will be able to experience it firsthand, often without leaving home.

For scientists, an eclipse offers more than an interesting experience, though. It’s a time to study the corona. Though some of it is visible all of the time to a few telescopes in space, the region where the corona meets the surface is masked by the sun’s intensity. “Only on days of eclipses can we put together a complete view of the sun,” Pasachoff explains. For researchers, the 2017 eclipse is thus another chance to connect what they see on the surface of the sun to what’s happening in the outer reaches of its corona.

One enduring mystery relates to temperatures on the sun. The sun’s surface is a relatively balmy 5,500° Celsius (nearly 10,000° Fahrenheit). But the corona is millions of degrees hotter. Scientists still aren’t really sure why. “The consensus is that the sun’s magnetic field is responsible,” says Paul Bryans. “But it’s not clear how,” he adds. Bryans works as a solar physicist at the National Center for Atmospheric Research in Boulder, Colo.

The magnetic field in the corona is too tenuous to study directly. Instead, researchers hope one day to measure the effect of magnetism on certain wavelengths of infrared light emitted by the corona. Bryans is leading a team that will point a device called a spectrometer (Spek-TROM-eh-tur) at the sun during the eclipse to detect that light.

“The plan is to put us in the back of a trailer, drive north to Wyoming and just sit and stare at the sun,” says Bryans, for whom the 2017 eclipse will be his first. “People keep telling me it’s a terrible thing to do because I’ll be stuck in the back of the trailer.”

This experiment will test whether the corona emits light at the predicted wavelengths and, if so, how brightly. (Scientists will have to wait for improved instruments and another eclipse to see how these wavelengths are distorted by the magnetic field.) One of the advantages of a mobile observatory, Bryans says, is that the team can look at weather forecasts the day before and drive to clear skies.

Another option is to point an infrared spectrometer out the window of a Gulfstream V jet. The researchers could then cruise at an altitude of about 15 kilometers (9 miles) along the path of the eclipse and make measurements. That is what Jenna Samra will be doing. She is a physics graduate student at Harvard University in Cambridge, Mass. Aside from getting away from weather intrusions, the flying telescope will soar above much of Earth’s water vapor, which absorbs a lot of the sun’s infrared light.

The moon’s shadow will race across the country at about 2,700 kilometers (1,700 miles) per hour. Only the world’s fastest military planes are capable of flying that fast. “We won’t be able to keep up with it,” Samra says. The jet her team uses will collide with the shadow in southwest Kentucky. “We will be able to stay in for about four minutes,” she says. That’s more than a minute longer than for anyone stuck on the ground.

Viewing the eclipse

eclipse 2017
This animation shows the path the moon’s shadow will take during the 2017 eclipse. Wherever the gray shadow falls, people will see a partial eclipse. Only those standing in the path of the black dot will see a total eclipse. (Time is given in Universal Time. Central duration time, lower right, tracks how long the sun will appear blacked out to an observer on the ground.)
A. Sinclair/HM Nautical Almanac Office

For observers on Earth, the eclipse first touches U.S. soil at 10:16 a.m. Pacific time near Oregon’s Depoe Bay. The shadow will move through five state capitals — Salem, Ore.; Lincoln, Neb.; Jefferson City, Mo.; Nashville, Tenn.; and Columbia, S.C. It will even cross a few national parks: Grand Teton, Great Smoky Mountains and Congaree. A spot in the Shawnee National Forest (just southeast of Carbondale, Ill.) has the honor of longest time in darkness: about 2 minutes, 42 seconds. Cape Island, S.C., is the shadow’s final stop. The shadow will then leave the continent around 2:49 p.m. Eastern time, just about an hour and a half after it had entered Oregon.

Based on typical climate patterns in late August, the weather has a better chance of cooperating in the western half of the eclipse path, from Oregon to western Nebraska. That’s why Pasachoff will be setting up in Salem, Ore. He won’t be looking for elusive infrared light. Instead, he will be taking rapid-fire images of plasma loops arcing off the sun. For a brief time, they will peek out from behind the moon.

These loops are coils of ionized gas trapped in billowing magnetic fields. One idea for why the corona is so hot is that these loops subtly jiggle. That is thought to stir up the surrounding plasma and heat the corona. By looking for oscillations along the loops, Pasachoff’s team will see if this hypothesis holds up.

The sun won’t be the only thing that’s probed during the eclipse. Some researchers will be keeping an eye on Earth’s atmosphere to see how it responds to a sudden loss of sunlight. Angela Des Jardins is a solar physicist at Montana State University in Bozeman. She is leading the national Eclipse Ballooning Project. Its scientists will launch more than 100 weather balloons at various times along the path of totality. Those balloons will measure changes in such things as temperature and wind speed.

For those who can’t make it to the eclipse path, or who get stuck under cloudy skies, the ballooning project will serve up live feeds from a vantage point unlike any other. Those balloons will soar roughly 30 kilometers (18 miles) above the ground. More than 50 teams of high school and college students will launch cameras on additional balloons from 30 sites along the eclipse path. Video and photos will be transmitted as they’re taken. These will be accessible via a website.

From 30 kilometers up, “you can really see the curvature of Earth and the blackness of space,” says Des Jardins. “Seeing the shadow of the moon come across the Earth gives you an amazing perspective of what’s going on.”

This NASA animation shows the path the moon’s shadow will follow on August 21 as it crosses the United States.

Power Words

(for more about Power Words, click here)

atmosphere     The envelope of gases surrounding Earth or another planet.

coil     Concentric rings or spirals formed by winding wire or some other fiber around and around a core; or the shape that such a wire would make.

consensus     An opinion or conclusion shared by most, if not all, of a specific group.

continent     (in geology) The huge land masses that sit upon tectonic plates. In modern times, there are six geologic continents: North America, South America, Eurasia, Africa, Australia and Antarctica.

corona     The envelope of the sun (and other stars). The sun’s corona is normally visible only during a total solar eclipse, when it is seen as an irregularly shaped, pearly glow surrounding the darkened disk of the moon.

eclipse     This occurs when two celestial bodies line up in space so that one totally or partially obscures the other. In a solar eclipse, the sun, moon and Earth line up in that order. The moon casts its shadow on the Earth. From Earth, it looks like the moon is blocking out the sun. In a lunar eclipse, the three bodies line up in a different order — sun, Earth, moon — and the Earth casts its shadow on the moon, turning the moon a deep red.

field     (in physics) A region in space where certain physical effects operate, such as magnetism (created by a magnetic field), gravity (by a gravitational field) or mass (by a Higgs field).

graduate student     Someone working toward an advanced degree by taking classes and performing research. This work is done after the student has already graduated from college (usually with a four-year degree).

high school     A designation for grades nine through twelve in the U.S. system of compulsory public education. High-school graduates may apply to colleges for further, advanced education.

hypothesis     A proposed explanation for a phenomenon. In science, a hypothesis is an idea that must be rigorously tested before it is accepted or rejected.

infrared light     A type of electromagnetic radiation invisible to the human eye. The name incorporates a Latin term and means “below red.” Infrared light has wavelengths longer than those visible to humans. It tends to record heat signatures of an object or the environment.

magnetic field     An area of influence created by certain materials, called magnets, or by the movement of electric charges.

magnetism     The attractive influence, or force, created by certain materials, called magnets, or by the movement of electric charges.

mass     A number that shows how much an object resists speeding up and slowing down — basically a measure of how much matter that object is made from.

moon     The natural satellite of any planet.

observatory     (in astronomy) The building or structure (such as a satellite) that houses one or more telescopes.

Pacific     The largest of the world’s five oceans. It separates Asia and Australia to the west from North and South America to the east.

physicist     A scientist who studies the nature and properties of matter and energy.

planet     A celestial object that orbits a star, is big enough for gravity to have squashed it into a roundish ball and it must have cleared other objects out of the way in its orbital neighborhood. To accomplish the third feat, it must be big enough to pull neighboring objects into the planet itself or to sling-shot them around the planet and off into outer space.

plasma     (in chemistry and physics) A gaseous state of matter in which electrons separate from the atom. A plasma includes both positively and negatively charged particles.

solar eclipse     An event in which the moon passes between the Earth and sun and obscures the sun, at least partially. In a total solar eclipse, the moon appears to cover the entire sun, revealing on the outer layer, the corona. If you were to view an eclipse from space, you would see the moon’s shadow traveling in a line across the surface of the Earth.

spectrometer     An instrument that measures a spectrum, such as light, energy, or atomic mass. Typically, chemists use these instruments to measure and report the wavelengths of light that it observes. The collection of data using this instrument (a process is known as spectrometry) can help identify the elements or molecules present in an unknown sample.

subtly     An adverb to describe something that may be important, but can be hard to see or describe. For instance, the first cellular changes that signal the start of a cancer may be only subtly different — as in small and hard to distinguish from nearby healthy tissues.

sun     The star at the center of Earth’s solar system. It’s an average size star about 26,000 light-years from the center of the Milky Way galaxy. Or a sunlike star.

telescope     Usually a light-collecting instrument that makes distant objects appear nearer through the use of lenses or a combination of curved mirrors and lenses. Some, however, collect radio emissions (energy from a different portion of the electromagnetic spectrum) through a network of antennas.

totality    The period of an eclipse when one object is totally obscured by another. In a solar eclipse, this is when (as viewed from Earth) the moon appears to completely block out the sun’s light.

Universal Time    The time set for some standard location, such as Greenwich, England, against all local time zones will be measured. Unlike Greenwich Mean Time, which goes from midnight one day to midnight the next, Universal Time also can be measured from noon to noon.

water vapor     Water in its gaseous state, capable of being suspended in the air.

wavelength     The distance between one peak and the next in a series of waves, or the distance between one trough and the next. Visible light — which, like all electromagnetic radiation, travels in waves — includes wavelengths between about 380 nanometers (violet) and about 740 nanometers (red). Radiation with wavelengths shorter than visible light includes gamma rays, X-rays and ultraviolet light. Longer-wavelength radiation includes infrared light, microwaves and radio waves.

weather     Conditions in the atmosphere at a localized place and a particular time. It is usually described in terms of particular features, such as air pressure, humidity, moisture, any precipitation (rain, snow or ice), temperature and wind speed. Weather constitutes the actual conditions that occur at any time and place. It’s different from climate, which is a description of the conditions that tend to occur in some general region during a particular month or season.


Meeting: A.C. Des Jardins et al. National Eclipse Ballooning Project. 47th meeting of the American Astronomical Society Solar Physics Division, Boulder, Colo., June 1, 2016.

Meeting: P. Bryans et al. Measuring the IR solar corona during the 2017 eclipse. 47th meeting of the American Astronomical Society Solar Physics Division, Boulder, Colo., June 3, 2016.

Meeting: J. Samra et al. An airborne infrared spectrometer for solar eclipse observations. 47th meeting of the American Astronomical Society Solar Physics Division, Boulder, Colo., June 3, 2016.