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Spacecraft Enters the Sun’s Corona for the First Time in History

The Parker Solar Probe will help scientists learn more about how our closest star functions

by Harvard-Smithsonian Center for Astrophysics
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CAMBRIDGE, MA — A spacecraft launched by NASA has done what was once thought impossible. On April 28, the Parker Solar Probe successfully entered the corona of the Sun—an extreme environment that’s roughly 2 million degrees Fahrenheit.

The historic moment was achieved thanks to a large collaboration of scientists and engineers, including members of the Center for Astrophysics | Harvard & Smithsonian (CfA) who built and monitor a key instrument onboard the probe: the Solar Probe Cup. The cup collects particles from the Sun’s atmosphere that helped scientists verify that the spacecraft had indeed crossed into the corona. 

“The goal of this entire mission is to learn how the Sun works. We can accomplish this by flying into the solar atmosphere,” says Michael Stevens, an astrophysicist at the CfA who helps monitor the cup. “The only way to do that is for the spacecraft to cross the outer boundary, which scientists call the Alfvén point. So, a basic part of this mission is to be able to measure whether or not we crossed this critical point.”

The corona is the outermost layer of the Sun’s atmosphere where strong magnetic fields bind plasma and prevent turbulent solar winds from escape. The Alfvén point is when solar winds exceed a critical speed and can break free of the corona and the Sun’s magnetic fields. Prior to April 28, the spacecraft had been flying just beyond this point.

“If you look at close-up pictures of the Sun, sometimes you’ll see these bright loops or hairs that seem to break free from the Sun but then reconnect with it,” Stevens explains. “That’s the region we’ve flown into—an area where the plasma, atmosphere, and wind are magnetically stuck and interacting with the Sun.”

According to data collected by the cup, the spacecraft entered the corona three times on April 28, at one point for up to five hours. A scientific paper describing the milestone was published in the Physical Review Letters

CfA astrophysicist Anthony Case, the instrument scientist for the Solar Probe Cup, says the instrument itself is an incredible feat of engineering. 

“The amount of light hitting the Parker Solar Probe determines how hot the spacecraft will get,” Case explains. “While much of the probe is protected by a heat shield, our cup is one of only two instruments that stick out and have no protection. It’s directly exposed to the sunlight and operating at a very high temperature while it’s making these measurements; it's literally red-hot, with parts of the instrument at more than 1,800 degrees Fahrenheit [1,000 degrees Celsius], and glowing red-orange.”

To avoid degradation, the device is constructed of materials that have high melting points, like tungsten, niobium, molybdenum, and sapphire. 

But the success of the Parker Solar Probe represents much more than technological innovation. There are many mysteries about Earth’s closest star that scientists are hoping the probe can help solve. 

For example, “We don’t actually know why the outer atmosphere of the Sun is so much hotter than the Sun itself,” Stevens says. “The Sun is 10,000 degrees Fahrenheit [5,500 degrees Celsius], but its atmosphere is about 3.6 million degrees Fahrenheit [2 million degrees Celsius].”

He adds, "We know that the energy comes from the churning magnetic fields bubbling up through the surface of the sun, but we do not know how the Sun's atmosphere absorbs this energy."

In addition, outbursts from the Sun, like solar flares and high-speed solar winds, can have a direct impact on Earth, disrupting power grids and radio communication.

The Parker Solar Probe can help better understand all these phenomena as it continues to orbit the Sun and take measurements and data for scientists to analyze here on Earth.

Case says, "The plasma around the Sun can act as a laboratory that teaches us about processes taking place in almost every astronomical object across the entire universe."

- This press release was originally published on the Harvard-Smithsonian Center for Astrophysics website