NASA’s Next Solar Mission Will Use Six Spacecraft to Make One Giant Telescope

Want to build the largest radio telescope to fly in space? Here’s an easier technique: Design six tiny satellites to fly in formation and work together.

That’s the approach of a NASA’s new Sun Radio Interferometer Space Experiment (SunRISE) mission, which is scheduled to launch no earlier than July 2023. SunRISE aims to help scientists understand the complex relationship between the sun’s activity and a host of dangerous phenomena around Earth called space weather. The mission selection comes amid a burst of solar science and an emphasis on missions that incorporate space-weather prediction into plans for human spaceflight beyond low Earth orbit.

“We are so pleased to add a new mission to our fleet of spacecraft that help us better understand the sun, as well as how our star influences the space environment between planets,” Nicky Fox, director of NASA’s Heliophysics Division, said in a NASA statement. “The more we know about how the sun erupts with space weather events, the more we can mitigate their effects on spacecraft and astronauts.”

Scientists have watched the sun fling energy and material toward Earth in outbursts, and they have also seen the impacts that such events can have on orbiting satellites, particularly on communication and navigation instruments. But scientists don’t yet understand the nitty-gritty details of the connection between solar outbursts and space weather phenomena well enough to predict space weather.

If all goes well, the $63-million SunRISE mission should help to bridge that gap. 

The six telescopes that make up the mission are tailored to study the radio waves that the sun ejects during solar particle outbursts. In particular, SunRISE will target outbursts called coronal mass ejections, which can throw massive amounts of plasma, the soup of charged particles that makes up the sun, across the solar system.

The toaster-sized satellites will spread out across about 6 miles (10 kilometers), orbiting Earth at an altitude of 22,000 miles (35,000 km). That orbit will keep SunRISE well above the ionosphere, which blocks radio waves of the relevant frequencies from reaching Earth.  

From that perch, the flock of cubesats should be able to map the influence of the sun’s magnetic field across space. They should also be able to gather the data scientists need to understand how different parts of a coronal mass ejection dramatically speed up and which such events are accompanied by bursts of radiation, which are vital clues for space-weather prediction.

“We can see a solar flare start, and a coronal mass ejection start lifting off from the sun, but we don’t know if it is going to produce high energy particle radiation, and we don’t know if that high energy particle radiation is going to reach Earth,” Justin Kasper, a space scientist at the University of Michigan who leads the mission, said in a university statement. “One reason why is we can’t see the particles being accelerated. We just see them when they arrive at the spacecraft, which isn’t much of a warning.”

That situation is inconvenient when it comes to satellites, but downright dangerous when it comes to humans venturing beyond the safety of Earth, hence the impetus to better understand space weather.

“Knowing which part of a coronal mass ejection is responsible for producing the particle radiation will help us understand how the acceleration happens,” Kasper said. “It could also result in a unique warning system for whether an event will both produce radiation and release that radiation towards Earth or spacefaring astronauts.”

Copyright 2020 Space.com, a Future company. All rights reserved. This material may not be published, broadcast, rewritten or redistributed.