NASA's Parker Solar Probe mapped an unseen part of the sun at its most active moment

Data from NASA's Parker Solar Probe has enabled astronomers to map the unssen surface of the sun's atmosphere for the first time.

Illustration showing a bright yellow ring with rays of orange yellow light coming out of it, all surrounded by petals of blue and white light against a black background.
An illustration of the sun's elusive Alfvén surface, the point of no return beyond which solar particles stream away as solar wind. The graphic was made with new data collected by NASA's Parker Solar Probe.
(Image credit: CfA/Melissa Weiss)

For the first time, scientists have created detailed, 2D maps of the sun's outermost atmosphere. This feat was accomplished using data from NASA's Parker Solar Probe, which has been dipping in and out of the sun's atmosphere, called the corona, since 2021.

Parker is the first craft in history to fly so close to a star. This ability is largely thanks to its extraordinary heat shield, which can withstand temperatures in excess of 2,500 degrees Fahrenheit (1,370 degrees Celsius). The sun's corona is much hotter — around 1 million to 3 million F (555,000 C) — but it is extremely diffuse, meaning that objects moving swiftly through it don't encounter very many superheated particles. This allows Parker to skim through the outer boundary of the corona for brief periods.

Joanna Thompson
Live Science Contributor

Joanna Thompson is a science journalist and runner based in New York. She holds a B.S. in Zoology and a B.A. in Creative Writing from North Carolina State University, as well as a Master's in Science Journalism from NYU's Science, Health and Environmental Reporting Program. Find more of her work in Scientific American, The Daily Beast, Atlas Obscura or Audubon Magazine.

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