Space station telescope sees X-ray hot spots merge on supermagnetic star corpse

For the first time, a powerful NASA telescope aboard the International Space Station observed merging "hot spots" on a weird star, known as a magnetar.

The telescope is called the Neutron star Interior Composition Explorer (NICER), and seeks to understand more about the extreme conditions present in super-dense, city-sized neutron stars and their variants. (Magnetars, for example, are a type of neutron star with a strong magnetic field.)

"NICER tracked how three bright, X-ray-emitting hot spots slowly wandered across the object's surface while also decreasing in size, providing the best look yet at this phenomenon," lead researcher George Younes, who has affiliations at George Washington University in Washington, D.C. and NASA's Goddard Space Flight Center in Greenbelt, Maryland, said in an agency statement Tuesday (March 8).

Related: There's a tiny, bright magnetar photobombing our galaxy's supermassive black hole

This plot tracks 37 days of change in SGR 1830’s peak X-ray emission as seen by NASA’s Neutron star Interior Composition Explorer (NICER). Green, yellow and red areas are thought to represent "hot spots" in the magnetar; these regions are producing the greatest number of X-rays. (Image credit: NASA/NICER/G. Younes et al. 2022)

"The largest spot eventually coalesced with a smaller one, which is something we haven’t seen before," Younes added. The team suggests the spots formed and moved due to crustal motion, in a similar process on the small star that the Earth experiences through tectonic plate motions that generate seismic activity.

The magnetar in question is called SGR 1830-0645 (SGR 1830 for short) and lies roughly 13,000 light-years away from Earth. The outburst was first spotted by NASA's cosmic burst-hunting Neil Gehrels Swift Observatory on Oct. 10, 2020. Swift found pulses coming from the object as it rotated every 10.4 seconds. NICER sprang into action the same day, detecting three closely-spaced peaks in the X-ray emission for each rotation of SGR 1830.

The peaks "were caused when three individual surface regions much hotter than their surroundings spun into and out of our view," NASA said. 

An artist’s illustration of the NICER telescope aboard the International Space Station.  (Image credit: NASA's Goddard Space Flight Center)

NICER continued watching SGR 1830 nearly daily between Oct. 10 to Nov. 17, until the sun creeped into the field of view and caused risks with observations. The telescope saw that emission peaks were starting to shift, causing them to happen at different moments in the magnetar's rotation, suggesting crustal motion.

"The crust of a neutron star is immensely strong, but a magnetar's intense magnetic field can strain it beyond its limits," co-author Sam Lander, an astrophysicist at the University of East Anglia in United Kingdom, added in the same statement.

"Understanding this process is a major challenge for theorists, and now NICER and SGR 1830 have brought us a much more direct look at how the crust behaves under extreme stress," Lander said.

The team suggests they saw a single region on the magnetar where the crust is now partly molten, and starting to deform due to extreme magnetic stress. Moreover, the three observed spots are likely locations for coronal loops, which we can see as plasma arcs on the sun connecting to the surface. "The interplay between the loops and crustal motion drives the drifting and merging behavior," NASA said.

A study based on the research was published Jan. 13 in Astrophysical Journal Letters.

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Elizabeth Howell
Staff Writer, Spaceflight

Elizabeth Howell (she/her), Ph.D., is a staff writer in the spaceflight channel since 2022 covering diversity, education and gaming as well. She was contributing writer for for 10 years before joining full-time. Elizabeth's reporting includes multiple exclusives with the White House and Office of the Vice-President of the United States, an exclusive conversation with aspiring space tourist (and NSYNC bassist) Lance Bass, speaking several times with the International Space Station, witnessing five human spaceflight launches on two continents, flying parabolic, working inside a spacesuit, and participating in a simulated Mars mission. Her latest book, "Why Am I Taller?", is co-written with astronaut Dave Williams. Elizabeth holds a Ph.D. and M.Sc. in Space Studies from the University of North Dakota, a Bachelor of Journalism from Canada's Carleton University and a Bachelor of History from Canada's Athabasca University. Elizabeth is also a post-secondary instructor in communications and science at several institutions since 2015; her experience includes developing and teaching an astronomy course at Canada's Algonquin College (with Indigenous content as well) to more than 1,000 students since 2020. Elizabeth first got interested in space after watching the movie Apollo 13 in 1996, and still wants to be an astronaut someday. Mastodon: