NASA's NICER telescope sees hot spots merge on a magnetar

NASA's NICER telescope sees hot spots merge on a magnetar
Scientists think SGR 1830's hot spots likely resembled the bases of coronal loops frequently seen on the Sun. In this extreme ultraviolet view from NASA's Solar Dynamics Observatory, loops of ionized gas trace magnetic fields emerging from the solar surface. Credit: NASA/SDO

For the first time, NASA's Neutron star Interior Composition Explorer (NICER) has observed the merging of multimillion-degree X-ray spots on the surface of a magnetar, a supermagnetized stellar core no larger than a city.

"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," said George Younes, a researcher at George Washington University in Washington and NASA's Goddard Space Flight Center in Greenbelt, Maryland. "The largest spot eventually coalesced with a smaller one, which is something we haven't seen before."

This unique set of observations, described in a paper led by Younes and published Jan. 13 in The Astrophysical Journal Letters, will help guide scientists to a more complete understanding of the interplay between the crust and magnetic field of these extreme objects.

A is a type of isolated neutron star, the crushed core left behind when a massive star explodes. Compressing more mass than the Sun's into a ball about 12 miles (20 kilometers) across, a neutron star is made of matter so dense that a teaspoonful would weigh as much as a mountain on Earth.

What sets magnetars apart is that they sport the strongest magnetic fields known, up to 10 trillion times more intense than a refrigerator magnet's and a thousand times stronger than a typical neutron star's. The magnetic field represents an enormous storehouse of energy that, when disturbed, can power an outburst of enhanced X-ray activity lasting from months to years.

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). In this graph, the star's rotational phase advances from left to right, with the measured energy shown vertically. The green, yellow, and red areas indicate regions producing the greatest numbers of X-rays and are thought to represent the magnetar's hot spots. They change in intensity and in their positions relative to one another as time goes on. For the first time, astronomers recorded two such spots merging. Credit: NASA/NICER/G. Younes et al. 2022

On Oct. 10, 2020, NASA's Neil Gehrels Swift Observatory discovered just such an outburst from a new magnetar, called SGR 1830-0645 (SGR 1830 for short). It's located in the constellation Scutum, and while its distance is not precisely known, astronomers estimate that the object lies about 13,000 light-years away. Swift turned its X-Ray Telescope to the source, detecting repeated pulses that revealed the object was rotating every 10.4 seconds.

NICER measurements from the same day show that the X-ray emission exhibited three close peaks with every rotation. They were caused when three individual surface regions much hotter than their surroundings spun into and out of our view.

NICER observed SGR 1830 almost daily from its discovery to Nov. 17, after which the Sun was too close to the field of view for safe observation. Over this period, the emission peaks gradually shifted, occurring at slightly different times in the magnetar's rotation. The results favor a model where the spots form and move as a result of crustal motion, in much the same way as the motion of tectonic plates on Earth drives seismic activity.

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

The team thinks these observations reveal a single active region where the crust has become partially molten, slowly deforming under magnetic stress. The three moving hot spots likely represent locations where —similar to the bright, glowing arcs of plasma seen on the Sun—connect to the surface. The interplay between the loops and crustal motion drives the drifting and merging behavior.

"Changes in pulse shape, including decreasing numbers of peaks, previously have been seen only in a few 'snapshot' observations widely separated in time, so there was no way to track their evolution," said Zaven Arzoumanian, the NICER science lead at Goddard. "Such changes could have occurred suddenly, which would be more consistent with a lurching magnetic field than wandering ."

NICER is an Astrophysics Mission of Opportunity within NASA's Explorers Program, which provides frequent flight opportunities for world-class scientific investigations from space utilizing innovative, streamlined, and efficient management approaches within the heliophysics and science areas. NASA's Space Technology Mission Directorate supports the SEXTANT component of the mission, demonstrating pulsar-based spacecraft navigation.


Explore further

Properties of magnetar SGR 1830−0645 inspected with NICER

More information: George Younes et al, Pulse Peak Migration during the Outburst Decay of the Magnetar SGR 1830-0645: Crustal Motion and Magnetospheric Untwisting, The Astrophysical Journal Letters (2022). DOI: 10.3847/2041-8213/ac4700
Journal information: Astrophysical Journal Letters

Citation: NASA's NICER telescope sees hot spots merge on a magnetar (2022, March 8) retrieved 14 August 2022 from https://phys.org/news/2022-03-nasa-nicer-telescope-hot-merge.html
This document is subject to copyright. Apart from any fair dealing for the purpose of private study or research, no part may be reproduced without the written permission. The content is provided for information purposes only.
624 shares

Feedback to editors