• NASA's NICER telescope sees hot spots me

    From ScienceDaily@1:317/3 to All on Tuesday, March 08, 2022 21:30:40
    NASA's NICER telescope sees hot spots merge on a magnetar

    Date:
    March 8, 2022
    Source:
    NASA/Goddard Space Flight Center
    Summary:
    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.



    FULL STORY ==========================================================================
    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 magnetar 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.

    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
    coronal loops - - 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 hot spots." 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 astrophysics science areas. NASA's
    Space Technology Mission Directorate supports the SEXTANT component of
    the mission, demonstrating pulsar-based spacecraft navigation.


    ========================================================================== Story Source: Materials provided by
    NASA/Goddard_Space_Flight_Center. Original written by Francis Reddy. Note: Content may be edited for style and length.


    ========================================================================== Related Multimedia:
    * YouTube_video:_NASA's_NICER_Tracks_a_Magnetar's_Hot_Spots ========================================================================== Journal Reference:
    1. George Younes, Samuel K Lander, Matthew G. Baring, Teruaki Enoto,
    Chryssa
    Kouveliotou, Zorawar Wadiasingh, Wynn C. G. Ho, Alice K. Harding,
    Zaven Arzoumanian, Keith Gendreau, Tolga Gu"ver, Chin-Ping Hu,
    Christian Malacaria, Paul S. Ray, Tod E. Strohmayer. Pulse Peak
    Migration during the Outburst Decay of the Magnetar SGR 1830-0645:
    Crustal Motion and Magnetospheric Untwisting. The Astrophysical
    Journal Letters, 2022; 924 (2): L27 DOI: 10.3847/2041-8213/ac4700 ==========================================================================

    Link to news story: https://www.sciencedaily.com/releases/2022/03/220308130555.htm

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