Magnetars

Magnetars


News: Scientists have detected an incredibly energetic flare from a magnetar in the galaxy Messier 82 (M82), marking the most distant such event observed. In just one-tenth of a second, this magnetar released energy equivalent to the Sun\'s output over about 10,000 years, showcasing the immense power of these cosmic phenomena.


About:

• Characteristics of M82
o Located 12 million light-years away in the Ursa Major constellation.
o Known as the cigar galaxy due to its elongated shape when viewed edge-on.
o Exhibits high rates of star formation, making it an active starburst galaxy.
• Giant Flares
o Rare eruptions of gamma rays, releasing immense energy.
o Only two confirmed instances observed in the Milky Way and one in the neighboring Large Magellanic Cloud prior to this discovery.
o Despite at least 30 known magnetars in the Milky Way, giant flares are rarely observed events.
o Giant Flare Mechanism: Originates from reconfiguration and reconnection of the magnetars magnetic field.
• Neutron Stars
o Neutron stars form from the explosive collapse of massive stars.
o Remarkably dense, compressing one or two solar masses into a sphere the size of a city.
• Magnetars
o A type of neutron star characterized by extremely strong magnetic fields, among the most powerful
observed in the universe.
o Powered by their own magnetic energy, distinguishing them from ordinary neutron stars.
o Relatively small and dense objects, with diameters of about 10-15 kilometers, similar to other neutron stars.


Characteristics:


Magnetar Characteristics
Formation and Observed Phenomena
Strong Magnetic Fields:Formation of Magnetars: 
Magnetars have magnetic field strengths
ranging from 1,000 to 10,000 trillion Gauss.
Magnetars are believed to form from the
remnants of massive stars undergoing
supernova explosions
These intense magnetic fields distort the
neutron star\'s structure and exert powerful
forces on its surroundings.
The collapse of the star\'s core during
supernova results in the formation of a
neutron star.
 If the progenitor star had a strong magnetic
field, the neutron star may become a
magnetar. 
Rapid Rotation:Observed Phenomena
Magnetars typically rotate rapidly, with periods
ranging from a few seconds to several seconds.
Magnetars emit sporadic and intense bursts
of X-ray and gamma-ray radiation.
Rapid rotation coupled with strong magnetic
fields generates intense electromagnetic
radiation and energy release.
These bursts can be thousands of times
more energetic than typical neutron star
emissions.
 Magnetars experience seismic-like
disturbances called \'magnetar quakes\' or
\'starquakes.\'
 Some magnetars are associated with
gamma-ray bursts (GRBs), the most
energetic explosions in the universe
 The exact mechanism by which magnetars
produce GRBs is still under investigation. 
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