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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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