What exactly are Magnetars? I've heard the term used before, and all I

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In summary, magnetars are neutron stars with very strong magnetic fields, which are the result of the decay of their magnetic fields. They form as a result of the supernova explosion of a massive star, and can be detected by their emission of high energy x-rays or gamma rays.
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fillipeano
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What exactly are Magnetars? I've heard the term used before, and all I remember about them are that they have very powerful magnetic fields.
What are they? How do they form and how do we detect them?
 
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They arehttp://en.wikipedia.org/wiki/Neutron_star" with extraordinarily large magnetic fields.
 
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How do they get such a large magnetic field? I'm really intrigued by strange objects :)
 
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fillipeano said:
What exactly are Magnetars?
Wikipedia said:
A magnetar is a type of neutron star with an extremely powerful magnetic field, the decay of which powers the emission of copious amounts of high-energy electromagnetic radiation, particularly X-rays and gamma rays.
fillipeano said:
How do they get such a large magnetic field?
Wikipedia said:
Magnetars are primarily characterized by their extremely powerful magnetic field, which can often reach the order of ten gigateslas.

A 10 gigatesla field, by contrast, has an energy density of [tex]4.0 \times 10^{25} \; \frac{\text{J}}{\text{m}^3}[/tex].

Although most common magnetic phenomena are electromagnetic, a second source of magnetism occurs due to the spin magnetic moment of sub-atomic particles. Spin magnetic moment is responsible for the magnetic field of magnetars.

Reference:
http://en.wikipedia.org/wiki/Neutron_star"
http://en.wikipedia.org/wiki/Magnetar"
http://en.wikipedia.org/wiki/Spin_magnetic_moment"
 
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fillipeano said:
... How do they form and how do we detect them?

Magnetars are a special type of neutron stars, which are a result of the evolution of a massive star. The star undergoes a supernova explosion, and a neutron star is left from the core of the star.

Magnetars have specific timing properties like radio pulsars. Unlike pulsars, however, magnetars have long spin periods (2-8 seconds or so) and are not very bright in radio emission. The magnetic field is so strong that it will deform the crust of the neutron star periodically. This results in the emission of high energy x-rays (hard x-rays) or lower energy gamma rays (soft gamma rays). These objects are respectively called anomalous X-ray pulsars (AXP) and soft gamma repeaters (SGR)
 

FAQ: What exactly are Magnetars? I've heard the term used before, and all I

What are magnetars?

Magnetars are a type of neutron star, which is the extremely dense core of a star that has undergone a supernova explosion. They are known for having incredibly strong magnetic fields, up to a thousand trillion times stronger than Earth's magnetic field.

How are magnetars different from other neutron stars?

Magnetars are distinguishable from other neutron stars because of their extremely strong magnetic fields. They also rotate very quickly, with some magnetars spinning hundreds of times per second.

What causes magnetars to have such strong magnetic fields?

The exact cause of magnetars' strong magnetic fields is still not fully understood, but it is thought to be a combination of their rapid rotation and the extreme conditions inside the star's core.

What are some of the unique properties of magnetars?

Magnetars are known for their flares, which are incredibly powerful bursts of X-rays and gamma rays. They also have a very high surface temperature, estimated to be around a million degrees Celsius. Additionally, the strong magnetic fields of magnetars can influence the behavior of matter in their surroundings.

How do scientists study magnetars?

Scientists study magnetars using various telescopes and instruments that can detect and measure X-rays and gamma rays. They also use models and simulations to better understand the physics behind magnetars and their behavior. Some scientists also study the effects of magnetars on their surrounding environment, such as the formation of nebulae.

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