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Because moving charges generate magnetic fields, I would think that a neutron star’s axis of rotation and axis of the magnetic field would line up; Why don’t they?

Thomas Knost, Mills River, North Carolina
RELATED TOPICS: NEUTRON STARS
Neutron star
The original massive star that formed into a neutron star (like that illustrated here) had a magnetic field produced by collective fluid-like motions of charged particles. Perhaps such a “fossil” field could have survived the massive sun’s evolution and eventual collapse into a neutron star. While this is one theory as to what creates a neutron star’s magnetic field, astronomers aren’t sure if it’s correct.
NASA/CXC/M. Weiss
A neutron star is the extremely compressed leftover core of a star that began life with between 10 and 30 times the Sun’s mass. Moving charges do generate magnetic fields, as you suggest; however, the rotation of the neutron star moves both positive charges (ions) and negative charges (electrons) together. Therefore, the overall rotation of the neutron star doesn’t generate a net electrical current or magnetic field.

The magnetic fields of stars and planets typically arise from “dynamo” processes that involve local currents generating an overall field. For example, the dynamo involving currents near Earth’s core produces a field that is misaligned with our planet’s rotation axis.

Astronomers don’t yet understand how neutron stars’ magnetic fields originate. We know that the suns that will eventually become neutron stars can generate magnetic fields through convective dynamo processes, which are collective fluid-like motions of charged particles that generate a field. However, it is unclear if a neutron star’s magnetic field comes from this “fossil” field condensing as the star’s core collapses or if a new field is generated during the core collapse (while the rest of the sun explodes as a supernova).

If a supernova explosion is asymmetrical, some of the energy also can affect the rotation of a new neutron star and give it high velocity — a process that we call a “kick.” For example, we know that these kicks can fire newborn neutron stars away from their birthplaces at potentially hundreds of miles per second. If the kicks occur slightly off-center, they also can impart a completely different rotation axis to the neutron star than that of the original star.
Dave Tsang
McGill University, Montreal
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