Our galaxy is filled with magnetic fields. They come not just from stars and planets, but from dusty stellar nurseries and the diffuse hydrogen gas of interstellar space. We’ve long known of this galactic magnetic field, but mapping it in detail has posed a challenge. Now a new study gives us a detailed 3-dimensional map of these fields, with a few surprises.
Magnetic fields don’t emit light on their own, so we can’t simply scan the sky with optical telescopes to see where they are. Instead, we must look for ways in which magnetic fields cause charged particles to emit light, or how distant light is affected by interstellar gas within the magnetic field.
For objects such as stars and planets, we mostly map their magnetic fields by charged particles. Ions can become trapped by magnetic field lines, spiraling along them as they emit light. It’s how we first mapped the magnetic field of Jupiter, and how we can study the magnetic fields of the accretion disks of black holes. But galactic magnetic fields are much weaker and diffuse. While charged particles can spiral along galactic magnetic fields, the light they emit is often too faint for us to detect. So instead we use a trick of polarized light.
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