
A unit of magnetic flux density, commonly used in astrophysics to measure field strength.The gauss (symbol G) is a unit of magnetic flux density, also known as magnetic induction, in the centimeter-gram-second (CGS) system of units. It measures the strength of a magnetic field — specifically, how many field lines pass through a given area. In astrophysics, the gauss is the standard unit for describing magnetic fields across cosmic scales, from the faint fields in interstellar space (microgauss, 10⁻⁶ G) to the intense fields on the surfaces of neutron stars and white dwarfs (up to 10⁹ G or more). One tesla, the SI unit, equals 10,000 gauss, so the gauss is convenient for the relatively weak fields found in most astronomical environments.
The unit is named after Carl Friedrich Gauss, the German mathematician and physicist who made foundational contributions to the theory of magnetism in the 1830s. The name was formally adopted in the late 19th century as part of the CGS system.
Magnetic flux density is defined by the force a magnetic field exerts on a moving charge: a charge of one statcoulomb moving at one centimeter per second perpendicular to a field of one gauss experiences a force of one dyne. In practice, astronomers infer magnetic field strengths indirectly. They measure the Zeeman splitting of spectral lines, the polarization of light, or the synchrotron radiation from charged particles spiraling in the field. Each technique yields a value in gauss, allowing comparisons across different objects and phenomena.
Beyond astrophysics, the gauss is used in magnetometry for geophysical surveys, in the calibration of magnetic sensors, and in the design of magnetic shielding for sensitive equipment.
The Earth's magnetic field at the surface is about 0.5 gauss, while a typical refrigerator magnet is around 100 gauss — a thousand times stronger.



