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The term "glitch" in astronomy does not refer to a specific astronomical phenomenon. Instead, a glitch, in its common usage, refers to a minor malfunction or a temporary setback. This term is often used in the context of technology and engineering, such as in spacecraft or electronic systems.1

In astronomy, the closest related concept might be the sudden "glitches" observed in the rotation of some neutron stars. These are not malfunctions but rather abrupt changes in their spin rate. Neutron stars are incredibly dense remnants of massive stars, typically about 20 km in diameter, with masses around 1.35 times that of the Sun. They possess extremely strong magnetic fields and rotate rapidly, sometimes emitting pulses of radiation that are detected as pulsars. When a neutron star glitches, its rotation speeds up slightly, a phenomenon that scientists are still working to fully understand.2

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2 Britannica Sources
  1. neutron star
  2. glitch

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