Vacuum Birefringence

Neutron stars have magnetic fields strong enough to bend light. This causes patterns of light and dark to form on the surface of the neutron star. The patterns depend on the tilt of the magnetic field compared to the rotation axis and the view angle [1]. If you were to tilt your head, you would see the patterns change. The patterns would change rapidly as the neutron star spins.

Neutron stars are very powerful. Neutron starquakes can repeatedly produce enough radiation to make space uninhabitable for several light years, with effects on planetary atmospheres extending out several tens of thousands of light years. When they aren't exploding, they emit enough radiation to ionize surrounding nebulae. Getting close enough to see a neutron star is difficult.

References:
[1] Thi H., etal. 2026, "Pulsed, Polarized X-Ray Emission from Neutron Star Surfaces: The Effects of Vacuum Birefringence in the Magnetosphere". The Astrophysical Journal, Volume 1000, Number 1. DOI, 10.3847/1538-4357/ae313c