In astronomical photos of stars, there are sharp lines that emanate from the center of the stars that are point sources of light.
What is the physical effect that causes these spikes?
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The spikes are also observed in particular on photos of the Hubble telescope , which is located in outer space. Therefore, the atmosphere can be excluded as a cause, so that the spikes must be created by the imaging in the telescope itself. In the case of lenses and mirrors, aberrations are referred to as deviations of the ideal spherical shape, which cause a blurred or distorted image. These effects can be understood in the context of geometric optics. But stars are point light sources and a distorted point would still have to be imaged as a point, so that aberrations can be excluded as a cause.
The cause of the spikes is the wave nature of the light, which leads to light diffraction at the opening of the telescope ( diffraction spikes ). Diffraction refers to the deflection of waves on an obstacle. A simple circular aperture on the lens causes a point light source to be imaged as a circle surrounded by diffraction rings (airy disk). However, the spikes in the photos of reflecting telescopes are caused by the suspension of the secondary mirror inside the tube, which acts as an aperture for the incident light rays. Depending on the number and arrangement of the supports, you can observe a different number of spikes, so that a star photographed with different telescopes can have two, four or six beams. Even when looking into the night sky with the naked eye, you can perceive a pointy star-like-shape because of diffraction. This is ultimately the reason why we represent stars in symbols and illustrations since the beginning of human history also with points.
This problem was inspired by this minutephysics video .