Diffraction spike

Diffraction spikes from various stars seen on image taken by HST

Diffraction spikes are lines radiating from bright light sources in reflecting telescope images. They are artifacts caused by light diffracting around the support vanes of the secondary mirror. Refracting telescopes and their photographic images do not have the same problem.

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Reflection telescope. Note the smaller mirror in the path of the light; this mirror's struts cause the diffraction spikes

The secondary mirror in a reflecting telescope has to be positioned at the central axis of the telescope and so has to be held by struts within the telescopes tube. No matter how fine these support rods are they diffract the incoming light from a subject star and this appears as diffraction spikes which are the Fourier transform of the support struts. The spikes represent a loss of light that could have been used to image the star. ^{[1] [2]}

Although diffraction spikes can obscure parts of a photograph and are undesired in professional contexts, some amateur astronomers like the visual effect they give to bright stars - the "Star of Bethlehem" appearance - and even modify their refractors to exhibit the same effect,^[3] or to assist with focusing when using a CCD.^[4]

External links

• Diffraction spikes explained by Astronomy Picture of the Day.

References

1. ^ Diffraction spikes explained by Astronomy Picture of the Day. 15-04-01
2. ^ Internal Reflections and Diffraction Spikes. Caltech. Accessed April 2010
3. ^ http://homepage.ntlworld.com/jan.rek/equipment.htm#starspike
4. ^ http://astronomy.qteaser.com/diffspike.html