TS-Optics Spike Mask for the Lens of the Seestar S50 Ingrandisci

TS-Optics Spike Mask for the Lens of the Seestar S50

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This spike mask generates the spikes known from Newtonians (and other telescopes with spider vanes) for a more dramatic effect of the astrophotos.

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SEESTAR-SPIKE

Disponibilità 3-4 gg lavorativi+ tempo di trasporto

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25,50 € 25.5 EUR 2024-06-09

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Codice articolo: SEESTAR-SPIKE

TS-Optics Spike Mask for the Lens of the Seestar S50 from ZWO

 This spike mask generates the spikes known from Newtonians (and other telescopes with spider vanes) for a more dramatic effect of the astrophotos. [EN]
Newtonian spikes are created by the interference of light rays passing through the aperture of the telescope and the spike mask. The mask consists of a series of thin, parallel lines that focus the light into these lines. When the light then hits the lens, a diffraction pattern is created which produces the spikes.

The Spike Mask is a simple and effective tool that can add a dramatic effect to images. It is a good choice for anyone who wants to have the Newtonian spikes in their astrophotographs without having to deal with image post-processing.

To use the Spike Mask, simply place the mask in front of the telescope objective and then move the telescope to a bright object such as the moon or a star cluster. The spikes should then be visible.

 This spike mask generates the spikes known from Newtonians (and other telescopes with spider vanes) for a more dramatic effect of the astrophotos. [EN]

Here are some tips for using the Spike Mask:

♦ Make sure that the mask is clean before you use it. Dirt or dust can impair the image quality.
♦ Make sure that the mask is perfectly aligned. If the mask is not aligned, the spikes may be blurred or distorted.

With a little practice, you can take beautiful pictures with Newtonian spikes using the Spike Mask:

♦ Attach the mask to the telescope and align it with the object to be photographed.
♦ Get the classic spikes of a Newtonian telescope in live view.
♦ The spikes will be more clearly visible on the images.

 This spike mask generates the spikes known from Newtonians (and other telescopes with spider vanes) for a more dramatic effect of the astrophotos. [EN]

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