Galileoscope
The Galileoscope is a small mass-produced refractor telescope, designed with the intention of increasing public interest in astronomy and science. It was developed for the International Year of Astronomy 2009. It is meant to be an inexpensive means by which millions of people can view the same things seen by Galileo Galilei, such as the craters of Earth's Moon, four of Jupiter's moons, and the Pleiades.
Galileoscope

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- refracting telescope.
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- United States.
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wikidata · Q615234 · wikipedia · Galileoscope
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Design and configurations
Design and configurations
The small telescope has an aperture of 50 mm and a relatively long focal length of 500 mm, for a focal ratio of f/10. • Illustration — Galileoscope
• Illustration — At the front, left: The four-lens main eyepiece. Middle: Barlow tube. Right: The two lens auxiliary eyepiece. Background: The focus tube and main telescope tube containing the achromatic doublet objective lens. The Galileoscope uses a 1+1/4 in focuser, giving the telescope a great deal of versatility, since this is the standard size for eyepieces used in most amateur and some professional telescopes. This means the Galileoscope can be used with relatively cheap extra eyepieces to produce magnifications up to 100, or even 200 times (with a 5 mm in combination with the included 2× Barlow lens). However, a magnification of more than 125× would not be recommended for a scope this size because its focal ratio limits sharpness beyond this. Additionally, the design of the slide-in/out focusing tube, without any gears or knobs, makes it nearly impossible to focus above the 125× limit. It also utilizes achromat glass lenses in the objective-lens – the large 2 in one in front – as well as in the eyepiece (4 lenses of two types of high quality plastic, known as a Plossl configuration) to prevent chromatic aberration, producing a clearer image. This is because single lenses, as are often used in cheap scopes, refract light of different colors in different angles (chromatic aberration). In practice this means all images will have blueish blurred edges on one side, reddish on the other, making the image very unclear. By using two types of glass for the two lenses this gets compensated to some degree, resulting in a sharper and clearer image. Depending on the configuration, 4, 6 or 8 lenses are used. The 4-lens configuration results in a telescope in some ways similar to Galileo's, with 17× magnification and a very small field of view. The 6-lens configuration provides 25× magnification, and the 8-lens configuration allows for 50× magnification. The user may easily switch between these configurations by changing the eyepiece.
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United States.
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The biographical narrative on this page is based on the Wikipedia article Galileoscope, revision 1213765161 (EN edition), by its contributors. VALÉORINE has edited that text and built its own documentary record around it. The reused material is available under CC BY-SA 4.0, and this page's reuse of it is offered under the same licence. Everything else on this page — the chronology, the holdings, the evidence, the plates and the connections — is VALÉORINE's own record. Sources and licences.
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1- refracting telescopeTerminology
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The Encyclopedia exists whether or not anything is for sale. Corrections are recorded rather than overwritten, and every version of this record is kept. Published 14 August 2026.
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