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DETAILS OF GALILEO'S LENSES


Basic Optical Parameters


In the following tables, Galileo's five surviving lenses are identified by the Lens ID codes explained on our page about Building a Galilean Telescope. The Thickness and Full Diameter refer to the whole lens. All the lenses are mounted with stops, and the Clear Aperture is the size of the central diameter actually used in the telescope. Front Radius and Rear Radius refer to the radii of curvature of the front and rear optical surfaces, respectively. A positive radius on the front indicates a convex (outward bulging) surface. On the rear surface a positive radius indicates a concave (inward bulging) surface. The Focal Length is a measured parameter. The Refractive Index of the glass is inferred by computation based on the measured radii, thickness and focal length. The refractive index is dimensionless; all other parameters are given in millimeters.

As Measured by Vasco Ronchi (1923)


Lens IDFull DiameterClear ApertureThicknessFront RadiusRear RadiusFocal LengthRefractive Index
GAL 1A 51 26 2.5 995.5 -3,465 1,327 1.580
GAL 1B 26 11 3.0 infinite 48.5 -95.2 1.509
GAL 2A 37 16 2.0 535 -50,500 956 1.550
GAL 2B 22 16 1.8 -51.5 51.5 -48.8 1.527
GAL 3 58 38 4.0 941.6 -14,363 1,689 1.523

As Measured by Greco, Molesini and Quercioli (1992, 1993)


Lens IDFull DiameterClear ApertureThicknessFront RadiusRear RadiusFocal LengthRefractive Index
GAL 1A 51 26 2.5 950 -2,700 1,330 1.528
GAL 1B 26 11 3.0 infinite -- -94.0 1.516
GAL 2A 37 16 2.0 -- infinite 980 1.546
GAL 2B 22 16 1.8 -- -- -47.5 1.539
GAL 3 58 38 4.0 940 -12,000 1,710 1.510

In the cases indicated by "--", Greco, Molesini and Quercioli did not attempt to repeat Ronchi's measurements. They state they found the refractive indices to range from 1.510 to 1.546, but do not identify which numbers go with which lenses. We have independently calculated the refractive index of each lens based on values given in the table. Ronchi thought that the glass of GAL 1A had an anomalously high index. Greco, Molesini and Quercioli apparently believe this was due to an erroneous measurement, by Ronchi, of the radius of its first surface (995 vs. 950 mm). Please note that the eyepiece designated here as GAL 2B is known to be a later replacement for the missing original eyepiece, and is, therefore, not connected with Galileo.



Dispersion


The only dispersion measurements we know of are those made by Ronchi on the three objective lenses.

Variation of Focal Length [mm] with Wavelength for the Three Objectives (Ronchi, 1923)


Wavelength [Å] GAL 1A GAL 2A GAL 3
4500 1,304 938 1,663
5000 1,317 950 1,678
5500 1,327 956 1,689
6000 1,333 962 1,697
6500 1,337 965 1,702
7000 1,339 969 1,705

The focal length of a singlet lens is completely determined by its thickness, the radii of its front and back surfaces, and the refractive index of the glass. Hence, given the measured thickness, radii and focal length the refractive index of the glass can be deduced. A graph of the refractive indices of Galileo's glasses, and how they vary with wavelength (their "dispersion"), as inferred from Ronchi's focal length measurements together with his measured thicknesses and radii, is given on our Building a Galilean Telescope page. Somewhat different indices, particularly for GAL 1A, are inferred if the newer radius measurements are used.



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Last modified: July 14, 2006