Kepler’s telescope and Galileo’s telescope

VP5.1.4.2
Kepler’s telescope and Galileo’s telescope
Kepler’s telescope and Galileo’s telescope Ray path through the Kepler telescope (P5.1.4.2)
Kepler’s telescope and Galileo’s telescope

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Description

The aim of the experiment P5.1.4.2 is to observe distant objects using a telescope. The objective and the ocular of a telescope are arranged so that the back focal point of the objective coincides with the front focal point of the ocular. A distinction is made between the Galilean telescope, which uses a dispersing lens as an ocular and produces an erect image, and the Kepler telescope, which produces an inverted image because its ocular is a collecting lens. In both cases, the total magnification can be determined as:

Components of equipment sets

1 46002  4  Lens in frame, f=50 mm LD
1 46003  4  Lens in frame, f=100 mm LD
1 46004  4  Lens in frame, f=200 mm LD
1 46005  8  Lens in frame, f=500 mm LD
1 46006  8  Lens in frame, f=-100 mm LD
1 460310  8  Optical bench, S1 profile, 1 m LD
2 460312  4  Clamp rider with clamp 45/35 LD
1 31122  4  Vertical rule LD
1 30011  4  Saddle base LD

Experiment Instructions

PDF (Experiment description) PDF (Experiment description) P5.1.4.2 Kepler’s telescope and Galileo’s telescope
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