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Optik & Wellenlehre · GCSE Physics Topic 6

Lochkamera & Finsternis-Simulator

Lochkamera & Sonnenfinsternis-Simulator: Geradlinige Lichtausbreitung und Kernschatten

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  • Echtzeit-Herleitung
  • Projektormodus
  • A4-Arbeitsblatt
Lokale Berechnung · Privat
Interaktives Wissenschaftslabor Reine clientseitige Berechnung physikalischer Gesetze. Die Verarbeitung erfolgt lokal ohne Erfassung persönlicher Daten.
3D-Simulationsfenster● 60 FPS
Voreinstellungen & typische Fallen:

Experimentelle Steuerungsparameter

cm
cm
mm

Echtzeit-Herleitung & Kennzahlen

Abbildungsmaßstab M
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Bildqualität und -art
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Bildlage
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Modus Sonnenfinsternis
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Echtzeit-Formelherleitung
Grundformel: --
Einsetzungsschritte: --
Physikalischer Zustand: --

Typische Beispielaufgaben & Prüfungsfallen

Worked Problem

Aufgabe: A 6cm candle is 10cm from pinhole, screen is 25cm away. Find image height and nature.
Schrittweise Herleitung:
  1. By similar triangles: H / 6 = 25 / 10 => H = 15cm. The image is inverted, magnified and real.

Worked Problem

Aufgabe: Under sunny tree canopy, circular spots cover the ground. What are they? What shape during partial solar eclipse?
Schrittweise Herleitung:
  1. Circular patches are pinhole images of the round sun. During a partial solar eclipse, they all turn into crescents.

Arbeitsblatt für den Unterricht & Hausaufgaben

Q1. Variant 1: Does pinhole inversion also flip left and right? How to verify experimentally?
Q2. Variant 2: What is the spatial alignment order of Sun, Earth, and Moon during solar and lunar eclipses?
Q3. Variant 3: What is the speed of light in vacuum? Is it faster or slower in water and glass?

Häufige Fragen & typische Missverständnisse

Why is a pinhole camera image always a real image?
Real images are formed by intersecting actual light rays and can be captured on physical screens or photographic film.
Why does an excessively large aperture blur out the image?
A large hole acts like thousands of overlapping tiny pinholes, blurring individual inverted images into an unstructured illumination blob.
What distinguishes total, annular, and partial solar eclipses?
Total: observer in lunar umbra. Annular: in antumbra (golden ring left). Partial: in penumbra (crescent bite).
Why are there annular solar eclipses but no "annular lunar eclipses"?
Earth is much larger than the Moon; Earth's umbral shadow at the Moon is 2.7x Moon's diameter, completely enveloping it.