Light bends round a narrow slit and spreads. We study the single slit and the width of its central maximum, then the double slit and the grating with diffraction included. The Rayleigh limit decides what a telescope, a microscope or an eye can tell apart. It serves the Indian syllabus (NCERT, JEE Main) and the matching topic of A-Level, IB and AP.
3 lessons, about 1 h 50 min3 simulations10 problems7 practice questionsPython in every lesson
Light spreads out when it passes through a slit about as narrow as its wavelength. The pattern of a single slit has a wide central maximum and weak maxima on both sides, with dark places at . The central maximum is wide, so a narrower slit gives a wider pattern.
A real double slit shows fringes inside the single-slit pattern of each slit, and some orders are missing. A diffraction grating has a great number of slits. It gives sharp bright lines at and a spectrum of each order for white light.
A star seen through a telescope is not a point but a small disc with rings, because of diffraction at the round aperture. Two stars can be told apart only if their angle is at least , the Rayleigh limit. A bigger aperture and a shorter wavelength resolve more detail.
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