BOUNDLESS EXPANSE 3D

🔭 Telescope Resolution & Diffraction

Rayleigh criterion · Airy disk · seeing · resolving binary stars
Key formula: θ_R = 1,22 · λ / D θ_eff = √(θ_R² + θ_seeing²)

A larger telescope is sharper because diffraction shrinks with aperture. Rayleigh criterion: θ = 1.22 λ/D. Shorter wavelengths and larger apertures resolve smaller angles. Atmospheric seeing adds blur in quadrature, so a space telescope or adaptive optics can outperform a much larger ground telescope in ordinary seeing. The simulator shows two Airy-like profiles merging or separating as parameters change.

🚀 Simulate in the browser

Related simulators

All physics simulators