object

optical microscopy

Optical microscopy is a technique that uses visible light and lenses to magnify and resolve small objects or structures.
48 related articles · 2 formulas · 6 who worked here

Description

An optical microscope forms an image by refracting visible light through a series of lenses. Resolution is limited by diffraction: according to the Rayleigh criterion, two points are distinguishable if the distance between them is at least half the wavelength divided by the numerical aperture of the objective. Modern methods—fluorescence microscopy, confocal, super-resolution (STED, PALM)—overcome this limit, allowing visualization of structures down to single molecules.

History

Zacharias Janssen is credited with constructing a compound microscope (1590). Antonie van Leeuwenhoek (1674) achieved 300x magnification with single lenses, discovering microorganisms. Robert Hooke in 'Micrographia' (1665) described cells. In 1873, Ernst Abbe developed the theory of image formation and the sine condition. Carl Zeiss and Otto Schott established industrial production of high-quality objectives. In the 20th century, Frits Zernike invented the phase-contrast microscope (1935, Nobel 1953), Marvin Minsky patented the confocal principle (1957). Super-resolution emerged in the 2000s: STED by Stefan Hell (2014 Nobel), PALM by Eric Betzig and Harold Hess.

How it works

A beam of light from the source is focused by the condenser onto the specimen. Scattered and directly transmitted light is collected by the objective, which forms a primary image in the plane of the field diaphragm. The eyepiece further magnifies it for viewing by eye or transmission to a detector. Contrast in brightfield microscopes arises from absorption or scattering; phase contrast converts a phase shift into an amplitude change. In fluorescence microscopes, the specimen is illuminated at the excitation wavelength, and emitted radiation is separated by a dichroic mirror and filters. In confocal microscopy, a point source and a detector with a pinhole provide optical sectioning. Super-resolution overcomes the diffraction limit by turning off fluorophores at the periphery of the excitation spot (STED) or by precise localization of single photoactivatable molecules (PALM/STORM).

In practice

Used in biology and medicine for cell analysis, in materials science for inspecting microchips, and in forensics for examining fibers and prints.

Fun fact

With an optical microscope, you can not only look but also move objects: laser tweezers can hold and move individual cells or bacteria.

Concept graph →

Formulas

$$\tau = n \sigma l$$
Optical depth equals column density times cross-section.
What is in the formula
τvariableoptical depth — optical depth
nvariablenumber density of absorbers — number density per cubic metre
σvariablecross-section per absorber — cross section square metre
lvariablepath length through the medium — length metre
τ=n_{{hi}}*σ_{{ly}α} · 2606.02711v1
τ_ν=\frac{\kappa_ν\sigma}{\cosi} · 2607.02660v1
τ_w(r)=\kappaa(\frac{1}{r}-\frac{1}{r_{\rmout}}) · 2607.24045v1
τ_{{ice}}=\langle-\ln\frac{f(λ)}{f_{{cont}}(λ)}\rangle · 2607.24934v1
$$\tau_d \propto \frac{M_d}{\rho_d v_{\text{ej}}^2 t^2}$$
Optical depth scales with dust mass, grain density, ejection speed, and time.
What is in the formula
\tau_dvariableoptical depth due to dust — optical depth
M_dvariabletotal dust mass — mass kilogram
\rho_dvariablemass density of individual dust grains — mass density kilogram per cubic metre
v_{\text{ej}}variableejection speed of the dust — velocity metre per second
tvariabletime since ejection — time second
τ_d\approx(\frac{m_d}{10^{-3}m_\odot})(\frac{ρ_d}{20{gcm}^{-3}})^{-1}(\frac{v_{{ej}}}{0.1c})^{-2}(\frac{t}{29{day}})^{-2} · 2607.00433
τ_d\approx1(\frac{m_d}{10^{-3}m_\odot})(\frac{v_{\rmej}}{0.1c})^{-2}(\frac{t}{29\rmday})^{-2} · 2607.00433v1

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