Telescopes and Optics Review

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A set of vocabulary flashcards covering key terms and definitions related to telescopes and optics.

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42 Terms

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Telescope

An optical instrument designed to make distant objects appear closer and clearer.

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Objective

The optical component of a telescope, typically a lens or mirror that collects light.

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Refraction

The bending of light rays when they pass from one medium to another.

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Chromatic Aberration

Optical distortion in lenses where different colors of light are focused at different points.

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Concave Mirror

A mirror that curves inward, used in reflecting telescopes to gather light.

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Focal Point

The point where light rays converge after passing through a lens or reflecting off a mirror.

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Magnification

The degree to which an image is enlarged as compared to the original object size.

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Angular Size

The apparent size of an object as seen from a given distance, measured in angles.

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Snellā€™s Law

A formula used to describe the relation between the angles of incidence and refraction.

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Eyepiece Lens

The lens that magnifies the image in a telescope.

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Field of View (FoV)

The extent of the observable area seen through a telescope or camera.

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Total Internal Reflection

The complete reflection of a light ray within a medium as it strikes the boundary with a less dense medium at a critical angle.

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Thin Convex Lens

A lens that is thicker at the center than at the edges, used in telescopes to converge light.

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Light Divergence

The spreading out of light rays as they move away from a source.

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Myopia

A condition where distant objects appear blurry because light is focused in front of the retina.

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Hyperopia

A condition where nearby objects appear blurry because light is focused behind the retina.

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Reflection

The bouncing back of light rays when they hit a surface.

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Reflecting Telescope

A telescope that uses mirrors to gather and focus light.

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Refracting Telescope

A telescope that uses lenses to gather and focus light.

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Ray Tracing

A method for representing the path of light rays as they pass through optical devices.

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Focal Length (ft)

The distance from the lens or mirror to the point where it focuses light.

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Spectroscopy

The study of the interaction of light and matter to analyze the composition of substances.

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Continuum Spectrum

A spectrum that shows all wavelengths emitted by a hot, dense light source.

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Emission Spectrum

The spectrum of light emitted by a substance when it is excited or heated.

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Absorption Spectrum

The spectrum that shows dark lines or gaps indicating wavelengths absorbed by a substance.

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Camera Obscura

An early device used to project an image onto a surface, a precursor to modern cameras.

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Optical Axis

An imaginary line that defines the path along which light travels through a lens or mirror.

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Irradiance

The amount of light energy received per unit area.

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Light Transmission

The passage of light through a medium.

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Diverging Lens

A lens that causes light rays to spread apart.

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Primary Mirror

The main mirror in a reflecting telescope, usually concave, that gathers light.

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Secondary Mirror

A smaller mirror in a reflecting telescope that redirects light to the eyepiece.

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Flat Mirror

A mirror with a flat reflective surface, used for simple reflection.

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Optic Nerve

The nerve that transmits visual information from the retina to the brain.

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Parallax

The apparent shift in position of an object when viewed from different angles.

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Infrared Telescopes

Telescopes designed to detect infrared radiation from celestial objects.

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Galilean Telescope

A refractive telescope designed by Galileo, using a concave eyepiece lens.

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Keplerian Telescope

A type of refracting telescope with an inverted image produced by two convex lenses.

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White Light Dispersion

The process whereby white light is split into different colors upon passing through a prism.

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Light Ray

An idealized model representing a narrow beam of light.

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Telescope Aperture

The diameter of the telescope's objective lens or mirror, which determines how much light is collected.

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Newton's Prisms Experiment

Isaac Newton's demonstration that white light consists of multiple colors by splitting light with prisms.