Optics of the Human Eye & Related Atmospheric Phenomena

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Vocabulary flashcards covering structure and function of the human eye, common vision defects and their corrections, optical phenomena such as dispersion and total internal reflection, and atmospheric effects on light.

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37 Terms

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Human Eye

Sense organ that enables vision; situated in skull eye sockets with a constant diameter of about 2.3 cm throughout life.

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Sclera

The tough, opaque, outermost white layer of the eye that protects and maintains its shape.

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Cornea

Transparent, outermost part of the eye that provides most of the eye’s refraction of incoming light.

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Eye Lens

Convex, flexible, jelly-like structure that focuses a real, inverted image on the retina by changing curvature.

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Iris

Dark, muscular diaphragm that controls pupil size and thus regulates the amount of light entering the eye.

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Pupil

Central aperture within the iris—often called the "window" of the eye—that admits light.

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Ciliary Muscles

Muscles that hold the lens and alter its curvature to adjust focal length during accommodation.

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Retina

Delicate, light-sensitive membrane containing rods and cones where images are formed for transmission to the brain.

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Optic Nerve

Nerve bundle that carries visual information from the retina to the brain’s visual centers.

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Blind Spot

Point on the retina where the optic nerve exits; contains no photoreceptors, so no image is detected there.

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Aqueous Humour

Clear fluid between cornea and lens that helps focus light on the retina and nourishes eye tissues.

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Vitreous Humour

Gel-like fluid filling the space between the lens and retina, helping maintain eyeball shape.

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Far Point

Maximum distance at which the eye can see clearly; for a normal eye, effectively at infinity.

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Near Point (Least Distance of Distinct Vision)

Minimum distance (about 25 cm for a normal eye) at which an object can be seen clearly without strain.

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Accommodation

Process by which ciliary muscles change lens curvature and focal length to keep images focused on the retina.

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Focusing on Far Objects

Ciliary muscles relax, lens becomes thin, focal length increases to bring distant images onto the retina.

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Focusing on Near Objects

Ciliary muscles contract, lens thickens, focal length decreases to focus nearby images on the retina.

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Myopia (Near-Sightedness)

Defect where nearby objects appear clear but distant ones appear blurred because images form in front of the retina.

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Causes of Myopia

Excessive curvature of the eye lens or elongation (stretching) of the eyeball.

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Correction of Myopia

Use of a concave (diverging) lens to form a virtual image at the eye’s far point, shifting focus onto the retina.

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Hypermetropia (Far-Sightedness)

Defect where distant objects are clear but near ones are blurred because images form behind the retina.

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Causes of Hypermetropia

Eye lens focal length too long or eyeball too short.

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Correction of Hypermetropia

Use of a convex (converging) lens to help form a real image of a near object directly on the retina.

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Dispersion of Light

Splitting of white light into constituent colours when passing through a prism due to different refractive indices.

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Prism

Transparent optical element with flat, polished surfaces that refracts and disperses light into a spectrum.

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Total Internal Reflection (TIR)

Phenomenon in which light incident on a boundary from a denser to a rarer medium reflects entirely back when the incidence angle exceeds the critical angle.

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Conditions for TIR

(1) Light travels from denser to rarer medium; (2) angle of incidence is greater than the critical angle.

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Rainbow Formation

Sequence of refraction, internal reflection, and dispersion of sunlight in water droplets producing a visible spectrum arc.

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Atmospheric Refraction

Bending of light as it travels through layers of air with varying optical densities, causing apparent position shifts of celestial objects.

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Blue Colour of Sky

Due to Rayleigh scattering: shorter-wavelength blue light is scattered more by tiny atmospheric particles than longer wavelengths.

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Reddish Sunrise & Sunset

Sun’s rays traverse more atmosphere near the horizon; shorter wavelengths scatter away, leaving predominantly red light.

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Red for Danger Signals

Red light has the longest wavelength, scatters least, and remains visible over longer distances in atmosphere, enhancing safety.

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Yellow School Buses

Yellow has high visibility and peripheral detection; its medium wavelength scatters moderately, making buses noticeable in various conditions.

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Apparent Raising of Celestial Bodies

Stars and Sun appear slightly higher than actual positions because atmospheric refraction bends their light downward.

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Early Sunrise & Delayed Sunset

Atmospheric refraction allows the Sun to be seen about two minutes earlier at dawn and later at dusk than its geometric position.

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Twinkling of Stars

Rapid changes in apparent brightness caused by atmospheric turbulence refracting starlight along varying paths.

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Planets Do Not Twinkle

Planets’ apparent disks average out atmospheric fluctuations, so their brightness appears steady compared to point-like stars.