Physics Study of a Ray of Light

Physics: Study of Light

 

  • Light is in the form of - an electromagnetic wave
  • The visible light has wavelengths stretches between - 400–700 nanometers.
  • The primary source of light is - sun.
  • Optics is a branch of physics that deals with the properties and behavior of light, along with its interactions with - the matter.
  • Light exhibits various properties which are - Reflection, Refraction, Total internal reflection,
  • Dispersion.
  • Light speed is 3 x 108 m/s which is the form of - energy.
  • Light is a - transverse wave.
  • When light falls on the surface of an object it can either be- Absorbed, Transmitted, Reflected
  • If an object absorbs all the light falling on it, then it will appear perfectly black for example - a blackboard.
  • An object is said to transmit light if it allows light to pass through itself and such objects are - transparent.
  • If an object sends back light rays falling on its surface then it is said to - have reflected the light.
  • When a ray of light falls on a boundary separating two media comes back into the same media, then this phenomenon is called - the reflection of light.
  • The angle of incidence is equal to - the angle of reflection.
  • The incident ray, the reflected ray and the normal to the mirror at the point of incidence all lie in the - same plane.
  • To see his full image in a plane mirror, a person required a mirror of - at least half of his height
  • Laws of reflection are applicable to all types of reflecting surfaces including - spherical surfaces.
  • The reflecting surface of a spherical mirror may be curved - inwards or outwards.
  • A spherical mirror, whose reflecting surface is curved inwards, that is, faces towards the centre of the sphere, is called - a concave mirror.
  • A spherical mirror whose reflecting surface is curved outwards, is called - a convex mirror.
  • The reflecting surface of a spherical mirror forms a part of a sphere which has a centre - That point is called the centre of curvature of the spherical mirror.
  • The centre of curvature is not a part of the mirror. It lies - outside its reflecting surface.
  • The centre of curvature of a concave mirror lies - in front of it.
  • The centre of curvature of a convex mirror lies - behind the mirror.
  • The phenomenon of deviation of light rays from its path when it travels from one transparent medium to another medium is called - refraction of light.
  • The cause of refraction is due to the different speed of light - in different medium.
  • When a ray of light enters from one medium to another medium, its frequency and phase do not change, but - wavelength and velocity change.
  • Due to refraction from Earth's atmosphere - the stars appear twinkle.
  • The incident ray, the refracted ray and the normal at the point of incidence all three lie in - the same plane in refraction of light.
  • When light travels through a denser medium towards a rarer medium it deviates away from the normal, therefore - a pond appears shallower.
  • A coin appears at lesser - depth in water.
  • The angle of incidence in a denser medium for which the angle of refraction in rarer medium becomes 90°, is called the critical angle.
  • When a light ray travelling from a denser medium to the rarer medium, in this incident at the interface at an angle of incidence greater than
  • critical angle, then light rays reflected into the denser medium, this phenomenon is known as total internal reflection
  • Sparkling of diamond, mirage and looming, shinning of the air bubble in water and optical Fibre are examples of total internal reflection.
  • The image formed by a concave mirror is generally real and inverted
  • The image formed by a convex mirror is always virtual, erect and diminished.
  • The radius of Curvature (R): The radius hollow sphere of which the mirror is a part.
  • Pole (P): The mid-point of a spherical mirror is called pole.
  • Focus (F): when a parallel beam of light rays is incident on a spherical mirror then after reflection it meets or appears to meet at a point on the principal axis, called focus of the spherical mirror.
  • Focal length (f): Focal length d= R/2
  • Prism is a uniform transparent refracting medium bounded by plane surfaces inclined at some angles forming a triangular shape.
  • When a light is incident on a glass prism, it disperses into its seven colour components in the following sequence VIBGYOR, and this is known as the dispersion of white light.
  • The refractive index of glass is maximum for violet colour
  • The refractive index of glass is minimum for the red colour
  • Rainbow is caused by dispersion of sunlight by tiny water droplets, present in the atmosphere.
  • The water droplets act like small prisms in rainbow formation.
  • The twinkling of a star is due to atmospheric refraction of starlight.
  • The apparent position of the star is slightly different from its actual position.
  • The Sun is visible to us about 2 minutes before the actual sunrise, and about 2 minutes after the actual sunset because of atmospheric refraction.
  • Hotter air is less dense and has smaller refractive index than the cooler air.
  • The earth’s atmosphere is a heterogeneous mixture of minute particles like smoke, tiny water droplets, suspended particles of dust and molecules of air.
  • When a beam of light strikes such fine particles, the path of the beam becomes visible which is known as Tyndall Effect
  • The colour of the scattered light depends on the size of the scattering particles.
  • The order of colours in light, arranged from shortest wavelength to longest, is called the visible spectrum of light.
  • Ultraviolet light and x-rays have wavelengths shorter than violet light
  • infrared (heat) and radio waves have wavelengths longer than red light.
  • The full range of wavelengths for light is called the "electromagnetic spectrum.
  • Wavelength of White Light: The white light extends from the 400 nm to 750 nm.
  • Since, the speed of light, remains constant, as frequency goes up, wavelength must go down.
  • violet has the highest frequency and the shortest wavelength of the visible colours of light.
  • red has the lowest frequency and the longest wavelength of the visible colours of light.
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