Light in 25 Minutes🔥| Class 10th | Rapid Revision | Prashant Kirad

Exphub 9th &10th32 minutes read

Prashant introduces a rapid revision of the chapter on light, covering theory, diagrams, and numerical problem-solving in 15 to 20 minutes, with a detailed video for further study. The concept of light, reflection, spherical mirrors, ray diagrams, uses of concave and convex mirrors, and sign convention rules for object distance and focal length are explained thoroughly.

Insights

  • Light travels straight at a speed of 3 * 10^8 meters per second, with reflection involving bouncing off shiny surfaces following two laws. Plane mirrors create virtual, erect images with equal size and distance from the mirror.
  • Spherical mirrors (concave and convex) are discussed in detail, focusing on poles, principal axis, center of curvature, focus, and focal length. Ray diagrams illustrate image formation based on object positions, with concave mirrors producing real and inverted images and convex mirrors creating virtual and erect images.

Get key ideas from YouTube videos. It’s free

Recent questions

  • What is light's speed?

    3 * 10^8 meters per second

  • What is reflection in light?

    Bouncing back from shiny surfaces

  • What are the properties of a plane mirror?

    Virtual, erect images, equal size

  • What are concave and convex mirrors?

    Spherical mirrors with different curvatures

  • What is the refractive index formula?

    c/v, inversely proportional to light speed

Related videos

Summary

00:00

Rapid Light Chapter Revision with Prashant

  • Prashant bhaiya introduces the rapid revision of the chapter on light, emphasizing its significance and complexity.
  • The revision aims to cover the chapter quickly within 15 to 20 minutes, focusing on theory, diagrams, and numerical problem-solving.
  • Prashant mentions a detailed video for in-depth study and practice, providing a link for further reference.
  • Light is defined as always traveling straight, with a speed of 3 * 10^8 meters per second.
  • The concept of reflection is explained as the bouncing back of light from a shiny surface, following two laws of reflection.
  • Properties of a plane mirror are discussed, including virtual and erect images, equal image size, and distance from the mirror.
  • Spherical mirrors, concave and convex, are introduced, with details on poles, principal axis, center of curvature, focus, and focal length.
  • Ray diagrams for concave and convex mirrors are explained, highlighting image formation based on object positions.
  • A trick for remembering ray diagrams is shared, emphasizing the importance of understanding image characteristics based on mirror types.
  • The uses of concave and convex mirrors are outlined, focusing on image enlargement and reduction, with practical examples provided.

11:16

Mirror and Lens Sign Conventions Explained

  • Left side is negative, right side is positive for objects in relation to a mirror or lens.
  • Objects above a line are positive, below are negative.
  • Sign convention rules apply to mirrors and lenses.
  • Object distance (u) is always negative.
  • Focal length of a concave mirror is negative, convex mirror is positive.
  • Mirror formula: 1/v + 1/u = 1/f.
  • Magnification formula: m = -v/u.
  • Questions involve finding v using mirror formula and determining image nature through magnification.
  • Refraction involves bending of light when passing between mediums.
  • Refractive index formula: c/v, inversely proportional to speed of light.

21:56

Image Formation in Concave Lenses Explained

  • Object is at 2f 1, i.e. third. If it is on number then where will our image be made? 2 will be made on f1.
  • Whenever the object is between these two, where will the image be made? Beyond will be made, it will be made behind.
  • If the object is on the top, where will the image be made? It will be made far behind, on the fifth number.
  • If the object is in the center of focus, where will the image be formed? It will be formed behind, virtually.
  • Concave lens has two cases: parallel light rays will meet at the focus, and other positions will form images between the optical center and focus.
Channel avatarChannel avatarChannel avatarChannel avatarChannel avatar

Try it yourself — It’s free.