Physics > Refraction of Light > 9.0 Optical instruments
Refraction of Light
1.0 Introduction
2.0 Laws of refraction
3.0 Apparent shift of an object
4.0 Thin lenses
4.1 Sign convention
4.2 Some important terms
4.3 Ray tracing
4.4 Image formed by covex lens
4.5 Image formed by concave lens
5.0 Lens makers formula & Other Functions of lens.
5.1 Thin Lens Formula
5.2 Magnification and Power of lens
5.3 Combination of lenses
5.4 Displacement method to find focal length.
5.5 Silvering of lens
6.0 Total internal reflection
7.0 Refraction through prism
8.0 Scattering of light
9.0 Optical instruments
9.1 Spectrometer
9.2 Simple microscope
9.3 Compound microscope
9.4 Astronomical telescope (Refracting type)
9.5 Terrestrial telescope
9.6 Galileo's terrestrial telescope
9.7 Reflecting type telescope
9.2 Simple microscope
4.2 Some important terms
4.3 Ray tracing
4.4 Image formed by covex lens
4.5 Image formed by concave lens
5.2 Magnification and Power of lens
5.3 Combination of lenses
5.4 Displacement method to find focal length.
5.5 Silvering of lens
9.2 Simple microscope
9.3 Compound microscope
9.4 Astronomical telescope (Refracting type)
9.5 Terrestrial telescope
9.6 Galileo's terrestrial telescope
9.7 Reflecting type telescope
It is also known as magnifying glass or simple magnifier. It consists of a convergent lens with object between its focus and optical centre and eye close to it. The image formed by it is erect, virtual, enlarged and on same side of lens between its focus and optical centre and eye close to it. The image formed by it is erect, virtual, enlarged and on same side of lens between object and infinity.
- Magnifying power $(M)$ is defined as the ratio of angle subtended by image at the eye $(\beta )$ to the angle subtended by the object at the eye $(\alpha )$.
$$M = \frac{{{\text{angle subtended by image at the eye}}}}{{{\text{angle subtended by the object at the eye}}}}$$ $$M = \frac{{\tan \beta }}{{\tan \alpha }} \approx \frac{\beta }{\alpha }$$
where both object and image are situated at the least distance of distinct vision.
- When the image is formed at infinity (far point), $$M = \frac{D}{f}$$
- When the image is formed at the least distance of distinct vision $D$ (near point), $$M = 1 + \frac{D}{f}$$