
Light - Reflection
Science ยท Grade 9 ยท Week 38 ยท 25 questions
Light travels in straight lines, bounces off mirrors, and bends through lenses. Understanding how light behaves explains everything from rainbows to eyeglasses to cameras.
What you'll practise
- Work with angles
- Explain reflection and refraction of light
- Describe how mirrors and lenses form images
- Understand the visible spectrum and colours
All 25 questions in this Light - Reflection quiz
Grade 9 Science โ Light - Reflection: 25 practice questions with instant scoring and explanations.
- The laws of reflection state that the angle of incidence:
- A plane mirror produces an image that is:
- The magnification produced by a plane mirror is:
- A concave mirror converges light at a point called:
- The focal length (f) of a mirror is related to radius of curvature (R) by:
- For a mirror with R = 40 cm, the focal length is:
- A convex mirror always produces:
- The mirror formula is:
- For a concave mirror with f = 10 cm, if u = 20 cm (object distance), then image distance (v) is:
- Magnification (m) is calculated as:
- A real, magnified, inverted image is formed when object is placed:
- A virtual, magnified, upright image is formed by concave mirror when object is:
- A convex mirror with f = 15 cm and u = 30 cm produces an image at:
- The magnification for a plane mirror is always:
- In the sign convention for mirrors, the focal length of a concave mirror is:
- The radius of curvature of a convex mirror is considered:
- When an object is at the focal point of a concave mirror, the image is:
- A concave mirror is used in:
- A convex mirror is commonly used in:
- For a concave mirror with f = 8 cm, u = 16 cm, the magnification is:
- The light ray parallel to principal axis of a concave mirror reflects through:
- A ray passing through the focal point of a concave mirror reflects:
- The power of a mirror (P) is defined as:
- A concave mirror with f = 0.5 m has a power of:
- Spherical aberration in mirrors is minimized when:
Question 1 of 250 correct so far