Rectilinear Propagation Of Light ICSE Class-6th Goyal Brothers Physics Solutions Chapter-5 Unit-2
WhatsApp Group
Rectilinear Propagation Of Light ICSE Class-6th Goyal Brothers Physics Solutions Chapter-5 Unit-2 We provide step-by-step answers to objective questions, true/false statements, incorrect and correct statements, fill in the blanks, match the following, and study questions of Chapter-5 (Light, Unit-2: Rectilinear Propagation Of Light, Pinhole Camera, and Shadows).
Light
Camera
CISCECISCE

Rectilinear Propagation Of Light Pinhole Camera And Shadows ICSE Class-6th Goyal Brothers Physics Solutions Chapter-5 Unit-2
List : high, solar, shadow, straight lines, inverted
An opaque body as a screen is necessary in the formation of a shadow because a shadow is formed when an object blocks light and a surface is needed to show the dark region. Without a screen (or surface) the dark region cannot be clearly observed.
The image formed by a pinhole camera is always real and inverted. Light from each point of the object crosses through the pinhole and falls on the opposite side of the box, producing a real image on the screen which is upside down.
Solar eclipse takes place less frequently than the lunar eclipse. This is because the Moon's shadow on the Earth is very small and lies along a narrow path, whereas the Earth's shadow on the Moon is much larger and easier for the Moon to enter.
The size of the umbra decreases as the opaque body is moved away from the screen. When the object moves away from the screen, the fully dark region becomes smaller because the light from the source can reach more of the screen around the object.
Solar eclipse lasts for a shorter time than a lunar eclipse. The Moon's shadow moves quickly across the Earth and the area of totality is small, so totality at any given place lasts only a few minutes, while a lunar eclipse can be seen from the whole night side of Earth and therefore lasts longer.
Answer:
Answer:

Answer:
Answer:
Rectilinear Propagation Of Light Pinhole Camera And Shadows ICSE Class-6th Goyal Brothers Physics Solutions Chapter-5 Unit-2
Materials: Three identical cardboard sheets, a pin or small hole, a candle or small lamp and a stand.
Procedure:
Observation: You can see the candle flame only when all three holes are exactly aligned. If any one cardboard is moved slightly so the holes are not in a straight line, the flame is no longer visible.
Conclusion: This shows that light travels in straight lines because only when the holes form a straight path can rays from the candle reach the eye.
The principle of a pinhole camera is that light travels in straight lines (rectilinear propagation). Rays of light from different points of an object pass through the pinhole and form corresponding points on the screen, producing an image which is real and inverted.
Construction:
Working:
Note: A clear diagram showing rays from the top and bottom of an object crossing at the pinhole and forming an inverted image on the screen should be drawn to support this explanation.
(i) If the distance between the pinhole and the screen increases, the image size on the screen increases because rays travel a longer distance and spread out more. However, the image becomes dimmer since the same light energy spreads over a larger area.
(ii) If the object is moved farther from the pinhole, the image size on the screen becomes smaller because the rays from the object spread less by the time they reach the pinhole. The image may also become slightly less bright.
A shadow is a dark region formed on a surface when light from a source is blocked by an opaque object.
Three conditions necessary for the formation of a shadow:
When the source is smaller than the object, there is a clear umbra (completely dark region) behind the object and a smaller penumbra around it. As the screen is moved farther from the object, the umbra becomes smaller because more rays from different parts of the source can reach around the object, while the penumbra becomes larger and fainter. If the screen is moved very far, the umbra may shrink and eventually disappear, leaving mostly penumbra.
When the source is larger than the object there is a large penumbra and a small or sometimes no umbra. The penumbra is wide because different parts of the large source send rays that are partially blocked. As the screen moves away, the penumbra grows wider and the umbra (if present) becomes smaller and may disappear altogether, leaving only a faint, large penumbra.
Birds flying very high appear not to cast noticeable shadows on the ground because the distance between the bird and the ground is large. Light rays from the Sun come from many directions (the Sun is effectively an extended source) so the small umbra produced by the bird is tiny by the time it reaches the ground and the penumbra is very spread out and faint. Thus any shadow becomes too small or too faint to see.
Fluorescent tube lights are called shadowless lights because the tube is an extended source of light. Light comes from many points along the tube so the shadows from these many points overlap. This makes the umbra very small or absent and produces only a faint penumbra, so distinct sharp shadows are not visible.
A solar eclipse occurs when the Moon comes between the Sun and the Earth and blocks all or part of the Sun's light from reaching a part of the Earth. During a total solar eclipse the Moon completely covers the Sun as seen from a small region on Earth, producing a dark area called the umbra on Earth's surface.
A solar eclipse lasts for a short time at any one place because the Moon's shadow moves quickly over the Earth's surface and the path of totality is narrow. The Moon's shadow travels across the Earth at high speed, so the period of totality at a given location is only a few minutes.
A total solar eclipse is not frequent because the Moon's orbit is tilted by about 5° to the Earth's orbit. This tilt means that the Moon's shadow does not fall on the Earth every new moon. Only when the Moon is near the plane of Earth's orbit during a new moon do eclipses occur, making total solar eclipses uncommon.
A lunar eclipse happens when the Earth comes between the Sun and the Moon so that the Moon passes into the Earth's shadow. During a total lunar eclipse the whole Moon moves into the Earth's umbra and appears dark or reddish.
A lunar eclipse lasts longer because the Earth's shadow is much bigger than the Moon's shadow, and the Moon moves more slowly through the Earth's shadow compared with the speed of the Moon's shadow over the Earth's surface. As a result, the Moon can remain in the shadow for a longer time.
Lunar eclipses are more frequent from any one place because the Earth's shadow is large and a lunar eclipse can be seen by anyone on the night side of Earth when it occurs. The Moon more often passes through Earth's larger shadow than the Moon's small shadow falls on the Earth, so solar eclipses are rarer.
Direct viewing of a solar eclipse with the naked eye is dangerous because the Sun's bright visible light and invisible ultraviolet rays can damage the retina and may cause permanent blindness.
Safe ways to observe a solar eclipse:
Never look directly at the Sun through unfiltered optical devices or ordinary glasses.
- : End Rectilinear Propagation Of Light Pinhole Camera And Shadows ICSE Class-6th Goyal Brothers Physics Solutions Chapter-5 Unit-2 :--
Return to- ICSE Class -6 Goyal Brothers Physics Solutions
Return to- ICSE Class -6 Goyal Brothers Physics SolutionsICSE Class -6 Goyal Brothers Physics Solutions
Thanks
Please share with your friends if you find it useful
