A small telescope has an objective lens of a focal length \(144~\text{cm}\) and an eyepiece of focal length \(6.0~\text{cm}.\) What is the magnifying power of the telescope?
1. | \(30\) | 2. | \(20\) |
3. | \(24\) | 4. | \(32\) |
Assertion (A): | If objective and eye lenses of a microscope are interchanged, then it can work as telescope. |
Reason (R): | The objective lens of telescope has small focal length. |
1. | Both (A) and (R) are True and (R) is the correct explanation of (A). |
2. | Both (A) and (R) are True but (R) is not the correct explanation of (A). |
3. | (A) is True but (R) is False. |
4. | Both (A) and (R) are False. |
(A) | The length of the telescope tube is \(20.02~\text{m}\). |
(B) | The magnification is \(1000\). |
(C) | The image formed is inverted. |
(D) | An objective of a larger aperture will increase the brightness and reduce chromatic aberration of the image. |
1. | (A) and (D) only |
2. | (A), (B) and (C) only |
3. | (B) and (D) only |
4. | (C) and (D) only |
1. | \(6\) cm and \(48\) cm |
2. | \(48\) cm and \(6\) cm |
3. | \(8\) cm and \(64\) cm |
4. | \(64\) cm and \(8\) cm |
A lens of large focal length and large aperture is best suited as an objective of an astronomical telescope since:
1. | a large aperture contributes to the quality and visibility of the images. |
2. | a large area of the objective ensures better light-gathering power. |
3. | a large aperture provides a better resolution. |
4. | all of the above. |
A giant refracting telescope at an observatory has an objective lens of focal length \(15\) m. If an eyepiece of focal length \(1.0\) cm is used, what is the angular magnification of the telescope?
1. | \(1175\) | 2. | \(1250\) |
3. | \(1300\) | 4. | \(1500\) |
(a) | the distance between the objective and the eyepiece is \(20.02\text{m}.\) |
(b) | the magnification of the telescope is \(-1000\). |
(c) | the image of the planet is erect and diminished. |
(d) | the aperture of the eyepiece is smaller than that of the objective. |
1. | (a), (b), and (c) | 2. | (b), (c), and (d) |
3. | (c), (d), and (a) | 4. | (a), (b), and (d) |