(a) | the distance between the objective and the eyepiece is 20.02m. |
(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) |
In an astronomical telescope in normal adjustment, a straight line of length L is drawn on the inside part of the objective lens. The eye-piece forms a real image of this line. The length of this image is l. The magnification of the telescope is:
1. Ll+1
2. Ll−1
3. L+1l−1
4. Ll
An astronomical refracting telescope will have large angular magnification and high angular resolution when it has an objective lens of:
1. | small focal length and large diameter. |
2. | large focal length and small diameter. |
3. | large focal length and large diameter. |
4. | small focal length and small diameter. |
1. | 46.0cm | 2. | 50.0cm |
3. | 54.0cm | 4. | 37.3cm |