| 1 |
Who attempted to measure the speed of light |
Gallileo
Michelson
Newton
None of these
|
| 2 |
The refracting edge of the prism must be parallel to the axis of rotation of the telescope, so that the turn table is leveled using |
Screws of the spectrometer
Leveling screws
Turn table screw
None of these
|
| 3 |
A telescope is rotatable about the same vertical axis as the turntable, with a scale which is |
Main scale
Vernier scale
Half degree scale
None of these
|
| 4 |
A circular scale is attached and graduated in |
One degree
2 degrees
Half degree
None of these
|
| 5 |
Turn table is the plateform over which we place |
Diffraction grating
Prism
Glass slab
a and b
|
| 6 |
The function of colimator is |
To converge the incoming rays
To make the parallel rays from source
In which the source of light is kept
None of these
|
| 7 |
The different parts of spectrometer |
Collimator
Turn table
Telescope
All of these
|
| 8 |
Spectrometer using diffraction grating can measure |
Wavelength of light
Frequency of light
Intensity of light
None of these
|
| 9 |
Spectrometer can measure quite accurately prism |
Deviation of light by a glass prism
Angle of prism
Refractive index of the material of prism
None of these
|
| 10 |
A spectrometer is an optical device used to study the spectra from different sources of light which is |
Absorption spectra
Emission spectra
Discrete spectra
None of these
|
| 11 |
In normal adjustment, the length of the telescope is |
f<sub>e</sub> + f<sub>o</sub>
f<sub>o</sub> - f<sub>e</sub>
f<sub>e</sub> - f<sub>o</sub>
None of these
|
| 12 |
When an image formed by the objective lies at the focus of both the objective and the eye-piece, the telescope is said to be in |
Final adjustment
Normal adjustment
Initial adjustment
None of these
|
| 13 |
When an image is placed at the focal length of the eye piece, the final image formed at |
2 F
4 F
6 F
Infinity
|
| 14 |
The image formed after objective lens of an astronomical telescope is |
Inverted
Diminished
Real
All of these
|
| 15 |
In an astronomical telescope the eye piece has the focal length fe if |
Short
Long
Extremely long
None of these
|
| 16 |
In an astronomical telescope is the objective has the focal length fo is |
Small
Very small
Long
None of these
|
| 17 |
A simple telescope is consists of |
One convex lens
Two convex lenses
Three convex lenses
None of these
|
| 18 |
In viewing the distant objects the angle subtended at the telescope is |
Smaller
Bigger
Very large
None of these
|
| 19 |
Telescope is an optical device used for viewing |
Near objects
Not far distance
Distant objects
b and c
|
| 20 |
If the magnification M1 = 20.0 for objective and M2 = 12.0 then total magnification is |
200
240
260
280
|
| 21 |
If the focal length of the eye piece 25.0 mm find its magnification |
12.0
14.0
- 11.0
- 13.0
|
| 22 |
If the focal length of objective is 10 mm find its magnification |
18
19
20
21
|
| 23 |
A microscope has an objective lens of 10 mm focal length and an eye piece of 25.0 mm focal length what is the distance between the lenses |
≈ 200 mm
≈ 210 mm
≈ 213 mm
≈ 233 mm
|
| 24 |
A compound microscope is consists of objective of |
Long focal length and short focal length of eye piece
Objective of very short focal length and eye piece of long focal length
Objective of very short focal length end eye piece of also short focal length
None of these
|
| 25 |
A compound microscope is consists of an eye piece of focal length |
Short
Very short
Large
Very large
|
| 26 |
A compound microscopes consists of objective of |
Very short focal length
Large focal length
Very large focal length
None of these
|
| 27 |
A compound microscope is consists of |
One convex lens
Two convex lenses
Two concave lenses
None of these
|
| 28 |
Whenever high magnification is desired |
A telescope is used
A compound microscope is used
A microscope is used
None of these
|
| 29 |
Magnification of a convex lens is |
M = p/d
M = p/q
M = q/p
None of these
|
| 30 |
If N is the number of rulings on the grating, then the resolving power in the mth order diffraction equals to |
R = N × m
R = N/m
R = m/N
R = N × m<sup>2</sup>
|
| 31 |
The optical resolution of microscope or a telescope tells us how close together, the two point sources of light can be so that they are still seen as two separate sources |
Angular magnification
Resolution
Magnification
None of these
|
| 32 |
When the object is closer to eye or near point, the image becomes |
Sharp
Clear visible
Blurred
None of these
|
| 33 |
The ratio of size of the image to the size of the object is called |
Resolving power
Magnification
Power
None of these
|
| 34 |
If f = 5 cm and d = 25 cm then the magnification will be |
2
4
5
6
|
| 35 |
The maximum size of an object as seen by the naked eye is obtained when it is placed of |
Far point
Near point
Distant point None of these
|
| 36 |
The apparent size of an object depends on the angle subtended but it at the eye. As the angle increases the size of the object |
Smaller
Larger
Very large
None of these
|
| 37 |
As the object is brought from a far off point to he focus, the magnification goes on |
Increasing
Decreasing
Do not change
None of these
|
| 38 |
The least distance of distinct vision changes with |
Time
Health
illness
Age
|
| 39 |
The least distance of he distinct vision is |
20 cm
22 cm
25 cm
30 cm
|
| 40 |
The normal human eye can focus a sharp image of an object located anywhere form infinity to a certain point called |
Far point
Near point
distant point
None of these
|