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This section includes 195 Mcqs, each offering curated multiple-choice questions to sharpen your Surveying knowledge and support exam preparation. Choose a topic below to get started.
| 101. |
The polaris remains below horizon at |
| A. | 10° N |
| B. | 50° N Latitude |
| C. | equator |
| D. | 5° S latitude. |
| Answer» E. | |
| 102. |
Circumpolar stars |
| A. | rotate round the north pole |
| B. | rotate round the celestial pole |
| C. | remain always above the horizon |
| D. | are seldom seen near the pole star |
| Answer» D. are seldom seen near the pole star | |
| 103. |
At western elongation, the pole star moves |
| A. | eastward |
| B. | westward |
| C. | northward |
| D. | southward. |
| Answer» E. | |
| 104. |
Places having same latitude |
| A. | lie on the parallel of the latitude |
| B. | are equidistant from the nearer pole |
| C. | are equidistant from both the poles |
| D. | all the above. |
| Answer» E. | |
| 105. |
The latitude of a place was obtained by subtracting the declination of a star from its zenith distance, the observed star was between |
| A. | horizon and equator |
| B. | zenith and pole |
| C. | equator and zenith |
| D. | pole and horizon. |
| Answer» B. zenith and pole | |
| 106. |
If θ and δ be the latitude of a place and declination of a star respectively, the upper culmination of the star will be north of zenith if its zenith distance, is |
| A. | δ - θ |
| B. | θ - δ |
| C. | θ + δ |
| D. | (θ + δ)/2 |
| Answer» B. θ - δ | |
| 107. |
By raising the z-column of right projector, maximum y-parallax is introduced in the model at |
| A. | position 1 |
| B. | position 2 |
| C. | position 4 |
| D. | position 4 and 6. |
| Answer» E. | |
| 108. |
The height displacement on a vertical photograph |
| A. | increases as the horizontal distance increases from the principal point |
| B. | increases as the ground elevation increases |
| C. | decreases as the flying height increases |
| D. | all the above. |
| Answer» E. | |
| 109. |
For plane ground the scale of a vertical photograph will be same as that of a tiled photograph along the photo parallel through |
| A. | isocentre |
| B. | plumb point |
| C. | principal point |
| D. | none of these. |
| Answer» B. plumb point | |
| 110. |
An aerial photograph may be assumed as |
| A. | parallel projection |
| B. | orthogonal projection |
| C. | central projection |
| D. | none of these. |
| Answer» D. none of these. | |
| 111. |
The latitude of a place was obtained by subtracting the zenith distance of a star from its declination, the observed star was between |
| A. | horizon and equator |
| B. | equator and zenith |
| C. | zenith and pole |
| D. | pole and horizon. |
| Answer» D. pole and horizon. | |
| 112. |
The latitude (λ) of a place and the altitude (α) of the pole are related by |
| A. | λ = α |
| B. | λ = 90° - α |
| C. | λ = α - 90° |
| D. | λ = 180° - α. |
| Answer» B. λ = 90° - α | |
| 113. |
The station which is selected close to the main triangulation station, to avoid intervening obstruction, is not known as |
| A. | satellite station |
| B. | eccentric station |
| C. | false station |
| D. | pivot station. |
| Answer» E. | |
| 114. |
Assuming human normal vision distance 25 cm, smallest measurable angle 20", and introcular distance 6.5 cm, the smallest depth to be discerned is |
| A. | 0.1 mm |
| B. | 0.5 mm |
| C. | 1.00 mm |
| D. | 1.1 mm. |
| Answer» B. 0.5 mm | |
| 115. |
The solar tidal force divided by lunar tidal force is |
| A. | 1/3 |
| B. | 1/2 |
| C. | 3/4 |
| D. | 5/4 |
| Answer» C. 3/4 | |
| 116. |
If the general ground level of any area is 10% of the flying height, the principal points may be used as the centres of radial directions for small scale mapping even in tilted photograph up to |
| A. | 1° |
| B. | 2° |
| C. | 3° |
| D. | 4° |
| Answer» D. 4° | |
| 117. |
In triangulation surveys |
| A. | the area is divided into triangular figures |
| B. | control stations are located from which detailed surveys are carried out |
| C. | sides are not measured excepting the base line |
| D. | all the above. |
| Answer» E. | |
| 118. |
The stereo plotting instruments are generally manufactured on the principle of |
| A. | optical projection |
| B. | optical mechanism projection |
| C. | mechanical projection |
| D. | all the above. |
| Answer» E. | |
| 119. |
Latitude of a place is the angular distance from |
| A. | Greenwich to the place |
| B. | equator to the poles |
| C. | equator to the nearer pole |
| D. | none of these. |
| Answer» E. | |
| 120. |
The point at which sun's declination changes from north to south, is known as |
| A. | first point of Aeries |
| B. | first point of Libra |
| C. | autumnal Equinox |
| D. | both (b) and (c) of the above. |
| Answer» E. | |
| 121. |
The point where vertical line passing through the perspective centre intersects the plane of the photograph, is known as |
| A. | photo plumb point |
| B. | plumb point |
| C. | nadir point |
| D. | isocentre |
| Answer» B. plumb point | |
| 122. |
If δ is the declination of the star and φ is the latitude of the observer then the hour angle of the star at elongation is given by |
| A. | sin H = tan φ . cot δ |
| B. | cos H = tan φ . cot δ |
| C. | tan H = tan φ . cot δ |
| D. | none of these. |
| Answer» C. tan H = tan φ . cot δ | |
| 123. |
Triangulation surveys are carried out for locating |
| A. | control points for surveys of large areas |
| B. | control points for photogrammetric surveys |
| C. | engineering works, i.e. terminal points of long tunnels, bridge abutments, etc. |
| D. | all the above. |
| Answer» E. | |
| 124. |
The method of surveying by triangula-tion was first introduced by the Dutchman Snell in |
| A. | 1600 |
| B. | 1615 |
| C. | 1630 |
| D. | 1650 |
| Answer» C. 1630 | |
| 125. |
From the principal point the horizon point lies on the principal line at a distance of |
| A. | f tan θ |
| B. | f sin θ |
| C. | f cot θ |
| D. | f cos θ. |
| Answer» B. f sin θ | |
| 126. |
The principal plane contains |
| A. | nadir point |
| B. | iso centre |
| C. | principal point |
| D. | all the above.. |
| Answer» E. | |
| 127. |
The equation which is obtained by multiplying each equation by the coefficient of its un-knowns and by adding the equations thus formed, is known as |
| A. | observation equation |
| B. | conditional equation |
| C. | normal equation |
| D. | none of these. |
| Answer» D. none of these. | |
| 128. |
The most convenient co-ordinate system for specifying the relative positions of heavenly bodies on the celestial sphere, is |
| A. | altitude and azimuth system |
| B. | declination and hour angle system |
| C. | declination and right ascension system |
| D. | declination and altitude system |
| Answer» D. declination and altitude system | |
| 129. |
The relief displacement of a minar 72 m high on photograph is 7.2 mm and its top appears 10 cm away from principal point. The flying height of the camera, is |
| A. | 500 m |
| B. | 1000 m |
| C. | 1500 m |
| D. | 2000 m. |
| Answer» C. 1500 m | |
| 130. |
Pick up the correct statement from the following. The difference between the longitudes of the places is obtained. |
| A. | by subtracting their longitudes if places are in the same hemisphere |
| B. | by adding their longitudes if places are in the different hemispheres |
| C. | by subtracting the sum of their longitudes exceeding 180° from 360° if places are in different hemispheres |
| D. | all the above. |
| Answer» D. all the above. | |
| 131. |
In a tropical year, the number of sidereal days, are |
| A. | 365 |
| B. | 365.2224 |
| C. | 365.2422 |
| D. | 366.2422 |
| Answer» E. | |
| 132. |
The declination and right ascension of the sun are each equal to zero on |
| A. | March 21 |
| B. | June 21 |
| C. | September 21 |
| D. | December 22. |
| Answer» B. June 21 | |
| 133. |
Spring tides are caused when |
| A. | sun and moon are in line with earth |
| B. | solar tidal force acts opposite to lunar tidal force |
| C. | solar tidal force and lunar tidal force both coincide |
| D. | none of these. |
| Answer» D. none of these. | |
| 134. |
If f is the focal length of the camera lens and θ is the angle of tilt, the distance of the plumb point from the principal point will be |
| A. | f sin θ |
| B. | f cos θ |
| C. | f tan θ |
| D. | f sec θ. |
| Answer» D. f sec θ. | |
| 135. |
If the distance between the projectors is altered by a movement along X-axis of one projector, |
| A. | the length of the air base is increased |
| B. | the scale of the model is altered |
| C. | y-parallax is not affected |
| D. | all the above. |
| Answer» E. | |
| 136. |
The elevation of the star at elongation is obtained by |
| A. | sin α = sin φ cosec δ |
| B. | sin α = sin φ sec δ |
| C. | sin α = cos φ sec δ |
| D. | sin α = cos φ cosec δ. |
| Answer» B. sin α = sin φ sec δ | |
| 137. |
For mapping any country |
| A. | geodetic triangulation of greatest possible sides and accuracy is carried out |
| B. | primary triangles are broken down into secondary triangles of somewhat lesser accuracy |
| C. | secondary triangles are further broken into third and fourth order triangles, the points of which are used for detail surveys |
| D. | all the above. |
| Answer» E. | |
| 138. |
The angle between the plane of the equator and the plane of the ecliptic, is known as obliquity of the ecliptic and its value is |
| A. | 22° 30' |
| B. | 23° 27' |
| C. | 23° 30' |
| D. | 24° 0'. |
| Answer» C. 23° 30' | |
| 139. |
While making astronomical observations, the observer is mainly concerned with |
| A. | the direction of the vertical, the axis of rotation of the instrument |
| B. | the direction of the poles of the celestial sphere |
| C. | the direction of the star from the instrument |
| D. | all the above. |
| Answer» E. | |
| 140. |
The altitude of a heavenly body is its angular distance, measured on the vertical circle passing through the body, above |
| A. | equator |
| B. | horizon |
| C. | pole |
| D. | none of these. |
| Answer» C. pole | |
| 141. |
At lower culmination, the pole star moves |
| A. | eastward |
| B. | westward |
| C. | northward |
| D. | southward. |
| Answer» B. westward | |
| 142. |
In a truly vertical photograph, |
| A. | principal point coincides the isocentre |
| B. | iso-centre coincides the plumb point |
| C. | plumb point coincides the principal point |
| D. | all the above. |
| Answer» E. | |
| 143. |
If S is the sum of three angles of a spherical triangle, the spherical excess equals |
| A. | S - 90° |
| B. | S - 180° |
| C. | S - 270° |
| D. | S - 360°. |
| Answer» C. S - 270° | |
| 144. |
In a spherical triangle ABC right angled at C, sin b equals to |
| A. | sin c sin B |
| B. | cos c cos B |
| C. | tan c tan B |
| D. | sin c cos B |
| Answer» B. cos c cos B | |
| 145. |
The nautical mile is the length of |
| A. | 1 minute of latitude |
| B. | 1 minute of longitude |
| C. | 1 degree of latitude |
| D. | 1 degree of longitude. |
| Answer» C. 1 degree of latitude | |
| 146. |
The scale of a tilted photograph of focal length f, taken from an altitude H, along the plate parallel through plumb point, is |
| A. | A |
| B. | B |
| C. | C |
| D. | D |
| Answer» C. C | |
| 147. |
To obtain photographs of an area of 1000 m average elevation, on scale 1 : 30, 000, with a camera of 30 cm focal length, the flying height is |
| A. | 4000 m |
| B. | 5000 m |
| C. | 6000 m |
| D. | 7000 m. |
| Answer» D. 7000 m. | |
| 148. |
On vertical photographs, height displacement is |
| A. | positive for points above datum |
| B. | negative for points below datum |
| C. | zero for points vertically below the air station |
| D. | all the above. |
| Answer» E. | |
| 149. |
The difference of parallax for a given difference in elevation is independent of |
| A. | focal length of the camera |
| B. | overall size of the photo graphs |
| C. | percentage of overlap |
| D. | all the above. |
| Answer» E. | |
| 150. |
α and β are the angles subtended by a point of elevation h at their air station with respective plumb points. Photo scale and focal length of the lens being S and f respectively. Parallax displacement of the point due to relief, is |
| A. | A |
| B. | B |
| C. | C |
| D. | D |
| Answer» D. D | |