First point of Aeries
First point of Libra
Vernal Equinox
Both (b) and (d) of the above
D. Both (b) and (d) of the above
Opposite corners of a photograph
Nodal points of the camera lens
Corresponding points on the ground and photograph
Plumb points of stereo pair of photographs
f/H
f/(H + h)
f/(H - h)
(H - h)/f
Photo plumb point
Plumb point
Nadir point
Isocenter
A great circle passing through the place and the poles
A great circle whose plane is perpendicular to the axis of rotation and it also passes through the place
A semi-circle which passes through the place and is terminated at the poles
An arc of the great circle which passes through the place and is perpendicular to the equator
52 m
62 m
72 m
82 m
Standard meridian
Greenwich meridian
Equator
180° longitude
Nadir point
Iso centre
Principal point
All the above
Rational horizon
True horizon
Celestial horizon
All the above
The east point of the horizon
The west point of the horizon
The zenith point of the observer
All the above
29 days
29.35 days
29.53 days
30 days
- 8.8 cos α
+ .8 sin α
+ 8.8 cos α
- 8.8 cos α
58 mm
60 mm
62 mm
64 mm
Normal to base line
Parallel to base line
Both (a) and (b)
Neither (a) nor (b)
At culmination
At elongation
Neither at culmination nor at elongation
Either at culmination or at elongation
Declination
Altitude
Zenith distance
Co-latitude
58 cot α
58 tan α
58 sin α
58 cos α
One less than mean solar days
One more than mean solar days
Equal to mean solar days
None of these
2 mm
4 mm
6 mm
10 mm
Horizon and equator
Zenith and pole
Equator and zenith
Pole and horizon
The star's movement is apparent due to the actual steady rotation of the earth about its axis
The stars move round in circular concentrated parts
The centre of the circular paths of stars is the celestial pole
All the above
sin a cos A
cos a sin A
tan a cot A
cot A tan a
1 in 12
1 in 10
1 in 8
1 in 6
1000 km
800 km
600 km
500 km
10°
20°
30°
40°
Astronomical latitude
Astronomical longitude
Astronomical bearing
All of these
One degree of longitude has greatest value at the equator
One degree of longitude has greatest value at the poles
One degree of longitude has the same value everywhere
One degree of latitude decreases from the equator to the poles
Principal point
Isocenter
Plumb point
Perspective centre
80°
70°
60°
40°
1°
2°
3°
4°
Parallel lines do not appear parallel in central projection
The two sides of a road meet at the vanishing point
The lines parallel to the negative plane are projected as parallel lines
All the above