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
D. All the above
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
80°
70°
60°
50°
24 hours 10 minutes
20 hours 25 minutes
24 hours 50 minutes
23 hours 50 minutes
cos H = tan λ/tan δ
sin α = sin λ/sin δ
sin A = cos δ/cos λ
All the above
Zenith
Celestial point
Nadir
Pole
Do not follow any definite mathematical law
Cannot be removed by applying corrections to the observed values
Are generally small
All the above
North end of the polar axis is known as North Pole
South end of the polar axis is known as South Pole
Point where polar axis when produced northward intersects the celestial sphere, is known as north celestial pole
All the above
The horizontal direction of the pole is called astronomical north
The angle between the direction of true north and the direction of a survey line is called astronomical bearing
The astronomical bearing is generally called azimuth
All the above
Isocenter
Principal point
Perspective centre
Plumb line
Photo plumb point
Plumb point
Nadir point
Isocenter
29 days
29.35 days
29.53 days
30 days
22° 30'
23° 27'
23° 30'
24° 0'
Optical projection
Optical mechanism projection
Mechanical projection
All the above
0.1 mm
0.5 mm
1.00 mm
1.1 mm
Normal to base line
Parallel to base line
Both (a) and (b)
Neither (a) nor (b)
Co-declination
Co-altitude
Co-latitude
Polar distance
sin H = tan φ . cot δ
cos H = tan φ . cot δ
tan H = tan φ . cot δ
None of these
f tan θ
f sin θ
f cot θ
f cos θ
1 m
2 m
4 m
8 m
Increases as the horizontal distance increases from the principal point
Increases as the ground elevation increases
Decreases as the flying height increases
All the above
30°
35°
40°
45°
Photo principal point
Ground principal point
Ground isocenter
All the above
Photo principal point and ground principal point
Photo isocenter and ground isocenter
Photo plumb point and ground plumb point
All the above
Latitudes north of the equator are taken as positive
Latitudes south of the equator are taken as negative
Longitudes east of Greenwich are taken as negative
Longitudes west of Greenwich are taken as positive
Isocenter
Plumb point
Principal point
None of these
High oblique
Low oblique
Vertical
None of these
The measured stereoscopic base of photographs is obtained by dividing the air base in metres by the mean scale of the photograph
The difference between the absolute parallax of two points depends upon the difference in their elevations
The line joining the principal point of a photograph and the transferred principal point of the adjoining photograph, is called stereoscopic base
All the above
Parallel to the principal line
Perpendicular to the principal line
Along the bisector of the angle between the principal line and a perpendicular line through principal plane
None of these
Is the period of time taken by the earth in making a complete rotation with reference to stars
Is slightly shorter than an ordinary solar day
Is divided into the conventional hours, minutes and seconds
All the above
Meridian
Vertical circle
Prime vertical
None of these