Equator
Horizon
Pole
None of these
B. Horizon
Visible horizon
Sensible horizon
Celestial horizon
True horizon
Swing
Tilt
Tip
None of these
52 m
62 m
72 m
82 m
B = bH/f
B =f/bH
B = b/fH
B = H/bf
fB/(H - h)
fB/(H - h)2
fB/(H + h)
fB/(H + h)2
May have tilt up to 30°
May include the image of the horizon
May not include the image of the horizon
None of these
Observation equation
Conditional equation
Normal equation
None of these
Satellite station
Subsidiary station
Pivot station
Main station
Greater than the longitude of the place
Less than the latitude of the place
Equal to the latitude of the place
None of these
10 km
25 km
30 km
50 km
Photo plumb point
Plumb point
Nadir point
Isocenter
1°
2°
3°
4°
Optical projection
Optical mechanism projection
Mechanical projection
All the above
Eastward
Westward
Northward
Southward
The plane passing through the perspective centre of a stereo pair and a ground point, is known as basal plane
Each pair of image points on stereo pair have their own basal plane
Relative orientation means reconstructing the basal plane
All the above
Length of the equator between their longitudes
Length of the parallel between their longitudes
Length of the arc of the great circle passing through them
None of these
sin α = sin φ cosec δ
sin α = sin φ sec δ
sin α = cos φ sec δ
sin α = cos φ cosec δ
Is the point in the celestial sphere where zero meridian crosses the celestial equator
Is usually denoted by the Greek letter γ
Is located near the very conspicuous rectangle of stars in the constellations of Pegasus and Andromeda
All the above
Every angle is less than two right angles
Sum of the three angles is equal to two right angles
Sum of the three angles less than six right angles and greater than two right angles
Sum of any two sides is greater than the third
1600
1615
1630
1650
S - 90°
S - 180°
S - 270°
S - 360°
When the star momentarily moves vertically
When the angle at the star of the spherical triangle is 90°
When the star's declination is greater than the observer's latitude
All the above
One minute arc of the great circle passing through two points
One minute arc of the longitude
1855.109 m
All the above
By subtracting their longitudes if places are in the same hemisphere
By adding their longitudes if places are in the different hemispheres
By subtracting the sum of their longitudes exceeding 180° from 360° if places are in different hemispheres
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
58 cot α
58 tan α
58 sin α
58 cos α
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
1/3
1/2
3/4
5/4
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
sin H = tan φ . cot δ
cos H = tan φ . cot δ
tan H = tan φ . cot δ
None of these