365
365.2224
365.2422
366.2422
D. 366.2422
One minute arc of the great circle passing through two points
One minute arc of the longitude
1855.109 m
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
0.50 sq km
0.56 sq km
0.60 sq km
0.64 sq km
δ - θ
θ - δ
θ + δ
½ (θ - δ)
θ = z + δ
θ = δ - z
θ = 180° - (z + δ)
θ = (z + δ) - 180°
Planimetric control
Height control
Both planimetric and height control
None of these
The area is divided into triangular figures
Control stations are located from which detailed surveys are carried out
Sides are not measured excepting the base line
All the above
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
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
Lengths
Angles
Heights
All of these
Swing
Tilt
Tip
None of these
1/3
1/2
3/4
5/4
The east point of the horizon
The west point of the horizon
The zenith point of the observer
All the above
The direction of the vertical, the axis of rotation of the instrument
The direction of the poles of the celestial sphere
The direction of the star from the instrument
All the above
Eastward
Westward
Northward
Southward
April 15
June 14
September 1
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
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
22° 30'
23° 27'
23° 30'
24° 0'
8,000 m
10,000 m
12,000 m
14,000 m
First point of Aeries
First point of Libra
Vernal Equinox
Both (b) and (d) of the above
Geodetic triangulation of greatest possible sides and accuracy is carried out
Primary triangles are broken down into secondary triangles of somewhat lesser accuracy
Secondary triangles are further broken into third and fourth order triangles, the points of which are used for detail surveys
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
1600
1615
1630
1650
cos H = tan λ/tan δ
sin α = sin λ/sin δ
sin A = cos δ/cos λ
All the above
East of observer
West of observer
North of observer
South of observer
Greenwich to the place
Equator to the poles
Equator to the nearer pole
None of these
Zenith
Celestial point
Nadir
Pole
1 : 10,000
1 : 15,000
1 : 20,000
1 : 30,000
Swing
Tilt
Tip
None of these