sin α = sin φ cosec δ
sin α = sin φ sec δ
sin α = cos φ sec δ
sin α = cos φ cosec δ
A. sin α = sin φ cosec δ
Centre of the celestial sphere is taken as the position of the observer
Centre of the celestial sphere is taken as the centre of the earth
Stars move and maintain their relative positions
All the above
Horizon and equator
Zenith and pole
Equator and zenith
Pole and horizon
- 8.8 cos α
+ .8 sin α
+ 8.8 cos α
- 8.8 cos α
Positive for points above datum
Negative for points below datum
Zero for points vertically below the air station
All the above
East of observer
West of observer
North of observer
South of observer
cos δ/cos λ
cos (90° - δ)/cos (90° - λ)
sin (90° - δ)/sin (90° - λ)
tan (90° + δ)/tan (90° + λ)
High oblique
Low oblique
Vertical
None of these
First point of Aeries
First point of Libra
Vernal Equinox
Both (b) and (d) of the above
sin a cos A
cos a sin A
tan a cot A
cot A tan a
Eastward
Westward
Northward
Southward
δ - θ
θ - δ
θ + δ
½ (θ - δ)
sin λ
cos λ
tan λ
cot λ
1 : 10,000
1 : 15,000
1 : 20,000
1 : 30,000
sin H = tan φ . cot δ
cos H = tan φ . cot δ
tan H = tan φ . cot δ
None of these
Apparent solar time is measured from the lower transit of the true sun
Mean solar time is measured from the lower transit of the mean sun
Sidereal time is measured from the lower transit of the first point of Aries
Sidereal time is measured from the upper transit of the first point of Aries
B = bH/f
B =f/bH
B = b/fH
B = H/bf
Sidereal time at any instant is equal to the hour angle of the first point of Aries
Local sidereal time of any place is equal to the right ascension of its meridian
Sidereal time is equal to the right ascension of a star at its upper transit
All the above
Ursa Minor's remains always north of pole star
Polar star remains always north of Polaris
Polaris remains always north of Ursa Minor's
Ursa Minor's pole star and Polaris are the names of the same star
Declination must be 0°
Declination must be 90°
Distance from the pole must be less than the latitude of the observer
Hour angle must be 180°
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
Swing
Tilt
Tip
None of these
50 %
60 %
70 %
75 %
Sidereal time
Apparent solar time
Mean solar time
All the above
500 m
1000 m
1500 m
2000 m
Isocenter
Plumb point
Principal point
None of these
Altitude and azimuth system
Declination and hour angle system
Declination and right ascension system
Declination and altitude system
58 cot α
58 tan α
58 sin α
58 cos α
Plane surveying
Geodetic surveying
Star observations
Planet observations
Correction for refraction is always negative
Correction for parallax is always positive
Correction for semi-diameter is always negative
Correction for dip is always negative
f/H sec θ
f sec θ/H
f/H
f/H cos ½θ