The sun's right ascension increases for 0 h to 24 h when it returns to the First point of Aries
The maximum declination of the sun increases up to 23 ½° N on about 21st June
The minimum declination of the sun is zero' on 22nd September
All the above
D. All the above
7 h 00 m
7 h 30 m
8 h 00 m
9 h 00 m
The east point of the horizon
The west point of the horizon
The zenith point of the observer
All the above
Astronomical latitude
Astronomical longitude
Astronomical bearing
All of these
24 hours 10 minutes
20 hours 25 minutes
24 hours 50 minutes
23 hours 50 minutes
Do not follow any definite mathematical law
Cannot be removed by applying corrections to the observed values
Are generally small
All the above
sin z = sec φ . cos δ
cos z = sec φ . cos δ
tan z = sec φ . cos δ
None of these
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
Hour angle
Azimuth
Right ascension
Declination
One minute arc of the great circle passing through two points
One minute arc of the longitude
1855.109 m
All the above
f/H sec θ
f sec θ/H
f/H
f/H cos ½θ
The sum of the angles around a station should be 360°
The sum of the three angles of a plane triangle should be 180°
The sum of the eight angles of a braced quadrilateral should be 360°
All the above
Horizon and equator
Equator and zenith
Zenith and pole
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
Tension = (P - Ps)L/AE
Sag = L3w²/24P² where w is the weight of tape/m
Slope = (h²/2L) + (h4/8L3) where h is height difference of end supports
All the above
29 days
29.35 days
29.53 days
30 days
1/3
1/2
3/4
5/4
Eastward
Westward
Northward
Southward
30°
35°
40°
45°
cos δ/cos λ
cos (90° - δ)/cos (90° - λ)
sin (90° - δ)/sin (90° - λ)
tan (90° + δ)/tan (90° + λ)
58 cot α
58 tan α
58 sin α
58 cos α
Ground elevation
Flying height
Length of air base
All the above
Equator
Celestial equator
Ecliptic
None of these
When its altitude is maximum
When its azimuth is 180°
When it is in south
All the above
h tan α/S
h tan β/S
h (tan α + tan β)/S
h (tan α - tan β)/S
180° eastward
180° westward
180° east or westward
360° eastward
Elevation of the elevated pole
Declination of the observer's zenith
Angular distance along the observer's meridian between equator and the observer
All the above
Parallax
Height
Parallax difference
Height difference
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
4000 m
5000 m
6000 m
7000 m
Sun and moon are in line with earth
Solar tidal force acts opposite to lunar tidal force
Solar tidal force and lunar tidal force both coincide
None of these