Hour angle
Azimuth
Right ascension
Declination
A. Hour angle
sin a cos A
cos a sin A
tan a cot A
cot A tan a
May have tilt up to 30°
May include the image of the horizon
May not include the image of the horizon
None of these
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
First point of Aeries
First point of Libra
Vernal Equinox
Both (b) and (d) of the above
1 minute of latitude
1 minute of longitude
1 degree of latitude
1 degree of longitude
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
Triangulation surveying
Astronomical surveying
Hydrographical surveying
Photogrammetric surveying
The principal point coincides with plumb point on a true vertical photograph
The top of a hill appears on a truly vertical photograph at greater distance than its bottom from the principal point
The top of a hill is represented on a vertical photograph at larger scale than the area of a nearby valley
All the above
L.M.T. - East longitude in time
L.M.T. + East longitude in time
L.M.T. - West longitude in time
None of these
One less than mean solar days
One more than mean solar days
Equal to mean solar days
None of these
Principal point coincides the isocenter
Iso-centre coincides the plumb point
Plumb point coincides the principal point
All the above
Nadir
Isocenter
Principal point
Plumb point
North pole
Pole star
Celestial pole
All the above
1°
2°
3°
4°
8,000 m
10,000 m
12,000 m
14,000 m
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
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
Plane surveying
Geodetic surveying
Star observations
Planet observations
Rotate round the North Pole
Rotate round the celestial pole
Remain always above the horizon
Are seldom seen near the pole star
Co-declination
Co-latitude
Declination
Latitude
1 in 12
1 in 10
1 in 8
1 in 6
9 cos α
9 sin α
9 tan α
9 cot α
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
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
Hour angle
Azimuth
Right ascension
Declination
Isocenter
Plumb point
Principal point
None of these
At culmination
At elongation
Neither at culmination nor at elongation
Either at culmination or at elongation
Rational horizon
True horizon
Celestial horizon
All the above
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
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