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4

If the image of a triangulation station of R.L. 500 m is 4 cm from the principal point of a vertical photo taken from an altitude of 2000 m, above datum, the height displacement will be

A. 2 mm

B. 4 mm

C. 6 mm

D. 10 mm

Correct Answer :

D. 10 mm


Related Questions

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4

The altitude of a circumpolar star is maximum when it is

A. At east elongation

B. At upper culmination

C. At west elongation

D. At lower culmination

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4

If δ is the declination of the star and φ is the latitude of the observer, then the azimuth of the star at elongation is given by

A. sin z = sec φ . cos δ

B. cos z = sec φ . cos δ

C. tan z = sec φ . cos δ

D. None of these

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4

The average eye base is assumed as

A. 58 mm

B. 60 mm

C. 62 mm

D. 64 mm

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4

Triangulation surveys are carried out for locating

A. Control points for surveys of large areas

B. Control points for photogrammetric surveys

C. Engineering works, i.e. terminal points of long tunnels, bridge abutments, etc.

D. All the above

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4

At western elongation, the pole star moves

A. Eastward

B. Westward

C. Northward

D. Southward

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4

If the altitudes of a star at its upper and lower transits are 60° 30' and 19° 30' respectively, the latitude of the place, is

A. 30°

B. 35°

C. 40°

D. 45°

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4

The point at which sun's declination changes from north to south, is known as

A. First point of Aeries

B. First point of Libra

C. Vernal Equinox

D. Both (b) and (d) of the above

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4

A star in northern sphere is said to transit

A. When its altitude is maximum

B. When its azimuth is 180°

C. When it is in south

D. All the above

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4

A star is said to elongate

A. When the star momentarily moves vertically

B. When the angle at the star of the spherical triangle is 90°

C. When the star's declination is greater than the observer's latitude

D. All the above

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4

The distance between the projection centre and the photograph, is called

A. Principal distance

B. Principal line

C. Isocentric distance

D. Focal length

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4

If two points differing by 1° of latitude and of the same longitude is 110 km apart on the earth, then two astronomical positions on the moon is about

A. 10 km

B. 25 km

C. 30 km

D. 50 km

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4

The longitudes of two places at latitude 60° N are 93° E and 97° W. Their departure is

A. 5100 nautical miles

B. 5700 nautical miles

C. 120 nautical miles

D. 500 nautical miles

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4

The scale of a vertical photograph of focal length f taken from height of H metres above M.S.L., at a point of reduced level h, is

A. f/H

B. f/(H + h)

C. f/(H - h)

D. (H - h)/f

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4

The sun's declination remains north between

A. March 21 to June 21

B. June 21 to September 21

C. September 21 to December 21

D. Both (a) and (b) of above

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4

The main object of the astronomer to obtain

A. Astronomical latitude

B. Astronomical longitude

C. Astronomical bearing

D. All of these

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4

Latitude of a place is the angular distance from

A. Greenwich to the place

B. Equator to the poles

C. Equator to the nearer pole

D. None of these

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4

If the equatorial distance between two meridians is 100 km, their distance at 60° latitude will be

A. 1000 km

B. 800 km

C. 600 km

D. 500 km

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4

Equation of time which is the difference between apparent solar time and mean solar time at any instant, vanishes during one year

A. Once

B. Twice

C. Thrice

D. Four times

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4

The coverage is least if photography is

A. High oblique

B. Low oblique

C. Vertical

D. None of these

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4

From the principal point the horizon point lies on the principal line at a distance of

A. f tan θ

B. f sin θ

C. f cot θ

D. f cos θ

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4

The equation which is obtained by multiplying each equation by the coefficient of its un-knowns and by adding the equations thus formed, is known as

A. Observation equation

B. Conditional equation

C. Normal equation

D. None of these

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4

The station which is selected close to the main triangulation station, to avoid intervening obstruction, is not known as

A. Satellite station

B. Eccentric station

C. False station

D. Pivot station

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4

The moon rotates round the earth once in every

A. 29 days

B. 29.35 days

C. 29.53 days

D. 30 days

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4

The scale of a tilted photograph of focal length f, taken from an altitude H, along the plate parallel through plumb point, is

A. f/H sec θ

B. f sec θ/H

C. f/H

D. f/H cos ½θ

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4

The angle between the plane of the equator and the plane of the ecliptic, is known as obliquity of the ecliptic and its value is

A. 22° 30'

B. 23° 27'

C. 23° 30'

D. 24° 0'

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4

Pick up the correct statement from the following:

A. The vertical plane containing the zenith, the station of observation and the celestial pole is the observer's meridian plane

B. The angle between the direction of star in vertical plane and the direction of the star in horizontal plane is called the altitude of the star

C. The complement of the altitude of star is called the zenith distance of the star

D. All the above

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4

α and β are the angles subtended by a point of elevation h at their air station with respective plumb points. Photo scale and focal length of the lens being S and f respectively. Parallax displacement of the point due to relief, is

A. h tan α/S

B. h tan β/S

C. h (tan α + tan β)/S

D. h (tan α - tan β)/S

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4

Pick up the correct statement from the following:

A. If the applied tension to the tape is more than the standard, the tension correction is positive

B. If the applied tension to the tape is less than the standard, the tension correction is negative

C. If the temperature during measurement is greater than the standard temperature, the temperature correction is positive

D. All the above

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4

At eastern elongation, the pole star moves

A. Eastward

B. Westward

C. Northward

D. Southward

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4

The most convenient co-ordinate system for specifying the relative positions of heavenly bodies on the celestial sphere, is

A. Altitude and azimuth system

B. Declination and hour angle system

C. Declination and right ascension system

D. Declination and altitude system