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4

The circle in which a plane tangent to the earth's surface at the point of observation, intersects the celestial sphere, is called

A. Visible horizon

B. Sensible horizon

C. Celestial horizon

D. True horizon

Correct Answer :

B. Sensible horizon


Related Questions

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Perspective centre relates to

A. Parallel projection

B. Orthogonal projection

C. Central projection

D. None of these

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4

The meridian of a place is

A. A great circle passing through the place and the poles

B. A great circle whose plane is perpendicular to the axis of rotation and it also passes through the place

C. A semi-circle which passes through the place and is terminated at the poles

D. An arc of the great circle which passes through the place and is perpendicular to the equator

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4

Pick up the correct statement from the following:

A. The measured stereoscopic base of photographs is obtained by dividing the air base in metres by the mean scale of the photograph

B. The difference between the absolute parallax of two points depends upon the difference in their elevations

C. The line joining the principal point of a photograph and the transferred principal point of the adjoining photograph, is called stereoscopic base

D. All the above

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Homologous points are

A. Opposite corners of a photograph

B. Nodal points of the camera lens

C. Corresponding points on the ground and photograph

D. Plumb points of stereo pair of photographs

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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

23 cm × 23 cm photographs are taken from a flying height with a camera of focal length of 3600 m and 15.23 cm respectively. A parallax difference of 0.01 mm represents

A. 1 m

B. 2 m

C. 4 m

D. 8 m

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4

The angle between the direction of star and the direction of earth's axis of rotation is called

A. Co-declination

B. Co-latitude

C. Declination

D. Latitude

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4

Sidereal day

A. Is the period of time taken by the earth in making a complete rotation with reference to stars

B. Is slightly shorter than an ordinary solar day

C. Is divided into the conventional hours, minutes and seconds

D. All the above

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4

The stereo plotting instruments are generally manufactured on the principle of

A. Optical projection

B. Optical mechanism projection

C. Mechanical projection

D. All the above

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4

The product of the distances of plumb point and horizon point of a vertical photograph from its principal point, is

A. f2

B. 2f2

C. 3f2

D. ½f

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4

The circle in which a plane tangent to the earth's surface at the point of observation, intersects the celestial sphere, is called

A. Visible horizon

B. Sensible horizon

C. Celestial horizon

D. True horizon

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4

The method of surveying by triangulation was first introduced by the Dutchman Snell in

A. 1600

B. 1615

C. 1630

D. 1650

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4

Pick up the correct statement from the following:

A. Aerial photographs may be either vertical or oblique

B. Vertical photographs are taken with the axis of camera pointing vertically downward

C. Vertical photographs are used for most accurate maps

D. All the above

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4

Pick up the correct statement from the following:

A. Sidereal time at any instant is equal to the hour angle of the first point of Aries

B. Local sidereal time of any place is equal to the right ascension of its meridian

C. Sidereal time is equal to the right ascension of a star at its upper transit

D. All the above

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4

The flying height of the camera is 1, 000 m above mean ground level, the distance of the top of a building from a nadir point is 10 cm and the relief displacement of building is 7.2 mm. The height of the building, is

A. 52 m

B. 62 m

C. 72 m

D. 82 m

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4

The time interval between successive transits of the moon, is

A. 24 hours 10 minutes

B. 20 hours 25 minutes

C. 24 hours 50 minutes

D. 23 hours 50 minutes

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4

The normal longitudinal overlap is generally kept

A. 50 %

B. 60 %

C. 70 %

D. 75 %

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The principal line is the line joining the principal point and

A. Nadir

B. Isocenter

C. Perspective centre

D. None of these

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4

The station where observations are not made, but the angles at the station are used in triangulation series, is known as

A. Satellite station

B. Subsidiary station

C. Pivot station

D. Main station

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4

Pick up the correct statement from the following:

A. The horizontal direction of the pole is called astronomical north

B. The angle between the direction of true north and the direction of a survey line is called astronomical bearing

C. The astronomical bearing is generally called azimuth

D. All the above

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4

The net ground area of a vertical photograph 20 cm × 20 cm on scale 1 : 10,000 having overlaps 60% and 30%, is

A. 0.50 sq km

B. 0.56 sq km

C. 0.60 sq km

D. 0.64 sq km

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4

The Polaris remains below horizon at

A. 10° N

B. 50° N Latitude

C. Equator

D. 5° S latitude

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4

The sidereal day is the time interval between two successive upper transits of

A. Mean sun

B. First point of Aries

C. First point of Libra

D. The polar star

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4

The value of geo-centric parallax to be added to the observed altitude of sun is

A. 9 cos α

B. 9 sin α

C. 9 tan α

D. 9 cot α

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4

With standard meridian as 82° 30' E the standard time at longitude 90° E is 8 h 30 m. The local mean time at the place will be

A. 7 h 00 m

B. 7 h 30 m

C. 8 h 00 m

D. 9 h 00 m

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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

At the first point of Aeries, the sun moves

A. Northward

B. Southward

C. From south to north of the equator

D. From north to south of the equator

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4

The maximum error in radial line assumption, is

A. h/H f tan θ

B. h/H f² tan θ

C. h/H f² sin θ

D. h/H f cos θ

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4

In a tropical year, the numbers of sidereal days are

A. 365

B. 365.2224

C. 365.2422

D. 366.2422

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4

While making astronomical observations, the observer is mainly concerned with

A. The direction of the vertical, the axis of rotation of the instrument

B. The direction of the poles of the celestial sphere

C. The direction of the star from the instrument

D. All the above