Q. The distance between the points in a celestial body can be determined by using __________

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Q. Determine the zenith distance if the declination of star is given as 74˚32ꞌ and the latitude of the observer as 54˚21ꞌ.

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Q. If the zenith distance is given as 26˚57ꞌ, find the altitude of the star at upper culmination.

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Q. Correction for parallax is given as ___________

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Q. Express the 24˚12ꞌ42ꞌꞌ in hours, minutes and seconds.

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Q. Determine the local time if the standard time is 19ʰ 42ᵐ 7ˢ and the difference in longitude can be given as 3ʰ 9ᵐ towards west.

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Q. Find G.M.T of a place if the L.M.T is given as 9ʰ 24ᵐ 17ˢ and the longitude 10ʰ 23ᵐ 32ˢ towards east.

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Q. Which of the following indicate the standard time meridian of India?

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Q. The mean time associated with the standard meridian can be given as _________

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Q. The formula of mean solar time can be given as ____________

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Q. Express the hours (19ʰ 42ᵐ 16ˢ) in angles.

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Q. Which of the following indicates formula for green witch mean time?

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Q. Calculate mean solar time if the hour angle of the sun is 34ʰ 21ᵐ 15ˢ.

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Q. Which of the following doesn’t belong to the set of corrections applied in astronomical corrections?

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Q. Magnitude of refraction depends upon which of the following factors?

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Q. Correction to the dip is always_____________

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Q. Determine the index error for face right, if the face left and face right readings were given as 18˚24ꞌ52ꞌꞌ and 18˚23ꞌ24ꞌꞌ.

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Q. Find the altitude correction for semi-diameter which is having index error 25˚46ꞌ21ꞌꞌ and semi-diameter 0˚26ꞌ21ꞌꞌ.

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Q. Determine the correction for refraction if the angle of azimuth is given as 62˚21ꞌ24ꞌꞌ.

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Q. Determine the correction for parallax which has to be applied to 29˚42ꞌ31ꞌꞌ for obtaining altitude of the sun, which is given as 32˚41ꞌ15ꞌꞌ.

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