Related Questions

The hour angle of the heavenly body for Greenwich meridian equals the hour angle of the body for any other meridian + longitude:
A Mean sun
B True sun
C Vernal equinox
D All the above
If θ and δ be the latitude of an observer and declination of a heavenly body respectively, the upper culmination of the body will be south of zenith if its zenith distance, is
A δ - θ
B θ - δ
C θ + δ
D $$\frac{1}{2}$$ (θ - δ)
The angular distance of a heavenly body from the equator, measured along its meridian, is called
A Declination
B Altitude
C Zenith distance
D Co-latitude
The altitude of a heavenly body is its angular distance, measured on the vertical circle passing through the body, above
A Equator
B Horizon
C Pole
D None of these
The horizontal angle between the true meridian and magnetic meridian at a place is called
A azimuth
B declination
C local attraction
D magnetic bearing
A negative declination shows that the magnetic meridian is to the
A eastern side of the true meridian
B western side of the true meridian
C southern side of the true meridian
D none of the above
A heavenly body which takes nearly the same time to complete one rotation and one revolution is
A an asteroid
B a comet
C moon
D mars
Heavenly body- এর বাংলা পরিভাষা কোনটি?
A স্বর্গীয় দেহ
B জ্যোতিষ্ক
C প্রেরিত দূত
D ভারী দেহ
Right ascension of a heavenly body is its equatorial angular distance measured
A Westward from the first point of Libra
B Eastward from the first point of Aeries
C Westward from the first point of Aeries
D Eastward from the first point of Libra
The position of a heavenly body on the celestial sphere can be completely specified by
A Its altitude and azimuth
B Its declination and hour angle
C Its declination and right ascension
D All the above

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