Q. G.M.T. corresponding to given mean time, equals

View solution

Q. Pick up the correct statement from the following :

View solution

Q. Latitude of the observer's position is equal to altitude of

View solution

Q. A star in northern sphere is said to transit

View solution

Q. In observations of equal precision, the most probable values of the observed quantities are those that render the sum of the squares of the residual errors a minimum, is the fundamental principle of

View solution

Q. Pick up the incorrect statement from the following. The angular distance of hevenly bodies on observer's meridian measured from the pole, is

View solution

Q. Pick up the correct statement from the following :

View solution

Q. Parallax bar measures

View solution

Q. Stellar astronomy deals with

View solution

Q. If a star whose declination is 60° N culminates at zenith, its altitude at the lower culmination, is

View solution

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

View solution

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

View solution

Q. Pick up the incorrect statement from the following :

View solution

Q. 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

View solution

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

View solution

Q. The zenith is the point on the celestial sphere

View solution

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

View solution

Q. To have greatest coverage of the area, the type of photography used, is

View solution

Q. The angle between the observer's meridian and declination circle of a heavenly body, is known as

View solution

Q. Pick up the correct statement from the following :

View solution