Surveying The difference in longitude of two places expressed in time is equal to the difference in their Apparent solar time Mean solar time All listed here Sidereal time Apparent solar time Mean solar time All listed here Sidereal time ANSWER DOWNLOAD EXAMIANS APP
Surveying When a star is between the pole and the horizon, the relationship between latitude (λ), zenith distance (z) and declination δ, is θ = z + δ θ = 180° - (z + δ) θ = δ - z θ = (z + δ) - 180° θ = z + δ θ = 180° - (z + δ) θ = δ - z θ = (z + δ) - 180° ANSWER DOWNLOAD EXAMIANS APP
Surveying The latitude of a place was obtained by subtracting the zenith distance of a star from its declination, the observed star was between Pole and horizon Zenith and pole Equator and zenith Horizon and equator Pole and horizon Zenith and pole Equator and zenith Horizon and equator ANSWER DOWNLOAD EXAMIANS APP
Surveying A star may culminate at zenith if its declination is Less than the latitude of the place Equal to the latitude of the place None of these Greater than the longitude of the place Less than the latitude of the place Equal to the latitude of the place None of these Greater than the longitude of the place ANSWER DOWNLOAD EXAMIANS APP
Surveying For a well-conditioned triangle, no angle should be less than 45° 20° 30° 60° 45° 20° 30° 60° ANSWER DOWNLOAD EXAMIANS APP
Surveying The length of a parallel of λ latitude between two meridians is equal to difference in longitudes multiplied by cos λ sin λ tan λ cot λ cos λ sin λ tan λ cot λ ANSWER DOWNLOAD EXAMIANS APP
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