Geography · Physics
Geodesy and Celestial Mechanics
984 Questions
Geodesy and celestial mechanics questions explore Earth measurements, great circles, and planetary motions. These concepts form a crucial part of physical geography and astronomy in competitive exams. Practice these questions to grasp longitudinal and latitudinal calculations.
Longitude and latitude calculationsGreat circle conceptEarths axial precessionLagrangian pointsAtmosphere boundary
Geodesy and Celestial Mechanics Questions
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Pole star appears to move from east to west.
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Pole star appears to move from west to east.
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Pole star does not appear to move.
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Pole star appears as the brightest star in the sky.
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Pole star appears very faintly in the sky.
C
Correct answer
Explanation
Pole star is situated in the direction of the earth's axis. Due to this, it does not appear to move.
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oval
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ceres
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planetai
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geoid
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circular
D
Correct answer
Explanation
Correct option. Geoid means Earth like shape, slightly flattened at the poles.
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3452 km
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1290 km
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6371 km
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5400 km
C
Correct answer
Explanation
Earth's mean radius is approximately 6,371 kilometers (about 3,959 miles). This value represents the average distance from Earth's center to its surface. The other options are either too small (like 1,290 km, which is closer to the Moon's radius) or don't match the accepted scientific value.
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vernier callipers
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spherometer
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screw gauge
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parallax method
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None of these
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106 km
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111 km
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120 km
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None of these
B
Correct answer
Explanation
Earth's circumference at the equator is approximately 40,075 km. With 360 degrees of longitude, each degree spans about 111.3 km at the equator (40,075 / 360 = 111.3 km). This is a standard geographical fact and an important value for understanding the scale of Earth's coordinate system. The distance between meridians decreases as you move toward the poles due to the convergence of longitude lines.
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5.23 light years
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5 light years
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4.24 light years
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None of these
C
Correct answer
Explanation
Proxima Centauri is the closest known star to the Sun and part of the Alpha Centauri star system. It is located approximately 4.24 light-years away from Earth, making it the nearest stellar neighbor to our solar system.
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82° 30' E longitude
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82° 50' E longitude
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82° E longitude
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83° 30' E longitude
A
Correct answer
Explanation
India's Standard Meridian is 82° 30' E, passing through Mirzapur (Uttar Pradesh). This longitude was chosen to balance the time difference between eastern and western India, giving a single time zone (IST) for the entire country.
B
Correct answer
Explanation
She went 360 km away from the earth.
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We can see lines on the earth.
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We can see the curved shape of the earth.
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We can see people roaming here and there.
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We can see large objects like huge trees only.
B
Correct answer
Explanation
We can see the curved shape of the earth. We cannot recognise lines on the earth like in the map.
C
Correct answer
Explanation
This option is correct because;
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λ = h / mv .
and from conservation of angular momentum we have = mvr = nh / 2π . => 2πr = nλ .
in this case value of n is 4 .
hence, this option is correct.
D
Correct answer
Explanation
Earth takes 365 rotations on its axis when it moves around the Sun once. Earth completes its one revolution around the sun in 365 days, i.e, a Year. It takes 23 hours, 59 minutes and 4 seconds for the Earth to make one complete rotation on its axis.
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300 and 400 latitude
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400 and 500 latitude
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500 and 600 latitude
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600 and 700 latitude
B
Correct answer
Explanation
The percentage of land surface in the Northern Hemisphere is the maximum between 400 and 500 latitude.
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south
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north
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east
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northeast
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none of these
A
Correct answer
Explanation
Magnetic north pole of earth will be found in gemetrical south pole direction.
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7000 km
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6000 km
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5000 km
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4000 km
B
Correct answer
Explanation
The Earth's equatorial radius is approximately 6,378 km, which is roughly 6,000 km. This is the distance from Earth's center to the equator. The polar radius is slightly smaller at about 6,357 km, giving Earth its slightly flattened shape.
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along the Equator
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along the Tropic of Cancer
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along the Arctic Circle
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at the North Pole
A
Correct answer
Explanation
Earth's rotational speed is highest at the Equator because the circumference is greatest there (approximately 40,075 km). Since Earth completes one full rotation in 24 hours everywhere, points on the Equator must travel the longest distance in the same time, resulting in the highest linear speed (about 1,670 km/h). At the poles, rotational speed approaches zero.