Geography · Physics
Geodesy and Celestial Mechanics
1,049 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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6375.1
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6377.1
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6378.1
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6379.1
C
Correct answer
Explanation
Earth's equatorial radius is 6378.1 km, which is the distance from Earth's center to the equator. Earth is not a perfect sphere but an oblate spheroid, so the equatorial radius is larger than the polar radius of approximately 6357 km.
D
Correct answer
Explanation
The Sun's surface area is approximately 12,000 times that of Earth. However, the question asks how many Earths would fit ON THE SURFACE (2D arrangement), which is about 109 Earths. This is based on the Sun's diameter being about 109 times Earth's diameter.
D
Correct answer
Explanation
The Pacific tectonic plate is moving northwestward at approximately 4 inches (about 10 cm) per year, carrying the Hawaiian islands with it toward Japan. This plate motion is driven by mantle convection and causes earthquakes and volcanic activity in the region.
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82 east
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82.5 east
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81.5 west
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83 east
B
Correct answer
Explanation
India uses Indian Standard Time (IST) which is UTC+5:30, corresponding to 82.5°E longitude as the central meridian.
D
Correct answer
Explanation
Latitude is represented by the Greek letter phi (φ) in mathematical and geographical notation.
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66,700
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70,000
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55,500
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85,600
A
Correct answer
Explanation
Earth's orbital speed around the Sun is approximately 66,700 miles per hour (about 107,000 km/h or 30 km/s). This is Earth's average velocity through space as it travels along its orbit.
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Celestial Coordinate System
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Declination
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Right ascension
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Celestial sphere
B
Correct answer
Explanation
Declination in astronomy is analogous to latitude on Earth - it's measured in degrees north or south of the celestial equator. Right ascension is analogous to longitude, the celestial coordinate system is the overall framework, and the celestial sphere is the imaginary sphere surrounding Earth.
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384,403 KM ( center to center)
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150000 KM ( center to center)
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195630 KM ( center to center)
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1 light year( center to center)
A
Correct answer
Explanation
The average distance from Earth to Moon's center is about 384,400 km. This varies between 363,300 km at perigee and 405,500 km at apogee due to elliptical orbit. 1 light year is vastly larger, and other values are incorrect.
A
Correct answer
Explanation
One billion seconds equals approximately 31.7 years, which rounds to 32 years. Calculate: 1,000,000,000 ÷ (60 × 60 × 24 × 365.25) ≈ 31.7 years.
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6400 km
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10200 km
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12800 km
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3200 km
A
Correct answer
Explanation
Earth's radius is approximately 6,371 km, commonly rounded to 6,400 km. This value represents the distance from Earth's center to its surface. The diameter is about 12,742 km (option C shows a confused diameter value). Earth is not a perfect sphere but an oblate spheroid.
A
Correct answer
Explanation
Approximately one-fifth (about 20%) of Earth's land surface is classified as desert, defined by very low precipitation (less than 250mm annually). This includes both hot deserts like the Sahara and cold deserts like Antarctica. One-quarter, one-third, or one-half would overestimate desert coverage.
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astronomical unit
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light year
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parallactic second
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none of these
A
Correct answer
Explanation
An astronomical unit (AU) is the average distance between Earth and Sun, about 93 million miles. A light year is the distance light travels in a year. Parallactic second (parsec) is a unit of interstellar distance. AU is specifically defined by Earth-Sun distance.
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5 km
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5 km north
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5 km per hour
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5 cm
B
Correct answer
Explanation
Displacement is a vector quantity that includes both magnitude AND direction. '5 km north' specifies both the distance (5 km) and the direction (north), making it a measure of displacement. Options A and D are distances (scalars), while C is speed.
A
Correct answer
Explanation
True. The Kármán line at 100 km altitude is internationally recognized as the boundary between Earth's atmosphere and outer space. This definition was established by the Fédération Aéronautique Internationale (FAI) and represents the altitude where aeronautics ends and astronautics begins.
D
Correct answer
Explanation
Approximately one-third (about 33%) of Earth's land surface is classified as desert or arid/semi-arid land. This includes hot deserts like the Sahara as well as cold deserts like Antarctica. Deserts are defined by low precipitation levels rather than temperature.