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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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.
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5,280 miles
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186,000 miles
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240,250 miles
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320,486 miles
C
Correct answer
Explanation
The average distance from Earth to the Moon is approximately 240,000 miles (384,400 km). This distance varies because the Moon's orbit is elliptical, ranging from about 225,000 miles at perigee to 252,000 miles at apogee. Option C is the closest to the average.
B
Correct answer
Explanation
The North Pole experiences approximately 186 days of continuous darkness (polar night) annually, centered around the December solstice. This occurs because Earth's axial tilt prevents sunlight from reaching the Arctic region during winter months.
B
Correct answer
Explanation
Moonlight takes approximately 1.25 seconds to travel from the Moon to Earth, covering the average distance of 384,400 km at the speed of light. This slight delay means we always see the Moon as it was 1.25 seconds ago.