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

Multiple choice general knowledge science & technology
  1. 6375.1

  2. 6377.1

  3. 6378.1

  4. 6379.1

Reveal answer Fill a bubble to check yourself
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.

Multiple choice general knowledge
  1. 1

  2. 2

  3. 3

  4. 4

Reveal answer Fill a bubble to check yourself
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.

Multiple choice general knowledge science & technology
  1. Celestial Coordinate System

  2. Declination

  3. Right ascension

  4. Celestial sphere

Reveal answer Fill a bubble to check yourself
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.

Multiple choice general knowledge science & technology
  1. 384,403 KM ( center to center)

  2. 150000 KM ( center to center)

  3. 195630 KM ( center to center)

  4. 1 light year( center to center)

Reveal answer Fill a bubble to check yourself
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.

Multiple choice general knowledge science & technology
  1. 6400 km

  2. 10200 km

  3. 12800 km

  4. 3200 km

Reveal answer Fill a bubble to check yourself
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.

Multiple choice general knowledge science & technology
  1. astronomical unit

  2. light year

  3. parallactic second

  4. none of these

Reveal answer Fill a bubble to check yourself
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.

Multiple choice general knowledge
  1. True

  2. False

Reveal answer Fill a bubble to check yourself
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.

Multiple choice general knowledge
  1. 1/4

  2. 1/5

  3. 1/6

  4. 1/3

Reveal answer Fill a bubble to check yourself
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.