Geography ยท 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
What was the distance to GW150914?
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400 million light-years
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1.3 billion light-years
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2.4 billion light-years
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3.5 billion light-years
B
Correct answer
Explanation
GW150914 was located 1.3 billion light-years away from Earth.
What was the distance to GW151226?
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440 million light-years
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1.4 billion light-years
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2.3 billion light-years
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3.2 billion light-years
B
Correct answer
Explanation
GW151226 was located 1.4 billion light-years away from Earth.
What was the distance to GW170104?
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880 million light-years
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1.2 billion light-years
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1.9 billion light-years
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2.6 billion light-years
A
Correct answer
Explanation
GW170104 was located 880 million light-years away from Earth.
What is the Hubble Space Telescope's field of view?
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0.1 square degrees
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1 square degree
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10 square degrees
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100 square degrees
A
Correct answer
Explanation
The Hubble Space Telescope's field of view is 0.1 square degrees. This means that it can only see a small portion of the sky at any given time.
What is the Hubble Space Telescope's angular resolution?
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0.1 arcseconds
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1 arcsecond
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10 arcseconds
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100 arcseconds
A
Correct answer
Explanation
The Hubble Space Telescope's angular resolution is 0.1 arcseconds. This means that it can see objects that are very close together.
What is the average distance between Earth and the Sun?
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149.6 million kilometers
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152.1 million kilometers
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158.7 million kilometers
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147.1 million kilometers
A
Correct answer
Explanation
The average distance between Earth and the Sun is approximately 149.6 million kilometers, also known as one astronomical unit (AU).
What is the approximate time it takes for Earth to complete one rotation on its axis?
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23 hours 56 minutes
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24 hours
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25 hours 6 minutes
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26 hours 12 minutes
B
Correct answer
Explanation
Earth completes one rotation on its axis in approximately 24 hours, which is equivalent to one day.
What is the approximate time it takes for Earth to complete one revolution around the Sun?
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365.24 days
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366.24 days
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367.24 days
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364.24 days
A
Correct answer
Explanation
Earth completes one revolution around the Sun in approximately 365.24 days, which is equivalent to one year.
What is the tilt of Earth's axis?
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23.5 degrees
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24.5 degrees
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25.5 degrees
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26.5 degrees
A
Correct answer
Explanation
Earth's axis is tilted at an angle of approximately 23.5 degrees, which causes the seasons.
What is the approximate time it takes for Earth's precession to complete one cycle?
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26,000 years
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27,000 years
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28,000 years
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29,000 years
A
Correct answer
Explanation
Earth's precession takes approximately 26,000 years to complete one cycle.
What is the approximate value of Earth's obliquity?
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23.5 degrees
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24.5 degrees
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25.5 degrees
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26.5 degrees
A
Correct answer
Explanation
Earth's obliquity is approximately 23.5 degrees.
What is the approximate value of Earth's eccentricity?
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0.0167
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0.0177
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0.0187
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0.0197
A
Correct answer
Explanation
Earth's eccentricity is approximately 0.0167.
What was the value of the Earth's circumference calculated by Aryabhata?
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40,000 miles
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24,000 miles
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36,000 miles
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32,000 miles
B
Correct answer
Explanation
Aryabhata calculated the Earth's circumference to be 24,000 miles.
What is the term for the point on the Earth's surface directly below a celestial object?
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Nadir
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Zenith
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Horizon
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Substellar point
D
Correct answer
Explanation
The substellar point is the point on the Earth's surface directly below a celestial object.
What is the name of the imaginary line that divides the celestial sphere into two equal hemispheres?
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Celestial equator
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Ecliptic
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Tropic of Cancer
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Tropic of Capricorn
A
Correct answer
Explanation
The celestial equator is the imaginary line that divides the celestial sphere into two equal hemispheres.