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
How does the period of the Earth's true anomaly affect the Earth's oceans?
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The period of the Earth's true anomaly does not affect the Earth's oceans.
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The period of the Earth's true anomaly causes the Earth's oceans to become warmer.
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The period of the Earth's true anomaly causes the Earth's oceans to become cooler.
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The period of the Earth's true anomaly causes the Earth's oceans to become unpredictable.
A
Correct answer
Explanation
The period of the Earth's true anomaly does not affect the Earth's oceans because the Earth's oceans are heated by the Sun. The Earth's orbit around the Sun does not affect the amount of sunlight that reaches the Earth, so the period of the Earth's true anomaly does not affect the Earth's oceans.
What is the formula for calculating the obliquity of the ecliptic?
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Obliquity = (23.4392911 - (0.0000004 * t))
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Obliquity = (23.4392911 + (0.0000004 * t))
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Obliquity = (23.4392911 - (0.0000004 * t^2))
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Obliquity = (23.4392911 + (0.0000004 * t^2))
A
Correct answer
Explanation
The formula for calculating the obliquity of the ecliptic is Obliquity = (23.4392911 - (0.0000004 * t)), where t is the number of years since the beginning of the Kali Yuga.
What is the formula for calculating the nutation in obliquity?
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Nutation in Obliquity = (9.2105 * cos(Ω) + 0.5532 * sin(Ω) - 0.0904 * cos(2Ω))
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Nutation in Obliquity = (9.2105 * sin(Ω) + 0.5532 * cos(Ω) - 0.0904 * sin(2Ω))
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Nutation in Obliquity = (9.2105 * cos(Ω) - 0.5532 * sin(Ω) - 0.0904 * cos(2Ω))
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Nutation in Obliquity = (9.2105 * sin(Ω) - 0.5532 * cos(Ω) - 0.0904 * sin(2Ω))
A
Correct answer
Explanation
The formula for calculating the nutation in obliquity is Nutation in Obliquity = (9.2105 * cos(Ω) + 0.5532 * sin(Ω) - 0.0904 * cos(2Ω)), where Ω is the longitude of the ascending node of the Moon.
What is the formula for calculating the true longitude of the Sun?
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True Longitude of the Sun = (Mean Longitude of the Sun + Nutation in Longitude)
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True Longitude of the Sun = (Mean Longitude of the Sun - Nutation in Longitude)
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True Longitude of the Sun = (Mean Longitude of the Sun + Nutation in Obliquity)
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True Longitude of the Sun = (Mean Longitude of the Sun - Nutation in Obliquity)
A
Correct answer
Explanation
The formula for calculating the true longitude of the Sun is True Longitude of the Sun = (Mean Longitude of the Sun + Nutation in Longitude).
What is the formula for calculating the true longitude of the Moon?
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True Longitude of the Moon = (Mean Longitude of the Moon + Nutation in Longitude + Evection + Variation + Annual Equation)
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True Longitude of the Moon = (Mean Longitude of the Moon - Nutation in Longitude + Evection + Variation + Annual Equation)
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True Longitude of the Moon = (Mean Longitude of the Moon + Nutation in Obliquity + Evection + Variation + Annual Equation)
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True Longitude of the Moon = (Mean Longitude of the Moon - Nutation in Obliquity + Evection + Variation + Annual Equation)
A
Correct answer
Explanation
The formula for calculating the true longitude of the Moon is True Longitude of the Moon = (Mean Longitude of the Moon + Nutation in Longitude + Evection + Variation + Annual Equation).
What is the formula for calculating the true latitude of the Moon?
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True Latitude of the Moon = (Mean Latitude of the Moon + Nutation in Latitude + Parallax in Latitude)
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True Latitude of the Moon = (Mean Latitude of the Moon - Nutation in Latitude + Parallax in Latitude)
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True Latitude of the Moon = (Mean Latitude of the Moon + Nutation in Obliquity + Parallax in Latitude)
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True Latitude of the Moon = (Mean Latitude of the Moon - Nutation in Obliquity + Parallax in Latitude)
A
Correct answer
Explanation
The formula for calculating the true latitude of the Moon is True Latitude of the Moon = (Mean Latitude of the Moon + Nutation in Latitude + Parallax in Latitude).
What is the formula for calculating the true latitude of the planets?
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True Latitude of the Planets = (Mean Latitude of the Planets + Nutation in Latitude + Perturbations in Latitude)
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True Latitude of the Planets = (Mean Latitude of the Planets - Nutation in Latitude + Perturbations in Latitude)
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True Latitude of the Planets = (Mean Latitude of the Planets + Nutation in Obliquity + Perturbations in Latitude)
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True Latitude of the Planets = (Mean Latitude of the Planets - Nutation in Obliquity + Perturbations in Latitude)
A
Correct answer
Explanation
The formula for calculating the true latitude of the planets is True Latitude of the Planets = (Mean Latitude of the Planets + Nutation in Latitude + Perturbations in Latitude).
What is the formula for calculating the distance of the Moon from the Earth?
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Distance of the Moon from the Earth = (Mean Distance of the Moon from the Earth + Evection + Variation + Annual Equation)
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Distance of the Moon from the Earth = (Mean Distance of the Moon from the Earth - Evection + Variation + Annual Equation)
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Distance of the Moon from the Earth = (Mean Distance of the Moon from the Earth + Nutation in Longitude + Evection + Variation + Annual Equation)
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Distance of the Moon from the Earth = (Mean Distance of the Moon from the Earth - Nutation in Longitude + Evection + Variation + Annual Equation)
A
Correct answer
Explanation
The formula for calculating the distance of the Moon from the Earth is Distance of the Moon from the Earth = (Mean Distance of the Moon from the Earth + Evection + Variation + Annual Equation).
What is the value of the Earth's circumference that Aryabhata calculated?
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24,900 miles
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25,000 miles
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25,100 miles
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25,200 miles
B
Correct answer
Explanation
Aryabhata calculated the Earth's circumference to be 25,000 miles.
What is the value of the distance to the Moon that Aryabhata calculated?
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238,855 miles
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238,900 miles
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239,000 miles
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239,100 miles
B
Correct answer
Explanation
Aryabhata calculated the distance to the Moon to be 238,900 miles.
What is the value of the distance to the Sun that Aryabhata calculated?
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93,000,000 miles
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93,100,000 miles
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93,200,000 miles
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93,300,000 miles
B
Correct answer
Explanation
Aryabhata calculated the distance to the Sun to be 93,100,000 miles.
What is the approximate distance of the Oort Cloud from the Sun?
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2,000 to 100,000 AU
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20,000 to 200,000 AU
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50,000 to 500,000 AU
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100,000 to 1,000,000 AU
A
Correct answer
Explanation
The Oort Cloud extends from about 2,000 to 100,000 AU from the Sun.
What is the typical size of a comet in the Oort Cloud?
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A few kilometers
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A few hundred kilometers
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A few thousand kilometers
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Tens of thousands of kilometers
A
Correct answer
Explanation
Most comets in the Oort Cloud are a few kilometers in size.
What is the period of the nutation of the Earth's axis?
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18.6 years
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23.5 years
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27.3 years
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365.25 days
A
Correct answer
Explanation
The period of the nutation of the Earth's axis is 18.6 years. This is the time it takes for the Earth's axis to complete one full cycle of nutation.
What is the amplitude of the nutation of the Earth's axis?
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9.2 arcseconds
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18.4 arcseconds
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27.6 arcseconds
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36.8 arcseconds
A
Correct answer
Explanation
The amplitude of the nutation of the Earth's axis is 9.2 arcseconds. This is the maximum angle by which the Earth's axis can deviate from its mean position.