Science General · Geography
Astronomy and Celestial Phenomena
1,839 Questions
This section provides practice questions on astronomy and celestial phenomena, focusing on eclipses, planetary movements, and tides. These concepts are commonly tested in general science sections of various competitive exams. Use this hub to practice questions related to the Earth, Moon, and solar system dynamics.
Solar and lunar eclipsesEquinoxes and solsticesPlanetary movementsOcean tidesCoriolis effectMeteor showers
Astronomy and Celestial Phenomena Questions
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the length of time taken by the sun to rotate
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sunspots
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variation in the total number of detected neutrinos
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the length of a cycle for the time taken by proton-proton cycle
B
Correct answer
Explanation
The sunspot cycle happens because of pole flip — North becomes South and South becomes North—approximately every 11 years. Some 11 years later, the poles reverse again back to where they started, making the full solar cycle actually a 22-year phenomenon. The Sun behaves similarly over the course of each 11-year cycle no matter which pole is on top.
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495 secs
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496 secs
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497 secs
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498 secs
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499 secs
E
Correct answer
Explanation
It takes 8 min 16 secs which is equal to 499 secs.
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Spring tide
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Neap tide
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Tropical tide
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Perigean tide
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Equinoctical spring tide
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at the start of a total solar eclipse
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at the end of a total solar eclipse
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only along the peripheral regions of the totality trail
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only in the central regions of the totality trail
C
Correct answer
Explanation
Diamond ring is observed in a solar eclipse, only along the peripheral regions of the totality trail.
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equator
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tropic of cancer
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tropic of Capricorn
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poles
A
Correct answer
Explanation
An equinox occurs when the sun is positioned directly over the equator, resulting in nearly equal day and night lengths globally. This happens twice a year.
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Cobra
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Upward Dog
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Chair
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Half Moon
A
Correct answer
Explanation
Cobra (or Upward Dog) is the backbend transition used in the Sun Salutation A sequence. While Upward Dog is also used, Cobra is a classic variation often taught in this sequence.
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The Sun revolves around the Earth every 365 days.
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The Earth revolves around the Sun every 365 days.
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The Earth's rotation every 24 hours.
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The amount of humidity the Sun creates in the atmosphere.
B
Correct answer
Explanation
Earth's seasons are caused by the tilt of the Earth's axis as it revolves around the Sun, which changes the angle at which sunlight hits different parts of the planet throughout the year.
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setting in the West in California
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rising in the east over Japan
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shining in the sky over Africa
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shining in the sky over Florida
D
Correct answer
Explanation
The Earth completes one full rotation on its axis in approximately 24 hours. Therefore, at the same time the next day, the Sun will be in the same position relative to the observer in Florida.
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full moon
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gibbous moon
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crescent moon
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new moon
D
Correct answer
Explanation
A solar eclipse occurs when the Moon passes directly between the Sun and Earth, which only happens during the new moon phase.
B
Correct answer
Explanation
A supermoon occurs when the Moon is at perigee, its closest point to Earth in its elliptical orbit, making it appear larger and brighter.
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umbra
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penumbra
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perigee
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apogee
B
Correct answer
Explanation
The penumbra is the lighter, outer part of the shadow where the light source is only partially obscured, resulting in a partial eclipse.
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umbra
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penumbra
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antumbra
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perigee
A
Correct answer
Explanation
The umbra is the darkest, central part of the shadow where the light source is completely blocked by the object.
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the Sun is orbiting Earth
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the Sun is orbiting the Moon
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the Earth & Moon are in constant motion
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the Earth is not moving at all
C
Correct answer
Explanation
The shadow changes because both the Earth and the Moon are in constant motion relative to each other and the Sun.
A
Correct answer
Explanation
The Moon's orbit around the Earth is not a perfect circle but an ellipse, which is why the distance between them varies.
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partial eclipse
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diamond ring
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Baily's Beads
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totality
C
Correct answer
Explanation
Baily's Beads are the points of light seen around the edge of the Moon just before or after totality, caused by sunlight shining through lunar valleys.