Science General · Geography

Astronomy and Celestial Phenomena

1,884 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

Multiple choice
  1. their blooming is controlled by low temperature

  2. they are sensitive to the phases of moon

  3. the desert insects eat away flowers during day time

  4. the desert insects are active during night time

Reveal answer Fill a bubble to check yourself
A Correct answer
Explanation

Correct Answer: their blooming is controlled by low temperature

Multiple choice
  1. the moon

  2. the pole star

  3. the sun

  4. Venus

Reveal answer Fill a bubble to check yourself
B Correct answer
Explanation

Earth's rotational axis currently points toward Polaris, known as the Pole Star or North Star. This happens because Polaris lies nearly directly above Earth's North Pole. The axis direction changes slowly over 26,000 years due to precession, but Polaris is our current pole star. The other options are gravitational bodies, not celestial alignment points.

Multiple choice
  1. moon and the earth have the same gravitational force

  2. moon cannot change its position

  3. the period of rotation of the moon on its axis and period of revolution around the earth is almost the same

  4. the period of rotation of the moon is not equal to the period of rotation of the earth

Reveal answer Fill a bubble to check yourself
C Correct answer
Explanation

The Moon exhibits tidal locking, meaning its rotational period equals its revolutionary period around Earth (approximately 27.3 days). This synchronization causes the same hemisphere to always face Earth. It is not due to equal gravitational forces or inability to change position, but rather a natural consequence of tidal forces over time.

Multiple choice
  1. 110 years

  2. 246 years

  3. 248 years

  4. 250 years

Reveal answer Fill a bubble to check yourself
C Correct answer
Explanation

Pluto has an extremely elongated orbit that takes it much farther from the Sun than the planets. At its average distance, it requires about 248 Earth years to complete one revolution around the Sun. This long orbital period is why Pluto was only discovered in 1930 despite being relatively bright compared to other distant objects.

Multiple choice
  1. the moon is at perigee

  2. the moon does not rotate

  3. only one side reflects light

  4. the periods of rotation and revolution of the moon are equal

Reveal answer Fill a bubble to check yourself
D Correct answer
Explanation

The Moon is tidally locked to Earth, meaning its rotational period (27.3 days) exactly equals its orbital period. This synchronous rotation causes the same lunar hemisphere to always face Earth. The far side was not seen until spacecraft missions in the 20th century. The Moon does rotate, just at the same rate it orbits.

Multiple choice
  1. the moon is nearest to the earth

  2. the moon does not rotate

  3. only one side reflects light

  4. the periods of rotation and revolution of the moon are equal

Reveal answer Fill a bubble to check yourself
A Correct answer
Multiple choice
  1. rotation of the earth

  2. revoluion of the earth

  3. elliptical path of the earth's orbit

  4. parallelism of inclined axis of the earth

Reveal answer Fill a bubble to check yourself
D Correct answer
Explanation

Singapore lies at 1°N latitude, between the Tropic of Cancer and Tropic of Capricorn. The sun is directly overhead twice annually (approximately once each when the sun crosses the zenith going north and south) due to the parallelism of Earth's inclined axis - the tilt direction stays fixed as Earth orbits, causing different latitudes to face the sun directly at different times. Options A, B, and C don't explain this phenomenon.

Multiple choice
  1. 1550

  2. 1530

  3. 1537

  4. 1543

Reveal answer Fill a bubble to check yourself
D Correct answer
Explanation

The heliocentric model (Sun as center of solar system) was published by Nicolaus Copernicus in 1543 in his work 'De revolutionibus orbium coelestium'. This marked a major shift from the geocentric view that had dominated for centuries.

Multiple choice
  1. 4th July

  2. 22nd December

  3. 22nd September

  4. None of these

Reveal answer Fill a bubble to check yourself
A Correct answer
Explanation

Earth reaches aphelion, its farthest point from the Sun, around July 4th each year. At this position, Earth is approximately 152 million kilometers from the Sun, compared to about 147 million kilometers at perihelion in early January. Despite being farther away, July is summer in the Northern Hemisphere because axial tilt is the dominant factor controlling seasons, not distance.