Earth's Seasons and Celestial Phenomena Quiz

Axial tilt causes varying exposure to the Sun, leading to seasons on Earth.

Perihelion is the point in Earth's orbit where it is closest to the Sun.

The Southern Hemisphere experiences summer when the North Pole is tilted away from the Sun.

The Earth's axial tilt is primarily caused by impacts from celestial bodies during its formation.

Axial tilt is the main factor causing variations in daylight length throughout the year.

During the Spring equinox, day and night have approximately equal length globally.

The Earth's rotation occurs around its axis, creating day and night cycles.

The Moon's gravitational pull is the main factor affecting Earth's tides.

Axial tilt results in the Midnight Sun phenomenon in polar regions, with continuous daylight during certain times.

The Zenith is the point in the sky directly above an observer.

The Summer solstice happens when the Sun is directly over the Tropic of Cancer, marking the longest day of the year.

The Southern Hemisphere experiences the Summer Solstice during its winter season.

A lunar eclipse can occur during a Full Moon when the Earth is positioned between the Sun and the Moon.

Aphelion is the farthest point in a planet's orbit from the Sun.

Perigee is the point in a satellite's orbit closest to the Earth.