Earth's Movement and Seasonal Changes Quiz

Earth's orbit around the Sun causes the changing position of the Sun.

Equal day and night occur during the Spring Equinox.

Earth rotates around its imaginary line called the Axis.

The rotation speed of Earth primarily determines the length of a day.

Differential heating leads to varied temperatures across Earth's regions.

The Moon exerts the greatest influence on Earth's tides.

The Earth's tilt is a result of past collisions with celestial bodies.

Solar zenith leads to the Sun's higher position in the summer sky.

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

Solstice results in maximum daylight for one hemisphere due to the axis's orientation.

Precession involves the Earth's axis tracing a circle in the sky over a long period.

Lunar eclipses occur during the Full Moon phase.

The Winter Solstice marks the Sun's farthest position from the celestial equator.

Seasonal changes on Earth are caused by variations in axial tilt.

Zenith occurs when the Sun is directly overhead at noon at the Tropic of Cancer.

Equilux is the period when day and night are of equal length.

Syzygy refers to the alignment of three celestial bodies, like during a solar eclipse.