Review the key concepts, formulae, and examples before starting your quiz.
🔑Concepts
Earth's Rotation: The Earth spins on its imaginary axis from West to East. This rotation takes approximately hours (rounded to hours) and is responsible for the cycle of day and night.
Earth's Axis: The Earth is tilted on its axis at an angle of relative to its orbital plane. This tilt remains constant as the Earth orbits the Sun.
Earth's Revolution: The movement of the Earth around the Sun in an elliptical orbit. One complete revolution takes days, which defines one solar year.
The Seasons: Seasons are caused by the tilt of the Earth's axis and its revolution around the Sun. When a hemisphere is tilted toward the Sun, it experiences summer; when tilted away, it experiences winter.
Solstices and Equinoxes: A solstice occurs when the Sun reaches its highest or lowest point in the sky at noon (Summer Solstice and Winter Solstice). An equinox occurs when day and night are of approximately equal length ( hours each).
Leap Year: Because a revolution takes days, the extra day is accumulated over four years to add an extra day ( ) to the calendar, maintaining seasonal alignment.
📐Formulae
💡Examples
Problem 1:
Calculate how many degrees the Earth rotates in hours.
Solution:
Explanation:
Since the Earth completes a rotation in hours, it rotates every hour. Multiplying the hourly rate by gives the total rotation.
Problem 2:
If it is the Summer Solstice in the Northern Hemisphere, which way is the North Pole tilting relative to the Sun?
Solution:
The North Pole is tilted at toward the Sun.
Explanation:
During the Summer Solstice in the Northern Hemisphere, the axial tilt causes the North Pole to lean towards the Sun, resulting in the longest day of the year for that hemisphere.
Problem 3:
Why do we have a leap year every years?
Solution:
Explanation:
The Earth's actual orbital period is days. To keep our -day calendar synchronized with the solar year, we add one day every four years.