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, completing one rotation in approximately hours, which causes day and night.
Earth's Revolution: The Earth travels around the Sun in a fixed elliptical path called an orbit. This journey takes approximately days (one year).
Axial Tilt: The Earth's axis is tilted at an angle of from the vertical. This tilt is the primary reason for the changing seasons.
Summer Solstice: Occurs around June 21st, when the Northern Hemisphere is tilted towards the Sun, resulting in the longest day of the year and the start of summer.
Winter Solstice: Occurs around December 22nd, when the Northern Hemisphere is tilted away from the Sun, resulting in the shortest day of the year and the start of winter.
Equinoxes: Occurring in March (Spring) and September (Autumn), these are dates when the Sun is directly above the equator, making day and night of equal length ( hours each).
Angle of Sunlight: When sunlight hits the Earth at a angle (direct), it is more intense and warmer. Slanting rays spread over a larger area and are less warm.
📐Formulae
💡Examples
Problem 1:
If a regular year has days and a leap year occurs every years to account for the extra day, calculate the total number of days in a -year cycle.
Solution:
Explanation:
To find the total days in a -year cycle, we add three regular years of days and one leap year of days. The sum is days.
Problem 2:
A scientist measures the angle of the Earth's tilt as . If the tilt is , and for a hypothetical experiment, she doubles this tilt, what would the new angle be?
Solution:
Explanation:
By multiplying the current axial tilt of by , we find that the hypothetical tilt would be . This would cause much more extreme seasonal changes.
Problem 3:
Calculate the difference in the number of hours of daylight between an Equinox (12 hours) and a Summer Solstice day that has 14 hours and 30 minutes of daylight.
Solution:
Explanation:
Subtracting the hours of an equinox from the hours (14 hours 30 mins) of the solstice gives a difference of hours (or 2 hours and 30 minutes).