Questions and Answers
How are seasons caused?
By the combination of Earth's tilted axis and its revolution around the Sun.
How does Earth move?
Earth moves through space in two major ways: rotation and revolution.
What does rotation mean?
The spinning on Earth's axis; one full rotation equals one day.
What does revolution mean?
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Where does sunlight hit Earth's surface most directly?
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How does sunlight hit the Earth near the poles?
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What would happen if Earth's axis was straight up-and-down in relation to the Sun?
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Why does Earth have seasons?
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How are summer and winter caused?
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Which hemisphere tilts towards the Sun in our summer?
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Which hemisphere tilts away from the Sun in our winter?
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When is the Sun at its maximum height in the sky in the northern hemisphere?
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What month is Earth the farthest from the Sun?
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When does the northern hemisphere experience more hours of daylight than darkness?
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The combination of direct rays and more hours of sunlight heats the surface more in what month than at any other time of the year?
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In June, the southern hemisphere is experiencing what season?
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During what month is Earth the closest to the Sun?
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What does solstice mean?
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When does solstice occur?
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What happens to the days when solstice occurs?
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What does equinox mean?
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When does equinox occur?
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Study Notes
Earth's Seasons
- Seasons result from the tilt of Earth's axis combined with its revolution around the Sun.
- Earth's movements include rotation (spinning on its axis) and revolution (orbiting around the Sun).
Rotation and Revolution
- Rotation explains the cycle of day and night; one complete rotation equals one day.
- Revolution describes Earth’s orbit around the Sun; one complete revolution equals one year.
Sunlight Distribution
- The equator receives sunlight most directly, leading to warmer temperatures.
- Sunlight at the poles strikes at a shallow angle, spreading over a larger area, resulting in colder climates.
Impact of Earth's Axis
- A vertically aligned axis would lead to minimal temperature variation throughout the year.
- Seasons are defined by the tilt of Earth's axis as it orbits the Sun, influencing temperature variations.
Seasonal Changes
- Summer occurs in the Northern Hemisphere when it tilts towards the Sun.
- Conversely, winter in the Northern Hemisphere occurs when it tilts away from the Sun.
Key Dates and Events
- The June solstice marks the Sun's maximum height in the Northern Hemisphere.
- Earth is farthest from the Sun in June, during summer in the Northern Hemisphere.
- The Southern Hemisphere experiences winter during June as it tilts away from the Sun.
Daylight Variations
- From March to September, the Northern Hemisphere enjoys more hours of daylight than darkness.
- June experiences the highest temperatures due to a combination of direct sunlight and extended daylight hours.
Distance to the Sun
- Earth is closest to the Sun in December, during winter in the Northern Hemisphere.
Solstices and Equinoxes
- Solstice refers to the points when the Sun is farthest north or south of the equator, occurring twice a year.
- Solstices result in the year's longest and shortest days.
- Equinox means "equal night," occurring twice a year when neither hemisphere tilts toward or away from the Sun; this happens in March and September, with the noon Sun directly overhead at the equator.
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Description
Explore the fundamental concepts of Earth's seasons through these informative flashcards. Learn how the tilted axis and the movement of the Earth create the seasons, along with the definitions of rotation and revolution. Perfect for students wanting to solidify their understanding of Earth's dynamics.