Lesson Sequence
Key Resources
Quizlet Flashcards: 6thSci 02 Astronomy
Holt California Astronomy Textbook Section
Optional Video Resource: Neil deGrasse Tyson Explains Leap Years
Earth's Revolution Around the Sun & The Four Seasons
Earth's Rotation Along Its Tilted Axis & Day/Night Cycle (Time Zones)
Discovery Education Video: Technology and the Electromagnetic Spectrum
Discovery Education Video: Four Seasons
Earth is tilted on an axis-- the North Pole is pointed towards Polaris, the North Star. This means that anyone in the Northern Hemisphere can see the North Star at night, and as such, astronomers and mariners have used this star as a guide for centuries to navigate the oceans.
This axial tilt can be observed on Earth when a camera is positioned at or near the North Pole. A time-lapse image will show Earth's rotation around a central star. Most stars leave a trail of light when their positions "change" relative to the camera, but the North Star is always found towards the center of the circular paths.
Even as Earth revolves around the sun, Earth is still tilted on its axis. In other words, the North Pole is still pointed towards Polaris. This axial tilt of 23.5° (relative to sun-earth equatorial plane) also contributes to the seasonal changes that can be observed on Earth.
The sun's most direct rays strike Earth in certain locations (between the Tropic of Cancer and the Tropic of Capricorn) at specific times during the year (solstices and equinoxes). Locations outside
Because we live in the Northern Hemisphere, the solar rays will never be perfectly overhead (at the zenith). Instead, the solar rays will always strike us at an angle, which means our shadow will always be visible. As shown in the figure above, our shadows will always point in some direction northward (northwest in the morning to northeast in the evening).
In the Northern Hemisphere, our shadow length will always be the longest in the winter months because of solar rays' low angle of incidence (sun is lower in the sky during the winter months). During the summer months, the sun is higher in the sky, so our shadows are shorter.
This angle of incidence is significant to architects who need to design roofs with solar panels, since the panels must be angled in such a way that it maximizes the absorption of sunlight. As shown in the figure above, they must be angled on the south side of the roof.
Depending on the position of Earth around the sun, the angle of solar rays can differ. This results in the seasonal changes that we observe on Earth.
The seasons are the result of Earth's revolution around the sun and the axial tilt. Depending on the location of Earth, the sun's direct rays will strike a different region (between the Tropic of Cancer, equator, and the Tropic of Capricorn). This means that when one hemisphere experiences summer (warm weather due to a higher angle of incidence of solar rays), the other experiences winter (colder weather due to a lower angle of incidence of solar rays).
On June 21, the sun's most direct rays strike the Tropic of Cancer (23.5°N). This is the official start of summer in the Northern Hemisphere (longest day of the year). In the Southern Hemisphere, however, this is the official start of winter (shortest day of the year).
On December 23, the sun's most direct rays strike the Tropic of Capricorn (23.5°S). This is the official start of summer in the Southern Hemisphere (longest day of the year). In the Northern Hemisphere, however, this is the official start of winter (shortest day of the year).
When Earth is in between the solstices, the sun's most direct rays strike the equator.
During these specific dates and locations, the sun is directly overhead (zenith) at noon. When this occurs, the shadow is directly on the ground below the object.
Earth's rotation about its axis causes day and night.
In the animation above, Earth is rotating from the west (left side) to the east (right side). Compass directions (north, south, west, east) are used because they have standardized definitions and don't change as long as north is "upwards." Clockwise and counterclockwise isn't used here because they must have a reference point: west to east rotation is counterclockwise with respect to the North Pole, but is clockwise when viewed from the South Pole.
Since Earth rotates west to east, it appears as if "day" (bright side) and "night" (dark side) are "traveling" westward. In other words, the East Coast experiences day and night before the West Coast. This causes a three-hour time difference (time zones) between New York and Los Angeles.
Time zones occur on Earth because different areas are located in different regions of the bright and dark side of Earth. Since different parts of Earth enter and exit daylight/night at different times, specific zones are necessary to standardize the time.
The moon revolves around Earth approximately once every four weeks. The sun always illuminates half of the moon. However, depending on where the moon is located, different portions of the moon are visible. The visible portion of the moon increases during the first half of the cycle (waxing stage) and decreases during the second half (waning stage).
A solar eclipse can occur if a new moon is perfectly aligned and casts a shadow on Earth. People in the umbra will experienced a few minutes to darkness during the day.
A lunar eclipse can occur if Earth is in between the sun and a full moon. Earth will cast a shadow on a full moon, causing the moon to become red in color. Note that the moon will still be visible because some sunlight is still being reflected off the moon's surface.
An incoming high tide leads to rush of water flowing towards land (flood current). Approximately 6 hours later (a quarter of Earth's rotation), an impending low tide results in the water rushing seaward (ebb current).
The relative position of the sun and moon affects tidal changes. When the graivtational forces line up, they combine to pull water towards it, resulting in a high tide for locations at these tidal bulges. At locations that don't receive this pull, a low tide event occurs. Note that there are two high tide events and two low tide events every day.