The movement of the Earth around the Sun can be described by the following statements:
1. The Earth revolves around the Sun in an elliptical orbit: This means that the Earth's path around the Sun is not a perfect circle but rather an elongated circle called an ellipse. This elliptical orbit causes variations in the distance between the Earth and the Sun throughout the year.
2. The Earth takes approximately 365.25 days to complete one orbit: This period of time is known as a year. The extra .25 days accumulate over four years and are accounted for in a leap year with 366 days.
3. The Earth's orbit is tilted relative to its axis: This tilt, known as the axial tilt, is about 23.5 degrees. This tilt is responsible for the changing seasons on Earth as different parts of the planet receive varying amounts of sunlight throughout the year.
4. The Earth's orbit is counterclockwise: When viewed from above the North Pole, the Earth moves around the Sun in a counterclockwise direction.
These statements collectively describe the movement of the Earth around the Sun and the key characteristics of this orbital motion that impact our planet's seasons and year.
