Earth Moon and the Sun Class 7 Notes
hardEarth Moon and the Sun Class 7 Notes
Earth Moon and the Sun Class 7 Notes
- Rotation: The spinning motion of the Earth around its own axis, which takes approximately 24 hours to complete one full turn. This motion causes day and night.
- Revolution: The movement of the Earth around the Sun in an elliptical orbit, taking about 365.25 days to complete one full cycle. This motion is responsible for the changing seasons.
- Equator: An imaginary line that divides the Earth into the Northern and Southern Hemispheres, located equidistant from the poles. It is the reference point for latitude at 0 degrees.
- Celestial Objects: Natural objects in space, such as stars, planets, moons, and asteroids. These objects can be observed from Earth and exhibit apparent motion due to the Earth's rotation and revolution.
- Foucault Pendulum: A device that demonstrates the rotation of the Earth. It consists of a long string with a heavy bob that swings freely, showing the rotation of the Earth beneath it.
- Aryabhata: An ancient Indian mathematician and astronomer who made significant contributions to astronomy, including observations about the apparent motion of celestial objects.
- Apparent Motion: The perceived movement of celestial objects across the sky as observed from Earth, which is caused by the rotation of the Earth on its axis.
- Sunlight Intensity: The strength or brightness of sunlight that reaches the Earth's surface, which varies based on the angle of sunlight and the Earth's tilt. This affects climate and seasons.
- Northern Hemisphere: The half of the Earth that is north of the Equator, experiencing different seasons and daylight hours compared to the Southern Hemisphere.
- Southern Hemisphere: The half of the Earth that is south of the Equator, experiencing seasons and daylight hours that are opposite to those in the Northern Hemisphere.
- Seasons: The four divisions of the year (spring, summer, autumn, winter) that result from the tilt of the Earth's axis and its revolution around the Sun.
- Cosmos: The universe seen as a whole.
- Orientation: Position; direction; or location.
- Astrophotographer: A person who takes photographs of celestial objects, phenomena, and events, such as stars, planets, and eclipses.
- Astronomer: A scientist who studies the objects in the sky, including planets, galaxies, black holes, and stars.
- Indigenous: Occurring naturally in a particular place; native.
- Autumn equinox: Marks the end of summer and the beginning of autumn.
- Summer solstice: Marks the official start of astronomical summer and the longest day of the year.
- Winter solstice: The day with the shortest period of daylight and longest night of the year.
- Transit: Passage from one place to another.
1. Earth's Rotation:
Observation: The Sun appears to rise in the East and set in the West due to this rotation.
2. Day and Night Cycle:
Description: The cycle created by Earth's rotation, leading to day time when a location is facing the Sun and night time when it is turned away.
3. Sun's Position:
Morning: The Sun rises in the East.
Noon: The Sun is at its highest point in the sky.
Evening: The Sun sets in the West.
4. Shadows:
Observation: Shadows change in length and direction throughout the day due to the Sun's apparent movement across the sky.
5. Lunar Eclipse:
Types:
- Total Lunar Eclipse: The Moon is completely in the Earth's shadow, appearing red.
- Partial Lunar Eclipse: Only part of the Moon is in the Earth's shadow.
6. Solar Eclipse:
Observation: The Moon can appear to cover the Sun, despite being smaller, due to its position.
Scientific Understanding: Modern science explains the mechanics behind eclipses, allowing for safe observation.
7. Foucault Pendulum:
Purpose: Demonstrates Earth's rotation through the changing direction of the pendulum's swing.
8. Astronomical Observatories:
Example: Kodaikanal Solar Observatory, which has contributed to solar studies for over a century.
9. Stellarium App:
Function: A tool for predicting and observing solar and lunar eclipses.