Friday, July 5, 2019

LONG ESSAY ON SOLAR SYSTEM AND PLANETS 3 (600 WORDS)

LONG ESSAY ON SOLAR SYSTEM AND PLANETS 3 (600 WORDS)

Introduction
Our solar system consists of eight planets that revolve around the Sun, which is central to our solar system. These planets have broadly been classified into two categories – inner planets and outer planets. There are four inner planets, Mercury, Venus, Earth and Mars. The inner planets are closer to the Sun and smaller in size as compared to the outer planets. These are also referred to as the Terrestrial planets. Jupiter, Saturn, Uranus and Neptune are termed as the outer planets. These are massive in size and are often referred to as Giant planets.
Here is brief information about each of these planets:
Mercury
The smallest planet in our solar system, Mercury is also the closest to the Sun. Its geological features consist of lobed ridges and impact craters. Being closest to the Sun, Mercury’s temperature sores extremely high during the day time. It can go as high as 450 degree Celsius. Surprisingly, the nights here are freezing cold.
Mercury has a diameter of 4,878 km. It does not have any natural satellite.
Venus
Venus is said to be the hottest planet of our solar system. It has a toxic atmosphere that traps heat. It is also the brightest planet and is visible to the naked eye. It has a thick silicate layer around an iron core which is similar to that of Earth. Astronomers have seen traces of internal geological activity on this planet.
Venus has a diameter of 12,104 km. Just like Mars, Venus also does not have any natural satellite.
Earth
Earth is the largest inner planet. Two-third of this planet is covered with water. It is the only planet in our solar system where life is known to exist. Earth’s atmosphere, which is rich in nitrogen and oxygen, makes it fit for the survival of various species of flora and fauna. However, human activities are having negative impact on its atmosphere.
Earth has a diameter of 12,760 km. It has one natural satellite, the moon.
Mars
Mars, the fourth planet from Sun, is often referred to as the Red Planet. The iron oxide present on this planet gives it a reddish appeal. The planet is cold and has geological features similar to that of Earth. This is the reason why it has captured the interest of astronomers like no other planet. Traces of frozen ice caps have been found on the planet.
Mars has a diameter of 6,787 km and two natural satellites.
Jupiter
Jupiter is the largest planet in our solar system. It has a strong magnetic field. It largely consists of helium and hydrogen. It has a Great Red Spot and cloud bands. A giant storm is believed to have raged here for hundreds of years.
Jupiter has a diameter of 139,822 km and has as many as 79 natural satellites.
Saturn
Saturn is known for its ring system. These rings are made of tiny particles of ice and rock. Its atmosphere is quite like that of Jupiter as it is also largely composed of hydrogen and helium.
Saturn has a diameter of 120,500 km. It has 62 natural satellites that are mainly composed of ice.
Uranus
Uranus, the seventh planet from Sun, is the lightest of all the giant, outer planets. It has a blue tint which is because of the presence of Methane in the atmosphere. Its core is colder than the other giant planets. The planet orbits on its side.
Uranus has a diameter of 51,120 km and 27 natural satellites.
Neptune
The last planet in our solar system, Neptune is also the coldest of all. It is around the same size as the Uranus but is much more massive and dense. Neptune’s atmosphere is composed of helium, hydrogen, methane and ammonia. It experiences extremely strong winds. It is the only planet in our solar system which is found by mathematical prediction.
Neptune has a diameter of 49,530 km. It has 14 natural satellites.
Conclusion
Scientists and astronomers have been studying our solar system for centuries and the findings are quite interesting. Various planets that form a part of our solar system have their own unique geological features and are different from each other in several ways.

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