Categorized | Earth, Featured, Our Solar System

Planet Earth

Earth

 

Earth, one of nine planets in the solar system, the only planet known to harbor life, and the “home” of human beings. From space Earth resembles a big blue marble with swirling white clouds floating above blue oceans. About 71 percent of Earth’s surface is covered by water, which is essential to life. The rest is land, mostly in the form of continents that rise above the oceans.

Earth’s Atmosphere

An oxygen-rich and protective atmosphere, moderate temperatures, abundant water, and a varied chemical composition enable Earth to support life, the only planet known to harbor life. The planet is composed of rock and metal, which are present in molten form beneath its surface.

Earth’s surface is surrounded by a layer of gases known as the atmosphere, which extends upward from the surface, slowly thinning out into space. Below the surface is a hot interior of rocky material and two core layers composed of the metals nickel and iron in solid and liquid form.

Life on Earth

Unlike the other planets, Earth has a unique set of characteristics ideally suited to supporting life as we know it. It is neither too hot, like Mercury, the closest planet to the Sun, nor too cold, like distant Mars and the even more distant outer planets — Jupiter, Saturn, Uranus, Neptune, and tiny Pluto. Earth’s atmosphere includes just the right amount of gases that trap heat from the Sun, resulting in a moderate climate suitable for water to exist in liquid form. The atmosphere also helps block radiation from the Sun that would be harmful to life. Earth’s atmosphere distinguishes it from the planet Venus, which is otherwise much like Earth. Venus is about the same size and mass as Earth and is also neither too near nor too far from the Sun. But because Venus has too much heat-trapping carbon dioxide in its atmosphere, its surface is extremely hot — 462°C (864°F) — hot enough to melt lead and too hot for life to exist.

Although Earth is the only planet known to have life, scientists do not rule out the possibility that life may once have existed on other planets or their moons, or may exist today in primitive form. Mars, for example, has many features that resemble river channels, indicating that liquid water once flowed on its surface. If so, life may also have evolved there, and evidence for it may one day be found in fossil form. Water still exists on Mars, but it is frozen in polar ice caps, in permafrost, and possibly in rocks below the surface.

For thousands of years, human beings could only wonder about Earth and the other observable planets in the solar system. Many early ideas — for example, that the Earth was a sphere and that it traveled around the Sun — were based on brilliant reasoning. However, it was only with the development of the scientific method and scientific instruments, especially in the 18th and 19th centuries, that humans began to gather data that could be used to verify theories about Earth and the rest of the solar system. By studying fossils found in rock layers, for example, scientists realized that the Earth was much older than previously believed. And with the use of telescopes, new planets such as Uranus, Neptune, and Pluto were discovered.

Space Exploration

In the second half of the 20th century, more advances in the study of Earth and the solar system occurred due to the development of rockets that could send spacecraft beyond Earth. Human beings were able to study and observe Earth from space with satellites equipped with scientific instruments. Astronauts landed on the Moon and gathered ancient rocks that revealed much about the early solar system. During this remarkable advancement in human history, humans also sent unmanned spacecraft to the other planets and their moons. Spacecraft have now visited all of the planets except Pluto. The study of other planets and moons has provided new insights about Earth, just as the study of the Sun and other stars like it has helped shape new theories about how Earth and the rest of the solar system formed.

As a result of this recent space exploration, we now know that Earth is one of the most geologically active of all the planets and moons in the solar system. Earth is constantly changing. Over long periods of time land is built up and worn away, oceans are formed and re-formed, and continents move around, break up, and merge.

Life itself contributes to changes on Earth, especially in the way living things can alter Earth’s atmosphere. For example, Earth at one time had the same amount of carbon dioxide in its atmosphere as Venus now has, but early forms of life helped remove this carbon dioxide over millions of years. These life forms also added oxygen to Earth’s atmosphere and made it possible for animal life to evolve on land.

A variety of scientific fields have broadened our knowledge about Earth, including biogeography, climatology, geology, geophysics, hydrology, meteorology, oceanography, and zoogeography. Collectively, these fields are known as Earth science. By studying Earth’s atmosphere, its surface, and its interior and by studying the Sun and the rest of the solar system, scientists have learned much about how Earth came into existence, how it changed, and why it continues to change.

[Image] – www.nasa.org

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  2. [...] planet Venus is nearest neighbor of Earth. It took the name from the Greek God named Venus and was also called Evening Star. The planet Venus [...]

  3. [...] our atmosphere, there would be no life on Earth. A relatively thin envelope, the atmosphere consists of layers of gases that support life and [...]

  4. [...] surface. The largest of these are the oceans, which contain over 97 percent of all water on Earth. Glaciers and the polar ice caps contain just over 2 percent of Earth’s water in the form of [...]

  5. [...] Pluto, which is technically not a planet anymore anyway. Mercury is the second densest planet after Earth, having a large iron core with a radius of 1,100 to 1,200 miles – roughly about 75% of the [...]

  6. [...] with magnetic fields. It’s a diameter of about 1,392,000 km, about 109 times that of Earth, and its mass (about 2×1030 kilograms, 330,000 times that of Earth) accounts for about 99.86% of [...]

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  100. [...] with magnetic fields. It has a diameter of about 1,392,000 km, approximately 109 times that of Earth, and its mass (about 2×1030 kg, 330,000 times that of Earth) accounts for about 99.86% of the [...]

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  103. [...] with magnetic fields. It’s a diameter of about 1,392,000 kilometers, about 109 times that of Earth, and its mass (about 2×1030 kilograms, 330,000 times that of Earth) accounts for about 99.86% of [...]

  104. [...] with magnetic fields. It’s a diameter of about 1,392,000 km, about 109 times that of Earth, and its mass (about 2×1030 kg, 330,000 times that of Earth) accounts for roughly 99.86% of the [...]

  105. [...] with magnetic fields. It has a diameter of about 1,392,000 kilometers, about 109 times that of Earth, and its mass (about 2×1030 kilograms, 330,000 times that of Earth) accounts for about 99.86% of [...]

  106. [...] magnetic fields. It has a diameter of about 1,392,000 kilometers, approximately 109 times that of Earth, and its mass (about 2×1030 kilograms, 330,000 times that of Earth) accounts for roughly 99.86% of [...]

  107. [...] with magnetic fields. It has a diameter of about 1,392,000 km, roughly 109 times that of Earth, and its mass (about 2×1030 kg, 330,000 times that of Earth) accounts for roughly 99.86% of the [...]

  108. [...] interwoven with magnetic fields. It has a diameter of about 1,392,000 km, roughly 109 times that of Earth, and its mass (about 2×1030 kilograms, 330,000 times that of Earth) accounts for about 99.86% of [...]

  109. [...] with magnetic fields. It’s a diameter of about 1,392,000 km, roughly 109 times that of Earth, and its mass (about 2×1030 kg, 330,000 times that of Earth) accounts for roughly 99.86% of the [...]

  110. [...] with magnetic fields. It’s a diameter of about 1,392,000 km, approximately 109 times that of Earth, and its mass (about 2×1030 kilograms, 330,000 times that of Earth) accounts for roughly 99.86% of [...]

  111. [...] war of the ancient Romans. Mars is the only planet whose surface can be observed in detail from the Earth. It is the fourth closest planet to the Sun and is the second nearest planet to the Earth and will [...]

  112. [...] similar in size, mass, density, composition and gravity. These were the similarities. But unlike Earth, Venus has no oceans and is covered by a thick, rapidly spinning atmosphere composed primarily of [...]

  113. [...] Diameter: 12,100 km. Venus is about 1040km smaller in diameter than Earth [...]

  114. [...] planet or binary system. These two are just 12,200 miles away from each other. Charon takes 6.4 Earth days to orbit around Pluto and one Pluto rotation, or a Pluto day, also takes 6.4 Earth days. Due [...]

  115. [...] planet of our Solar system is the fifth planet from the Sun. It is over 11 times the size of Earth and is so large that it can fit 1,400 Earths. It is assumed that if Jupiter was larger, it might [...]

  116. [...] in the main Asteroid Belt and is approximately 117 million miles (188 million kilometres) from Earth. It has a circumference of 329 [...]

  117. [...] system. They rotate around the Sun in the following order, starting from the Sun: Mercury, Venus, Earth, Mars, Jupiter, Saturn, Uranus and Neptune. In addition to the full size planets there are 5 dwarf [...]

  118. [...] of Jupiter: 85,788 miles. Jupiter is the largest planet of the solar system – more than 12 Earths could line up across [...]

  119. [...] the Solar System came into being. That makes the Moon more than 4.527 billion years old – the Earth itself is 4.54 billion years old. Some researchers and computer simulations suggest that in the [...]


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