How will the end of the Earth happen? Hints given to scientists

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Know about the latest study in which scientists have found indications of how the end of the Earth might happen by observing an exoplanet. Read on to understand the life cycle of planets and what happens when an outer planet collides with its star. Discover the similarities between the observed exoplanet and Jupiter, and find out how this study will help scientists improve their theories of tidal physics.

Introduction

  • The role of the Sun in the existence of the Earth
  • Scientists’ recent study on an outer planet gives hints on how the Earth will end

The Exoplanet Kepler 1658b

  • Discovery and confirmation of Kepler 1658b
  • Similarities between Kepler 1658b and Jupiter
  • Difference between the two planets

The Decreasing Orbit of Kepler 1658b

  • The decreasing orbit of Kepler 1658b
  • The rate of decrease
  • The role of gravitational force between the planet and the Sun

The End of Kepler 1658b

  • Kepler 1658b’s end process
  • Laboratory for scientists
  • Improvement of theories of tidal physics

The Possibility of Earth’s End

  • The common belief of Earth’s end caused by a meteorite impact
  • Scientists’ ongoing research and study for the correct answer

Conclusion

  • The significance of the study on Kepler 1658b for understanding the life cycle of planets
  • The importance of the ongoing research on Earth’s end

The Earth is a planet that has been existing for billions of years, and its existence is highly dependent on the Sun. As long as the Earth receives light from the Sun, it will continue to exist. However, scientists have recently discovered an outer planet that is losing its orbit, which gave them hints on how the Earth will end.

The exoplanet Kepler 1658b, which was discovered by NASA with the help of a telescope in 2009, is similar in size and weight to Jupiter. The only difference is that it has reached very close to its star, which is causing it to gradually lose its orbit. The distance between Kepler 1658b and its star is only equal to the 8th part of the distance between the Sun and Mercury.

The orbit of Kepler 1658b is decreasing every year at a rate of 131 milliseconds, which is caused by the gravitational force between the planet and its Sun. This force causes a change in the size of each other, and tremendous energy is released as a result. Scientists have found that similar energy is also generated due to the gravitational force between the planet Jupiter and its moons.

When Kepler 1658b reaches the end of its orbit, it will merge into its star, which will serve as a laboratory for scientists to improve their theories of tidal physics. This study is significant in understanding the life cycle of planets.

People often believe that a huge rock or meteorite from space will hit the Earth and cause it to be divided into many pieces and destroyed. However, scientists have been conducting ongoing research and study to find the correct answer to this question.

In conclusion, the recent study on Kepler 1658b has given scientists valuable hints on how planets can come to an end, and this ongoing research on Earth’s end is significant in understanding the life cycle of planets.

As we learn more about the end of Kepler 1658b, we can start to apply that knowledge to our own planet. While the destruction of our planet by a meteorite is a popular theory, it’s important to understand that this is not the only way in which the Earth could meet its end. In fact, the end of the Earth is likely to happen much more slowly and gradually.

One possibility is that the Earth’s orbit could decay over time. As the Earth continues to orbit the Sun, the gravitational forces between the two celestial bodies cause a small amount of energy to be transferred from the Earth to the Sun. Over time, this energy loss could cause the Earth’s orbit to decay and eventually collide with the Sun. This process is estimated to take billions of years, but it could still happen in the distant future.

Another possibility is that the Sun itself will eventually run out of fuel and expand, consuming the inner planets, including the Earth. This process, known as a “red giant” phase, is estimated to occur in about 5 billion years. During this phase, the Sun will grow to be so large that it will engulf Mercury, Venus, and possibly the Earth.

Ultimately, the end of the Earth is not something that we need to worry about in our lifetimes or even our children’s lifetimes. However, it is important for scientists to continue studying the life cycles of planets so that we can better understand the universe and our place in it.

In conclusion, the recent discovery of Kepler 1658b and its eventual collision with its star provides valuable insight into the life cycle of planets. While the end of the Earth may not happen for billions of years, it’s important for scientists to continue studying the phenomenon so that we can better understand our place in the universe.

FAQs:

  1. Will the Earth end in my lifetime?

No, the end of the Earth is not something that we need to worry about in our lifetimes or even our children’s lifetimes.

  1. How long will it take for the Earth to collide with the Sun?

If the Earth’s orbit decays over time, it could collide with the Sun in billions of years. However, this is not the only possibility for the end of the Earth.

  1. Will a meteorite destroy the Earth?

While it’s a popular theory, a meteorite is not the only way in which the Earth could be destroyed. The end of the Earth is likely to happen much more slowly and gradually.

  1. What is a red giant phase?

A red giant phase is when a star, such as the Sun, runs out of fuel and expands, consuming the inner planets, including the Earth. This process is estimated to occur in about 5 billion years.

  1. Why is it important for scientists to study the end of planets?

Studying the life cycles of planets provides valuable insight into the universe and our place in it. By understanding how planets end, we can better understand the future of our own planet and the universe as a whole?

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