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The Sun’s core will shrink but keep its massive size, becoming a White Dwarf and surrounded by a planetary nebula. The Sun accounts for 99.86% of the Solar System’s mass and is composed of 75% Hydrogen and 25% Helium, with less than 0.1% of other metals. Its plasma aura, called the corona, extends millions of kilometers and is most visible during a total solar eclipse. A coronagraph telescope can view close objects near the Sun by blocking its bright surface. The distance between the Sun and Earth fluctuates yearly due to the Earth’s elliptical orbit, ranging from 147 to 152 million kilometers. The Sun is almost a perfect sphere and rotates on its axis once every 25 days at the equator and 36 days at the poles. The energy output of the Sun is roughly 386 billion Megawatts, generated through nuclear fusion of Hydrogen into Helium.

The core of the Sun can reach temperatures of 150 million degrees Celsius during the nuclear fusion process, while the surface is cooler at approximately 5,500 degrees Celsius. The Sun has a powerful magnetic field causing magnetic storms, which give rise to dark spots known as Sunspots. The number of Sunspots visible varies significantly, occurring in a cycle every 11 years. Solar winds, streams of charged particles, are created when the particle stream builds up enough kinetic energy to escape the Sun’s center of gravity. These winds can cause radio interference and alter spacecraft trajectories. However, they also create beautiful phenomena such as the Aurora Borealis. The Sun has played a significant role in ancient religions, with early cultures often worshiping it as a deity. Astrologers once believed that the Earth was the center of the Universe, with the Sun as a planet orbiting it. Finally, if the Sun’s surface were removed, it would be pitch black, as only the outer surface glows brightly enough to burn retinas.

FAQ

1. What is the Sun?

The Sun is a star that is located at the center of the Solar System. It is the closest star to Earth, and it is the largest object in the Solar System, making up 99.86% of its total mass.

2. How hot is the Sun?

The Sun’s temperature at its core is about 15 million degrees Celsius (27 million degrees Fahrenheit). However, the temperature at the surface of the Sun is about 5,500 degrees Celsius (9,932 degrees Fahrenheit).

3. How old is the Sun?

The Sun is about 4.6 billion years old, which is about halfway through its lifespan. It is believed that the Sun will continue to shine for another 5 billion years before it reaches the end of its life cycle.

4. Does the Sun have any impact on Earth?

Yes, the Sun has a significant impact on Earth. It provides the energy that drives the Earth’s weather and climate, and it is responsible for the existence of life on our planet. However, the Sun can also have a negative impact, such as causing sunburns and damaging the ozone layer.

5. Can we harness the power of the Sun?

Yes, we can harness the power of the Sun through solar energy. Solar panels can convert the energy from the Sun into electricity, which can be used to power homes and businesses. As technology advances, solar energy is becoming more efficient and cost-effective.

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