About Sun in our solar system
The Sun is theat the center of the . It is a massive, nearly perfectof hot , heated tobyreactions in its core, radiating the energy from itsmainly asandwith 10% atenergies. It is by far the most important source of energy foron . The Sun has been anin many cultures. It has been a central subject for astronomical research since . The Sun is the only star and the center of our solar system1234. It is a hot ball of hydrogen and helium24that is about 100 times wider than Earth and 10 times wider than Jupiter14. The Sun's gravity holds the solar system together1and its energy makes life possible on Earth2. The Sun is about 93 million miles (150 million kilometers) from Earth24and it takes light about 8 minutes and 20 seconds to reach us3.
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6 FAQs about [Sun in our solar system]
Why is the Sun a dominant body of the Solar System?
Sun, star around which Earth and the other components of the solar system revolve. It is the dominant body of the system, constituting more than 99 percent of its entire mass. The Sun is the source of an enormous amount of energy, a portion of which provides Earth with the light and heat necessary to support life.
How did the Sun become a planet?
Eventually, the gases heated up enough to begin nuclear fusion, and became the sun in our solar system. Other parts of the molecular cloud cooled into a disc around the brand-new sun and became planets, asteroids, comets, and other bodies in our solar system. The sun is about 150 million kilometers (93 million miles) from Earth.
What is the main body of the Solar System?
Get a special academic rate on Britannica Premium. Sun, star around which Earth and the other components of the solar system revolve. It is the dominant body of the system, constituting more than 99 percent of its entire mass.
What is the energy produced by the Sun?
The energy produced by the Sun is essential for life on Earth and is a driving force behind the Earth’s weather. The Sun is all the colours mixed together, this appears white to our eyes. The Sun is composed of hydrogen (70%) and Helium (28%). The Sun is a main-sequence G2V star (or Yellow Dwarf).
What part of the Sun do we see from Earth?
The part of the Sun we see from Earth – the part we call the surface – is the photosphere. The Sun doesn’t actually have a solid surface because it’s a ball of plasma. Above the Sun’s surface are its thin chromosphere and the huge corona (crown). This is where we see features such as solar prominences, flares, and coronal mass ejections.
Why is the Sun important to astrophysics?
The Sun is the engine behind much of Earth’s environment, providing energy for everything from ocean currents and weather patterns to the plants and algae that form the base of many food chains. The Sun is the easiest star for us to study, making it very useful to the field of astrophysics.
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