Our Sun is a 4.5 billion-year-old star – a hot glowing ball of hydrogen and helium at the center of our solar system. The Sun is about 93 million miles (150 million kilometers) from Earth, and without its energy, life as we know it could not exist here on our home planet.
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The Sun is the largest object in our solar system. The Sun’s volume would need 1.3 million Earths to fill it. Its gravity holds the solar system together, keeping everything from the biggest planets to the smallest bits of debris in orbit around it. The hottest part of the Sun is its core, where temperatures top 27 million degrees Fahrenheit (15 million degrees Celsius). The Sun’s activity, from its powerful eruptions to the steady stream of charged particles it sends out, influences the nature of space throughout the solar system.
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Heliovie
Heliovie is the study of the Sun and its various aspects. This can include studying the Sun's structure, composition, and behavior, as well as its effects on Earth and other planets. Scientists who specialize in heliovie use various instruments, such as telescopes and solar probes, to gather data and make observations of the Sun. Heliovie also involves studying phenomena such as solar flares, sunspots, and solar wind, which can have significant impacts on space weather and our technological systems.
I'm sorry, but I couldn't find any information on "Heliovie." Could you please provide more context or clarify your question?
The term "Heliovie" is not recognized as a known term or concept related to the Sun or astronomy. It is possible that it is a misspelling or a term that is not commonly used in the field.
To know more about the Sun, its characteristics, and its role in our solar system, you can refer to credible sources such as scientific articles, textbooks, or reliable websites that focus on astronomy or space science. These sources will provide detailed information about the Sun's composition, age, size, and its significance in sustaining life on Earth.