Helium is named after the Greek god of the Sun, Helios.
A star is a huge celestial body composed mainly of hydrogen and helium gases undergoing nuclear fusion in its core that produces light and heat through the release of energy.
The Sun is the celestial body that undergoes nuclear fusion, where hydrogen atoms combine to form helium, releasing energy in the process.
A large celestial body composed of gas that emits light is a star. Stars, like our Sun, are primarily made up of hydrogen and helium and produce energy through nuclear fusion in their cores, which generates light and heat. They vary in size, temperature, and brightness, and are fundamental components of galaxies.
Merriam-Webster Dictionary defines "star" as "a self-luminous gaseous spheroidal celestial body of great mass which produces energy by means of nuclear fusion reactions." So, yes, in more simple terms, it is a big ball of burning gas.
Helium is named after the Greek god of the Sun, Helios.
A star is a huge celestial body composed mainly of hydrogen and helium gases undergoing nuclear fusion in its core that produces light and heat through the release of energy.
The Sun is the celestial body that undergoes nuclear fusion, where hydrogen atoms combine to form helium, releasing energy in the process.
Helium
The sun is mainly composed of hydrogen and helium gas. These elements undergo nuclear fusion in the sun's core, converting hydrogen into helium and releasing immense amounts of energy in the form of light and heat.
Fusion occurs naturally in the core of the Sun, our nearest star, which is a celestial body in the solar system. This process involves the combination of hydrogen atoms into helium, releasing huge amounts of energy in the form of heat and light.
No sun doesn't revolve to any celestial body, but the celestial body revolve around the sun.
sun
Helium is a gas and is not found in the body
satellite
The moonMoon is the closet celestial body.
To derive the escape velocity of an object from a celestial body, you can use the formula: escape velocity (2 gravitational constant mass of celestial body / distance from the center of the celestial body). This formula takes into account the gravitational pull of the celestial body and the distance of the object from its center. By calculating this value, you can determine the minimum velocity needed for an object to escape the gravitational pull of the celestial body.