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  1. The solar mass (M ☉), 1.988 92 × 10 30 kg, is a standard way to express mass in astronomy, used to describe the masses of other stars and galaxies. It is equal to the mass of the Sun, about 333 000 times the mass of the Earth or 1 048 times the mass of Jupiter.

  2. en.wikipedia.org › wiki › Solar_SystemSolar System - Wikipedia

    The Sun is the Solar System's star and by far its most massive component. Its large mass (332,900 Earth masses), which comprises 99.86% of all the mass in the Solar System, produces temperatures and densities in its core high enough to sustain nuclear fusion of hydrogen into helium.

  3. en.wikipedia.org › wiki › SunSun - Wikipedia

    The Sun is the star at the center of the Solar System.It is a massive, hot ball of plasma, inflated and heated by energy produced by nuclear fusion reactions at its core. Part of this energy is emitted from its surface as visible light, ultraviolet, and infrared radiation, providing most of the energy for life on Earth.The Sun has been an object of veneration in many cultures.

  4. In astronomy, planetary mass is a measure of the mass of a planet -like astronomical object. Within the Solar System, planets are usually measured in the astronomical system of units, where the unit of mass is the solar mass ( M☉ ), the mass of the Sun.

  5. Sep 15, 2018 · At about 864,000 miles (1.4 million kilometers) wide, the sun is 109 times wider than Earth, and it accounts for more than 99.8 percent of the solar system's total mass. If it was a hollow ball,...

  6. en.wikipedia.org › wiki › Earth_massEarth mass - Wikipedia

    One Solar mass is close to 333 000 Earth masses. The Earth mass excludes the mass of the Moon. The mass of the Moon is about 1.2% of that of the Earth, so that the mass of the Earth+Moon system is close to 6.0456 × 1024 kg .

  7. en.wikipedia.org › wiki › MassMass - Wikipedia

    the solar mass (M ☉), defined as the mass of the Sun, primarily used in astronomy to compare large masses such as stars or galaxies (≈ 1.99 × 10 30 kg) the mass of a particle, as identified with its inverse Compton wavelength (1 cm −1 ≘ 3.52 × 10 −41 kg)

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