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  2. Sun - Wikipedia

    en.wikipedia.org/wiki/Sun

    The Sun is about halfway through its main-sequence stage, during which nuclear fusion reactions in its core fuse hydrogen into helium. Each second, more than four billion kilograms of matter are converted into energy within the Sun's core, producing neutrinos and solar radiation. At this rate, the Sun has so far converted around 100 times the ...

  3. Solar wind - Wikipedia

    en.wikipedia.org/wiki/Solar_wind

    The total number of particles carried away from the Sun by the solar wind is about 1.3 × 10 36 per second. [32] Thus, the total mass loss each year is about (2–3) × 10 −14 solar masses, [33] or about 1.3–1.9 million tonnes per second. This is equivalent to losing a mass equal to the Earth every 150 million years. [34]

  4. Solar phenomena - Wikipedia

    en.wikipedia.org/wiki/Solar_phenomena

    A solar flare is a sudden flash of brightness observed over the Sun's surface or the solar limb, which is interpreted as an energy release of up to 6 × 10 25 joules (about a sixth of the total Sun's energy output each second or 160 billion megatons of TNT equivalent, over 25,000 times more energy than released from the impact of Comet ...

  5. Solar core - Wikipedia

    en.wikipedia.org/wiki/Solar_core

    The core contains 34% of the Sun's mass, but only 3% of the Sun's volume, and it generates 99% of the fusion power of the Sun. There are two distinct reactions in which four hydrogen nuclei may eventually result in one helium nucleus: the proton–proton chain reaction – which is responsible for most of the Sun's released energy – and the ...

  6. Solar constant - Wikipedia

    en.wikipedia.org/wiki/Solar_constant

    More specifically, it is a flux density measuring mean solar electromagnetic radiation (total solar irradiance) per unit area. It is measured on a surface perpendicular to the rays, one astronomical unit (au) from the Sun (roughly the distance from the Sun to the Earth). The solar constant includes radiation over the entire electromagnetic ...

  7. Solar mass - Wikipedia

    en.wikipedia.org/wiki/Solar_mass

    The solar mass (M ☉) is a standard unit of mass in astronomy, equal to approximately 2 × 10 30 kg (2 nonillion kilograms in US short scale). It is approximately equal to the mass of the Sun. It is often used to indicate the masses of other stars, as well as stellar clusters, nebulae, galaxies and black holes. More precisely, the mass of the ...

  8. Heliosphere - Wikipedia

    en.wikipedia.org/wiki/Heliosphere

    Voyager 1 surpassed the radial distance from the Sun of Pioneer 10 at 69.4 AU on 17 February 1998, because it was traveling faster, gaining about 1.02 AU per year. [70] On July 18, 2023, Voyager 2 overtook Pioneer 10 as the second most distant human-made object from the Sun. [ 71 ] Pioneer 11 , launched a year after Pioneer 10 , took similar ...

  9. Orders of magnitude (energy) - Wikipedia

    en.wikipedia.org/wiki/Orders_of_magnitude_(energy)

    Mass-energy of the Andromeda galaxy (M31), ~0.8 trillion solar masses. [344] [345] 10 62 1–2×10 62 J: Total massenergy of the Virgo Supercluster including dark matter, the Supercluster which contains the Milky Way [346] 10 70: 1.462×10 70 J: Rough estimate of total massenergy of ordinary matter (atoms; baryons) present in the ...