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  2. Stellar evolution - Wikipedia

    en.wikipedia.org/wiki/Stellar_evolution

    Representative lifetimes of stars as a function of their masses The change in size with time of a Sun-like star Artist's depiction of the life cycle of a Sun-like star, starting as a main-sequence star at lower left then expanding through the subgiant and giant phases, until its outer envelope is expelled to form a planetary nebula at upper right Chart of stellar evolution

  3. Stellar mass loss - Wikipedia

    en.wikipedia.org/wiki/Stellar_mass_loss

    The sun loses mass due to the solar wind at a very small rate, (2–3) × 10 −14 solar masses per year. [2] The solar wind carries trace amounts of the nuclei of heavy elements fused in the core of the sun, revealing the inner workings of the sun while also carrying information about the solar magnetic field. [3]

  4. Tau Ceti - Wikipedia

    en.wikipedia.org/wiki/Tau_Ceti

    Tau Ceti, Latinized from τ Ceti, is a single star in the constellation Cetus that is spectrally similar to the Sun, although it has only about 78% of the Sun's mass.At a distance of just under 12 light-years (3.7 parsecs) from the Solar System, it is a relatively nearby star and the closest solitary G-class star.

  5. G-type main-sequence star - Wikipedia

    en.wikipedia.org/wiki/G-type_main-sequence_star

    The Sun, the star in the center of the Solar System to which the Earth is gravitationally bound, is an example of a G-type main-sequence star (G2V type). Each second, the Sun fuses approximately 600 million tons of hydrogen into helium in a process known as the proton–proton chain (4 hydrogens form 1 helium), converting about 4 million tons ...

  6. List of nearest stars - Wikipedia

    en.wikipedia.org/wiki/List_of_nearest_stars

    The closest encounter to the Sun so far predicted is the low-mass orange dwarf star Gliese 710 / HIP 89825 with roughly 60% the mass of the Sun. [4] It is currently predicted to pass 0.1696 ± 0.0065 ly (10 635 ± 500 au) from the Sun in 1.290 ± 0.04 million years from the present, close enough to significantly disturb the Solar System's Oort ...

  7. The sun actually pelts itself with colossal 'shooting stars'

    www.aol.com/news/sun-actually-pelts-itself...

    The weather forecast on the sun: rainy with a chance of space fireballs. Astronomers have discovered a phenomenon that causes the sun to form enormous objects similar to meteors or "shooting stars ...

  8. Formation and evolution of the Solar System - Wikipedia

    en.wikipedia.org/wiki/Formation_and_evolution_of...

    The Sun remains a main-sequence star today. [33] As the early Solar System continued to evolve, it eventually drifted away from its siblings in the stellar nursery, and continued orbiting the Milky Way's center on its own. The Sun likely drifted from its original orbital distance from the center of the galaxy.

  9. How Did the “Dubai Bling” Cast Get So Rich? All About the ...

    www.aol.com/did-dubai-bling-cast-rich-163000632.html

    Neville Hopwood/Getty. The cast of Netflix's 'Dubai Bling' attend an exclusive celebration at the INTI Edition on Oct. 20, 2022, in Dubai, United Arab Emirates.