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  2. Betelgeuse - Wikipedia

    en.wikipedia.org/wiki/Betelgeuse

    With a radius between 640 and 764 times that of the Sun, [14] [11] if it were at the center of our Solar System, its surface would lie beyond the asteroid belt and it would engulf the orbits of Mercury, Venus, Earth, and Mars. Calculations of Betelgeuse's mass range from slightly under ten to a little over twenty times that of the Sun.

  3. 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 ...

  4. Scholz's Star - Wikipedia

    en.wikipedia.org/wiki/Scholz's_Star

    The system has an apparent magnitude of 18.3, [2] and is estimated to be between 3 and 10 billion years old. [2] With a parallax of 166 mas (0.166 arcseconds), about 80 star systems are known to be closer to the Sun. [9] It is a late discovery, as far as nearby stars go, because past efforts concentrated on high-proper-motion objects. [citation ...

  5. Astronomers discover strange new type of star hidden in the ...

    www.aol.com/news/never-seen-old-smoker-stars...

    In about 5 or 6 billion years, our sun will become a red giant, puffing up and expanding as it releases layers of material and likely evaporating the solar system’s inner planets, although Earth ...

  6. VY Canis Majoris - Wikipedia

    en.wikipedia.org/wiki/VY_Canis_Majoris

    It has probably evolved from a hot, dense O9 main sequence star of 5–20 R ☉ (solar radii). [28] [30] [64] The star has evolved rapidly because of its high mass. The time spent to the red hypergiant phase is estimated to be between 100,000 and 500,000 years, and thus VY CMa most likely left its main sequence phase more than a million years ...

  7. Alpha Centauri - Wikipedia

    en.wikipedia.org/wiki/Alpha_Centauri

    Alpha Centauri B, also known as Toliman, is the secondary star of the binary system. It is a main-sequence star of spectral type K1-V, making it more an orange colour than Alpha Centauri A; [97] it has around 90% of the mass of the Sun and a 14% smaller diameter.

  8. List of multiplanetary systems - Wikipedia

    en.wikipedia.org/wiki/List_of_multiplanetary_systems

    The stars with the most confirmed planets are the Sun (the Solar System's star) and Kepler-90, with 8 confirmed planets each, followed by TRAPPIST-1 with 7 planets. The 1,033 multiplanetary systems are listed below according to the star's distance from Earth. Proxima Centauri, the closest star to the Solar System, has three planets (b, c and d).

  9. List of largest stars - Wikipedia

    en.wikipedia.org/wiki/List_of_largest_stars

    Luminous red novae appear to expand extremely rapidly, reaching thousands to tens of thousands of solar radii within only a few months, significantly larger than the largest red supergiants. [ 2 ] Some studies use models that predict high-accreting Population III or Population I supermassive stars (SMSs) in the very early universe could have ...