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  2. Lists of astronomical objects - Wikipedia

    en.wikipedia.org/wiki/Lists_of_astronomical_objects

    Lists of stars. List of nearest stars; List of brightest stars; List of hottest stars; List of nearest bright stars; List of most luminous stars; List of most massive stars; List of largest known stars; List of smallest stars; List of oldest stars; List of stars with proplyds; List of variable stars; List of semiregular variable stars; List of ...

  3. Stellar classification - Wikipedia

    en.wikipedia.org/wiki/Stellar_classification

    Class S stars have excess amounts of zirconium and other elements produced by the s-process, and have more similar carbon and oxygen abundances to class M or carbon stars. Like carbon stars, nearly all known class S stars are asymptotic-giant-branch stars. The spectral type is formed by the letter S and a number between zero and ten.

  4. Asterism (gemology) - Wikipedia

    en.wikipedia.org/wiki/Asterism_(gemology)

    The stars are caused by the light reflecting from needle-like inclusions of rutile aligned perpendicularly to the rays of the star. The star-effect may be also caused by the inclusions of hematite . In black star sapphire hematite needles formed parallel to the faces of the second order prism produce asterism.

  5. Brittle star - Wikipedia

    en.wikipedia.org/wiki/Brittle_star

    Brittle stars, serpent stars, or ophiuroids (from Latin ophiurus ' brittle star '; from Ancient Greek ὄφις (óphis) ' serpent ' and οὐρά (ourá) ' tail '; referring to the serpent-like arms of the brittle star) are echinoderms in the class Ophiuroidea, closely related to starfish. They crawl across the sea floor using their flexible ...

  6. Cat's Eye Nebula - Wikipedia

    en.wikipedia.org/wiki/Cat's_Eye_Nebula

    The Cat's Eye Nebula (also known as NGC 6543 and Caldwell 6) is a planetary nebula in the northern constellation of Draco, discovered by William Herschel on February 15, 1786. It was the first planetary nebula whose spectrum was investigated by the English amateur astronomer William Huggins , demonstrating that planetary nebulae were gaseous ...

  7. Astronomical symbols - Wikipedia

    en.wikipedia.org/wiki/Astronomical_symbols

    [47] [55] In modern renditions, the spearhead has a broader or narrower diamond shape. In 1802, it was given a cordate leaf shape. A variation has a triangular head, conflating it with the alchemical symbol for sulfur. [47] 3 Juno [48] [85] U+26B5 (dec 9909) ⚵ a scepter topped with a star [48] [42] [86] 4 Vesta [49] U+1F777 (dec 128887) 🝷

  8. Stellar structure - Wikipedia

    en.wikipedia.org/wiki/Stellar_structure

    Different layers of the stars transport heat up and outwards in different ways, primarily convection and radiative transfer, but thermal conduction is important in white dwarfs. Convection is the dominant mode of energy transport when the temperature gradient is steep enough so that a given parcel of gas within the star will continue to rise if ...

  9. Celestial spheres - Wikipedia

    en.wikipedia.org/wiki/Celestial_spheres

    In Greek antiquity the ideas of celestial spheres and rings first appeared in the cosmology of Anaximander in the early 6th century BC. [7] In his cosmology both the Sun and Moon are circular open vents in tubular rings of fire enclosed in tubes of condensed air; these rings constitute the rims of rotating chariot-like wheels pivoting on the Earth at their centre.