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  2. Sun in fiction - Wikipedia

    en.wikipedia.org/wiki/Sun_in_fiction

    The Sun received comparatively little specific attention in early science fiction; [2] prior to the late 1800s, when Mars became the most popular celestial object in fiction, the Sun was a distant second to the Moon. [3]

  3. Active region - Wikipedia

    en.wikipedia.org/wiki/Active_region

    In solar physics and observation, an active region is a temporary feature in the Sun's atmosphere characterized by a strong and complex magnetic field. They are often associated with sunspots and are commonly the source of violent eruptions such as coronal mass ejections and solar flares . [ 1 ]

  4. Solar System - Wikipedia

    en.wikipedia.org/wiki/Solar_System

    If the Sun–Neptune distance is scaled to 100 metres (330 ft), then the Sun would be about 3 cm (1.2 in) in diameter (roughly two-thirds the diameter of a golf ball), the giant planets would be all smaller than about 3 mm (0.12 in), and Earth's diameter along with that of the other terrestrial planets would be smaller than a flea (0.3 mm or 0. ...

  5. List of literary movements - Wikipedia

    en.wikipedia.org/wiki/List_of_literary_movements

    Literary movements are a way to divide literature into categories of similar philosophical, topical, or aesthetic features, as opposed to divisions by genre or period. Like other categorizations, literary movements provide language for comparing and discussing literary works.

  6. Hale's law - Wikipedia

    en.wikipedia.org/wiki/Hale's_law

    Hale's law states that bipolar active regions have the following properties depending on whether the region is located in the northern or southern solar hemisphere: [2] In the same hemisphere, regions tend to have the same leading polarity. In the opposite hemisphere, regions tend to have the opposite leading polarity.

  7. Sun - Wikipedia

    en.wikipedia.org/wiki/Sun

    The Sun is classed as a G2 star, [66] meaning it is a G-type star, with 2 indicating its surface temperature is in the second range of the G class. The solar constant is the amount of power that the Sun deposits per unit area that is directly exposed to sunlight.

  8. Solar plage - Wikipedia

    en.wikipedia.org/wiki/Solar_plage

    A plage / p l eɪ dʒ / is a bright region in the Sun's chromosphere, typically found in and around active regions. Historically, they have been referred to as bright flocculi, in contrast to dark flocculi, and as chromospheric faculae, in contrast to photospheric faculae. [1]

  9. Solar phenomena - Wikipedia

    en.wikipedia.org/wiki/Solar_phenomena

    In the spectral class label, G2 indicates its surface temperature, of approximately 5770 K ( the UAI will accept in 2014 5772 K) and V indicates that the Sun, like most stars, is a main-sequence star, and thus generates its energy via fusing hydrogen into helium. In its core, the Sun fuses about 620 million metric tons of hydrogen each second.