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  2. Solar luminosity - Wikipedia

    en.wikipedia.org/wiki/Solar_luminosity

    The Sun is a weakly variable star, and its actual luminosity therefore fluctuates. [3] The major fluctuation is the eleven-year solar cycle (sunspot cycle) that causes a quasi-periodic variation of about ±0.1%. Other variations over the last 200–300 years are thought to be much smaller than this. [4]

  3. Luminosity - Wikipedia

    en.wikipedia.org/wiki/Luminosity

    For example, consider a 10 W transmitter at a distance of 1 million metres, radiating over a bandwidth of 1 MHz. By the time that power has reached the observer, the power is spread over the surface of a sphere with area 4πr 2 or about 1.26×10 13 m 2, so its flux density is 10 / 10 6 / (1.26×10 13) W m −2 Hz −1 = 8×10 7 Jy.

  4. Sun - Wikipedia

    en.wikipedia.org/wiki/Sun

    Because energy transport in the Sun is a process that involves photons in thermodynamic equilibrium with matter, the time scale of energy transport in the Sun is longer, on the order of 30,000,000 years. This is the time it would take the Sun to return to a stable state if the rate of energy generation in its core were suddenly changed. [106]

  5. Sunlight - Wikipedia

    en.wikipedia.org/wiki/Sunlight

    Sunlight takes about 8.3 minutes to reach Earth from the surface of the Sun. [3] A photon starting at the center of the Sun and changing direction every time it encounters a charged particle would take between 10,000 and 170,000 years to get to the surface.

  6. Sun reaches Solar Maximum but it doesn’t mean peak activity ...

    www.aol.com/sun-reaches-solar-maximum-doesn...

    The Sun has reached a period of peak activity in an 11-year cycle known as the Solar Maximum, marked by recent geomagnetic storms and near-global aurora light displays.

  7. Orders of magnitude (illuminance) - Wikipedia

    en.wikipedia.org/wiki/Orders_of_magnitude...

    Factor ()Multiple Value Item 0 0 lux 0 lux Absolute darkness 10 −4: 100 microlux 100 microlux: Starlight overcast moonless night sky [1]: 140 microlux: Venus at brightest [1]: 200 microlux

  8. List of Arabic star names - Wikipedia

    en.wikipedia.org/wiki/List_of_Arabic_star_names

    However, some Arabic language star names sprang up later in history, as translations of ancient Greek language descriptions. The astronomer Claudius Ptolemy in his Almagest (2nd century) tabulated the celestial position and brightness (visual magnitude) of 1,025 stars. Ptolemy's book was translated into Arabic in the 8th and 9th centuries and ...

  9. Sunshine duration - Wikipedia

    en.wikipedia.org/wiki/Sunshine_duration

    Some places in the interior of the Arabian Peninsula receive 3,600–3,800 hours of bright sunshine annually. The largest sun-baked region in the world (over 3,000 hours of yearly sunshine) is North Africa. The sunniest month in the world is December in Eastern Antarctica, with almost 23 hours of bright sun daily. [7]