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  2. Sun - Wikipedia

    en.wikipedia.org/wiki/Sun

    Ernest Rutherford suggested that the Sun's output could be maintained by an internal source of heat, and suggested radioactive decay as the source. [196] However, it would be Albert Einstein who would provide the essential clue to the source of the Sun's energy output with his mass–energy equivalence relation E = mc 2. [197]

  3. Solar activity and climate - Wikipedia

    en.wikipedia.org/wiki/Solar_activity_and_climate

    Over the following approximately 4 billion years, the Sun's energy output increased and the composition of the Earth atmosphere changed. The Great Oxygenation Event around 2.4 billion years ago was the most notable alteration of the atmosphere.

  4. Solar energy - Wikipedia

    en.wikipedia.org/wiki/Solar_energy

    Solar energy is the radiant energy from the Sun's light and heat, ... solar thermal collectors, pumps, and fans to convert sunlight into useful output.

  5. Why the sun isn't causing today's climate change - AOL

    www.aol.com/news/why-sun-isnt-causing-todays...

    Climate 101 is a Mashable series that answers provoking and salient questions about Earth’s warming climate. Yes, the sun is a profoundly important factor in Earth's climate. It always will be ...

  6. Solar irradiance - Wikipedia

    en.wikipedia.org/wiki/Solar_irradiance

    The Sun's rays are attenuated as they pass through the atmosphere, leaving maximum normal surface irradiance at approximately 1000 W/m 2 at sea level on a clear day. When 1361 W/m 2 is arriving above the atmosphere (when the Sun is at the zenith in a cloudless sky), direct sun is about 1050 W/m 2 , and global radiation on a horizontal surface ...

  7. Solar constant - Wikipedia

    en.wikipedia.org/wiki/Solar_constant

    The angular diameter of the Earth as seen from the Sun is approximately 1/11,700 radians (about 18 arcseconds), meaning the solid angle of the Earth as seen from the Sun is approximately 1/175,000,000 of a steradian. Thus the Sun emits about 2.2 billion times the amount of radiation that is caught by Earth, in other words about 3.846×10 26 watts.

  8. Synchronised satellites to create artificial solar eclipse

    www.aol.com/synchronised-satellites-create...

    The Proba-3 mission will also play an important role in climate studies by performing ongoing monitoring of the Sun’s energy output. “Researchers used to talk about the ‘solar constant ...

  9. Orders of magnitude (energy) - Wikipedia

    en.wikipedia.org/wiki/Orders_of_magnitude_(energy)

    Total energy output of the Sun each day [240] [257] 10 32 1.71×10 32 J: Gravitational binding energy of the Earth [258] 3.10×10 32 J Yearly energy output of Sirius B, the ultra-dense and Earth-sized white dwarf companion of Sirius, the Dog Star. It has a surface temperature of about 25,200 K. [259] 10 33 2.7×10 33 J

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