One nominal solar luminosity is defined by the International Astronomical Union to be 3.828×1026 W. The Sun is a weakly variable star, and its actual luminosity therefore fluctuates. The major fluctuation is the eleven-year solar cycle (sunspot cycle) that causes a quasi-periodic variation of about ±0.1%.
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The table at right provides the magnitudes of the brightest bodies of the solar system sorted by the maximal visual magnitudes.Only the bodies brightest ...
The luminosity of the Sun is 3.846 × 1026 watts (or 3.846 × 1033 ergs per second). Luminosity is an absolute measure of radiant power; that is, its value is ...
Apr 1, 2024 · Solar luminosity, denoted as L☉, is a measure of the total amount of energy emitted by the Sun per unit time. It is a crucial parameter in ...
Solar radiation that reaches the Earth's surface is absorbed by the atmosphere. The amount of absorption depends on the elevation of the Sun above the horizon, ...