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Solar output is nearly, but not quite, constant. Variations in total solar irradiance were too small to detect with technology available before the satellite era. As the Earth rotates, the energy from the sun is distributed across the entire surface area. At any given moment, the amount of solar radiation received at a location on the Earth's surface depends on the state of the atmosphere, the location's latitude, and the time of day.

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Wiki User

12y ago
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AnswerBot

5mo ago

The sun's energy stays relatively constant due to a balance between gravitational forces pulling inwards and nuclear fusion reactions pushing outwards. Any fluctuations in energy output are typically small and occur over long time scales.

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Q: What makes the sun's energy stay the same?
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