Web1 mrt. 2024 · The sun’s luminosity is about 3.8 x 1026 Joules a second. In terms of mass, you can think of the total energy output as about 4,000,000 tons every second. When … Web25 jan. 2024 · The sun’s luminosity is about 3.8 x 1026 Joules a second. In terms of mass, you can think of the total energy output as about 4,000,000 tons every second. When the curvature of the Earth and the density of the luminosity that hits our planet is considered, we receive only about 4.5 pounds per second of that energy. What is solar radiation W m2?
Energy from the Sun - American Chemical Society
Web26 mrt. 2013 · Now, all we have to do is calculate the surface area (in meters) of a sphere with a radius of 16,300 light years and multiply that by the minimum 10^6 photons per … Web7 aug. 2024 · A wave with a higher frequency, or a longer wavelength, transmits more energy with each photon. Multiply the the Planck constant, 6.63 x 10^-34, by the wave's speed. Assuming the wave's speed to be the speed of light in a vacuum, which is 3 x 10^8 meters per second: 6.63 x 10^-34 x 3 x 10^8 = 1.99 x 10^-25. tennessee football coaching staff 2017
How to Calculate Photons Per Second Sciencing
The sun has about 5 x 1023 horsepower – which is 5 with 23 zeroes after it. This translates to about 8 x 1020 Corvettes running at full power per second. For comparison purposes, one billion only has nine zeroes. Keep in mind that the sun is almost 93 million miles from the Earth. This means that not … Meer weergeven Instead of continuing to rely on fossil fuels, it is time to turn to the sun, which provides an astronomical amount of energy (no pun intended). … Meer weergeven If ergs and joules are not a regular part of your vocabulary, then horsepower might be easier to understand. Historically, this term was … Meer weergeven It’s easy, but it requires a change from the norm. According to the US Energy Information Administration, 86% of our energy comes from coal, natural gas, and nuclear … Meer weergeven The core of the Sun has so much pressure that nuclear fusion occurs. That energy eventually gets to the surface of the sun and shows up as light. The sunlight we see is about 6000 Kelvin or 10340.33° Fahrenheit. A … Meer weergeven Web6 dec. 2024 · The Stefan-Boltzmann equation then gives the energy flux emitted at the sun’s surface. S S = (5.67 × 10 –8 W·m –2 ·K –4 ) (5800 K) 4 = 63 × 10 6 W·m –2 The … WebNone would exist without it. At the Earth's orbit, neglecting absorption by the atmosphere, each square meter of area facing the Sun receives about 1380 joules per second (nearly … trey hopkins