Webwhere T * is the apparent sun temperature as an exergy source. In this analysis, the value suggested by Petela (1964) is adopted, i.e., T * is approximately equal to ¾T s, where T s is the apparent blackbody temperature of the sun, which is about 5770 K. Therefore, the T * considered here is 4330 K. It should be noted that, in this analysis, T * is also considered … WebThe effective temperature, defined by the total radiative power per square unit, is 5772 K. [4] The color temperature of sunlight above the atmosphere is about 5900 K. [5] The Sun may appear red, orange, yellow, or white …
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Web10 Oct 2012 · Photosphere - The photosphere is the deepest layer of the Sun that we can observe directly. It reaches from the surface visible at the center of the solar disk to about 250 miles (400 km) above that. The … Web10 Jul 2024 · The above graph compares global surface temperature changes (red line) and the Sun's energy received by the Earth (yellow line) in watts (units of energy) per square meter since 1880. The lighter/thinner lines show the yearly levels, while the heavier/thicker lines show the 11-year average trends. fut fantasy futbin
Exact temperature to heat your home to stop mould and ... - The Sun
WebThe temperature in a sunspot is low compared with neighbour area, typically 4000 K (70% of normal T). Therefore sunspots only emit the fraction of 0,704= 24% of L. This is why sunspots look black, compared with the surrounding surface (Fig. 10). Figure 10 - Sunspot and granules. Energy transport and Granules WebThe Sun is a class G star; these are yellow, with surface temperatures of 5,000–6,000 K. Class K stars are yellow to orange, at about 3,500–5,000 … Webr=radius of the body=700000000 I'm using this equation to estimate the core temperature : (G*mp*M)/ (r* (3/2)*k) which nets 15653011 for the sun which is close enough given that that is the only star core temperature known (afaik). I'm using this to estimate the luminosity L: 4*PI* (r^2)*s* (Te^4) giving hands brierley hill