WebFactors affecting the Earth’s temperature. The temperature of the Earth depends on many factors including the concentration of greenhouse gases such as water vapour, … Blackbody temperature To find the effective (blackbody) temperature of a planet, it can be calculated by equating the power received by the planet to the known power emitted by a blackbody of temperature T. Take the case of a planet at a distance D from the star, of luminosity L. Assuming the star … See more The effective temperature of a body such as a star or planet is the temperature of a black body that would emit the same total amount of electromagnetic radiation. Effective temperature is often used as an estimate of a … See more The effective temperature of a star is the temperature of a black body with the same luminosity per surface area (FBol) as the star and is defined according to the Stefan–Boltzmann law FBol … See more • Star portal • Brightness temperature • Color temperature See more • Effective temperature scale for solar type stars • Surface Temperature of Planets • Planet temperature calculator See more
Black body temperature - Oxford Reference
WebThe radiation spectrum was measured by the COBE satellite and found to be a remarkable fit to a blackbody curve with a temperature of 2.725 K and is interpreted as evidence that the universe has been expanding and cooling for about 13.7 billion years. WebBy the Stefan-Boltzmann law, the black body temperature is given by where is . Using a planetary albedo of 0.3, this gives a black body temperature of 255 K or -18 C, very … green law firms
Greenhouse Effect Clarkson University
WebNov 17, 2024 · The average temperature of the Earth’s surface increased by about 1.4 °F (0.8 °C) over the past 100 years, with about 1.0 °F (0.6 °C) of this warming occurring over just the past three decades. [1] 14.9: Global Warming is shared under a not declared license and was authored, remixed, and/or curated by LibreTexts. Webmaximum wavelength for the earth's blackbody radiation. Solution: λmax = γ/T = (2.90 x 10-3 m K) / (300 K) = 9.7 mm. This is in the infrared. This is crucial for understanding the green-house effect. 4. The Solar Spectrum The radiation from the sun may be modeled by that of a black body at a temperature of WebInfrared radiation of Earth is 239 W⋅m −2, one of two outgoing energy values of Earth's energy budget, the other being the reflected energy of 102 W⋅m −2, and effectively being the 255 K calculated blackbody … greenlawformayor.ca