lamda = .0029/T
therefor, Lambda = .0029/21500 = 1.34 x 10^-7 meters
The Sun emits light in a broad range of wavelengths, peaking in the visible spectrum around 500 nanometers, which is green light. This peak intensity is a result of the Sun's temperature, which determines its blackbody radiation curve.
The temperature of a star can be calculated using Wien's law. Given the peak wavelength of 290nm, we can use the formula λmax = b/T, where b is a constant (2.898 x 10^-3 m K) to find the temperature of the star. In this case, the temperature would be approximately 10,000 K.
Astronomers determine the temperature of stars by analyzing the colors of light they emit. This is done using a tool called a spectrometer, which breaks down the light into its different wavelengths. By studying the distribution of these wavelengths, astronomers can calculate the temperature of a star.
64GB.
I can resolve 100 arc seconds. If craters are 60 arc seconds I'd bet that there are people whose eyes are good enough. 60 arc seconds is certainly within the 20 arc second maximum capability of the eye.
The Sun's wavelength of maximum energy emission falls within the visible light spectrum, specifically in the range of around 500 to 600 nanometers. This corresponds to the green to yellow part of the spectrum.
The maximum wavelength of absorbance for potassium permanganate is around 525 nanometers. At this wavelength, potassium permanganate exhibits a strong absorption peak due to its characteristic deep purple color. This absorption peak is often used in spectrophotometric analyses to quantify the concentration of potassium permanganate in solution.
The maximum wavelength of absorbance for sodium dichromate typically occurs around 350-370 nanometers (nm). This absorbance is primarily due to the presence of the chromate ion, which exhibits strong UV-visible absorbance characteristics. The specific wavelength can vary slightly depending on the concentration and the solvent used.
Resonance wavelength refers to the specific wavelength at which a material or system exhibits maximum absorption or emission of light. This wavelength is determined by the material's properties such as refractive index and the physical dimensions of the system. Resonance wavelength is important in various fields, including optics, photonics, and spectroscopy.
To find the wavelength at which an object radiates most strongly, you can use Wien's Law, which states that the wavelength of maximum intensity radiation (λmax) is inversely proportional to the temperature (T). In this case, for 20,000 K, the wavelength would be around 144.44 nanometers (nm).
The maximum wavelength at which electromagnetic radiation can occur is infinite.
Because red light has minimum frequency and thus it has maximum wavelength.
No.
The wavelength is the spatial period of the wave and it can be measured between any 2 points with the same phase. The maximum wavelength in the spectrum is 502 nm.
The maximum wavelength for cibacron Yellow FN2R dye is typically around 420-430 nm.
The wavelength of maximum emission intensity can be found using Wien's displacement law, which states that λ_max * T = 2.898 x 10^-3 m*K. Plugging in the temperature of 6000K, we get λ_max = 2.898 x 10^-3 / 6000 = 4.83 x 10^-7 meters or 483 nm.
The Sun emits light in a broad range of wavelengths, peaking in the visible spectrum around 500 nanometers, which is green light. This peak intensity is a result of the Sun's temperature, which determines its blackbody radiation curve.