I just learned this while researching grow lamps today.
The conversion from nm to K is:
SInce I'm typing this out on a computer, and don't really know how to turn on my funny math symbols, I'm going to rewrite the equation below, with everything in the same place, only replacing the funny symbols with other variable symbols that I can reproduce on a regular keyboard.
nm = 2,897,768 / K
In this equation:
nm = nanometers, or peak wavelength
K = Peak temperature, in degrees Kelvin.
2,897,768 = the number that needs to be in the equation according to some big science and math conference where a whole lot of nerds got together and decided things like the number that needs to be in that spot in the equation. I tried to understand it, but I don't know anything about math terminology and am not smart enough to learn about it tonight before I respond to this, so I can't explain why that number exists, only that it has to be there to complete the conversion.
This equation is called Wien's law, and it is actually a lot more complex than I'm making it here, but to use it properly would take more understanding than I have. This method is not as accurate as if you were to use the full equation, but it's so close that most people even simplify it further to nm = 3,000,000 / K, and still consider it accurate enough to be a practical reference tool.
I'll show a few examples.
A light bulb rated at 4500K translates to 644nm.
644 (nm) = 2,897,768 / 4500 (K)
A light bulb rated at 6500K translates to 446nm.
446 (nm) = 2,897,768 / 6500 (K)
A light bulb rated at 10.000K translates to 290nm.
290 (nm) = 2,897,768 / 10,000K
The sun puts out peak radiation at 5778K, which is approximately 502nm.
502 (nm) = 2,897,768 / 5778 (K)
Adversely, to convert the opposite direction, swap the position of the nm and the K to look like:
K = 2,897,768 / nm
The response to your question would look like this: K = 2,897,768 / 450
K = 6,439K
You'll notice that when you make it a little easier on yourself and use 3,000,000 instead of 2,897,768, the result is quite noticeably inaccurate, but I suppose if you needed that much accuracy, you'd be in a lab somewhere doing this yourself instead of asking a moron like me to explain it.
To find the temperature associated with light of a certain wavelength, we can use Wien's displacement law: λ_max = b / T, where λ_max is the peak wavelength, b is Wien's displacement constant (2.898 x 10^-3 m*K), and T is the temperature in Kelvin. Since the peak wavelength for 450 nanometer light is 450 x 10^-9 meters, we can rearrange the formula to solve for T. Plugging in the values, we find T ≈ 6444 K.
When light passes through a substance near 0 degrees Kelvin, it bends and becomes deformed.
the temperature of a UV light is 10nm-400 degrees fahrenheit
The "K" in 4057K bulb stands for Kelvin, which is a unit of measure for color temperature. It indicates the color appearance of the light emitted by the bulb, with higher Kelvin values corresponding to cooler (bluish-white) light and lower Kelvin values corresponding to warmer (yellowish-white) light.
A star like the sun has a surface temperature of about 5800 K to 6000 K. At this temperature, a star emits light in the visible spectrum, appearing white or yellow-white.
The term 2700K refers to the color temperature of a light source, measured in Kelvin. A 2700K light source typically produces a warm, yellowish light similar to traditional incandescent bulbs. This color temperature is suitable for creating a cozy and inviting atmosphere in residential spaces.
A temperature of 3000 Kelvin is equivalent to around 2726.85 degrees Celsius or 4940.33 degrees Fahrenheit. This temperature is high enough to produce a glowing red-orange light emission, making it commonly associated with hot objects such as molten metal or stars.
Dubhe is a star in the constellation Ursa Major, approximately 124 light-years away from Earth. It has a surface temperature of around 5,800 degrees Celsius (10,500 degrees Fahrenheit).
When light passes through a substance near 0 degrees Kelvin, it bends and becomes deformed.
Stars that are around 4000 degrees Kelvin typically appear red in color. This is because their surface temperature is cooler, causing them to emit more red and infrared light compared to higher temperature stars.
Light is usually measured in candle power or candellas. The temperature of the light is measured in degrees, kelvin. You'll find greater detail at the local library or through research on the internet.
The temperature of the core of a star can reach millions of degrees Kelvin due to nuclear fusion reactions that generate immense heat and light. This intense heat and pressure in the core are what sustain a star's energy output.
the temperature of a IR light is 6500 degrees fahrenheit
3000 Kelvin refers to the color temperature of light. It represents a warm white light that is slightly more yellowish in tone, similar to the light produced by traditional incandescent bulbs.
The temperature of the Sun's crust, known as the photosphere, is around 5,500°C (9,932°F). This is the layer from which most of the Sun's visible light is emitted.
The temperature at which a blackbody radiates primarily in the infrared region is around 300 K (27°C). At this temperature, the peak of the blackbody radiation curve falls within the infrared spectrum.
the temperature of a UV light is 10nm-400 degrees fahrenheit
Ah, isn't that a lovely temperature! To convert Celsius to Kelvin, you simply add 273. So, 34 degrees Celsius is equal to 307 Kelvin. Just like adding a touch of light to a painting, converting temperatures can bring a new perspective and understanding to the beauty of science.