The 'White Light' part.
We cannot see. UV. or shorter wavelengths. nor can we see IR (Infra-Red) or lomger wavelengths.
However, humans can be affected by unseen EM waves.
UV in small doses , gives us a 'tan'.
IR can transfer heat.
White Light was shown by Sir Isaac newton , in his Optics, to split into the colours of the rainbow. Blue at the shorter wavelength and red at the longer wavelength. With in order of wavelength , violet, indigo, blue, green, yellow, orange, red.
NB If you like to have a 'sun tan' , then sit in the shade. You will receive all the UV light you need for the tan, but, none of the IR light, which would heat you up and give you sun burn .
Yes - as with all other wavelengths on the em spectrum - however, not to a high intensity. You'd be surprised the moon is actually brighter than the sun when viewed in 'gamma ray vision'.
solar The sun releases electromagnetic energy in the entire EM spectrum from radio waves up to Gamma radiation
Electromagnetic (EM) radiation is the word we use for any sort of energy wave that propagates through space. We can measure the frequency of the wave, or the wavelength. The speed of light is 186,000 miles per second, which is about 300,000,000 meters per second. We can use this to convert frequency to wavelength; the frequency (in Hertz) times the wavelength (in meters) equals the speed of light. The EM spectrum includes radio, microwaves, heat, light, X-rays and gamma rays; it is all electromagnetic radiation, and the only difference is the frequency (or wavelength). So heat rays are part of the EM spectrum that is just below the red color of light, so "infra-" (below) red; infrared. Infrared (IR) is light that is a frequency a little below what our eyes can see, just as ultraviolet (UV) rays are just light that's a little higher in frequency than our eyes see. We see when light is reflected back to our eyes. When light hits vegetation, it reflects best in the IR range, so satellite photos in the IR range can see tiny changes in the way we see plants.
Stars produce energy through nuclear fusion, where hydrogen atoms combine to form helium in their cores. This process releases a tremendous amount of energy in the form of light and heat, which is what sustains a star's brightness and allows it to shine.
The color of a star is determined by its temperature. The sun's temperature (around 5,500°C) causes it to emit white light, with a peak in the yellow-green spectrum. Higher temperature stars appear blue or purple because they emit more energy in the ultraviolet and blue wavelengths.
Humans can see colors in the visible light portion of the electromagnetic spectrum, which ranges from approximately 400 nanometers (violet) to 700 nanometers (red).
It is certainly a very important part, but it is not a major part; 'visible light' makes up only a tiny part of the EM spectrum.
The visible light portion of the electromagnetic spectrum is most important to humans as it allows us to see our surroundings. This portion ranges from about 400 to 700 nanometers in wavelength and is the basis for our perception of colors and shapes.
Most of the EM spectrum is visible light.
That part is called "visible light", or just "light".
The smallest part of the electromagnetic spectrum is the gamma rays. They have the shortest wavelengths and highest frequencies among all types of electromagnetic radiation.
Sound is a mechanical wave, not an electromagnetic wave.
Visible light is a very small part of the EM spectrum and it is intellectual laziness to refer to all EM radiation as light.
frequency and heat. (Color can change, too)
Cosmic rays are not part of the EM spectrum -- they are high energy charged particles.
The part of the electromagnetic spectrum that we can see is visible light. Visible light consists of the colors of the rainbow, ranging from violet at shorter wavelengths to red at longer wavelengths. This portion of the spectrum is detected by our eyes and is responsible for our sense of sight.
The highest frequency part of the electromagnetic spectrum is gamma rays. Gamma rays have the shortest wavelengths and highest energy of all electromagnetic waves.