Stars emit various types of radiation, including visible light, ultraviolet radiation, and infrared radiation. They also emit X-rays and gamma rays. The type of radiation emitted depends on the temperature and composition of the star.
Long-lived stars are typically lower in mass, shine less brightly, and have longer lifespans compared to short-lived stars. Short-lived stars tend to be more massive, burn through their fuel more rapidly, and have shorter lifespans before evolving or ending in a supernova explosion.
Yes, there are some stars as small as earth. It depends, however, on where the stars are located and how long they have been burnt out.
UV-C, UV-A, and UV-B refer to different wavelengths of ultraviolet (UV) radiation. UV-C has the shortest wavelength and is mostly absorbed by the Earth's atmosphere. UV-B has a medium wavelength and can cause sunburn and skin damage. UV-A has the longest wavelength and can penetrate deeper into the skin, potentially causing long-term skin damage and aging.
4000billion years +
Long wavelength radiation, such as infrared radiation, is emitted by Earth's surface after absorbing solar radiation. Greenhouse gases in the atmosphere trap this long wavelength radiation, leading to a warming effect known as the greenhouse effect. This process helps regulate Earth's temperature by keeping the planet warm enough to support life.
Electromagnetic radiation, such as radio waves, microwaves, and infrared waves, fills space as long wavelength radiation. These forms of radiation have lower frequencies and longer wavelengths compared to visible light.
The wavelengths of electromagnetic radiation extend from any long wavelength, withno upper limit no matter how long, continuously through all possible wavelengths, withno gaps, down to any short wavelength, with no lower limit no matter how short.
Radio waves have the longest wavelength radiation from the sun. This type of radiation is lower in energy compared to other forms, such as visible light or ultraviolet rays.
This type of radiation would be classified as radio waves. Radio waves have long wavelengths and low frequencies, making them suitable for communication and broadcasting purposes.
Something having wavelike properties means that it exhibits characteristics of a wave, such as interference, diffraction, and superposition. This is commonly observed in phenomena involving light, sound, and matter at the quantum level.
Yes, long-wave heat radiation is given off by the Earth as it absorbs short-wave radiation from the Sun. This process is known as the Earth's energy balance, where incoming solar radiation is absorbed by the Earth's surface and later re-emitted as long-wave heat radiation.
Entropy - it wears everything down, ultimately converting it to long wavelength heat radiation.
By analogy with the spectrum of visible light from violet to red, with colours ordered in increasing wavelength, the electromagnetic spectrum is the collection of all types of electromagnetic radiation ordered by increasing wavelength. EM radiation that we can detect runs from ultra-long wavelength radio waves used to communicate with submarines, through long-wave, short-wave, VHF and UHF radio to microwaves, infra-red (heat radiation), visible light, UV, X-rays and gamma rays.
The sun gives off a range of wavelengths, including both short and long wavelengths. The majority of the sun's energy is in the form of visible light, which falls in the mid-range of the electromagnetic spectrum. However, the sun also emits shorter wavelength ultraviolet radiation and longer wavelength infrared radiation.
When a wave has high frequency, the wavelength is short. This is because frequency and wavelength are inversely proportional in waves. A higher frequency means more waves pass a given point in a given time, resulting in shorter wavelengths.
X-rays have the highest frequency in the electromagnetic spectrum.