That will depend a lot on the star's temperature. The highest frequencies can be infrared radiation, red light, blue light, ultraviolet, or even x-rays - all depending on the star's surface temperature.
The range of electromagnetic radiation produced by a star includes radio waves, microwaves, infrared, visible light, ultraviolet, X-rays, and gamma rays. The distribution of these wavelengths depends on the temperature and composition of the star.
Electromagnetic radiation.
Supernovas release a wide range of electromagnetic radiation, including visible light, X-rays, and radio waves. This emission is a result of the intense energy and heat created during the explosion of a star.
Our sun emits mostly visible and ultra-violet radiation
star produce radiation and it is usually gamma which is deadly and it affects the color of the star
Yes, radiation is produced in the sun as a result of nuclear fusion reactions occurring in its core. These reactions convert hydrogen atoms into helium, releasing energy in the form of electromagnetic radiation.
A star is any hydrostatically stable plasma that generates heat and electromagnetic radiation by nuclear fusion.
A star is a roughly spherical plasma that emits electromagnetic radiation by nuclear fusion, usually that of hydrogen into helium.
It is no longer a star but a cosmic body which hsa imploded into a black hole.
You would look for high-energy electromagnetic radiation like gamma rays emitted from the star. This type of radiation is produced during nuclear fusion reactions when light atomic nuclei combine to form heavier nuclei and release energy. Detection of gamma rays can provide evidence that nuclear fusion is taking place in the core of a star.
The radiation zone is a region in the interior of a star where energy is transported outward by electromagnetic radiation, primarily in the form of photons. In this zone, energy is carried through the star's layers by the absorption and re-emission of photons. The radiation zone is located between the core and the convection zone of a star.
In the radiation zone of a star, energy is transferred through electromagnetic radiation in the form of photons. These photons travel outward from the core of the star through the radiation zone, carrying thermal energy with them. This process allows the star to maintain its equilibrium by balancing the inward gravitational force with the outward pressure generated by this energy transfer.