When stars burn hydrogen, what type of radiation do they emit?

When stars burn hydrogen in their cores, they undergo a process known as nuclear fusion. This process primarily converts hydrogen into helium while releasing a significant amount of energy. This energy is emitted in the form of electromagnetic radiation, which spans a wide range of wavelengths, encompassing everything from radio waves to gamma rays.

Electromagnetic radiation is the mechanism by which energy is transported from the interior of the star to its surface and then into space. As nuclear fusion occurs, different forms of radiation are produced, including visible light, ultraviolet radiation, and even infrared radiation. However, it is the general category of electromagnetic radiation that encompasses all these forms, which is why it is the most accurate and complete answer to the question.

While ultraviolet radiation is indeed a component of what is emitted by stars, it does not fully encapsulate the range of emissions from hydrogen fusion. Gravitational radiation refers to waves in spacetime caused by massive objects moving through it and is not relevant to the fusion processes occurring in stars. Microwave radiation is a subset of electromagnetic radiation but does not adequately cover the broader spectrum involved in stellar processes. Thus, the key aspect of energy release in stars through nuclear fusion is correctly described as electromagnetic radiation.