Stars are the primary sources of luminous radiation in the universe, radiating energy across various temperatures, from 2700 K to as high as 10^24 K.
Highly evolved stars, such as Wolf-Rayet stars, can achieve extreme surface temperatures up to 210,000 K, showcasing the diverse thermal profiles of stellar bodies.
Neutron stars and their interiors reach staggering temperatures, with surfaces radiating at ~600,000 K and cores exceeding one trillion K, allowing for unique particle states.
The most extreme conditions of temperature and energy occur in supermassive black holes where particle acceleration causes energies reaching around 10^20 eV, suggesting temperatures of 10^24 K.
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