T CrB is a binary system comprising a red giant and a white dwarf, where the latter siphons material from its neighbor until a critical mass is reached, sparking a thermonuclear fusion on its surface.

Situated within a binary system alongside its larger counterpart, the unseen white dwarf J0526A, this stellar duo dances around each other with astonishing speed, completing one orbit in just 20 minutes.

This colossal image is a mosaic composed of hundreds of meticulously stitched-together frames, each captured through filters that allow different colors of light to pass through.

This newly found massive helium star may provide insights into the origins of magnetars – extremely dense remnants of dead stars with ultra-strong magnetic fields that have baffled scientists for years.

While this natural twinkle isn't visible to telescopes on Earth, the Northwestern University research team achieved a breakthrough. They accurately modeled the energy rippling caused by convection in a star's core and then translated these patterns into sound.

Since the age of the universe is approximately 13.8 billion years, diamond stars have not yet fully formed, but some are already starting to undergo this extraordinary metamorphosis. HD 190412 C is believed to be one such object.