The XRISM (X-ray Imaging and Spectroscopy Mission) recently captured data from the center of galaxy NGC 4151, where a supermassive black hole is actively consuming material from its surrounding accretion disk. The resulting spectrum obtained from this observation shows the presence of iron in the peak around 6.5 keV and dips around 7 keV, revealing light that is thousands of times more energetic than what the human eye can perceive.
The Resolve instrument aboard XRISM collected valuable insights into the physics and processes occurring at the center of NGC 4151 by studying the distribution of material and energy around the supermassive black hole. By examining these phenomena, scientists can deepen their understanding of how cosmic events interact and evolve over time.
When combined with X-ray, optical, and radio light, an image of NGC 4151 can be constructed. This comprehensive view allows researchers to see the galaxy in a new light, providing a complete picture of its structure and behavior.
Overall, XRISM’s Resolve instrument plays a crucial role in advancing our knowledge of supermassive black holes and their surrounding environments. By studying energetic processes in galaxies like NGC 4151, scientists can continue to unravel the mysteries of the universe and deepen our understanding of the forces that shape it.