# How Do You Take a Picture of a Black Hole? Astrophysicist Shep Doeleman explains the global collaboration required to image supermassive black holes. - **Source:** [Quanta Magazine](https://www.quantamagazine.org) - **Published:** 2026-10-29 - **Topic:** [science](https://brifing.si/c/science) - **Original article:** - **On Brifing:** https://brifing.si/s/e7e35729-71e4-4b20-a32f-002682f619ba ## The Elusive Cosmic Giant Black holes are exotic, dense objects that exert gravitational forces so strong that even light cannot escape their grasp. Despite their reputation as destructive monsters, they are elegant, compact systems that play a fundamental role in shaping galaxies. They act as both historical architects and future destinations for the cosmic structures we observe today. ## The First Direct Image For decades, evidence for black holes remained indirect, relying on X-ray binaries or orbital movements. In a landmark achievement, the Event Horizon Telescope network captured the first image of a supermassive black hole in the M87 galaxy. This project, involving 250 researchers, successfully visualized the shadow cast by a black hole's gravitational pull. ## Turning Earth into Optics To image an object as small as a black hole, scientists needed a telescope with unprecedented resolution. By linking radio telescopes across the globe, the team effectively created an Earth-sized instrument. This technique, known as interferometry, allows researchers to overcome the physical limitations of single-dish telescopes by combining data from multiple geographic locations. ## The Physics of Light Einstein’s theory of general relativity predicted that gas swirling into a black hole would heat to extreme temperatures, emitting light. This light is lensed by gravity, creating a distinct ring around the black hole's shadow. Capturing this ring allows scientists to measure the object's mass and verify fundamental predictions of gravitational physics. ## A Visionary's Early Inspiration Shep Doeleman’s interest in astronomy was sparked by a total solar eclipse in 1980. Watching the moon perfectly align with the sun demonstrated how rare cosmic coincidences can reveal hidden phenomena, such as the solar corona. This early experience shaped his belief that nature often provides specific windows for observing the otherwise invisible. ## Experimental Research Roots Doeleman’s path to astrophysics was non-linear, beginning with experimental work in Antarctica at age 19. Managing cosmic ray and electromagnetic experiments in harsh conditions provided him with the practical skills needed for complex field research. These experiences prepared him for the logistical challenges of coordinating a global network of radio observatories. ## Two Flavors of Holes Astrophysicists categorize black holes into two main types: stellar-mass and supermassive. Stellar-mass black holes form during the supernova collapse of massive stars. In contrast, supermassive black holes reside at the centers of galaxies. While stellar-mass versions are common, galaxies typically host only one or two of these massive, central gravitational anchors. ## Evidence from Radio Jets Before direct imaging, radio observations provided strong evidence for supermassive black holes. Astronomers observed oppositely directed jets of material moving at near-light speeds from the centers of galaxies. These jets, piercing through entire galaxies, suggested the presence of spinning supermassive black holes acting as engines for this high-energy, large-scale cosmic activity. ## The Power of Seeing While theoretical models are essential, direct imaging confers a unique reality to scientific objects. Seeing the ring of light around a black hole provides more than just a visual confirmation; it allows for precise measurements. These measurements serve as a rigorous test for the mathematical solutions derived by Schwarzschild during World War I. ## Resolution and Wavelengths The angular resolution of a telescope depends on the wavelength of light observed divided by the telescope's diameter. To see the smallest objects in the universe, researchers must either decrease the wavelength or increase the aperture size. The Event Horizon Telescope project pushed these parameters to their absolute limits to achieve necessary clarity. ## Future Cinematic Potential The current success in imaging static black holes is only the beginning of this research trajectory. Researchers are now looking toward the early 2030s, aiming to produce movies of black holes. Capturing dynamic changes in the accretion disk will provide even deeper insights into the behavior of matter near the event horizon. ## Science at Its Best The Event Horizon Telescope project represents a pinnacle of international scientific collaboration. By uniting observatories worldwide, researchers transformed a theoretical curiosity into a measurable reality. This achievement underscores how persistent, long-term experimental efforts can unlock the most profound mysteries of our universe, bridging the gap between abstract mathematics and observable physical phenomena. ## Sources covering this story - https://www.quantamagazine.org/how-do-you-take-a-picture-of-a-black-hole-20261029/ — --- _Summary written by Brifing from the original reporting. Copyright in the original article belongs to its publisher; read the full piece at the link above._