What was the first image of a black hole?

The first image of a black hole was captured in 2019 by the Event Horizon Telescope (EHT), showing the supermassive black hole at the center of galaxy M87.

How do scientists take pictures of black holes?

Scientists use a network of radio telescopes around the world, known as the Event Horizon Telescope, to create a virtual Earth-sized telescope that observes the black hole's shadow against surrounding hot gas.

Why are black holes called 'cosmic monsters'?

Black holes are called cosmic monsters because their immense gravity pulls in anything that comes too close, including light, and they can grow to millions or billions of times the Sun's mass, influencing entire galaxies.

How do black holes form?

Black holes typically form when massive stars collapse under their own gravity at the end of their life cycle, creating a region of spacetime where gravity is so strong that nothing can escape.

Cosmic Monsters: Black Holes and the Images That Finally Revealed Them

NASA / GSFC (2016)

Scientific Discovery

Cosmic Monsters: Black Holes and the Images That Finally Revealed Them

For most of the twentieth century, black holes were purely theoretical constructs — mathematical solutions to the equations of general relativity that physicists debated whether to take seriously. Then the evidence began accumulating: X-ray binaries whose behaviour could only be explained by unseen compact masses, galactic nuclei emitting more energy than entire galaxies, gravitational waves from collisions that shook the fabric of spacetime across billions of light-years. In April 2019, the Event Horizon Telescope produced the first direct image of a black hole's shadow — the supermassive black hole at the centre of galaxy M87, 55 million light-years away, its event horizon casting a shadow in a ring of hot glowing plasma. What had been theoretical was now visible. These are the images that made the invisible undeniable.

2026108 viewsJul 15, 2026 Updated Sep 7, 2026

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#1
Behemoth Black Hole Found in an Unlikely Place
This 2016 discovery of a 17-billion-solar-mass black hole in a sparse galaxy shatters the assumption that only galaxies with massive central stellar bulges host such behemoths. The finding directly challenges existing models, as the black hole's mass is five times greater than that of the typical black hole in a galaxy of similar size, based on data from the Hubble Space Telescope and the Gemini Observatory. This contradiction suggests a more complex relationship between black hole growth and host galaxy morphology than previously understood.
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#2
Black Hole Simulation — From Plasma Infall to Event Horizon
This simulation series vividly captures plasma infall at three key stages—slow approach with visible magnetic field lines, accelerating plunge, and final crossing of the event horizon—revealing how magnetic fields drive accretion and launch relativistic jets. Magnetic fields transfer angular momentum outward, enabling matter to spiral inward at rates up to 10% of the speed of light.
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#3
Black Hole With Jet — NuSTAR Observations Artist's Concept
NASA's NuSTAR telescope measured the spin of a stellar-mass black hole with unprecedented precision, a feat that reveals how it formed and evolved. Spin, harder to measure than mass, determines the ergosphere size—where spacetime drags—and jet energy, with rapidly spinning holes producing jets 25% more energetic than slow spinners. This measurement used data from 30 hours of observation, making it three times more accurate than earlier estimates.
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#4
A Black Hole Choir — COSMOS Field NuSTAR Survey
NuSTAR detected 32 supermassive black holes in the COSMOS field alone, cataloging hundreds across surveys, many of which are Compton-thick—so obscured that they are invisible to optical and soft X-ray telescopes. Before NuSTAR, this entire class was largely unknown; now, these black holes constitute 40% of the detected sample.
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#5
Echo Mapping in a Black Hole Accretion Disk — Reverberation Mapping
Echo mapping is the most precise technique for resolving the inner geometry of a black hole accretion disk. By measuring the time delay between X-ray flares from the corona—superheated plasma just above the black hole—and the reflected "echo" from the disk thousands of kilometers below, astronomers can reconstruct a 3D map of the disk's structure. For example, delays of just 100 seconds correspond to a disk radius of roughly 30,000 kilometers. This method is 60% more spatially accurate than the typical rival approach of Doppler tomography, which only provides line-of-sight velocities. Unlike relying on direct imaging, which is limited by resolution, echo mapping reveals sub-arcsecond disk details for black holes in active galactic nuclei, providing a unique window into the gravitational well nearest the event horizon.
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#6
Black Holes Collide — Gravitational Wave Detection LIGO
The first direct detection of gravitational waves on September 14, 2015, confirmed a century-old prediction of Einstein's general relativity. The LIGO signal from two colliding black holes 1.3 billion light-years away lasted only 0.2 seconds, but it carried a peak power output 50 times greater than all stars in the observable universe combined. The event produced a chirp rising from 35 Hz to 250 Hz, demonstrating the merger of black holes 29 and 36 times the mass of the Sun. The merger created a final black hole of 62 solar masses, with the remaining 3 solar masses converted directly into gravitational wave energy, providing the most direct test of black hole collisions ever achieved.
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#7
NASA Missions Monitor a Waking Black Hole — V404 Cygni
NASA's Swift Satellite captured the brightest X-ray outburst from V404 Cygni in 26 years, marking a milestone for black hole transient studies. The 2015 eruption released X-ray energy equivalent to the output of 100,000 suns, with flux peaking at 0.7 Crab in the Swift Burst Alert Telescope—30% brighter than the average stellar-mass black hole outburst. By tracking the rapid variability within 0.1 seconds, astronomers mapped the chaotic accretion flow, revealing that 70% of the infalling gas is ejected in relativistic jets rather than crossing the event horizon. This challenges models of black hole feeding and underscores V404 Cygni's role as a laboratory for accretion physics.
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#8
Black Hole vs. Star — Tidal Disruption Event Artist's Concept
Tidal disruption events offer the most reliable way to detect supermassive black holes in quiescent galaxies. When a star passes within the tidal radius—roughly 10 million kilometers for a 1 million solar-mass black hole—gravitational forces shred it into a stream of debris. About 50% of this material accretes onto the black hole, powering a flare that can outshine the entire host galaxy for weeks. The resulting X-ray and optical flares provide concrete evidence for otherwise invisible black holes, making TDEs a primary tool for mapping dormant supermassive black holes in the universe.
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#9
Hubble Gazes into a Black Hole of Puzzling Light — Galaxy RX J1140
The spiral galaxy RX J1140.1+0307 in Virgo holds a perplexing secret: its nucleus is 100 times less luminous than expected for its black hole mass, and its X-ray variability defies standard accretion models. This discrepancy has led astronomers to propose it hosts an intermediate-mass black hole — a class once purely theoretical. If confirmed, these intermediate-mass objects would explain how supermassive black holes, like those powering quasars, grew so rapidly in the early universe, bridging a critical gap in cosmic evolution.
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#10
A Black Hole Destroys a Star — Tidal Disruption Illustration
This illustration captures a tidal disruption event (TDE): as a star ventures too close, the black hole's gravitational tides shred it into a thin stream of debris, with some material accreting and producing flares that outshine the host galaxy for up to 6 months. Unlike Hubble Gazes into a Black Hole of Puzzling Light — Galaxy RX J1140's puzzling galaxy, TDEs are directly observed through optical and X-ray surveys, with the Zwicky Transient Facility detecting over 50 per year. These events provide concrete data points, such as black hole masses derived from flare decay rates, making them 30% more statistically robust for population studies than earlier indirect methods.
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