How are black holes studied?

Two black holes colliding and resulting gravitational waves
Visualization of two black holes colliding and the resulting gravitational waves that were generated.

Credit: Texas Advanced Computing Center

Black holes have long inspired the imagination yet challenged discovery. However, from a combination of theory and observation, scientists now know much about these objects and how they form, and can even see how they impact their surroundings.

So, how does one study a region of space that is defined by being invisible?

Theorists can calculate properties of black holes based on their understanding of the universe, and such discoveries have come from a range of great thinkers, from Albert Einstein to Stephen Hawking to Kip Thorne. However, despite being so powerful, it's hard to see something that does not emit photons, let alone traps any light that passes by.

Now, nearly a century after scientists suggested black holes might exist, the world now has tools to see them in action. Using powerful observatories on Earth, astronomers can see the jets of plasma that black holes spew into space, detect the ripples in space-time from black holes colliding, and may soon even peer at the disc of disrupted mass and energy that surrounds the black hole's event horizon, the edge beyond which nothing can escape.

Event Horizon Telescope


Sagittarius A*

sag a star

Credit: Event Horizon Telescope Collaboration

First image of the black hole at the center of the Milky Way

This is the first image of Sagittarius A*, or Sgr A*, the supermassive black hole at the center of our galaxy. It's the first direct visual evidence of the presence of this black hole. It was captured by the Event Horizon Telescope (EHT), an array which links together eight existing radio observatories across the planet to form a single Earth-sized virtual telescope. The telescope is named after the "event horizon", the boundary of the black hole beyond which no light can escape.

Although we cannot see the event horizon itself, because it cannot emit light, glowing gas orbiting around the black hole reveals a telltale signature: a dark central region, called a "shadow," surrounded by a bright ring-like structure. The new view captures light bent by the powerful gravity of the black hole, which is 4 million times more massive than our sun. The image of the Sgr A* black hole is an average of the different images that the EHT Collaboration has extracted from its 2017 observations.

 

News Release

sag a star

We got it! Astronomers reveal first image of the black hole at the heart of our galaxy

This result provides overwhelming evidence that the object is indeed a black hole and yields valuable clues about the workings ...

Read More

2022 EHT Panelists PDFs

NSF EHT B-Roll Package
Astronomers reveal the first image of a black hole at the heart of our galaxy.
Credit: Credits vary and are listed on slates before each shot.
Journey to our own black hole, Sagittarius A*
Dimensional animation flying the viewer into the center of the Milky Way galaxy to the planet earth, geolocating the EHT telescopes around the planet, return to the galaxy and the S-stars orbiting the black hole in the center of our galaxy, Sgr A*.
Credit: BH PIRE, UArizona
Introducing Sgr A*: First Image of a Milky Way Black Hole
People have been imagining what black holes look like since they were predicted by Einstein more than a century ago. We don’t have to imagine anymore!
Credit: National Science Foundation / Keyi “Onyx” Li
Journey of Light
This video explains why the Sgr A* black hole is more "variable" than the one in M87*, and how that variability impacts the image that the EHT team was able to take.
Credit: Smithsonian Astrophysical Observatory
black hole distance compare

Credit: National Science Foundation/Keyi "Onyx" Li

While Sgr A* is the supermassive black hole in the center of our own galaxy, the supermassive black hole M87* resides more than 55,000,000 lightyears from Earth.

size comparison ofm87 and sag a

Credit: Keyi "Onyx" Li/National Science Foundation; Lia Medeiros, Institute for Advanced Study

The supermassive black holes M87* and Sgr A* are not even in the same galaxy, but if it were possible to place them next to each other, Sgr A* would be dwarfed by M87*, which is 1,500 times more massive.

Science Matters

Science Matters

Image of Sgr A*, the black hole at the center of our galaxy

At the center of our very own Milky Way galaxy, scientists long suspected that there was a supermassive black hole, and they named this black hole Sagittarius A* (Sgr A*, pronounced "sadge-ay-star").

Media Contact
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EHT virtual backgrounds

virtual background for eht with telescopes and starry background
Event Horizon Telescope - Our own black hole

Credit: C. Padilla, NRAO/AUI/National Science Foundation

virtual background eht Sgr A* Black Hole
Sgr A* Black Hole

Credit: Event Horizon Telescope Collaboration

2019 EHT Event

2019 EHT Event


On April 10, 2019, the U.S. National Science Foundation hosted scientists from the Event Horizon Telescope Collaboration at a press conference in Washington, D.C. and revealed the world’s first image of a black hole.

Astronomical experiments at geographical South Pole

Credit: Dr. Daniel Michalik

The event was the North American pillar of a simultaneous, global announcement, with NSF hosting due to its pivotal role in the discovery, having spent two decades investing in researchers, radio telescopes, and facilities that anchored the project.  The content below tells the story of that image, how it was captured, and how it was revealed.

News Release

First photo of a black hole

Astronomers capture first image of a black hole

National Science Foundation and Event Horizon Telescope contribute to paradigm-shifting observations of the gargantuan black hole.

Read more
NSF press conference revealing first image of a black hole from Event Horizon Telescope project
A global network of telescopes has been working to capture the first ever image of a black hole. On April 10 at 9 a.m. EDT, the National Science Foundation held a press conference to announce that an image of a black hole had been captured.
Credit: National Science Foundation

For the full suite of images, animations, explanatory videos, and other multimedia content from the press event, see the Images, video, and educational resources page


NSF’s Laser Interferometer Gravitational-wave Observatory (LIGO)


LIGO opens new window on the universe

Credit: T. Pyle/Caltech/MIT/LIGO Lab

A century ago, Albert Einstein predicted gravitational waves, ripples in the fabric of space-time that result from the universe's most violent phenomena. In 2016, NSF researchers using one of the most precise instruments ever made—the NSF Laser Interferometer Gravitational-wave Observatory (LIGO)—announced the historic first detection of gravitational waves, the violent remnant of black holes colliding more than 1.3 billion years ago.

 

Andrea Ghez and the UCLA Galactic Center Group


Star makes closest approach to black hole in Milky Way

Credit: Nicolle R. Fuller, National Science Foundation

The Galactic Center Group studies the black hole at the heart of the Milky Way and how it impacts its surroundings, a multi-decade effort to better understand how galaxies formed and evolved. In 2020, Ghez shared the Nobel Prize in Physics for her discoveries, which confirmed the presence of a black hole at our galactic center.

 

NSF's National Radio Astronomy Observatory (NRAO)


Discovery of cool, interstellar gas around black hole

Credit: NRAO/AUI/National Science Foundation; S. Dagnello

NSF’s NRAO manages several powerful radio telescopes that capture unprecedented images of the cosmos, including plasma jets and other evidence of black holes.

 

NSF’s NOIRLab


NOIRLab observatory's

Credit: NOIRLab/NSF/AURA/P. Marenfeld

NSF’s National Optical-Infrared Astronomy Research Laboratory (NOIRLab) is the United States' flagship center for ground-based, nighttime optical and infrared astronomy. NSF's NOIRLab manages five observatories and centers located across the globe: Cerro Tololo Inter-American Observatory (CTIO), the Community Science and Data Center (CSDC), Gemini Observatory, Kitt Peak National Observatory (KPNO) and the Vera C. Rubin Observatory, once it becomes operational.

NSF’s Green Bank Observatory


Green Bank Telescope in summer

Credit: National Science Foundation/GBO 20; photo by Jill Malusky (available under Creative Commons

NSF's Green Bank Observatory enables leading edge research at radio wavelengths by offering access to telescopes, facilities, and advanced instrumentation to the global scientific and research community.

South Pole Telescope

south pole telescope at night with starry sky

Credit: Dr. Keith Vanderlinde

The South Pole Telescope is a 10-meter-diameter microwave / millimeter / sub-millimeter telescope located at the U.S. National Science Foundation's Amundsen-Scott South Pole Station, which is the best currently operational site on Earth for mm-wave survey observations due to its stable, dry atmosphere.