Uploaded May 2025 | Updated September 2026, 2 weeks ago
For the first time, astronomers have probed the physical environment of repeating X-ray outbursts near monster black holes thanks to data from NASA’s NICER (Neutron star Interior Composition Explorer) and other missions.
Scientists have only recently encountered this class of X-ray flares, called QPEs, or quasi-periodic eruptions. A galaxy astronomers have nicknamed Ansky is only the eighth QPE source discovered, and it produces the most energetic outbursts seen to date. Ansky also sets records in terms of timing and duration, with eruptions every 4.5 days or so that last approximately 1.5 days.
Ansky’s name comes from ZTF19acnskyy, the moniker of a visible-light outburst seen in 2019. It was located in a galaxy about 300 million light-years away in the constellation Virgo. This event was the first indication that something unusual might be happening.
A leading theory suggests that QPEs occur in systems where a relatively low-mass object passes through the disk of gas surrounding a supermassive black hole that holds hundreds of thousands to billions of times the Sun’s mass.
When the lower-mass object punches through the disk, its passage drives out expanding clouds of hot gas that we observe as QPEs in X-rays.
Scientists think their quasi-periodicity occurs because the smaller object’s orbit is not perfectly circular and spirals toward the black hole over time. Also, the extreme gravity close to the black hole warps the fabric of space-time, altering the object’s orbits so they don’t close on themselves with each cycle. Scientists’ current understanding suggests the eruptions repeat until the disk disappears or the orbiting object disintegrates, which may take up to a few years.
Scientists think Ansky’s extreme properties may be due to the nature of the disk around its supermassive black hole, which may be much larger and therefore involve objects farther away than previous examples, creating longer timescales.
Astronomers used data from NICER and ESA’s (European Space Agency’s) XMM-Newton space telescope to map the rapid evolution of the ejected material driving the observed QPEs in unprecedented detail by studying variations in X-ray intensity during the rise and fall of each eruption.
The researchers found that each impact resulted in about a Jupiter’s worth of mass reaching expansion velocities around 15% of the speed of light.
NICER’s ability to frequently observe Ansky from the space station and its unique measurement capabilities also made it possible for researchers to measure the size and temperature of the roughly spherical bubble of debris as it expanded.
For more information about this story: science.nasa.gov/universe/nasas-nicer-maps-debris-from-recurring-cosmic-crashes
Music credit: “Superluminal,” Lee Groves and Peter George Marett [PRS], Universal Production Music
Credit: NASA’s Goddard Space Flight Center
Producer: Scott Wiessinger (eMITS)
Science Writer: Jeanette Kazmierczak (University of Maryland College Park)
Narrator: Scott Wiessinger (eMITS)
Graphics: Scott Wiessinger (eMITS)
This video can be freely shared and downloaded at svs.gsfc.nasa.gov/14819. While the video in its entirety can be shared without permission, the music and some individual imagery may have been obtained through permission and may not be excised or remixed in other products. Specific details on such imagery may be found here: svs.gsfc.nasa.gov/14819. For more information on NASA’s media guidelines, visit nasa.gov/multimedia/guidelines.
If you liked this video, subscribe to the NASA Goddard YouTube channel: youtube.com/NASAGoddard
Follow NASA’s Goddard Space Flight Center
· Instagram instagram.com/nasagoddard
· X twitter.com/NASAGoddard
· Facebook: facebook.com/NASAGoddard
· Flickr flickr.com/photos/gsfc
For the first time, astronomers have probed the physical environment of repeating X-ray outbursts near monster black holes thanks to data from NASA’s NICER (Neutron star Interior Composition Explorer) and other missions.
Scientists have only recently encountered this class of X-ray flares, called QPEs, or quasi-periodic eruptions. A galaxy astronomers have nicknamed Ansky is only the eighth QPE source discovered, and it produces the most energetic outbursts seen to date. Ansky also sets records in terms of timing and duration, with eruptions every 4.5 days or so that last approximately 1.5 days.
Ansky’s name comes from ZTF19acnskyy, the moniker of a visible-light outburst seen in 2019. It was located in a galaxy about 300 million light-years away in the constellation Virgo. This event was the first indication that something unusual might be happening.
A leading theory suggests that QPEs occur in systems where a relatively low-mass object passes through the disk of gas surrounding a supermassive black hole that holds hundreds of thousands to billions of times the Sun’s mass.
When the lower-mass object punches through the disk, its passage drives out expanding clouds of hot gas that we observe as QPEs in X-rays.
Scientists think their quasi-periodicity occurs because the smaller object’s orbit is not perfectly circular and spirals toward the black hole over time. Also, the extreme gravity close to the black hole warps the fabric of space-time, altering the object’s orbits so they don’t close on themselves with each cycle. Scientists’ current understanding suggests the eruptions repeat until the disk disappears or the orbiting object disintegrates, which may take up to a few years.
Scientists think Ansky’s extreme properties may be due to the nature of the disk around its supermassive black hole, which may be much larger and therefore involve objects farther away than previous examples, creating longer timescales.
Astronomers used data from NICER and ESA’s (European Space Agency’s) XMM-Newton space telescope to map the rapid evolution of the ejected material driving the observed QPEs in unprecedented detail by studying variations in X-ray intensity during the rise and fall of each eruption.
The researchers found that each impact resulted in about a Jupiter’s worth of mass reaching expansion velocities around 15% of the speed of light.
NICER’s ability to frequently observe Ansky from the space station and its unique measurement capabilities also made it possible for researchers to measure the size and temperature of the roughly spherical bubble of debris as it expanded.
For more information about this story: science.nasa.gov/universe/nasas-nicer-maps-debris-from-recurring-cosmic-crashes
Music credit: “Superluminal,” Lee Groves and Peter George Marett [PRS], Universal Production Music
Credit: NASA’s Goddard Space Flight Center
Producer: Scott Wiessinger (eMITS)
Science Writer: Jeanette Kazmierczak (University of Maryland College Park)
Narrator: Scott Wiessinger (eMITS)
Graphics: Scott Wiessinger (eMITS)
This video can be freely shared and downloaded at svs.gsfc.nasa.gov/14819. While the video in its entirety can be shared without permission, the music and some individual imagery may have been obtained through permission and may not be excised or remixed in other products. Specific details on such imagery may be found here: svs.gsfc.nasa.gov/14819. For more information on NASA’s media guidelines, visit nasa.gov/multimedia/guidelines.
If you liked this video, subscribe to the NASA Goddard YouTube channel: youtube.com/NASAGoddard
Follow NASA’s Goddard Space Flight Center
· Instagram instagram.com/nasagoddard
· X twitter.com/NASAGoddard
· Facebook: facebook.com/NASAGoddard
· Flickr flickr.com/photos/gsfc
