Black Hole Beams Promote Stellar Eruptions | Hubble Space Telescope
Giant galaxy M87 shows a 3,000-light-year-long jet of plasma blasting from the galaxy's 6.5-billion-solar-mass central black hole
Black hole jet and accompanying erupting nova (artist's concept)
In a surprise finding, astronomers using the NASA/European Space Agency Hubble Space Telescope have discovered that the blowtorch-like jet from a supermassive black hole at the core of a huge galaxy seems to cause stars to erupt along its trajectory. The stars, called novae, are not caught inside the jet, but are apparently in a dangerous neighborhood nearby.
The finding confounds researchers searching for an explanation. "We don't know what's going on, but it's just a very exciting finding," said lead author Alec Lessing of Stanford University. "This means there's something missing from our understanding of how black hole jets interact with their surroundings."
A nova erupts in a double-star system where an ageing, swelled-up, normal star spills hydrogen onto a burned-out white dwarf companion star. When the dwarf has tanked up a mile-deep surface layer of hydrogen that layer explodes like a giant nuclear bomb. The white dwarf is not destroyed by the nova eruption. It ejects its surface layer and then goes back to syphoning fuel from its companion, and the nova-outburst cycle starts over again.
Hubble found twice as many novae going off near the jet as elsewhere in the giant galaxy during the surveyed time period. The jet is launched by a 6.5-billion-solar-mass central black hole surrounded by a disc of swirling matter. The black hole, engorged with infalling matter, launches a 3,000-light-year-long jet of plasma blazing through space at nearly the speed of light. Anything caught in the energetic beam would be sizzled. However, being near its blistering outflow is apparently also risky, according to the new Hubble findings.
The finding of twice as many novae near the jet implies that there are twice as many nova-forming double-star systems near the jet or that these systems erupt twice as often as similar systems elsewhere in the galaxy.
"There's something that the jet is doing to the star systems that wander into the surrounding neighborhood. Maybe the jet somehow snowplows hydrogen fuel onto the white dwarfs, causing them to erupt more frequently," said Lessing. "But it's not clear that it's a physical pushing. It could be the effect of the pressure of the light emanating from the jet. When you deliver hydrogen faster, you get eruptions faster. Something might be doubling the mass transfer rate onto the white dwarfs near the jet." Another idea the researchers considered is that the jet is heating the dwarf's companion star, causing it to overflow further and dump more hydrogen onto the dwarf. However, the researchers calculated that this heating is not nearly large enough to have this effect.
"We're not the first people who've said that it looks like there's more activity going on around the M87 jet," said co-investigator Michael Shara of the American Museum of Natural History in New York City. "But Hubble has shown this enhanced activity with far more examples and statistical significance than we ever had before."
Shortly after Hubble's launch in 1990, astronomers used its first-generation Faint Object Camera (FOC) to peer into the center of M87 where the monster black hole lurks 54 million light years away. They noted that unusual things were happening around the black hole. Almost every time Hubble looked, astronomers saw bluish "transient events" that could be evidence for novae popping off like camera flashes from nearby paparazzi. Unfortunately, the FOC's view was so narrow that Hubble astronomers could not look away from the jet to compare with the near-jet region. For over two decades, the results remained mysteriously tantalizing.
Compelling evidence for the jet's influence on the stars of the host galaxy was collected over a nine-month interval when Hubble observed with newer, wider-view cameras to count the erupting novae. This was a challenge for the telescope's observing schedule because it required revisiting M87 precisely every five days for another snapshot. Adding up all of the M87 images led to the deepest images of M87 that have ever been taken.
Hubble found 94 novae in the one-third of M87 that its camera can encompass. "The jet was not the only thing that we were looking at—we were looking at the entire inner galaxy. Once you plotted all known novae on top of M87 you did not need statistics to convince yourself that there is an excess of novae along the jet. This is not rocket science. We made the discovery simply by looking at the images. And while we were really surprised, our statistical analyses of the data confirmed what we clearly saw," said Shara.
“We are witnessing an intriguing but puzzling phenomenon,” commented Chiara Circosta, a European Space Agency Research Fellow, who studies the impact that accreting supermassive blackholes have on the galaxies hosting them in the distant Universe. “I was very surprised by this discovery. Such detailed observations of nearby galaxies are precious to expand our understanding of how jets interact with their host galaxies and potentially affect star formation”
This accomplishment is entirely due to Hubble's unique capabilities. Ground-based telescope images do not have the clarity to see novae deep inside M87. They cannot resolve stars or stellar eruptions close to the galaxy's core because the black hole's surroundings are far too bright. Only Hubble can detect novae against the bright M87 background.
Novae are remarkably common in the Universe. One nova erupts somewhere in M87 every day. Moreover, since there are at least 100 billion galaxies throughout the visible universe, around one million novae erupt every second somewhere out there.
Image Credit: NASA, ESA, J. Olmsted (STScI)
Release Date: Sept. 26, 2024
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