태양계는 10,000년에 감마선 1번 폭발하는 강력한 방사선 펄스에 맞았습니다.

감마선 폭발은 우주에서 가장 밝은 폭발입니다. 천문학자들은 이 애니메이션에서 볼 수 있듯이 거대한 별의 핵이 핵연료를 다 써버리고 자중으로 붕괴하여 블랙홀을 형성할 때 대부분이 일어난다고 생각합니다. 그런 다음 블랙홀은 거의 빛의 속도로 붕괴하는 별을 파고드는 입자 폭발을 일으킵니다. 이 제트는 별을 뚫고 우주를 통해 흐르면서 X선과 감마선(자주색)을 방출합니다. 그런 다음 불운한 별을 둘러싼 물질에 파고들어 점차 사라지는 다중 파장 배경 광선을 생성합니다. 이 평면 중 하나를 가까이서 볼수록 더 밝게 나타납니다. 크레딧: NASA의 고다드 우주 비행 센터

2022년 10월 9일 일요일, 유난히 강렬한 복사의 맥박이 천문학자들이 역사상 가장 밝은 BOAT라고 명명한 태양계를 휩쓸었습니다.

그 원인은 우주에서 가장 강력한 종류의 폭발인 감마선 폭발(GRB)이었습니다.

폭발은 많은 우주선의 감지기를 작동시켰고 전 세계의 관측소가 뒤따랐습니다. 이 모든 데이터를 샅샅이 조사한 후 천문학자들은 이제 그것이 얼마나 밝은지 결정하고 과학적 영향을 더 잘 이해할 수 있습니다.

허블 우주 망원경의 광시야 카메라 3은 BOAT GRB와 그 모은하의 적외선 빛(동그라미)을 감지했으며 거의 ​​가장자리에서 폭발의 오른쪽 상단까지 뻗어 있는 빛의 은색으로 보입니다. 이 합성 사진에는 분화 후 1개월과 2개월 후인 2022년 11월 8일과 12월 4일에 촬영된 이미지가 포함되어 있습니다. 밝기 때문에 잔광은 몇 년 동안 망원경으로 감지할 수 있습니다. 이 이미지는 1~1.5미크론의 파장에서 매일 촬영한 3개의 근적외선 이미지를 결합합니다. 이미지 제공: NASA, ESA, CSA, STScI, A. Levan(Radboud University); 이미지 처리: Gladys Cooper

“GRB 221009A는 인류 문명이 시작된 이래 발생한 X선 및 감마선 에너지의 가장 밝은 폭발일 가능성이 높습니다. 그는 약 7,000개의 GRB에 대한 분석을 이끌었습니다. 그 중 대부분은 NASA의 Fermi 감마선 우주 망원경과 러시아의 지구상 Konus 장비에 의해 발견되었습니다.[{” attribute=””>NASA’s Wind spacecraft – to establish how frequently events this bright may occur. Their answer: once in every 10,000 years.

The burst was so bright it effectively blinded most gamma-ray instruments in space, which means they could not directly record the real intensity of the emission. U.S. scientists were able to reconstruct this information from the Fermi data. They then compared the results with those from the Russian team working on Konus data and Chinese teams analyzing observations from the GECAM-C detector on their SATech-01 satellite and instruments on their Insight-HXMT observatory. Together, they prove the burst was 70 times brighter than any yet seen.

감마선 폭발은 우주에서 가장 밝은 폭발입니다. 천문학자들은 대부분 무거운 별의 핵이 핵연료가 고갈되고 자체 중량으로 붕괴되어 형태가 형성될 때 발생한다고 생각합니다.[{” attribute=””>black hole, as illustrated in this animation. The black hole then drives jets of particles that drill all the way through the collapsing star at nearly the speed of light. These jets pierce through the star, emitting X-rays and gamma rays (magenta) as they stream into space. They then plow into material surrounding the doomed star and produce a multiwavelength afterglow that gradually fades away. The closer to head-on we view one of these jets, the brighter it appears. Credit: NASA’s Goddard Space Flight Center

Burns and other scientists presented new findings about the BOAT at the High Energy Astrophysics Division meeting of the American Astronomical Society in Waikoloa, Hawaii. Observations of the burst span the spectrum, from radio waves to gamma rays, and include data from many NASA and partner missions, including the NICER X-ray telescope on the International Space Station, NASA’s NuSTAR observatory, and even Voyager 1 in interstellar space. Papers describing the results presented appear in a focus issue of The Astrophysical Journal Letters.

The signal from GRB 221009A had been traveling for about 1.9 billion years before it reached Earth, making it among the closest-known “long” GRBs, whose initial, or prompt, emission lasts more than two seconds. Astronomers think these bursts represent the birth cries of black holes formed when the cores of massive stars collapse under their own weight. As it quickly ingests the surrounding matter, the black hole blasts out jets in opposite directions containing particles accelerated to near the speed of light. These jets pierce through the star, emitting X-rays and gamma rays as they stream into space.

This chart compares the BOAT’s prompt emission to that of five previous record-holding long gamma-ray bursts. The BOAT was so bright it effectively blinded most gamma-ray instruments in space, but U.S. scientists were able to reconstruct its true brightness from Fermi data. Credit: NASA’s Goddard Space Flight Center and Adam Goldstein (USRA)

With this type of GRB, astronomers expect to find a brightening supernova a few weeks later, but so far it has proven elusive. One reason is that the GRB appeared in a part of the sky that’s just a few degrees above the plane of our own galaxy, where thick dust clouds can greatly dim incoming light.

“We cannot say conclusively that there is a supernova, which is surprising given the burst’s brightness,” said Andrew Levan, a professor of astrophysics at Radboud University in Nijmegen, Netherlands. Since dust clouds become more transparent at infrared wavelengths, Levan led near- and mid-infrared observations using NASA’s James Webb Space Telescope – its first use for this kind of study – as well as the Hubble Space Telescope to spot the supernova. “If it’s there, it’s very faint. We plan to keep looking,” he added, “but it’s possible the entire star collapsed straight into the black hole instead of exploding.” Additional Webb and Hubble observations are planned over the next few months.

As the jets continue to expand into material surrounding the doomed star, they produce a multiwavelength afterglow that gradually fades away.

This illustration shows the ingredients of a long gamma-ray burst, the most common type. The core of a massive star (left) has collapsed, forming a black hole that sends a jet of particles moving through the collapsing star and out into space at nearly the speed of light. Radiation across the spectrum arises from hot ionized gas (plasma) in the vicinity of the newborn black hole, collisions among shells of fast-moving gas within the jet (internal shock waves), and from the leading edge of the jet as it sweeps up and interacts with its surroundings (external shock). Credit: NASA’s Goddard Space Flight Center

“Being so close and so bright, this burst offered us an unprecedented opportunity to gather observations of the afterglow across the electromagnetic spectrum and to test how well our models reflect what’s really happening in GRB jets,” said Kate Alexander, an assistant professor in the department of astronomy at the University of Arizona in Tucson. “Twenty-five years of afterglow models that have worked very well cannot completely explain this jet,” she said. “In particular, we found a new radio component we don’t fully understand. This may indicate additional structure within the jet or suggest the need to revise our models of how GRB jets interact with their surroundings.”

The jets themselves were not unusually powerful, but they were exceptionally narrow – much like the jet setting of a garden hose – and one was pointed directly at us, Alexander explained. The closer to head-on we view a jet, the brighter it appears. Although the afterglow was unexpectedly dim at radio energies, it’s likely that GRB 221009A will remain detectable for years, providing a novel opportunity to track the full life cycle of a powerful jet.

XMM-Newton images recorded 20 dust rings, 19 of which are shown here in arbitrary colors. This composite merges observations made two and five days after GRB 221009A erupted. Dark stripes indicate gaps between the detectors. A detailed analysis shows that the widest ring visible here, comparable to the apparent size of a full moon, came from dust clouds located about 1,300 light-years away. The innermost ring arose from dust at a distance of 61,000 light-years – on the other side of our galaxy. GRB221009A is only the seventh gamma-ray burst to display X-ray rings, and it triples the number previously seen around one. Credit: ESA/XMM-Newton/M. Rigoselli (INAF)

The burst also enabled astronomers to probe distant dust clouds in our own galaxy. As the prompt X-rays traveled toward us, some of them reflected off of dust layers, creating extended “light echoes” of the initial blast in the form of X-ray rings expanding from the burst’s location. The X-ray Telescope on NASA’s Neil Gehrels Swift Observatory discovered the presence of a series of echoes. Detailed follow-up by ESA’s (the European Space Agency’s) XMM-Newton telescope, together with Swift data, revealed these extraordinary rings were produced by 21 distinct dust clouds.

“How dust clouds scatter X-rays depends on their distances, the sizes of the dust grains, and the X-ray energies,” explained Sergio Campana, research director at Brera Observatory and the National Institute for Astrophysics in Merate, Italy. “We were able to use the rings to reconstruct part of the burst’s prompt X-ray emission and to determine where in our galaxy the dust clouds are located.”

GRB 221009A is only the seventh gamma-ray burst to display X-ray rings, and it triples the number previously seen around one. The echoes came from dust located between 700 and 61,000 light-years away. The most distant echoes – clear on the other side of our Milky Way galaxy – were also 4,600 light-years above the galaxy’s central plane, where the solar system resides.

Lastly, the burst offers an opportunity to explore a big cosmic question. “We think of black holes as all-consuming things, but do they also return power back to the universe?” asked Michela Negro, an astrophysicist at the University of Maryland, Baltimore County, and NASA’s Goddard Space Flight Center in Greenbelt.

Her team was able to probe the dust rings with NASA’s Imaging X-ray Polarimetry Explorer to glimpse how the prompt emission was organized, which can give insights into how the jets form. In addition, a small degree of polarization observed in the afterglow phase confirms that we viewed the jet almost directly head-on.

Together with similar measurements now being studied by a team using data from ESA’s INTEGRAL observatory, scientists say it may be possible to prove that the BOAT’s jets were powered by tapping into the energy of a magnetic field amplified by the black hole’s spin. Predictions based on such models have already successfully explained other aspects of this burst.

References:

“Focus on the Ultra-luminous Gamma-Ray Burst GRB 221009A” March 2023, The Astrophysical Journal Letters.