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ОписаниеGRB 200522A (2020-48-4769).png	English: This image shows the glow from a kilonova caused by the merger of two neutron stars. The kilonova, whose peak brightness reaches up to 10,000 times that of a classical nova, appears as a bright spot (indicated by the arrow) to the upper left of the host galaxy. The merger of the neutron stars is believed to have produced a magnetar, which has an extremely powerful magnetic field. The energy from that magnetar brightened the material ejected from the explosion.
Дата	12 ноября 2020 (дата загрузки)
Источник	GRB 200522A
Автор	, , W. Fong (Northwestern University), and T. Laskar (University of Bath, UK)
Другие версии	TIF version

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This file is in the public domain because it was created by NASA and ESA. NASA Hubble material (and ESA Hubble material prior to 2009) is copyright-free and may be freely used as in the public domain without fee, on the condition that only NASA, STScI, and/or ESA is credited as the source of the material. This license does not apply if ESA material created after 2008 or source material from other organizations is in use.
The material was created for NASA by Space Telescope Science Institute under Contract NAS5-26555, or for ESA by the Hubble European Space Agency Information Centre. Copyright statement at hubblesite.org or 2008 copyright statement at spacetelescope.org. For material created by the European Space Agency on the spacetelescope.org site since 2009, use the {{ESA-Hubble}} tag.

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Автор	Space Telescope Science Institute Office of Public Outreach
Название изображения	Long ago and far across the universe, an enormous burst of gamma rays unleashed more energy in a half-second than the Sun will produce over its entire 10-billion-year lifetime. In May of this year, scientists detected the light from that flash as it finally reached Earth. They quickly trained NASA’s Hubble Space Telescope on the location to study the associated afterglow. Based on X-ray and radio observations from other observatories, the team was baffled by what they saw with Hubble — the near-infrared emission detected by Hubble was 10 times brighter than predicted.These results challenge conventional theories of what happens in the aftermath of a gamma-ray burst. One possibility is that the observations might point to the birth of a massive, highly magnetized neutron star called a magnetar.“These observations do not fit traditional explanations for short gamma-ray bursts,” said study leader Wen-fai Fong of Northwestern University in Evanston, Illinois. “Given what we know about the radio and X-rays from this blast, it just doesn’t match up. The near-infrared emission that we’re finding with Hubble is way too bright. In terms of trying to fit the puzzle pieces of this gamma-ray burst together, one puzzle piece is not fitting correctly.”Without Hubble, the gamma-ray burst (GRB) would have appeared like many other GRBs, and Fong and her team would not have known about the bizarre infrared behavior.“It’s amazing to me that after 10 years of studying the same type of phenomenon, that we can discover unprecedented behavior like this,” said Fong. “It just reveals the diversity of explosions that the universe is capable of producing, which is very exciting.”Light FantasticThe intense flashes of gamma rays from these bursts appear to come from jets of material that are moving extremely close to the speed of light. The jets do not contain a lot of mass— maybe a millionth of the mass of the Sun — but because they’re moving so fast, they release a tremendous amount of energy across all wavelengths of light. This particular gamma-ray burst was one of the rare instances in which scientists were able to detect light across the entire electromagnetic spectrum.“As the data were coming in, we were forming a picture of the mechanism that was producing the light we were seeing,” said the study’s co-investigator, Tanmoy Laskar of the University of Bath in the United Kingdom. “As we got the Hubble observations, we had to completely change our thought process, because the information that Hubble added made us realize that we had to discard our conventional thinking, and that there was a new phenomenon going on. Then we had to figure out about what that meant for the physics behind these extremely energetic explosions.”Gamma-ray bursts—the most energetic, explosive events known—live fast and die hard. They are split into two classes based on the duration of their gamma rays.If the gamma-ray emission lasts less than two seconds, it’s considered a short burst. This is thought to be caused by the merger of two neutron stars, extremely dense objects about the mass of the Sun compressed into the volume of a small city. A neutron star is so dense that on Earth, one teaspoonful would weigh a billion tons! A merger of two neutronstars is generally thought to produce a black hole.If the gamma-ray emission is greater than two seconds, then it’s called a long gamma-ray burst. This event is thought to result directly from the core collapse of a massive star. Scientists expect a supernova to accompany this longer type of burst.Neutron star mergers are very rare but are extremely important because scientists think that they are one of the main sources of heavy elements in the universe, such as gold and uranium.Along with a short gamma-ray burst, scientists expect to see a“kilonova” whose peak brightness reaches 1,000 times that of a classical nova. Kilonovae are an optical and infrared glow from the radioactive decay of these heavy elements and are unique to the merger of two neutron stars.Magnetic Monster?Fong and her team have discussed several possibilities to explain the unusual brightness that Hubble saw. While most short gamma-ray bursts probably result in a black hole, the two neutron stars that merged in this case may have combined to form a magnetar, a supermassive neutron star with a very powerful magnetic field.“You basically have these magnetic field lines that are anchored to the star that are whipping around at about a thousand times a second, and this produces a magnetized wind,” explained Laskar. “These spinning field lines extract the rotational energy of the neutron star formed in the merger,and deposit that energy into the ejecta from the blast, causing the ejecta to glow even brighter.”If the extra brightness seen by Hubble came from a magnetar, then within a period of a few years, the team expects the ejecta from the burst to produce light that shows up at radio wavelengths. Follow-up radio observations may ultimately prove that this was a magnetar, and this may explain the origin of such objects.When this short gamma-ray burst was discovered with NASA’s Neil Gehrels Swift Observatory, the team of scientists quickly enlisted other telescopes, including Hubble, the Very Large Array, the W. M. Keck Observatory, and the Las Cumbres Observatory Global Telescope (LCOGT) network to study the afterglow, kilonova, and host galaxy.“Hubble really sealed the deal in the sense that it was the only one to detect near-infrared light,” explained Fong. “Amazingly, Hubble was able to take an image only three days after the burst. You need another observation to prove that there is a fading counterpart associated with the merger, as opposed to a static source. When Hubble looked again at 16 days and 55 days, we knew we had not only nabbed the fading source, but that we had also discovered something very unusual. Hubble’s angular resolution was also key in disentangling the host galaxy from the position of the burst and to quantify the amount light coming from the merger.”NASA’s upcoming James Webb Space Telescope is particularly well-suited for this type of observation. “Webb will completely revolutionize the study of similar events,” said Edo Berger of Harvard University in Cambridge, Massachusetts, and principal investigator of the Hubble program. “With its incredible infrared sensitivity it will not only detect such
Краткое название	Kilonova
Поставщик, кто предоставил изображение	NASA, ESA, STScI, W. Fong (Northwestern)
Заголовок	NASA’s Hubble Sees Unexplained Brightness from Colossal Explosion
Источник	STScI
Условия использования	http://hubblesite.org/copyright/
Оригинальные дата и время	5 января 2020
Цветовое пространство	Некалиброванное
Версия Exif	2.31
Ширина изображения	609 пикс.
Высота изображения	609 пикс.
Глубина цвета	8 8 8
Высота	609 пикс.
Ширина	609 пикс.
Цветовая модель	RGB
Количество цветовых компонентов	3
Горизонтальное разрешение	72 точек на дюйм
Вертикальное разрешение	72 точек на дюйм
Контактная информация	outreach@stsci.edu http://hubblesite.org 3700 San Martin Drive Baltimore, MD, 21218 USA 410-338-4444
Ключевые слова	GRB 2005-22A
Дата и время оцифровки	04:38, 12 октября 2020
Программное обеспечение	Adobe Photoshop 21.2 (Macintosh)
Дата последнего изменения метаданных	05:36, 21 октября 2020
Дата и время изменения файла	04:54, 21 октября 2020
Уникальный идентификатор исходного документа	xmp.did:a5ef733a-4695-4a2f-8bfe-392ec80bf647

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