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黑洞可以很“温柔”?银河系中心黑洞首张照片发布

CGTN 2022-05-17


北京时间12日晚9时许,包括中国在内的全球多地天文学家同步公布了这个超大质量黑洞—人马座 A* (Sgr A*)的照片。相关研究成果以特刊形式发表在《天体物理学杂志通讯》上。
这是人类“看见”的第二个黑洞,也是银河系中心超大质量黑洞真实存在的首个直接视觉证据。这个超大质量黑洞距离太阳系约2.7万光年,质量超过太阳质量的400万倍。
这张银河系中心黑洞的照片,与人类看到的第一张黑洞照片拍摄者和拍摄时间均相同,都是由“事件视界望远镜”(EHT)合作组织,2017年通过分布在地球上8个射电望远镜组成的、一个等效于地球般口径大小的“虚拟望远镜”所拍摄。


EHT的科学家们对这个黑洞表示了喜爱,并称它比他们在过去十年模拟环境时所希望的“更温和、更合作”。


美国亚利桑那大学的欧泽尔在新闻发布会上表示,这个黑洞是“我们银河系中心的‘温柔巨人’”。

Astronomers presented the first image of the black hole at the center of our Milky Way galaxy for the first time on Thursday.


The image is a supermassive black hole that devours any matter within its huge gravitational pull but is currently on a bit of a diet.


The black hole – called Sagittarius A*, or Sgr A* – is only the second one ever to be imaged. The feat was accomplished by the same Event Horizon Telescope (EHT) international collaboration that in 2019 unveiled the first-ever photo of a black hole residing at the heart of a different galaxy.


The EHT collaboration revealed the blurry image at a press conference, saying that the black hole is "gentler, more cooperative" than they had hoped.


University of Arizona astronomer Feryal Özel, at a news conference in Washington, hailed "the first direct image of the gentle giant in the center of our galaxy," showing a glowing ring of red, yellow and white surrounding a darker center.


Sagittarius A* (pronounced Sagittarius "A" star) possesses 4 million times the mass of our sun and is located about 26,000 light years – the distance light travels in a year, 9.5 trillion km – from Earth.


Harvard-Smithsonian Center for Astrophysics astrophysicist Michael Johnson called Sagittarius A* "ravenous but inefficient," currently eating relatively little matter.


"If Sgr A* were a person, it would consume a single grain of rice every million years," Johnson said. It is putting out only a few hundred times the energy of the sun despite being much more massive.


Black holes are extraordinarily dense objects with gravity so strong that not even light can escape, making viewing them extremely challenging. A black hole's event horizon is the point of no return beyond which anything – stars, planets, gas, dust and all forms of electromagnetic radiation – gets dragged into oblivion.


The image was obtained using the EHT's global network of observatories working collectively to observe radio sources associated with black holes. It showed a ring of light – super-heated disrupted matter and radiation circling at tremendous speed at the edge of the event horizon – around a region of darkness representing the actual black hole. This is called the black hole's shadow or silhouette.


Imaging it was complicated by its dynamic environment including swirling gas around it – as Özel put it: "a source that burbled and gurgled as we looked at it."

"We love our black hole," Özel said.


The Milky Way is a spiral galaxy that contains at least 100 billion stars. Viewed from above or below it resembles a spinning pinwheel, with our sun situated on one of the spiral arms and Sagittarius A* located at the center. 

'Just trickling in'


Scientists are trying to better understand how supermassive black holes form early in a galaxy's history and evolve over time.


"They go through periods where there is a lot of material around them," Özel said. "... And then they go through these quiescent phases like the one at the center of our galaxy where matter is just trickling in."


The image released in 2019 showed the supermassive black hole in a galaxy called Messier 87, or M87. That one was far more distant and massive than Sagittarius A*, situated about 54 million light-years from Earth with a mass 6.5 billion times that of our sun.


Sagittarius A*, despite being much closer to our solar system than M87, was harder to image. The diameter of Sagittarius A* is about 17 times that of the sun, meaning it would sit within the innermost planet Mercury's solar orbit. In contrast, M87's diameter would encompass the entirety of our solar system.


Harvard-Smithsonian Center for Astrophysics radio astronomer Lindy Blackburn said that "the smaller physical size of Sgr A* also means that everything changes about a thousand times faster for Sgr A* than M87. We must also peer through the messy disk of our own galaxy to view Sgr A*, which blurs and distorts the image."


Johnson said both black hole images appear blurry because obtaining them pushed the capability of the telescopes "to the breaking point." MIT Haystack Observatory astronomer Vincent Fish said the researchers hope to obtain M87 black hole video in the future.


Thursday's announcement was made in news conferences at seven sites worldwide. EHT Project Director Huib Jan van Langevelde in Germany voiced excitement over finally unmasking the enigma that had been Sagittarius A*.


"I think it's just super exciting," said Caltech computer scientist Katie Bouman. "What's more cool than seeing the black hole at the center of our own Milky Way?"



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