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Following up on the first image of a supermassive black hole

Following up on the first image of a supermassive black hole

2025-01-23

Taiwan-based researchers in the Event Horizon Telescope Collaboration project on Thursday held a press conference highlighting their latest results. There are more than 400 astrophysicists worldwide participating in this international research project, observing two galactic center black holes. The focus of the Taiwanese researchers is the supper massive black hole at the center of the Messier 87 galaxy, known as M87. Let’s hear more.

Britton Harold Jeter
Academia Sinica postdoctoral fellow
In this case, the diameter corresponds to the mass of this black hole of six and a half billion suns. The asymmetry in brightness, that is, being bright at the bottom of the ring and dim at the top, comes from a combination of effects, from both the spin of the black hole, the rotation of the accretion flow, and effects from strong gravitational lensing and Doppler beaming, leading to one side being brighter than the other.

Pu Hung-yi
National Taiwan Normal University assistant professor
The clearer the image of a black hole, the deeper we get to understand the spacetime of a black hole and the surrounding spacetime. Each black hole behaves differently. For example, some have jets, while others don’t. The direction of jets and the speed of black hole spins are all related to the evolution of the universe, how a black hole affects its surroundings, and even the evolution of a galaxy.

The press conference at Academia Sinica explains the main findings of a recent publication in the latest volume of “Astronomy & Astrophysics,” a leading academic journal. A total of 180,000 simulation images were analyzed, 120,000 more than a previous research that resulted in the very first image of a black hole in 2019. The researchers found that their observation of rotating gas around the M87’s black hole could help scientists better understand the dynamics of black hole environments.

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M87黑洞新影像曝光!歷經7年研究有重大突破

2025-01-23

台師大與中研院天文所,參與的EHT「事件視界望遠鏡」團隊,今天公布18萬張M87黑洞的最新影像,這項研究證實,透過吸積盤中的湍流,解釋2017年與2018年黑洞偏移。

[[中研院天文所博後 紀柏特]]
“這個明亮的這個光圈的結構的大小,我們可以推算出這個黑洞,大概是有65億個太陽質量這麼重,周圍的這些光線它有個亮度不對稱的現象,那是因為在黑洞周圍,以高溫運行的物質所放出來的輻射,它受到黑洞的重力效應,以及都卜勒效應影響所造成的”

[[台師大物理系助理教授 卜宏毅]]
“把黑洞的影像看得更清晰的話,那我們可以對黑洞的時空,周圍的時空有更深入的了解,不同的黑洞它有不同的表現,譬如說有的黑洞有噴流,有的沒有,那它的噴流的方向會是什麼,或者是這些黑洞的轉速是什麼,那這些其實都跟宇宙的演化,還有黑洞怎麼影響周圍,甚至星系的演化相關”

今天公布18萬張M87黑洞的最新影像,這項研究證實,透過吸積盤中的湍流,解釋2017年與2018年黑洞偏移。透過18萬張黑洞影像分析,驗證黑洞光環與2017年所觀測的大小相同,符合廣義相對論的預測,而環的最亮處位置明顯偏轉,與理論預測黑洞周圍紊流的變異性一致。研究成果也發表於"天文與天文物理"國際期刊。

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