<\/div>\nOver five nights in April 2017, astronomers observed Sgr A* (pronounced \u201csadge-ay-star\u201d) in the constellation of Sagittarius with eight radio telescopes,<\/span> at six sites from Arizona to the South Pole and Spain to Hawaii.<\/p>\nPart of the EHT collaboration \u2013 a global network of synchronized radio dishes yielding an Earth-sized virtual telescope of planet-wide aperture \u2013 it was the result of decades of work involving more than 300 people and 80 institutions.<\/p>\n
Using the technique of very long baseline interferometry, the EHT offered the highest possible resolving power from the surface of Earth, capturing objects as small as 20 micro-arcseconds on the sky \u2013 that\u2019s equivalent to spying a doughnut on the Moon.<\/p>\n
The Event Horizon Telescope<\/span><\/strong><\/h2>\nThe EHT is a planet-wide network of 11 synchronized radio telescopes.<\/p>\n
A map showing the location of the various locations of the Event Horizon Telescope for the 2017 observing campaign.<\/span><\/figcaption><\/div>\n1.Atacama Large Millimeter Array (ALMA), Chile<\/p>\n
2. Atacama Pathfinder Experiment (APEX), Chile<\/p>\n
3. IRAM 30-m Telescope, Pico Veleta, Sierra Nevada, Spain<\/p>\n
4. James Clark Maxwell Telescope (JCMT), Hawaii, USA<\/p>\n
5. Submillimeter Array (SMA), Hawaii, USA<\/p>\n
6. Large Millimeter Telescope (LMT), Alfonso Serrano, Mexico<\/p>\n
7. South Pole Telescope (SPT)<\/p>\n
8. Submillimeter Telescope (SMT), Mount Graham, Arizona, USA<\/p>\n
Additional telescopes since 2017:\u00a0<\/span><\/strong><\/h3>\n9. IRAM NOEMA Telescope, French Alps<\/p>\n
10. Greenland Telescope (GLT)<\/p>\n
11. University of Arizona 12-meter Telescope, Kitt Peak, Arizona, USA<\/p>\n
Sagittarius A* vs the M87 black hole<\/strong><\/h2>\n To illustrate the huge difference in size between the two imaged\u00a0black holes, M87* is approximately 25,000 AU across, whereas Pluto orbits the Sun at an average of 39 AU\u2026<\/span><\/figcaption><\/div>\nDr Ziri Younsi from University College London is co-lead of the Fundamental Physics working group on the next generation EHT (ngEHT).<\/p>\n
He affirmed it was, \u201ca very challenging task compared to imaging M87* located 53 million lightyears away.\u201d<\/p>\n
Though Sgr A* is much closer than that, it is comparatively tiny, with a mass of four million Suns crammed into a region smaller than Mercury\u2019s orbit \u2013 1,500 times smaller than M87*, a behemoth weighing in at 6.5 billion Suns.<\/p>\n
For size comparison, if M87* was the size of Wembley Stadium, then Sgr A* would be a burger at the concession stand.\u00a0<\/span><\/p>\n \u2026this means it dwarfs our own galaxy\u2019s black hole which is a tiny spec in comparison at 32.2 million miles in diameter, or about one third of an AU, not far from the 29-million-mile orbit of Mercury<\/span><\/figcaption><\/div>\nThe challenge of trying to \u2018see\u2019 a black hole<\/strong><\/h2>\n\u201cGas circling Sgr A* and M87* moves at the same speed \u2013 almost the speed of light \u2013 but it circuits Sgr A* in a few minutes compared to M87*\u2019s days,\u201d says Younsi.<\/p>\n
\u201cObserving Sgr A*\u2019s turbulent gas flow, minute-by-minute, created \u2018motion blur\u2019. Moreover, we were looking through the entire Galactic plane stuffed with stars, gas and dust, all rapidly-changing over different timescales.\u201d<\/p>\n
\u201cThis created a screen of scattered radio waves. Trying to see Sgr A* was like standing in your garden in a rainstorm peering through a steamed-up kitchen window watching your frantic puppy \u2013 our supermassive black hole \u2013 careering around in circles chasing its tail.<\/p>\n
\u201cBy comparison, M87* is a puppy napping on a sunlit patio.\u201d<\/span><\/p>\nHow the Milky Way\u2019s black hole image was captured<\/strong><\/h2>\n The EHT Collaboration created a series of possible images of Sgr A* using ray-tracing based on Einstein\u2019s Theory of General Relativity. Credit: EHT collaboration<\/span><\/figcaption><\/div>\nIt has taken five years for the EHT team to figure it all out. It was a daunting task: collaboration members split into multiple teams, each using independent methods to reconstruct an image from the data.<\/p>\n
The result was uncertain; many images revealed a ring, but not all.<\/p>\n
To solve this dilemma, scientists used some of the most sophisticated computer algorithms ever written to simulate different images, and then used these to test what results their various image reconstruction methods would give.<\/p>\n
Eventually they were certain they had detected a ring, and what a spectacular, ground-breaking result! \u00a0<\/span><\/p>\nEHT\u2019s vision \u2013 three million times sharper than the human eye \u2013 revealed Sgr A* is strikingly similar in its overall morphology to M87*.<\/span><\/p>\nThere is a bright fuzzy ring of light \u2013 radio emission from electrons in the <\/span>gas swishing around the black hole \u2013 encircling a dark centre.<\/p>\nThis dark core is where the light, captured by immense gravity, has plunged past the event horizon never to be seen again, but leaving a \u2018shadow\u2019 of the black hole\u2019s presence.<\/p>\n
Sgr A*\u2019s appetite compared to M87* is surprisingly slow; it is effectively starving, surviving on whispers of gas from the winds of nearby stars \u2013 comparable to a human swallowing one grain of rice every million years.<\/p>\n
The infalling gas emits just a few hundred times as much energy as our Sun, so at a cosmically \u2018close\u2019 27,000 lightyears, Sgr A* cannot be considered bright.\u00a0<\/span><\/p>\nWhat can we learn from a black hole image?<\/strong><\/h2>\n Credit: EHT Collaboration<\/span><\/figcaption><\/div>\nThe measurement also allowed astronomers to measure the size of Sgr A*\u2019s event horizon, which according to Einstein\u2019s theory of gravity should be directly related to its mass.<\/p>\n
The EHT measured Sgr A*\u2019s event horizon spanning around 51.8 micro-arcseconds, precisely as the theory predicted.\u00a0<\/span><\/p>\nBut there are still several mysteries our black hole might be hiding.<\/p>\n
Sgr A* lies on its side so that we look down at its head, and it is spinning counter-clockwise at a yet to be determined rate in the same direction as its orbiting gas.<\/p>\n
This orientation may hide a relativistic jet. And the bright knots dotting the ring?<\/p>\n
These could be areas rich in gas, or artifacts from the observation process \u2013 it will take more work yet to determine what these mean.<\/p>\n
In fact, producing the image is just the start. Subsequent observing campaigns have generated data that also requires analysing.<\/p>\n
This artist\u2019s concept shows a black hole with an accretion disc expelling a jet of hot gas, called plasma.<\/div>\nMore dishes are being added to the telescope between now and 2030 to create the ngEHT.<\/p>\n
This will expand the current 230 GHz radio frequency to 345 GHz, improving image resolution by 50%.<\/p>\n
Movies will showcase how black hole silhouettes change over time, the \u2018slower\u2019 M87* offering a possible \u2018world premier\u2019.<\/p>\n
Who knows? Within a decade we may enjoy videos of Sgr A* in action.\u00a0<\/span><\/p>\nAs Dr Younsi so eloquently stated, \u201cblack holes play a fundamental role in the genesis of the Universe, our Galaxy and every other galaxy.<\/p>\n
\u201cThey are the bedrock, the gravitational anchors holding everything together so it\u2019s remarkable that we can actually see them now\u201d.<\/p>\n
Remarkable indeed, and so much more science is still to come!<\/p>\n
How interferometry works<\/strong><\/h2>\n Staff at the Max Planck Institute for Radio Astronomy evaluate data from the EHT. Credit: MPIfR.<\/span><\/figcaption><\/div>\nThe technique of very long baseline interferometry combines data from pairs of\u00a0EHT telescopes to reveal both\u00a0the small- and large-scale structure of the target.\u00a0<\/span><\/span><\/p>\nThe varying distances between the telescopes \u2013 known as the baseline \u2013 means they receive the signal from the black hole at slightly different times, which can be measured using very accurate clocks.<\/span><\/p>\nAs the planet turns, each telescope\u2019s view of the Galactic centre changes, as do the dishes\u2019 apparent separations as seen from the black hole.<\/span><\/p>\nSuch changes help \u2018fill in\u2019 the virtual antenna. To compile the image, a variety of baselines are needed, and the more the merrier.\u00a0<\/span><\/span><\/p>\nThe enormous volume of raw recorded data (3.5 petabytes, equivalent to 750,000 DVDs) from each EHT site is stored on high-performance helium-filled hard drives and transported by commercial freight aircraft to highly specialised supercomputers known as correlators at the Max Planck Institute for Radio Astronomy (MPIfRI) in Bonn, Germany and the Massachusetts Institute of Technology\u2019s (MIT) Haystack Observatory in Massachusetts, USA, where it is combined and calibrated to within trillionths of a second.<\/span><\/p>\nThis article originally appeared in the July 2022 issue of <\/strong><\/em>BBC Sky at Night Magazine<\/strong>.<\/strong><\/em><\/p><\/body><\/html>\nBy Jane Green Published: Wednesday, 17 August 2022 at 12:00 am On 12 May 2022 at 13:07 UT, the first ever direct visual image of our closest supermassive black hole was unveiled by the Event Horizon Telescope (EHT) team. It was a thrilling, profound moment. Though not the first black hole picture presented by the […]<\/p>\n","protected":false},"author":24,"featured_media":35887,"template":"","categories":[1],"acf":{"readingTimeMinutes":"8"},"uagb_featured_image_src":{"full":["https:\/\/c01.purpledshub.com\/uploads\/sites\/77\/2022\/08\/how-astronomers-photographed-the-milky-ways-central-black-hole.jpg",1500,1203,false],"thumbnail":["https:\/\/c01.purpledshub.com\/uploads\/sites\/77\/2022\/08\/how-astronomers-photographed-the-milky-ways-central-black-hole-150x150.jpg",150,150,true],"medium":["https:\/\/c01.purpledshub.com\/uploads\/sites\/77\/2022\/08\/how-astronomers-photographed-the-milky-ways-central-black-hole-300x241.jpg",300,241,true],"medium_large":["https:\/\/c01.purpledshub.com\/uploads\/sites\/77\/2022\/08\/how-astronomers-photographed-the-milky-ways-central-black-hole-768x616.jpg",768,616,true],"large":["https:\/\/c01.purpledshub.com\/uploads\/sites\/77\/2022\/08\/how-astronomers-photographed-the-milky-ways-central-black-hole-1024x821.jpg",800,641,true],"1536x1536":["https:\/\/c01.purpledshub.com\/uploads\/sites\/77\/2022\/08\/how-astronomers-photographed-the-milky-ways-central-black-hole.jpg",1500,1203,false],"2048x2048":["https:\/\/c01.purpledshub.com\/uploads\/sites\/77\/2022\/08\/how-astronomers-photographed-the-milky-ways-central-black-hole.jpg",1500,1203,false]},"uagb_author_info":{"display_name":"importmanagerhub@sprylab.com","author_link":"https:\/\/c01.purpledshub.com\/bbcskyatnight\/author\/importmanagerhubsprylab-com\/"},"uagb_comment_info":0,"uagb_excerpt":"By Jane Green Published: Wednesday, 17 August 2022 at 12:00 am On 12 May 2022 at 13:07 UT, the first ever direct visual image of our closest supermassive black hole was unveiled by the Event Horizon Telescope (EHT) team. It was a thrilling, profound moment. Though not the first black hole picture presented by the…","_links":{"self":[{"href":"https:\/\/c01.purpledshub.com\/bbcskyatnight\/wp-json\/wp\/v2\/rss_feed\/35886"}],"collection":[{"href":"https:\/\/c01.purpledshub.com\/bbcskyatnight\/wp-json\/wp\/v2\/rss_feed"}],"about":[{"href":"https:\/\/c01.purpledshub.com\/bbcskyatnight\/wp-json\/wp\/v2\/types\/rss_feed"}],"author":[{"embeddable":true,"href":"https:\/\/c01.purpledshub.com\/bbcskyatnight\/wp-json\/wp\/v2\/users\/24"}],"wp:featuredmedia":[{"embeddable":true,"href":"https:\/\/c01.purpledshub.com\/bbcskyatnight\/wp-json\/wp\/v2\/media\/35887"}],"wp:attachment":[{"href":"https:\/\/c01.purpledshub.com\/bbcskyatnight\/wp-json\/wp\/v2\/media?parent=35886"}],"wp:term":[{"taxonomy":"category","embeddable":true,"href":"https:\/\/c01.purpledshub.com\/bbcskyatnight\/wp-json\/wp\/v2\/categories?post=35886"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}
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