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German astronomers track stars orbiting Milky Way black hole


The central parts of our Galaxy, the Milky Way, as observed in the near-infrared with the NACO instrument on ESO's Very Large Telescope. By following the motions of the most central stars over more than 16 years, astronomers were able to determine the mass of the supermassive black hole that lurks there.

MUNICH (BNS): A team of German astronomers have unravelled the mysteries surrounding the Milky Way Galaxy's heart, a super massive black hole known as Sagittarius A*, by mapping the orbits of almost 28 stars, a five-fold increase over previous studies.


In a period spanning 16 years studying the motions of the stars orbiting the Milky Way black hole, the astronomers have revealed information about the enigmatic formation of these stars and the black hole to which they are bound. One of the stars has now completed a full orbit, according to an ESO release.

Reinhard Genzel, leader of the team from the Max-Planck-Institute for Extraterrestrial Physics in Garching near Munich said that the centre of the Galaxy is a unique laboratory where one can study the fundamental processes of strong gravity, stellar dynamics and star formation that are of great relevance to all other galactic nuclei, with a level of detail that will never be possible beyond the Galaxy.

Explaining about the discovery, he said that the interstellar dust that fills the Galaxy blocks the direct view of the Milky Way's central region in visible light. To study the region, the astronomers used infrared wavelengths that could penetrate the dust to probe the region. One of the study's author, Stefan Gillessen said the Galactic Centre harbours the closest super massive black hole known, which is the best place to experiment.

The astronomers said they used the central stars as 'test particles' by watching how they move around Sagittarius A*. "Just as leaves caught in a wintry gust reveal a complex web of air currents, so does tracking the central stars show the nexus of forces at work at the Galactic Centre. These observations can then be used to infer important properties of the black hole itself, such as its mass and distance.

The new study also showed that at least 95 per cent of the mass sensed by the stars has to be in the black hole. ''There is thus little room left for other dark matter," they said.

"Undoubtedly the most spectacular aspect of the long term study is that it has delivered what is now considered to be the best empirical evidence that super massive black holes do really exist. The stellar orbits in the Galactic Centre show that the central mass concentration of four million solar masses must be a black hole, beyond any reasonable doubt," said Genzel.

The observations also allow astronomers to pinpoint the distance to the centre of the Galaxy with great precision, which is now measured to be 27,000 light-years.

Max-Planck-Institute astronomer said the ESO still had much to look forward to. "For future studies in the immediate vicinity of the black hole, we need higher angular resolution than is presently possible," Genzel said.

According to Frank Eisenhauer, principal investigator of the next generation instrument GRAVITY, ESO will soon be able to obtain that much needed resolution. "The next major advance will be to combine the light from the four 8.2-metre VLT unit telescopes a technique known as inter-ferometry. This will improve the accuracy of the observations by a factor 10 to 100 over what is currently possible. This combination has the potential to directly test Einstein's general relativity in the presently unexplored region close to a black hole."

The ESO said that to build this unparalleled picture of the Milky Way's heart and calculate the orbits of the individual stars, the team had to study the stars there for many years. "These latest groundbreaking results therefore represent 16 years of dedicated work, which started with observations made in 1992 with the SHARP camera attached to ESO's 3.5-metre New Technology Telescope located at the La Silla observatory in Chile. More observations have subsequently been made since 2002 using two instruments mounted on ESO's 8.2 m Very Large Telescope (VLT). A total of roughly 50 nights of observing time with ESO telescopes, over the 16 years, has been used to complete this incredible set of observations.''

The new work improved the accuracy by which the astronomers can measure the positions of the stars by a factor of six compared to previous studies. The final precision is 300 microarcseconds, equivalent at seeing a one euro coin from a distance of roughly 10,000 km, the astronomers said.

For the first time the number of known stellar orbits is now large enough to look for common properties among them. The study's author said the stars in the innermost region are in random orbits, like a swarm of bees. "However, further out, six of the 28 stars orbit the black hole in a disc. In this respect, the new study has also confirmed explicitly earlier work in which the disc had been found, but only in a statistical sense. Ordered motion outside the central light-month, randomly oriented orbits inside that's how the dynamics of the young stars in the Galactic Centre are best described," Gillessen said.

Shedding more light on the study, he said that one particular star, known as S2, orbits the Milky Way's centre so fast that it completed one full revolution within the 16-year period of the study. "Observing one complete orbit of S2 has been a crucial contribution to the high accuracy reached and to understanding this region. Yet the mystery still remains as to how these young stars came to be in the orbits they are observed to be in today. They are much too young to have migrated far, but it seems even more improbable that they formed in their current orbits where the tidal forces of the black hole act. Excitingly, future observations are already being planned to test several theoretical models that try to solve this riddle," the ESO said.


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