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Paris, July, 26, 2018

GRAVITY confirms predictions of general relativity near the Galactic Centre Massive Black Hole

Observations made with the Very Large Telescope (VLT) of the European Southern Observatory (ESO) have, for the first time, detected the effects of general relativity predicted by Einstein, in the movement of a star passing into the intense gravitational field of Sagittarius A*, a massive black hole at the centre of the Milky Way. These results were obtained by the GRAVITY consortium1, led by the Max Planck Institute for Extraterrestrial Physics (MPE) in Germany and also involving the CNRS, the Paris Observatory (PSL), the Université Grenoble-Alpes and several French universities. These findings, the culmination of 26 years of observations using telescopes at the ESO in Chile, were published by the GRAVITY consortium on 26 July 2018 in Astronomy & Astrophysics.

Sagittarius A* (Sgr A*) sits at the centre of our galaxy, 26,000 light-years from Earth. This black hole, which has a mass 4 million times that of the sun, is surrounded by a star cluster – the S stars – which reach mind-boggling speeds when they approach the hole. General relativity describes the effects of matter on the movement of stars, and more specifically, in this case, the effects of a black hole on the stars surrounding it. The stars of Sgr A*, located in the Milky Way's most powerful gravitational field, are a perfect laboratory in which to test Einstein's general theory of relativity.

Astronomers used three VLTs – NACO, SINFONI, and more recently GRAVITY – to follow one particular star in the Sgr A* system – S2 – before and after it passed close to the black hole on 19 May 2018. GRAVITY achieved a resolution of 50 microarcseconds: the angle at which a tennis ball placed on the moon would be visible from Earth. This accuracy made it possible to detect the hour-by-hour movement of S2 as close as possible to the black hole. When S2 passed by Sgr A* at a distance just 120 times that of the Earth from the Sun, it reached an orbital velocity of 8000 km/s: 2.7 % of the speed of light. These extreme conditions suffice for the S2 star to be subjected to the effects of general relativity.

By combining previous measurements made using NACO and SINFONI with GRAVITY's precision on the position of S2, astronomers were able to detect the gravitational redshift which Einstein predicted. Redshift affects light sources that are in a gravitational field; in this case, the black hole. The phenomenon produces a shift in wavelength toward the red part of the spectrum which is detected by a measuring instrument. This is the first time the effect has been measured in the gravitational field of a black hole.

These results are perfectly in line with the theory of general relativity (and not explained by Newton's theory, which excludes such a shift). They are a major breakthrough towards better understanding the effects of intense gravitational fields. Shifts in the trajectory of S2 due to gravity will be detected in a few months, and could yield information on mass distribution around the black hole.

 

sgr A*

© Paris Observatory / LESIA

Centre: Sagittarius A* and its star cluster


 

 

Download the press release : CP Gravity Anglais

Notes:

1GRAVITY is a second-generation VLT interferometer (VLTI) developed by the GRAVITY consortium:
- Max Planck Institute for Extraterrestrial Physics (MPE) in Garching, Germany
- Laboratory for Space Science and Astrophysical Instrumentation (LESIA) of the Paris Observatory – PSL/CNRS/Sorbonne Université/Université Paris Diderot
- Institut de Planétologie et d'Astrophysique de Grenoble (IPAG, Université Grenoble Alpes/CNRS)
- Max Planck Institute for Astronomy (MPIA) in Heidelberg, Germany
- University of Cologne (Germany)
- Centro Multidisciplinar de Astrofísica (CENTRA), Lisbon and Porto, Portugal
- European Southern Observatory (ESO), Garching, Germany

Bibliography:

“Detection of the Gravitational Redshift in the Orbit of the Star S2 near the Galactic Centre Massive Black Hole”, GRAVITY Collaboration, Astronomy & Astrophysics, July 2018. DOI: 10.1051/0004-6361/201833718

Contacts:

CNRS researchers

Guy Perrin, researcher Observatoire de Paris l guy.perrin@obspm.fr l T +33(0)1 45 07 79 63

Karine Perraut, researcher Observatoire des sciences de l'Univers de Grenoble l karine.perraut@univ-grenoble-alpes.fr l T +33(0)4 76 63 55 15

Thibaut Paumard, CNRS Researcher l T +33(0)1 45 07 75 45 l thibaut.paumard@obspm.fr

Press

CNRS Press l Juliette Dunglas l T +33(0)1 44 96 51 51 l T +33(0)1 44 96 46 34 l juliette.dunglas@cnrs.fr


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