Global Gaia campaign reveals secrets of stellar pair
2020-01-21
Information from the Astronomical Observatory of the University of Warsaw
A 500-day global observation campaign spearheaded more than three years ago by ESA’s galaxy-mapping powerhouse Gaia has provided unprecedented insights into the binary system of stars that caused an unusual brightening of an even more distant star.
The brightening of the star, located in the Cygnus constellation, was first spotted in August 2016 [MOU1] by the Gaia Photometric Science Alerts programme.
This system, maintained by the Institute of Astronomy at the University of Cambridge, UK, scans daily the huge amount of data coming from Gaia and alerts astronomers to the appearance of new sources or unusual brightness variations in known ones, so that they can quickly point other ground and space-based telescopes to study them in detail. The phenomena may include supernova explosions and other stellar outbursts.
In this particular instance, follow-up observations performed with more than 50 telescopes worldwide revealed that the source – since then named Gaia16aye after Ayers Rock, the famous landmark in Australia – was behaving in a rather strange way.
“We saw the star getting brighter and brighter and then, within one day, its brightness suddenly dropped,” says Lukasz Wyrzykowski from the Astronomical Observatory at the University of Warsaw, Poland, who is one of the scientists behind the Gaia Photometric Science Alert programme.
“This was a very unusual behaviour. Hardly any type of supernova or other star does this.”
Lukasz and collaborators soon realised that this brightening was caused by gravitational microlensing – an effect predicted by Einstein’s theory of general relativity, caused by the bending of spacetime in the vicinity of very massive objects, like stars or black holes.
When such a massive object, which may be too faint to be observed from Earth, passes in front of another, more distant source of light, its gravity bends the fabric of spacetime in its vicinity. This distorts the path of light rays coming from the background source – essentially behaving like a giant magnifying glass.
Gaia16aye is the second micro-lensing event detected by ESA’s star surveyor. However, the astronomers noticed it behaved strangely even for this type of event.
“If you have a single lens, caused by a single object, there would be just a small, steady rise in brightness and then there would be a smooth decline as the lens passes in front of the distant source and then moves away,” says Lukasz.
“In this case, not only did the star brightness drop sharply rather than smoothly, but after a couple of weeks it brightened up again, which is very unusual. Over the 500 days of observation, we have seen it brighten up and decline five times.”
This sudden and sharp drop in brightness suggested that the gravitational lens causing the brightening must consist of a binary system – a pair of stars, or other celestial objects, bound to one another by mutual gravity.
The combined gravitational fields of the two objects produce a lens with a rather intricate network of high magnification regions. When a background source passes through such regions on the plane of the sky, it lights up, and then dims immediately upon exiting it.
From the pattern of subsequent brightenings and dimmings, the astronomers were able to deduce that the binary system was rotating at a rather fast pace.
“The rotation was fast enough and the overall micro-lensing event slow enough that the background star entered the high magnification region, left it and then entered it again,” says Lukasz.
The long period of observations, which lasted until the end of 2017, and the extensive participation of ground-based telescopes from around the globe enabled the astronomers to gather a large amount of data – almost 25 000 individual data points.
In addition, the team also made use of dozens of observations of this star collected by Gaia as it kept scanning the sky over the months. These data have undergone preliminary calibration and were made public as part of the Gaia Science Alerts programme.
From this data set, Lukasz and his colleagues were able to learn a great deal of detail about the binary system of stars.
“We don’t see this binary system at all, but from only seeing the effects that it created by acting as a lens on a background star, we were able to tell everything about it,” says co-author Przemek Mróz, who was a PhD student at the University of Warsaw when the campaign started, and is currently a postdoctoral scholar at the California Institute of Technology.
“We could determine the rotational period of the system, the masses of its components, their separation, the shape of their orbits – basically everything – without seeing the light of the binary components.”
The pair consists of two rather small stars, with 0.57 and 0.36 times the mass of our Sun, respectively. Separated by roughly twice the Earth-Sun distance, the stars orbit around their mutual centre of mass in less than three years.
“If it wasn’t for Gaia scanning the whole sky and then sending the alerts straight away, we would never have known about this microlensing event,” says co-author Simon Hodgkin from the University of Cambridge, who leads the Gaia Science Alerts programme.
“Maybe we would have found it later, but then it might have been too late.”
The detailed understanding of the binary system relied on the extensive observation campaign and on the broad international involvement that the Gaia16aye event attracted.
“We acknowledge the professional astronomers, amateur astronomers and volunteers from all around the globe who have been observing this event: without the dedication of all those people we wouldn’t have been able to obtain such results,” says Lukasz.
“Microlensing events like this can shed light on celestial objects that we would otherwise not be able to see,” says Timo Prusti, Gaia Project Scientist at ESA.
“We are delighted that Gaia’s detection triggered the observation campaign that made this result possible.”
Publication:
“Full Orbital Solution for the Binary System in the Northern Galactic Disk Microlensing Event Gaia16aye” by L. Wyrzykowski et al is published in Astronomy and Astrophysics.
[DOI: 10.1051/0004-6361/201935097].
Contact:
Łukasz Wyrzykowski (pron. Woo-cash Vi-zhi-kov-ski)
Gaia Photometric Science Alerts Team
Astronomical Observatory
University of Warsaw
Al. Ujazdowskie 4
00-478 Warszawa
e-mail: lw@astrouw.edu.pl
Tel: +48 608648817
Przemek Mróz (pron. Pshe-mek Mrooz)
California Institute of Technology
Pasadena, CA, USA, USA
e-mail: pmroz@astrouw.edu.pl
Simon Hodgkin
Gaia Photometric Science Alerts Team
Institute of Astronomy
Cambridge, UK
e-mail: sth@ast.cam.ac.uk
Timo Prusti
Gaia Project Scientist
Institute of Astronomy
European Space Agency
e-mail: tprusti@cosmos.esa.int
Images:
OA200121b_fot01s.jpg, HR: https://www.fuw.edu.pl/press/images/2020/OA200121b_fot01.jpg
Artists impression on the binary system discovered in the microlensing event Gaia16aye.
It was not the light of the stars, but their mass what caused the space-time to bend in a sophisticated way. The light rays from a distant star travelled to the Gaia space mission and observers on the ground via perturbed space-time, which resulted in the lensing (magnification) of the background star.
Credit: Maciej Rębisz
OA200121b_fot02ens.png, HR:
https://www.fuw.edu.pl/press/images/2020/OA200121b_fot02en.png
Map of the sky with the localisation of the Gaia16aye event. The top figure shows the entire Northern part of the Milky Way, lower left shows the zoom-in as seen with a small telescope and on the right the view seen by a large telescope. Author: Lukasz Wyrzykowski and Mariusz Gromadzki (OAUW)
OA200121b_fot03s.png, HR: https://www.fuw.edu.pl/press/images/2020/OA200121b_fot03.png
Microlensing observation campaign spearheaded by Gaia
This graph shows the variation of brightness of the star Gaia16aye caused by a microlensing event, as a foreground massive object – a binary system of stars – passed across its line of sight. The brightness is indicated on the vertical axis in terms of the astronomical magnitude, with smaller values (towards the top) indicating higher brightness; time is indicated on the horizontal axis.
The graph shows data collected over a period of almost two years with more than 50 telescopes worldwide, as part of a global observation campaign spearheaded by ESA’s Gaia satellite. Brightness measurements obtained with Gaia are shown as large black diamond symbols, whereas ground-based observations performed with a variety of telescopes across the world are shown as smaller circles, squares, diamonds and triangles of different colours.
The first detection of the source’s sudden brightening, made by Gaia in August 2016, is marked with a red arrow. The detection was made as part of the Gaia Photometric Science Alerts programme, a system that scans daily the huge amount of data coming from Gaia and alerts astronomers to the appearance of new sources or unusual brightness variations in known ones, so that they can quickly point other ground and space-based telescopes to study them in detail.
Follow-up observations of the source, since then named Gaia16aye after Ayers Rock, the famous landmark in Australia, revealed that the source was behaving in a rather strange way: after getting brighter and brighter, its luminosity suddenly dropped within one day.
Astronomers soon realised that this brightening was caused by gravitational microlensing – an effect predicted by Einstein’s theory of general relativity, caused by the bending of spacetime in the vicinity of very massive objects, like stars or black holes.
The Gaia alert led to a 500-day long global observation campaign, which lasted until the end of 2017, monitoring the star as it brightened up and subsequently declined five times. Extensive participation of ground-based telescopes from around the world enabled astronomers to gather a large amount of data – almost 25 000 individual data points – which were used to study the foreground object that was acting as a lens on the more distant star.
The data revealed the gravitational lens is actually a binary stellar system, consisting of two rather small stars, with 0.57 and 0.36 times the mass of our Sun, respectively. Separated by roughly twice the Earth-Sun distance, the stars orbit around their mutual centre of mass in less than three years.
Gaia16aye is the second micro-lensing event detected by the Gaia mission.
The ground-based observations were performed with different filters at a variety of visible and near-infrared wavelengths. In the graph, the different filters are indicated with the following letters: B standing for blue; g for green; V for visual (corresponding to intermediate wavelengths between green and red); R and r for red; I and i for infrared.
Credit: Adapted from Wyrzykowski et al. 2020, author: Kris Rybicki.
Videos:
http://www.astrouw.edu.pl/~wyrzykow/Gaia16ayePR/Gaia-launch-video.mov
Gaia launch in December 2013. Credit: ESA
http://www.astrouw.edu.pl/~wyrzykow/Gaia16ayePR/Gaia-launch-orbit.mov
Gaia launch, animation of the launch, trajectory and operation. Credit: ESA