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The Future of Alpha Centauri

A rare opportunity for planet hunting in Alpha Centauri A predicted for 2028

20 października 2016

A very rare gravitational lensing event, set to occur in 2028, has been predicted by a team of French astronomers led by Pierre Kervella of the CNRS/Universidad de Chile. It will provide an ideal opportunity to look for evidence of a planet around a nearby star.

Using both new and archive data obtained with a range of ESO telescopes [1], the team has predicted the trajectories of the fast-moving stellar duo known as the Alpha Centauri A and B, with negligible error. That has allowed them to predict every close alignment until 2050 between the Alpha Centauri pair and the stars which lie close to them on the sky — but which are in fact a great deal further away in space [2].

Whilst it is satisfying to see into the future with such impressive accuracy, that is not the real prize in these results; they provide a unique opportunity for planet hunting in the Alpha Centauri system, by allowing us to search for secondary gravitational lensing events. Gravitational lensing occurs because a massive object, such as a star, warps the very fabric of the space around it. Light — coming from a distant object — that passes close to the star on its way to us follows a curved path through the warped space. The nearer star acts like a lens, bending the light from the distant object. In the most impressive cases, this can generate an Einstein ring, a circle of light around the foreground star. Because the amount of mass in this nearby star determines exactly how the light deflection occurs, deviations from the expected gravitational lensing effect can be used to determine the presence, and the masses, of planets.

One of the most exciting alignments predicted by this study is between the more massive star in the Alpha Centauri pair, named Alpha Centauri A, and a distant background star — probably a red giant — nicknamed S5. In May 2028, there is a strong chance that the light from S5 will create an Einstein ring around Alpha Centauri A, observable with ESO’s telescopes [3]. This would provide a unique opportunity to look for planetary or low-mass objects in our nearest star system. This is particularly exciting in the light of the recent discovery of the planet Proxima b, which orbits the third star in the same star system, known as Proxima Centauri.

Notes

[1] Because of the vast distances involved, measuring the true motions of most stars is extremely difficult and requires incredibly precise measurements and extensive observations. The team of astronomers used data collected in 2007 from the New Technology Telescope (NTT) and new observations from the NACO instrument on the Very Large Telescope (VLT). This was complemented with data from the Atacama Large Millimeter/submillimeter Array (ALMA) to obtain high-precision measurement of the relative positions of Alpha Centauri A and B.

[2] Because of the Alpha Centauri system’s proximity to the plane of the Milky Way, the distant star field is very densely populated; this gave the team a good chance of finding a background star which would almost perfectly align with one of the Alpha Centauri binary pair.

[3] The event will be observable by the GRAVITY instrument on the Very Large Telescope Interferometer (VLTI), Atacama Large Millimeter/submillimeter Array (ALMA), and the forthcoming European-Extremely Large Telescope (E-ELT), providing a good chance of ascertaining the mass of any planet to a high degree of accuracy.

ALMA, an international astronomy facility, is a partnership of ESO, the U.S. National Science Foundation (NSF) and the National Institutes of Natural Sciences (NINS) of Japan in cooperation with the Republic of Chile.

More Information

This research was presented in a paper to appear on 19 October 2016 in the journal Astronomy and Astrophysics (Kervella et al. 2016, A&A, 594, A107)

The team is composed of: P. Kervella, CNRS UMI 3386, University of Chile and LESIA, Paris Observatory; F. Mignard, Côte d’Azur Observatory, France; A. Mérand, ESO; and F. Thévenin, Côte d’Azur Observatory, France.