Credit: University of Warwick

A giant gas planet – up to fifty times the mass of Jupiter, encircled by a ring of dust – is likely hurtling around a star more than a thousand light years away from Earth, according to new research by an international team of astronomers, led by the University of Warwick.

Hugh Osborn, a researcher from Warwick's Astrophysics Group, has identified that the light from this rare young star is regularly blocked by a large object – and predicts that these eclipses are caused by the orbit of this as-yet undiscovered planet.

Using data from the Wide Angle Search for Planets (WASP) and Kilodegree Extremely Little Telescope (KELT), Osborn and fellow researchers from Harvard University, Vanderbilt University, and Leiden Observatory analysed fifteen years of the star's activity.

"We found a hint that this was an interesting object in data from the WASP survey," said Hugh Osborn, lead author, who discovered the unusual light curve, "but it wasn't until we found a second, almost identical eclipse in the KELT survey data that we knew we had something special."

They discovered that every two and a half years, the light from this distant star - PDS 110 in the Orion constellation, which is same temperature and slightly larger than our sun - is reduced to thirty percent for about two to three weeks. Two notable eclipses observed were in November 2008 and January 2011.

"What's exciting is that during both eclipses we see the light from the star change rapidly, and that suggests that there are rings in the eclipsing object, but these rings are many times larger than the rings around Saturn," says Leiden astronomer Matthew Kenworthy.

Assuming the dips in starlight are coming from an orbiting planet, the next eclipse is predicted to take place in September this year – and the star is bright enough that amateur astronomers all over the world will be able to witness it and gather new data. Only then will we be certain what is causing the mysterious eclipses.

If confirmed in September, PDS 110 will be the first giant ring system that has a known orbital period.

"September's eclipse will let us study the intricate structure around PDS 110 in detail for the first time, and hopefully prove that what we are seeing is a giant exoplanet and its moons in the process of formation," comments Hugh Oborn.

The researchers suggest that there are moons could be forming in the habitable zone around PDS 110 – pointing to the possibility that life could thrive in this system.

The eclipses can also be used to discover the conditions for forming planets and their moons at an early time in the life of a star, providing a unique insight into forming processes that happened in our solar system.

The research, 'Periodic Eclipses of the Young Star PDS 110 Discovered with WASP and KELT Photometry', is due to be published in the Monthly Notices of the Royal Astronomical Society.

More information: H. P. Osborn et al. Periodic Eclipses of the Young Star PDS 110 Discovered with WASP and KELT Photometry, Monthly Notices of the Royal Astronomical Society (2017). Journal information: Monthly Notices of the Royal Astronomical Society H. P. Osborn et al. Periodic Eclipses of the Young Star PDS 110 Discovered with WASP and KELT Photometry,(2017). DOI: 10.1093/mnras/stx1249