A planet – as massive as Jupiter – has been spotted in a triple-star system and according to astronomers who imaged the planet, it most probably witnesses three sunrises and sunsets every day.
Named HD 131399Ab, the planet is located 340 light years from Earth in the constellation Centaurus and orbits three stars. Published in journal Science, the study about the planet was carried out by astronomers led by those at University of Arizona in Tucson, Arizona. The astronomers involved with the find also manged to directly image the planet.
The plane HD 131399Ab is believed to be about 16 million years old, making it one of the youngest exoplanets discovered to date. Analysis of the data collected by astronomers indicate that the planet has a rather harsh environment with temperatures of 850 Kelvin (about 1,070 degrees Fahrenheit or 580 degrees Celsius). Weighing in at an estimated four Jupiter masses, it is also one of the coldest and least massive directly imaged exoplanets.
“For about half of the planet’s orbit, which lasts 550 Earth-years, three stars are visible in the sky, the fainter two always much closer together, and changing in apparent separation from the brightest star throughout the year,” said Kevin Wagner, a first-year PhD student in Apai’s research group and the paper’s first author, who discovered HD 131399Ab. “For much of the planet’s year the stars appear close together, giving it a familiar night-side and day-side with a unique triple-sunset and sunrise each day. As the planet orbits and the stars grow further apart each day, they reach a point where the setting of one coincides with the rising of the other – at which point the planet is in near-constant daytime for about one-quarter of its orbit, or roughly 140 Earth-years.”
Wagner identified the planet among hundreds of candidate planets and led the follow-up observations to verify its nature.
The planet marks the first discovery of an exoplanet made with SPHERE, one of the world’s most advanced instruments dedicated to finding planets around other stars. SPHERE, which stands for the Spectro-Polarimetric High-Contrast Exoplanet Research Instrument, is sensitive to infrared light, making it capable to detect the heat signatures of young planets, along with sophisticated features correcting for atmospheric disturbances and blocking out the otherwise blinding light of their host stars. The instrument is part of the Very Large Telescope operated by the European Southern Observatory on Cerro Paranal in the Atacama Desert of northern Chile.
Although repeated and long-term observations will be needed to precisely determine the planet’s trajectory among its host stars, observations and simulations seem to suggest the following scenario: At the center of the system lies a star estimated to be eighty percent more massive than the sun and dubbed HD 131399A, which itself is orbited by the two remaining stars, B and C, at about three-hundred AU (one AU, or astronomical unit, equals the average distance between the earth and the sun). All the while, B and C twirl around each other like a spinning dumbbell, separated by a distance roughly equal to that between our sun and Saturn
In this scenario, planet HD 131399Ab travels around the central star, A, in an orbit about twice as large as Pluto’s if compared to our solar system, and brings the planet to about one-third of the separation of the stars themselves. The authors point out that a range of orbital scenarios is possible, and the verdict on long-term stability of the system will have to wait for planned follow-up observations that will better constrain the planet’s orbit.
“If the planet was further away from the the most massive star in the system, it would be kicked out of the system,” Apai explained. “Our computer simulations showed that this type of orbit can be stable, but if you change things around just a little bit, it can become unstable very quickly.”
Planets in multi-star systems are of special interest to astronomers and planetary scientists because they provide an example of how planet formation functions in these more extreme scenarios. While multi-star systems seem exotic to us in our orbit around our solitary star – multi-star systems are in fact just as common as single stars.
“It is not clear how this planet ended up on its wide orbit in this extreme system, and we can’t say yet what this means for our broader understanding of the types of planetary systems out there, but it shows there is more variety out there than many would have deemed possible,” Wagner said. “What we do know is that planets in multi-star systems are much less explored, and potentially just as numerous as planets in single-star systems.”
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