One Planet, Four Stars
Artist’s conception of the 30 Ari star system. The system is composed of four stars. The distant companion 30 Ari A is actually a pair of stars in a close orbit. The research team discovered the fourth star in the system (the left-most star in the image). That star is a small red dwarf. A massive planet orbits the star named 30 Ari B in a nearly year-long orbit. Art by Karen Teramura, UH IfA.
Researchers, including IfA’s Christoph Baranec, who want to know more about the influences of multiple stars on exoplanets have found only the second known case of a planet in a four-star system. Although the star system, 30 Ari, was previously known to scientists, the new study increases the number of stars in it from three to four.
The system is located 136 light-years away in the constellation Aries. Its gaseous planet is enormous, with 10 times the mass of Jupiter, and orbits its primary star every 335 days. The newly discovered fourth star, whose distance from the planet is 23 times the Sun-Earth distance, does not appear to have impacted the orbit of the planet. The exact reason for this is uncertain, so the team is planning further observations to better understand the orbit of the newly discovered star and its complicated family dynamics.
Were it possible to see the skies from this world, the four stars would look like one small sun and two very bright stars that would be visible in daylight. If viewed with a large enough telescope, one would see that one of those bright stars is actually a binary system—two stars orbiting each other.
In recent years, dozens of planetary systems with two or three host stars have been found, which isn’t too much of a surprise, considering that binary stars are more common in our galaxy than single stars such as our Sun. “About four percent of solar-type stars are in quadruple systems, which is up from previous estimates because observational techniques are steadily improving,” said Andrei Tokovinin (Cerro Tololo Inter-American Observatory, Chile), a co-author of the study.
Lead author Lewis Roberts (Jet Propulsion Laboratory) and his colleagues want to understand the effects that multiple stars can have on their developing youthful planets. Evidence suggests that stellar companions can influence the fate of planets by changing the planets’ orbits and even triggering some to grow more massive. The “hot Jupiter” planets that whip around their stars in just days, for example, might be gently nudged closer to their primary star by the gravitational hand of a stellar companion. “This result strengthens the connection between multiple star systems and massive planets,” said Roberts.
The discovery was made at Palomar Observatory using two new adaptive optics technologies that compensate for the blurring effects of Earth’s atmosphere: the robotic Robo-AO adaptive optics system, developed under the leadership of Baranec, and the PALM-3000 extreme adaptive optics system, developed by a team at Caltech and NASA’s Jet Propulsion Laboratory (JPL) that also included Baranec.
“The discovery of this exciting system is only possible when we quickly scan through large numbers of potential targets,” said Baranec. “At the moment, Robo-AO is the only instrument that can give us the necessary combination of resolution and efficiency. Once we discover something interesting with Robo-AO, we can follow up with the “Formula 1” systems, like PALM-3000 or the SCExAO system at the Subaru Telescope in Hawai‘i, to obtain the absolute sharpest images possible. Additionally, we’re planning to bring a new, more powerful Robo-AO system to the University of Hawai‘i 2.2-m telescope to leverage the pristine skies of Maunakea. We’ll use it for even larger surveys and follow-up observations of asteroids and supernovae discovered by ATLAS on Mauna Loa and Haleakalā.”