Original Image: NASA/Johns Hopkins University Applied Physics Laboratory/Southwest Research Institute/Goddard Space Flight Center

Exiled moons may explain astronomical mysteries

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Australian and South American researchers posit wandering “ploonets” as unseen actors in distant solar systems. Moons ejected from orbits around gas giant exoplanets could explain several astronomical mysteries, an international team of astronomers suggests. Researchers led by Mario Sucerquia, from the Universidad de Antioquia, Colombia, and Jaime Alvarado-Montes from Australia’s Macquarie University, modelled the likely behaviour of giant exomoons predicted to form around massive planets – and discovered that they would be expelled and sent packing.

Organisation/s: Macquarie University, Universidad de Antioquia

Funder: M.S. is supported by Colciencias (647) and the CODI/UdeA. J.A.M. acknowledges funding support from Macquarie University through the Macquarie University Research Excellence Scholarship (‘iMQRES MRES’). J.I.Z. is supported by Vicerrectoría de Docencia UdeA. N.C. acknowledges financial support provided by FONDECYT grant 3170680. The authors thank Jorge Cuadra for helpful remarks and partial funding from CONICYT-Chile through FONDECYT (1141175) and Basal (PFB0609) grants.

Media Release

From: Science In Public

Australian and South American researchers posit wandering “ploonets” as unseen actors in distant solar systems.

Moons ejected from orbits around gas giant exoplanets could explain several astronomical mysteries, an international team of astronomers suggests.

Researchers led by Mario Sucerquia, from the Universidad de Antioquia, Colombia, and Jaime Alvarado-Montes from Australia’s Macquarie University, modelled the likely behaviour of giant exomoons predicted to form around massive planets – and discovered that they would be expelled and sent packing.

Roughly 50% of these ejected moons would survive both the immediate expulsion and avoid any subsequent collision with the planet or the star, ending up as quasi-planets travelling around the host star, but in eccentric “Pluto-like” orbits.

These rogue moons – dubbed “ploonets” by Sucerquia, Alvarado-Montes and colleagues – could potentially explain several puzzling phenomena, not the least of which is why astronomers have so far confirmed the existence of at least 4098 exoplanets, but not a single exomoon.

Most of the planets discovered thus far are of a type known as Hot Jupiters, a fact that reflects mainly the limits of current detection technology. Previous research indicates that at least some of these should be orbited by large moons.

Their absence, the researchers write in a paper soon to be published in the journal Monthly Notices of the Royal Astronomical Society, could be explained by a scenario in which the angular momentum between the two bodies results in the moon escaping the gravitational pull of its parent.

“These moons would become planetary embryos, or even fully-fledged planets, with highly eccentric orbits of their own,” explains Alvarado-Montes.

While conceding that ploonets remain hypothetical, the researchers say their existence would offer a possible explanation for several challenging results produced by NASA’s now-retired Kepler space telescope.

These include the puzzling dips in the light-curves emanating from a formally known as KIC-8462852.

“It’s better known as Tabby Star,” says Alvarado-Montes, “and the strange changes in its light intensity have been observed for years, but are still not understood. Ploonets could be the answer.”

They might also explain apparent evidence of cannibalism between some stars, or the existence of “exocomets” around others.

Ploonets, thus, may be a vital piece of the planetary puzzle, but, as yet, their existence remains unproven.

Sucerquia, Alvarado-Montes and colleagues concede that even if they do exist, they may deteriorate too rapidly to ever be observed.

“If, on the other hand,” they write, “the timescales are large enough, we could have real chances to detect them in the near and middle future.”

The paper is currently available on arXiv, the preprint library maintained by Cornell University in the US.

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