New Low-Mass Objects Could Help Refine Planetary Evolution

When a star is young, it is often still surrounded by a primordial rotating disk of gas and dust, from which planets can form.
Astronomers like to find such disks because they might be able to catch the star partway through the planet-formation process, but it’s highly unusual to find such disks around brown dwarfs or stars with very low masses. New work from a team led by Anne Boucher of Université de Montréal, and including Carnegie’s Jonathan Gagné and Jacqueline Faherty, has discovered four new low-mass objects surrounded by disks. The results will be published by The Astrophysical Journal.

Three of the four objects discovered by these researchers are quite small, somewhere between only 13 and 18 times the mass of Jupiter. The fourth has about 120 times Jupiter’s mass. (For comparison the Sun is just over 1,000 times more massive than Jupiter.)

“Finding disks in low-mass systems is really interesting to us, because objects that exist at the lower limit of what defines a star and that still have disks that indicate planet formation can tell us a lot about both stellar and planetary evolution,” said first author Boucher, who works at her university’s Institute for Research on Exoplanets (iREx).

In a planet-forming disk, the dust grains collide and aggregate to form pebbles, which grow into boulders, and so on, increasing in size through planetesimals, planetary embryos, and finally rocky terrestrial planets (some of which then become the cores for gas giant planets). Astronomers are able to identify these types of planet-birthing disks, because the star heats up the surrounding dust, which affects the way it looks using a telescope with an infrared camera.

However, some disks indicate that planet formation isn’t ongoing, but has already finished. These disks are made up of the debris left behind by all the collisions during planet formation and by subsequent collisions of the newly formed planets. Eventually these dusty remains are swept away. But until that happens, a cooler, thinner ring of dust surrounds the star.

Some disks even represent an intermediate stage between the planet-forming and dusty remnant phases.

It’s important for astronomers to try to distinguish between these different types of disks, because then they can better chart the way planetary systems, including our own solar system, are born and change over time.

The research team was able to determine that the disks surrounding their four newly discovered low-mass objects were all likely in a phase of planet forming. None were in the dusty aftermath phase.

Even more interesting, two of the objects are possibly between 42 and 45 million years old. This would make them the oldest objects surrounded by active disk systems ever found.

“There is still so much to learn about disks around low-mass objects such as these four,” concluded Gagné, who is also a iREx collaborator. “Hopefully, we can conduct further research on them and be able to narrow down what kind of activity is happening in them and whether or not they would be good targets for future planet hunters.”

Reference: “BANYAN. VIII. New Low-Mass Stars and Brown Dwarfs with Candidate Circumstellar Disks,” Anne Boucher et al., 2016, to appear in the Astrophysical Journal [http://apj.aas.org, preprint: https://arxiv.org/abs/1608.08259]. The other co-authors are David Lafrenière and René Doyon of Université de Montréal, and Lison Malo of the Canada-France-Hawaii Telescope.

This work made use of the data products from: The Two Micron All Sky Survey, which is a joint project of the University of Massachusetts and the Infrared Processing and Analysis Center (IPAC)/California Institute of Technology (Caltech), funded by NASA and the National Science Foundation; the Wide-field Infrared Survey Explorer, which is a joint project of the University of California, Los Angeles, and the Jet Propulsion Laboratory (JPL)/Caltech, funded by NASA; and the DENIS I-band catalog. This research also made use of the SIMBAD database and VizieR catalogue access tool, operated at Centre de Données astronomiques de Strasbourg, France; as well as the NASA/IPAC Infrared Science Archive, which is operated by the JPL, Caltech, under contract with NASA. This paper is based on observations obtained at the Canada-France-Hawaii Telescope (CFHT) which is operated by the National Research Council of Canada, the Institut National des Sciences de l’Univers of the Centre National de la Recherche Scientique of France, and the University of Hawaii. It also includes data gathered with the 6.5 meter Magellan Telescopes located at Las Campanas Observatory, Chile, using the FIRE instrument.

The Carnegie Institution for Science (http://carnegiescience.edu) is a private, nonprofit organization headquartered in Washington, D.C., with six research departments throughout the U.S. Since its founding in 1902, the Carnegie Institution has been a pioneering force in basic scientific research. Carnegie scientists are leaders in plant biology, developmental biology, astronomy, materials science, global ecology, and Earth and planetary science.

The Institute for research on exoplanets (iREx, http://www.exoplanetes.umontreal.ca) brings together top researchers and their students who work to gain the most from current and upcoming major observational projects, with the ultimate goal of finding life elsewhere in the universe. The Institute is devoted to exploring new worlds and seeking life on other planets.