Why Do Aging Brown Dwarfs Sweep the Clouds Away?

An artist’s conception of a brown dwarf.

 Image is courtesy of NASA/JPL, slightly modified by Jonathan Gagné.

Because they are freely floating in space, the atmospheric properties of brown dwarfs are much easier to study than the atmospheres of exoplanets, where the light of a central star can be completely overwhelming.

In this paper, Gagné and his colleagues—Katelyn Allers of Bucknell University; Christopher Theissen of University of California San Diego; Jacqueline Faherty and Daniella Bardalez Gagliuffi of the American Museum of Natural History, and Etienne Artigau of Institute for Research on Exoplanets, Université de Montréal—focused on an unusually red brown dwarf called 2MASS J13243553+6358281, which they were able to determine is one of the nearest known planetary mass objects to our Solar System.

The redness of this object had previously been suggested to indicate that it was actually a binary system, but the research team’s findings indicate that it is a single free floating planetary mass object.

They confirmed that it is part of a group of roughly 80 stars of similar ages and compositions drifting together through space, called the AB Doradus moving group, which revealed that it is about 150 million years old.

 

By knowing the object’s age and measuring its luminosity and distance, the team could determine its likely radius, mass, and, most-importantly its temperature.

They could then compare its temperature to that of another previously studied brown dwarf in the same moving group—one that was still cloudy while 2MASS J1324+6358 was already cloudless. This allowed them to figure out the temperature at which the cloudy to cloudless transition happens.

“We were able to constrain the point in the cool-down process at which brown dwarfs like J1324transition from cloudy to cloud-free,” explained Gagné

The shift occurs about 1,150 degrees kelvin, or 1,600 degrees Fahrenheit, for planetary-mass objects that are 150 million years old like 2MASS J1324+6358 and other members of the AB Doradus moving group.

“Because brown dwarfs like this one are so analogous to gas giant planets, this information could help us understand some of the evolutionary processes that occurred right here in our own Solar System’s history,” Gagné added.

 

Citation: 2MASS J13243553 6358281 Is an Early T-type Planetary-mass Object in the AB Doradus Moving Group. Jonathan Gagné, Katelyn N. Allers, Christopher A. Theissen, Jacqueline K. Faherty, Daniella Bardalez Gagliuffi, Étienne Artigau.The Astrophysical Journal, 2018; 854 (2): L27 DOI: 10.3847/2041-8213/aaacfd