Brown dwarfs hiding in plain sight in our solar neighborhood

September 6, 2016, Carnegie Institution for Science

Cool brown dwarfs are a hot topic in astronomy right now. Smaller than stars and bigger than giant planets, they hold promise for helping us understand both stellar evolution and planet formation. New work from a team including Carnegie's Jonathan Gagné has discovered several ultracool brown dwarfs in our own solar neighborhood. Their findings are published in The Astrophysical Journal.

Brown dwarfs are sometimes called failed stars. They are too small to sustain the hydrogen fusion process that powers stars, so after forming they slowly cool, contract, and dim over time. Their temperatures can range from nearly as hot as a star to as cool as a planet and their masses also range between star-like and giant-planet-like.

They're fascinating to astronomers for a variety of reasons, mostly because they can serve as a bridge between stars and planets and how the former influences the latter, particular when it comes to composition and atmospheric properties. But much about them remains unknown.

"Everyone will benefit from the study of , because they can often be found in isolation, which means that we can more easily gather precise data on their properties without a bright star blinding our instruments," Gagné said, who is also a collaborator of the Institute for Research on Exoplanets (iREx) at Université de Montréal.

Discovering new brown dwarfs will help scientists to better quantify the frequency at which they occur both in our solar neighborhood and beyond. Knowing the abundance and distribution of brown dwarfs provides key information on the distribution of mass in the universe, and on the mechanism of brown dwarf formation, for example, whether they form in isolation or instead are ejected from larger planetary systems.

To that end, the team, led by Jasmin Robert of Université de Montréal, believed that although hundreds of ultracool brown dwarfs have already been discovered, the techniques used to identify them were overlooking those with more-unusual compositions, which would not show up in the color-based surveys generally used.

So they surveyed 28 percent of the sky and discovered 165 ultracool brown dwarfs, about a third of which have unusual compositions or other peculiarities. When talking about brown dwarfs, ultracool means temperatures under about 3,500 Fahrenheit or 2,200 kelvin

"The search for ultracool brown dwarfs in the neighborhood of our own Solar System is far from over," said Gagné. "Our findings indicate that many more are hiding in existing surveys."

Explore further: Brown dwarfs reveal exoplanets' secrets

More information: "A Brown Dwarf Census from the SIMP Survey," Jasmin Robert et al., 2016, to appear in the Astrophysical Journal: arxiv.org/abs/1607.06117

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MaxwellSmith
4 / 5 (4) Sep 06, 2016
I'm wondering what type of material you could scoop up on a Spectral Class Y Brown Dwarf, one cool enough to land on? Ultradense Hydrogen, prefusion?
I read that some Y class brown dwarfs are around the temperature of the human body.
Just curious.
Could planet X be a Y class brown dwarf?
wduckss
1 / 5 (1) Sep 07, 2016
"They're fascinating it astronomers for a variety of reasons, mostly because they can serve as a bridge between stars and planets .."

The conclusions should have been properly copied from the picture book (for a younger age), "The universe is rotating, after all," http://www.svemir....html#1b
The figure should correctly make ranking of (first planet ..) the same as in the picture book.

Article (arxiv.org/abs/1607.06117) has finally given appropriate attention to this matter.
antialias_physorg
5 / 5 (5) Sep 07, 2016
one cool enough to land on?

You would not want to land on one because they are still very large (i.e. have high surface gravity). This also comes with pretty dense atmospheres.

Could planet X be a Y class brown dwarf?

No. While these things are 'cool' by normal star standards it would still stand out like a lighthouse in any IR survey of the sky because of its size and proximity.

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