Skip to main content

Pair of brown dwarfs orbit each other 12 billion miles apart

It’s not uncommon for stars to be found in binary pairs, where two stars are gravitationally bound together and orbit each other. Sometimes, you even find triple star systems with three stars bound together. But typically, stars in these configurations are relatively close together. Now, though, astronomers have spotted a pair of brown dwarfs, which are objects in between planets and stars, which have the widest separation found to date.

The brown dwarf pair, called CWISE J014611.20-050850.0AB, are a mind-bending 12 billion miles apart — that’s more than three times the distance between Pluto and the sun. They are especially notable because brown dwarf pairs generally have less gravitational force binding them than a pair of full-blown stars would have. “Because of their small size, brown dwarf binary systems are usually very close together,” said lead author Emma Softich of Arizona State University in a statement. “Finding such a widely separated pair is very exciting.”

An artist’s rendition of a binary system of brown dwarfs like CWISE J014611.20-050850.0AB.
An artist’s rendition of a binary system of brown dwarfs like CWISE J014611.20-050850.0AB. William Pendrill

The pair were discovered with the W. M. Keck Observatory on Maunakea, Hawaiʻi, using its Near-Infrared Echellette Spectrometer, or NIRES instrument. “Keck’s exceptional sensitivity in the infrared with this instrument was critical for our measurements,” said co-author Adam Burgasser. “The secondary brown dwarf of this system is exceptionally faint, but with Keck we were able to obtain good enough spectral data to classify both sources and identify them as members of a rare class of blue L dwarfs.”

Citizen scientists played a role in helping this discovery come about as well. As part of NASA’s Backyard Worlds project, members of the public were invited to search astronomical data to look for indications of brown dwarfs. The researchers in this study looked through the Backyard World’s identified brown dwarfs and searched for companions to them.

When the researchers found indications of a binary pair, they used NIRES to confirm the pair, located around 130 light-years away.

“Binary systems are used to calibrate many relations in astronomy, and this newly discovered pair of brown dwarfs will present an important test of brown dwarf formation and evolution models,” said co-author Jennifer Patience.

The research is published in The Astrophysical Journal Letters.

Editors' Recommendations

Georgina Torbet
Georgina is the Digital Trends space writer, covering human space exploration, planetary science, and cosmology. She…
Hubble discovers over 1,000 new asteroids thanks to photobombing
This NASA/ESA Hubble Space Telescope image of the barred spiral galaxy UGC 12158 looks like someone took a white marking pen to it. In reality it is a combination of time exposures of a foreground asteroid moving through Hubble’s field of view, photobombing the observation of the galaxy. Several exposures of the galaxy were taken, which is evidenced by the dashed pattern.

The Hubble Space Telescope is most famous for taking images of far-off galaxies, but it is also useful for studying objects right here in our own solar system. Recently, researchers have gotten creative and found a way to use Hubble data to detect previously unknown asteroids that are mostly located in the main asteroid belt between Mars and Jupiter.

The researchers discovered an incredible 1,031 new asteroids, many of them small and difficult to detect with several hundred of them less than a kilometer in size. To identify the asteroids, the researchers combed through a total of 37,000 Hubble images taken over a 19-year time period, identifying the tell-tale trail of asteroids zipping past Hubble's camera.

Read more
Biggest stellar black hole to date discovered in our galaxy
Astronomers have found the most massive stellar black hole in our galaxy, thanks to the wobbling motion it induces on a companion star. This artist’s impression shows the orbits of both the star and the black hole, dubbed Gaia BH3, around their common centre of mass. This wobbling was measured over several years with the European Space Agency’s Gaia mission. Additional data from other telescopes, including ESO’s Very Large Telescope in Chile, confirmed that the mass of this black hole is 33 times that of our Sun. The chemical composition of the companion star suggests that the black hole was formed after the collapse of a massive star with very few heavy elements, or metals, as predicted by theory.

Black holes generally come in two sizes: big and really big. As they are so dense, they are measured in terms of mass rather than size, and astronomers call these two groups of stellar mass black holes (as in, equivalent to the mass of the sun) and supermassive black holes. Why there are hardly any intermediate-mass black holes is an ongoing question in astronomy research, and the most massive stellar mass black holes known in our galaxy tend to be up to 20 times the mass of the sun. Recently, though, astronomers have discovered a much larger stellar mass black hole that weighs 33 times the mass of the sun.

Not only is this new discovery the most massive stellar black hole discovered in our galaxy to date but it is also surprisingly close to us. Located just 2,000 light-years away, it is one of the closest known black holes to Earth.

Read more
Watch how NASA plans to land a car-sized drone on Titan
An artist's impression of NASA's Dragonfly drone.

 

A decision by NASA this week paved the way for the Dragonfly drone mission to continue to completion.

Read more