AUI News  >

Astronomers Discover Jupiter-sized Objects Drawn into Each Other’s Orbit

Recent News

NSF VLA Contributes Crucial Puzzle Piece to ‘Peculiar’ High Energy Transient

High-energy transient signals are most often determined to be gamma-ray burst events, but the recently-launched Einstein Probe has expanded astronomers’ ability to quickly respond to similar signals occurring at X-ray wavelengths. Now, a multi-wavelength study of EP240408a concludes that while many of the signal’s characteristics might lead to the conclusion that it is a gamma-ray burst, the non-detection at radio wavelengths precludes that possibility.

Students Contribute to New Understanding of ‘Twinkling’ Pulsars

The flexible observing setup of the Green Bank Observatory’s 20-meter telescope enabled frequent, long-duration observations of eight pulsars, spanning two and a half years for a student-driven study carried out by students in the Pulsar Science Collaboratory program.

Double the Disks, Double the Discovery: New Insights into Planet Formation in DF Tau

Tucked away in a star-forming region in the Taurus constellation, a pair of circling stars are displaying some unexpected differences in the circumstellar disks of dust and gas that surround them. A new study led by researchers at Lowell Observatory, combining data from the Atacama Large Millimeter/submillimeter Array (ALMA) and Keck Observatory, has unveiled intriguing findings about planet formation in this binary star system, known as DF Tau, along with other systems in this region.

Astronomers Discover Jupiter-sized Objects Drawn into Each Other’s Orbit

Two Free-floating binary Jupiter-mass objects

Credit: Gemini Observatory/Jon Lomberg

VLA & JWST observe binary system of free-floating JuMBOs

In our most basic understanding of our Solar System, planets are drawn into the orbit of our massive star, the Sun. But what happens to planet-sized objects that don’t have a star? A team of astronomers studying Jupiter-mass binary objects (JuMBOs) in the Orion Nebula are gaining a new understanding of these unusual systems. These massive, free-floating objects are being drawn into orbit with each other. These latest findings come from observations made by the Karl G. Jansky Very Large Array (VLA) at the U.S. National Science Foundation National Radio Astronomy Observatory, and NASA’s James Webb Space Telescope.

This groundbreaking discovery has been made in the field of astronomy, thanks to advancements in sensitivity that have allowed scientists to detect fainter and smaller objects in space. Using the VLA, astronomers searched for counterparts to a group of 40 Jupiter-mass binary objects known as JuMBOs, previously identified by Pearson and McCaughrean in 2023. Surprisingly, only one of these objects, JuMBO 24, exhibited a radio counterpart.

This remarkable finding challenges existing theories on the formation of stars and planets. The radio luminosity of the two planets in this binary system is significantly higher than that detected in brown dwarfs, which are objects that share similarities with these planets. This abnormality raises new questions and provides exciting research opportunities to further understand the nature of these free-floating planets. While it is possible that the association between infrared and radio signals is coincidental, the team considers this to be highly unlikely, with odds of only 1 in 10,000. This discovery builds upon the previous work of Kao et al., who, in 2018, detected a single planetary-mass system resembling the components of JuMBO 24 using the VLA.

Dr. Luis F. Rodriguez, Professor Emeritus at the National Autonomous University of Mexico, who participated in this research, emphasizes the significance of the discovery. “What’s truly remarkable is that these objects could have moons similar to Europa or Enceladus, both of which  have underground oceans of liquid water that could support life”, he stated.

The detection of radio waves originating from both components of a double system of free-floating planets represents a significant milestone in our exploration of the universe. It also presents an exciting opportunity for further research into the potential habitability of planets beyond our solar system. Read the entire published findings online.

About NRAO

The National Radio Astronomy Observatory (NRAO) is a National Science Foundation facility, operated under a cooperative agreement by Associated Universities, Inc.

NRAO Media Contacts
Corrina C. Jaramillo Feldman
Public Information Officer – New Mexico
VLA, VLBA, ngVLA
Tel: +1 505-366-7267
cfeldman@nrao.edu

Jill Malusky
NRAO & GBO News & Public Information Manager
Tel: +1 304-460-5608
jmalusky@nrao.edu

This news article was originally published on the NRAO website on February 12, 2024.

Recent News

NSF VLA Contributes Crucial Puzzle Piece to ‘Peculiar’ High Energy Transient

High-energy transient signals are most often determined to be gamma-ray burst events, but the recently-launched Einstein Probe has expanded astronomers’ ability to quickly respond to similar signals occurring at X-ray wavelengths. Now, a multi-wavelength study of EP240408a concludes that while many of the signal’s characteristics might lead to the conclusion that it is a gamma-ray burst, the non-detection at radio wavelengths precludes that possibility.

Students Contribute to New Understanding of ‘Twinkling’ Pulsars

The flexible observing setup of the Green Bank Observatory’s 20-meter telescope enabled frequent, long-duration observations of eight pulsars, spanning two and a half years for a student-driven study carried out by students in the Pulsar Science Collaboratory program.

Double the Disks, Double the Discovery: New Insights into Planet Formation in DF Tau

Tucked away in a star-forming region in the Taurus constellation, a pair of circling stars are displaying some unexpected differences in the circumstellar disks of dust and gas that surround them. A new study led by researchers at Lowell Observatory, combining data from the Atacama Large Millimeter/submillimeter Array (ALMA) and Keck Observatory, has unveiled intriguing findings about planet formation in this binary star system, known as DF Tau, along with other systems in this region.