'1000 light-years away': James Webb Telescope discovers six new rogue worlds that are not bound at any star
'1000 light-years away': James Webb Telescope discovers six new rogue worlds that are not bound at any star
Produced by: Tarun Mishra
Designed by: Manoj Kumar
Discovery of Rogue Worlds
The James Webb Space Telescope has identified six potential rogue worlds—objects with planetary masses not bound to any star. These are the lightest such objects ever detected and include one with a dusty disk.
Significance of Findings
The discovery provides new evidence that processes responsible for star formation may also create objects with masses slightly greater than Jupiter. This challenges previous assumptions about how such objects form.
Credit : ESA
Study Details
The research, led by Adam Langeveld of Johns Hopkins University, focused on the young nebula NGC1333, about 1,000 light-years from Earth. The findings are detailed in a paper accepted for publication in The Astronomical Journal.
Observations and Analysis
Webb's infrared observations indicate that the rogue worlds are gas giants 5-10 times the mass of Jupiter. These objects are among the lightest to form through processes typically associated with stars and brown dwarfs.
Credit : ESA
Role of Dusty Disks
One of the rogue worlds, the lightest identified, has a dusty disk, suggesting it formed like a star. This disk is a feature generally seen in early star formation stages and could indicate the potential for planet formation.
Implications for Star and Planet Formation
The findings suggest that objects forming from gas and dust clouds may also be capable of developing planetary systems. This has implications for understanding both stellar and planetary formation processes.
Credit : ESA
Future Research
The team plans to study the atmospheres of these faint objects and compare them to known brown dwarfs and giant planets. They will also use the Webb telescope to explore similar objects for potential mini planetary systems.
Broader Impact
The research challenges existing models of celestial formation and may reshape our understanding of how planetary and star-like objects are created in the universe.
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