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Astronomers have discovered the first known instance of a baby star ‘sneezing.‘ The cosmic discharge, which may have occurred as recently as a few hundred years ago, reveals how infant stars expel most of their magnetic energy very early in their evolution—a shedding mechanism that stops their high-spinning profiles from breaking apart.
Radio telescope researchers reached into the cosmic bassinet for a way to explain to themselves and to laypersons how an unexpected "interchange instability“ creates a detectable leaks of gases and dust in an emerging star. Anyone have a super-cosmic-sized hankie?
Context:
Astronomers have discovered the first known instance of a baby star Astronomers have discovered the first known instance of a baby star Astronomers have discovered the first known instance of a baby star 'sneezing.' The cosmic discharge, which may have occurred as recently as a few hundred years ago, reveals how infant stars expel most of their magnetic energy very early in their evolution — a shedding mechanism that stops their high-spinning profiles from breaking apart.
Researchers observed the cosmic sneeze in images captured by the Atacama Large Millimeter/submillimeter Array (ALMA) observatory, a set of radio telescopes located in Chile's Atacama Desert.
The star in question is a faint baby star embedded in a dense gas cloud named MC 27 roughly 450 light-years from Earth in the constellation Taurus. The cosmic cradle is a turbulent ring of gas and dust known as a protostellar disk, where unstable magnetic fields interact with gasses and intermittently blast out as spikes and arcs coated with gas and dust. This process, known as interchange instability, propels the leaked material away from the disk at roughly the speed of sound, the researchers reported in a study published Thursday (April 11) in The Astrophysical Journal.
"This discovery was unexpected," Kazuki Tokuda, an astronomer at Kyushu University in Japan and the lead author of the study, told Live Science. While previous telescope observations of the stellar nursery hadn't revealed the peculiar structures, ALMA spotted streamers not only escaping the disk but also much further away, revealing the baby star "sneezed" multiple times in the past. Such episodic behavior helps the baby star maintain a compact disk around it, the researchers say.sneezing.' The cosmic discharge, which may have occurred as recently as a few hundred years ago, reveals how infant stars expel most of their magnetic energy very early in their evolution — a shedding mechanism that stops their high-spinning profiles from breaking apart.
Researchers observed the cosmic sneeze in images captured by the Atacama Large Millimeter/submillimeter Array (ALMA) observatory, a set of radio telescopes located in Chile's Atacama Desert.
The star in question is a faint baby star embedded in a dense gas cloud named MC 27 roughly 450 light-years from Earth in the constellation Taurus. The cosmic cradle is a turbulent ring of gas and dust known as a protostellar disk, where unstable magnetic fields interact with gasses and intermittently blast out as spikes and arcs coated with gas and dust. This process, known as interchange instability, propels the leaked material away from the disk at roughly the speed of sound, the researchers reported in a study published Thursday (April 11) in The Astrophysical Journal.
"This discovery was unexpected," Kazuki Tokuda, an astronomer at Kyushu University in Japan and the lead author of the study, told Live Science. While previous telescope observations of the stellar nursery hadn't revealed the peculiar structures, ALMA spotted streamers not only escaping the disk but also much further away, revealing the baby star "sneezed" multiple times in the past. Such episodic behavior helps the baby star maintain a compact disk around it, the researchers say.sneezing.' The cosmic discharge, which may have occurred as recently as a few hundred years ago, reveals how infant stars expel most of their magnetic energy very early in their evolution — a shedding mechanism that stops their high-spinning profiles from breaking apart.
Researchers observed the cosmic sneeze in images captured by the Atacama Large Millimeter/submillimeter Array (ALMA) observatory, a set of radio telescopes located in Chile's Atacama Desert.
The star in question is a faint baby star embedded in a dense gas cloud named MC 27 roughly 450 light-years from Earth in the constellation Taurus. The cosmic cradle is a turbulent ring of gas and dust known as a protostellar disk, where unstable magnetic fields interact with gasses and intermittently blast out as spikes and arcs coated with gas and dust. This process, known as interchange instability, propels the leaked material away from the disk at roughly the speed of sound, the researchers reported in a study published Thursday (April 11 [2024]) in the Astrophysical Journal.
"This discovery was unexpected," Kazuki Tokuda, an astronomer at Kyushu University in Japan and the lead author of the study, told Live Science. While previous telescope observations of the stellar nursery hadn't revealed the peculiar structures, ALMA spotted streamers not only escaping the disk but also much further away, revealing the baby star ‘sneezed‘ multiple times in the past. Such episodic behavior helps the baby star maintain a compact disk around it, the researchers say.
Citation:
Kuthunur, Sharmila. “There's a Baby Star ‘Sneezing’ in the Constellation Taurus—and it Could Solve a Longstanding Cosmic Mystery.” LiveScience, livescience.com, 12 April 2024. Web..