Astronomy

Astronomers Were Fortunate Enough to Catch a Neutron Star Merging With Another Star

A team of astronomers have followed the evolution of a short duration gamma ray burst, one of the most intense explosions in the entire universe. This discovery makes a breakthrough for further observations of these rare events.

To say that gamma ray bursts are incredibly bright is an understatement. A single burst releases more energy in a few seconds then our Sun does over its entire lifetime. They are so bright that they can be seen from literally across the universe. 

But because of their fleeting nature they are very difficult to detect. Observatories must constantly monitor large swaths of the sky and tune in to catch the quickly fading afterglow of the explosion. 

But a team of astronomers have developed a different way to study these short but intense events. They used ALMA, the Atacama Large Millimeter/submillimeter Array, located in the high Atacama desert of Northern Chile. The array consists of 66 different telescopes all working together to provide high resolution images of the distant universe.

“This short gamma-ray burst was the first time we tried to observe such an event with ALMA,” said Northwestern’s Wen-fai Fong, principal investigator of the ALMA program. “Afterglows for short bursts are very difficult to come by, so it was spectacular to catch this event shining so brightly. After many years observing these bursts, this surprising discovery opens up a new area of study, as it motivates us to observe many more of these with ALMA and other telescope arrays in the future.”

The team targeted GRB 211106A after an initial detection of the event in the x-rays. They were able to study the afterglow of the event for much longer using millimeter wavelengths rather than gamma rays or X-rays .

“Millimeter wavelengths can tell us about the density of the environment around the GRB,” said Schroeder, study coauthor and graduate student in Fong’s research group. “And, when combined with the X-rays, they can tell us about the true energy of the explosion. Because emission at millimeter wavelengths can be detected for a longer time than in X-rays, the millimeter emission also can be used to determine the width of the GRB jet.”

“ALMA shatters the playing field in terms of its capabilities at millimeter wavelengths and has enabled us to see the faint, dynamic universe in this type of light for the first time,” Fong said. “After a decade of observing short GRBs, it is truly amazing to witness the power of using these new technologies to unwrap surprise gifts from the universe.”

Paul M. Sutter

Astrophysicist, Author, Host | pmsutter.com

Recent Posts

New Study Addresses how Lunar Missions will Kick up Moondust.

Before the end of this decade, NASA plans to return astronauts to the Moon for…

15 hours ago

How Warm Are the Oceans on the Icy Moons? The Ice Thickness Provides a Clue.

Scientists are discovering that more and more Solar System objects have warm oceans under icy…

16 hours ago

NASA Tests the New Starship Docking System

The Apollo Program delivered 12 American astronauts to the surface of the Moon. But that…

20 hours ago

China Has Built a Huge Space Simulation Chamber

Well it certainly caught my attention when I saw the headlines  “China’s first Space Environment…

1 day ago

The International Space Station’s Air Leaks are Increasing. No Danger to the Crew

Only the other week I had to fix my leaky tap. That was a nightmare. …

1 day ago

Planetary Atmospheres: Why study them? What can they teach us about finding life beyond Earth?

Universe Today has surveyed the importance of studying impact craters, planetary surfaces, exoplanets, astrobiology, solar…

1 day ago