Sixteen years of studying this rare object found it to be a ring of hydrogen gas, surrounding what looks like an ordinary star. However, the properties of this object suggest the star at the center of this object is, itself, the product of the merger of a pair of stars. This discovery of TYC 2597–735-1 could open up a new era of understanding the nature of binary star systems. “We were in the middle of observing one night, with a new spectrograph that we had recently built, when we received a message from our colleagues about a peculiar object composed of a nebulous gas expanding rapidly away from a central star. How did it form? What are the properties of the central star? We were immediately excited to help solve the mystery!” Guðmundur Stefánsson of Princeton University stated. [Read: Why this security engineer loves working in infosec]
It takes two to tango
Unlike our own Sun, most stars in the Milky Way are found in binary systems, dancing with another star around their common center of gravity. “Stellar mergers are a brief but common phase in the evolution of binary star systems. These events have many astrophysical implications; for example, they may lead to the creation of atypical stars… Although a handful of stellar mergers have been observed directly, the central remnants of these events were shrouded by an opaque shell of dust and molecules, making it impossible to observe their final state,” researchers wrote in an article in Nature detailing the study. In systems where stars are close enough can result in a collision between the stars, merging the bodies together into one massive star. Orbital energy once present in the former stars results in the ejection of large quantities of material from the newly-formed body. — Purple Haze, Jimi Hendrix “When neutron stars collide, all hell breaks loose. They start producing a tremendous amount of visible light, and also gamma rays, X-rays, radio waves,” describes Frans Pretorius, physics professor at Princeton.
Three eyes are better than two
Astronomers went to work studying the Blue Ring Nebula, using a pair of 10-meter telescopes — the HIRES optical spectrograph at the Keck Telescope in Hawaii, and the near-infrared Habitable-zone Planet Finder attached to the Hobby-Eberly Telescope in Texas. Analysis revealed TYC 2597–735–1 is the product of a stellar merger that took place thousands of years ago. The Blue Ring Nebula offers astronomers a unique target to study — a composite star caught still settling down from its birth in a cathartic stellar merger. Astronomy News with The Cosmic Companion is also available as a weekly podcast, carried on all major podcast providers. Tune in every Tuesday for updates on the latest astronomy news, and interviews with astronomers and other researchers working to uncover the nature of the Universe.
