Three mysterious debris rings surrounding Supernova 1987A were formed during an ancient two-star merger that eventually led to an enormous stellar explosion, a new computer model suggests.
The model, detailed in Friday's issue of the journal Science, was announced on the 20th anniversary of the supernova’s discovery.
Supernova 1987A, or SN1987A, was the closest and brightest supernova observed in more than 400 years. It blazed as brightly as 100 million suns before gradually fading. The explosion occurred in the Large Magellanic Cloud, a dwarf galaxy only 160,000 light-years away. It was first spotted on Feb. 23, 1987, and marked the first time modern astronomers could observe a star explosion in detail.
The discovery of three rings of gas around SN1987 led astronomers to propose that the supernova resulted from the merger of two stars — one about 15 solar masses and the other about 5 solar masses — into a red supergiant. According to this scenario, the red supergiant eventually shrunk into a blue supergiant, called Sanduleak-69 202, or SK-69, about 20,000 years ago before finally exploding. The entire process is thought to have taken a few hundred years.
Computer model re-creates star merger
This speculative theory is now bolstered by a new three-dimensional computer model that successfully re-created the star merger and the unusual three-ring nebula.
The model, developed by Thomas Morris and Philipp Podsiadlowski of the University of Oxford, suggests the triple rings were created by two minor explosions which occurred before SK-69 went supernova. One occurred during the initial merging of the two stars into a red supergiant.
“When the two stars merged, they released a lot of energy that ejected part of the (stellar) envelope, producing the two outer rings,” Podsiadlowski told SPACE.com in a phone interview.
The second explosion occurred immediately after the red supergiant transitioned to a blue supergiant.
“In that phase, the star ejected material in the equatorial plane, and this is what produced the inner ring,” Podsiadlowski said.
The researchers say their model is testable because it predicts mass and chemical differences among the three rings that could become apparent in future decades, when debris from the supernova blast catches up with material in the ring.
Star unions may not explain odd nebulas
“This process has already started,” Podsiadlowski said. “The ejecta will destroy the inner ring, and that will produce a lot of energy, which will lighten up the nebula again.”
Noam Soaker, an astronomer at the Technion Israel Institute of Technology who was not involved in the computer modeling, writes in an accompanying Science article that although the new “model has several advantages ... it cannot be considered as a general model for other similar objects, and it is not the last word on the formation of the rings of SN1987A.”
Nathan Smith, an astronomer at the University of California at Berkeley recently proposed a different formation scenario for SN1987A. Smith proposed that the supernova’s progenitor star belonged to a class of unstable blue supergiants, called luminous blue variables, that can go supernova without merging with other stars or going through a red supergiant phase.