Astronomers Watch Delayed Broadcast of a Rare Celestial Eruption

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Pasadena, CA— Eta Carinae, one of the most massive stars in our Milky Way galaxy, unexpectedly increased in brightness in the 19th century. For ten years in the mid-1800s it was the second-brightest star in the sky. (Now it is not even in the top 100.) The increase in luminosity was so great that it earned the rare title of Great Eruption. New research from a team including Carnegie’s Jose Prieto, now at Princeton University, has used a “light echo” technique to demonstrate that this eruption was much different than previously thought. Their work is published Feb. 16 in Nature.

Eta Carinae is a Luminous Blue Variable (LBV), meaning it has periods of dimness followed by periods of brightness. The variations in brightness of an LBV are caused by increased instability and loss of mass. The Great Eruption was an extreme and unique event in which the star, which is more than 100 times the mass of the Sun, lost several times the mass of the Sun. Scientists have believed that this rare type of eruption was caused by a stellar wind.

The team of scientists, led by Armin Rest of the Space Telescope Science Institute, used images of Eta Carinae over 8 years to study light echoes of the Great Eruption. For the first time, they observed light from the eruption that bounced, or echoed, off interstellar dust tens of light years from the star. Those extra tens of light years mean that the light is reaching Earth now rather than in the 1800s when people on Earth observed the light that traveled here directly.

They then used the Magellan and du Pont telescopes at Las Campanas Observatories, in Chile, to obtain spectra of the echoes of light. The spectra allow them to precisely separate the light into its constituents, much like a drop of rain naturally acts as a prism and separates sunlight into the colors of the rainbow. These observations give important information about the chemical composition, temperature, and velocity of the material ejected during the 19th century Great Eruption.

Most surprisingly, their observations show that the Great Eruption is different from so-called “supernova impostor,” events in nearby galaxies that are thought to be eruptions from LBVs. For example, the Great Eruption was significantly cooler than allowed by simple stellar-wind models used to explain supernova impostors.

“This star’s Giant Eruption has been considered a prototype for all supernova imposters in external galaxies,” Prieto said. “But this research indicates that it is actually a rather unique event.”

Thus, scientists still don’t know what phenomenon caused Eta Carinae to erupt and lose such a quantity of mass without being destroyed. Further research is necessary to determine whether other proposed models could have triggered this activity instead.

 

Caption: These images reveal light from a massive stellar outburst in the Carina Nebula reflecting off dust clouds surrounding a behemoth double-star system, a phenomenon called a light echo.
The color image at left shows the Carina Nebula, a star-forming region located 7500 light-years from Earth. The massive star Eta Carinae resides near the top of the image. The double-star system, about 120 times more massive than the Sun, produced a spectacular outburst that was seen on Earth from 1837 to 1858. But some of the light from the eruption took an indirect path and is just now reaching our planet. The light bounced off dust clouds (the box about 100 light-years away at the bottom of the image) and was rerouted to Earth. The image was taken by the U.S. National Optical Astronomy Observatory’s Curtis-Schmidt Telescope at the Cerro Tololo Inter-American Observatory (CTIO) in Chile.
The three black-and-white images at right show light from the eruption illuminating the dust clouds over an eight-year span as it moves through them. The effect is like shining a flashlight on different regions of a vast cavern. The images were taken by the U.S. National Optical Astronomy Observatory’s Blanco 4-meter telescope at the CTIO. Photo credits: NASA, NOAO, and A. Rest (STScI)

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Observations were made at the Blanco 4m telescope, a facility of the Cerro Tololo Inter-American Observatory, National Optical Astronomy Observatory, operated by the Association of Universities for Research in Astronomy, under contract with the National Science Foundation. Observations were also obtained at Las Cumbres Observatory Global Telescope Network and some of the scientists received support from LCOGT. The researchers used data from the UVES Paranal Observatory Project. The computations in this paper were run on the Odyssey cluster supported by the FAS Science Division Research Computing Group at Harvard University. Prieto received support from NASA’s Hubble fellowship.