NASA unravels mysteries of huge space explosion
In the constellation of Carina, lies the most luminous and mysterious star system within 10,000 light-years. The two massive stars, better known as Eta Carinae, erupted twice in the 19th 聽Century for reasons astronomers still don鈥檛 understand, and are now approaching the point where one might soon detonate as a supernova.
Astronomers from the 225th 聽meeting of the American Astronomical Society weighed in on this supermassive showoff earlier today. New findings include 3-D printed models that reveal never-before-seen features of the stars鈥� interactions.
But first, let鈥檚 better orient ourselves with this elusive system. The brighter, primary star has about 90 times the mass of the Sun and outshines it five million times. The properties of the smaller, companion star are still hotly contested. Both stars produce powerful gaseous outflows called stellar winds. Although these winds enshroud the stars, blocking all efforts to directly observe them, the gas is hot and dense enough to emit observable X-rays.
The X-ray emission, however, dramatically changes when the stars reach their point of closest approach, or periastron. As the stars approach one another, their X-ray output gradually brightens, reaching a maximum when the stars are as close as Mars is to the Sun. But just past periastron, the X-rays drop suddenly as the companion star quickly moves around the primary star.
Now, a research team has developed a 3-D simulation, looking at 11 years worth of data and three periastron passages, from multiple NASA satellites and ground-based telescopes.
According to the team鈥檚 model, the winds from each star have different properties. The primary star鈥檚 winds are extremely slow, blowing out at one million miles per hour, while the hotter companion star鈥檚 winds are much faster, clocking in at a speed six times greater. The primary star鈥檚 winds are also extremely dense, carrying away the equivalent mass of our Sun every thousand years, while the companion鈥檚 wind carries off 100 times less material.
But the research team didn鈥檛 stop there. 鈥淯sing a commercial 3-D printer 鈥� we have found a way to 3-D print the output from our computer simulations of Eta Car,鈥� said Thomas Madura, also from NASA Goddard Space Flight Center. 鈥淎nd as far as we are aware these are the world鈥檚 first 3-D prints of a supercomputer simulation of a complex astrophysical system.鈥�
The printed model can be separated into two sections: the dense wind from the primary star and the more tenuous wind from the companion star. Slicing the model in half therefore reveals the cavity carved by the companion star鈥檚 wind into the primary star鈥檚 wind.
鈥淎s a result of doing this 3-D printing work, we actually discovered these finger-like protrusions that extend radially out of the spiral wind-wind collision region,鈥� said Madura. 鈥淭hese are features that we didn鈥檛 even really know existed鈥� prior to this. They鈥檙e likely the result of physical instabilities that arise when the fast wind collides with the slower wind, which is essentially a wall of gas.
Both of the massive stars of Eta Carinae might one day end their lives in supernova explosions. 鈥淔or stars, mass determines their destiny. But for massive stars, mass loss determines their destiny,鈥� said Michael Corcoran from the NASA Goddard Space Flight Center.
Although the stars continue to lose mass at high rates, there is no evidence to suggest an imminent demise of either star.
聽is a freelance science journalist. She holds two B.A.'s from Whitman College in physics-astronomy and philosophy, and an M.S. in astronomy from the University of Wyoming. Currently, she is working toward a second M.S. from NYU's Science, Health and Environmental Reporting program. You can follow her on Twitter聽.
