A stunning image from the Hubble Space Telescope and Chandra X-ray Observatory reveals a planetary nebula come back to life.
This stunning image reveals the death throes of a star not unlike the Sun. The planetary nebula Abell 30 lies 5,500 light-years away, and its central star, less than eight times the mass of the Sun, is nearing the end of its life. But not before it has its final say.
Planetary nebulae are the often-beautiful (and sometimes mysterious) shells of gas ejected from a dying, low-mass star. Sun-like stars live long, steady lives as they burn through the hydrogen in their core. As the core runs out, the star — including our future Sun — continues fusing hydrogen in a thin shell surrounding the depleted center. The star puffs up to become a red giant, denying the inevitable with a roughly hundredfold increase in size and thousandfold increase in core temperature. (The heated core can’t account for the increase in size, so the stars’ visible surface cools, turning orange in color.)
Unavoidably, the shell of hydrogen runs out as well, and the core contracts once more while the star’s outer layers puff out in a slow-motion explosion. The gas shell glides outward, in the case of Abell 30 moving less than 100,000 miles per hour. The gasping core remains, no longer a red giant, but a hot cinder. Its ultraviolet radiation and fast stellar wind, flying outward at 6 million miles per hour, slams into the slower moving gas, setting it alight in what astronomers see as a planetary nebula.
That’s what happened 12,500 years ago in Abell 30 to create the outer spherical shell seen in the wide-field image. But 850 years ago, the dying star decided it hadn’t yet said its piece. It reverted briefly to a red giant phase, long enough to choke out knots of helium and carbon-rich gas. A second, small-scale planetary nebula formed inside the first. Martín A. Guerrero (IAA-CSIC, Spain) and his colleagues investigated this second phase by zooming in on Abell 30’s heart, in a view about one light-year across, using the Chandra and XMM-Newton X-ray observatories. In their observations, Guerrero’s team found that as the fast stellar wind rams into the knots, they heat up and erode to produce the X-ray emission.
This type of stellar “rebirth” is rarely seen — only three other examples are known. The exceptional resolution of Hubble and Chandra combine to give astronomers an exquisite view of an atypical event.
While the beautiful structures created by the dying star earn most of the attention in this stunning composite image, the X-ray emission from the star itself may be the real mystery. Guerrero’s team was unable to explain the dying star’s X-ray glow, ruling out some theories and declaring others implausible. The authors describe even the best theory, a hot bubble of gas created during the star’s second explosion, as “puzzling” and “implausible.”