Astronomers using the planet-hunting spacecraft Kepler have discovered a dying star with irregular pulsations that cause the star to get a few percent brighter and fainter every few minutes.
They also observed massive outbursts every few days that significantly heated up its surface for many hours.
The star, a white dwarf called PG1149+057, is in the constellation Virgo, which is roughly 120 light years from Earth. Our sun will eventually become a white dwarf in more than six billion years, after it runs out of its nuclear fuel.
“We have essentially found rogue waves in a pulsating star, akin to ‘irregular heartbeats,’ These were truly a surprise to see: we have been watching pulsating white dwarfs for more than 50 years now from the ground, and only by being able to stare uninterrupted for months from space have we been able to catch these events,” says JJ Hermes of the University of Warwick’s Astrophysics Group, who led the project.
15% brighter in an hour
White dwarfs have been known to pulsate for decades, and some are exceptional clocks, with pulsations that have kept nearly perfect time for more than 40 years. Pulsations are believed to be a naturally occurring stage when a white dwarf reaches the right temperature to generate a mix of partially ionized hydrogen atoms at its surface.
That mix of excited atoms can store up and then release energy, causing the star to resonate with pulsations characteristically every few minutes. Astronomers can use the regular periods of these pulsations just like seismologists use earthquakes on Earth, to see below the surface of the star into its exotic interior.
This was why astronomers targeted PG1149+057 with Kepler, hoping to learn more about its dense core. In the process, they caught a new glimpse at these unexpected outbursts.
“These are highly energetic events, which can raise the star’s overall brightness by more than 15 percent and its overall temperature by more than 750 degrees in a matter of an hour,” says Hermes. “For context, the sun will only increase in overall brightness by about 1 percent over the next 100 million years.”
Not the only star
Interestingly, this is not the only white dwarf to show an irregular pulse. Recently, the Kepler spacecraft witnessed the first example of these strange outbursts while studying another white dwarf, KIC 4552982, which was observed from space for more than 2 years.
There is a narrow range of surface temperatures where pulsations can be excited in white dwarfs, and so far irregularities have only been seen in the coolest of those that pulsate. Thus, these irregular outbursts may not be just an oddity; they have the potential to change the way astronomers understand how pulsations, the regular heartbeats, ultimately cease in white dwarfs.
“The theory of stellar pulsations has long failed to explain why pulsations in white dwarfs stop at the temperature we observe them to,” argues Keaton Bell of the University of Texas at Austin, who analyzed the first pulsating white dwarf to show an irregular heartbeat, KIC 4552982.
“That both stars exhibiting this new outburst phenomenon are right at the temperature where pulsations shut down suggests that the outbursts could be the key to revealing the missing physics in our pulsation theory.”
What’s going on?
Astronomers are still trying to settle on an explanation for these never-before-seen outbursts. Given the similarity between the first two stars to show this behavior, they suspect it might have to do with how the pulsation waves interact with themselves, perhaps via a resonance.
“Ultimately, this may be a new type of nonlinear behavior that is triggered when the amplitude of a pulsation passes a certain threshold, perhaps similar to rogue waves on the open seas here on Earth, which are massive, spontaneous waves that can be many times larger than average surface waves,” says Hermes. “Still, this is a fresh discovery from observations, and there may be more to these irregular stellar heartbeats than we can imagine yet.”
The research appears in the Astrophysical Journal Letters.
This text is published here under a Creative Commons License.
Author: Lee Page-University of Warwick
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