It may be a bit fanciful to suggest the universe has a heartbeat but if University of Warwick (UK) researchers can state that dying stars have ‘irregular heartbeats’ then why can’t the universe have a heartbeat of sorts? Getting back to the University of Warwick, their August 26, 2015 press release (also on EurekAlert) has this to say,
Some dying stars suffer from ‘irregular heartbeats’, research led by astronomers at the University of Warwick has discovered.
The research confirms rapid brightening events in otherwise normal pulsating white dwarfs, which are stars in the final stage of their life cycles.
In addition to the regular rhythm from pulsations they expected on the white dwarf PG1149+057, which cause the star to get a few percent brighter and fainter every few minutes, the researchers also observed something completely unexpected every few days: arrhythmic, massive outbursts, which broke the star’s regular pulse and significantly heated up its surface for many hours.
The discovery was made possible by using the planet-hunting spacecraft Kepler, which stares unblinkingly at a small patch of sky, uninterrupted by clouds or sunrises.
Led by Dr JJ Hermes of the University of Warwick’s Astrophysics Group, the astronomers targeted the Kepler spacecraft on a specific star in the constellation Virgo, PG1149+057, which is roughly 120 light years from Earth.
Dr Hermes explains:
“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.”
The star with the irregular beat, PG1149+057, is a pulsating white dwarf, which is the burnt-out core of an evolved star, an extremely dense star which is almost entirely made up of carbon and oxygen. Our Sun will eventually become a white dwarf in more than six billion years, after it runs out of its nuclear fuel.
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% and its overall temperature by more than 750 degrees in a matter of an hour,” said Dr Hermes. “For context, the Sun will only increase in overall brightness by about 1% over the next 100 million years.”
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 2.5 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 analysed 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.”
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 behaviour, 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 behaviour 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,” said Dr Hermes. “Still, this is a fresh discovery from observations, and there may be more to these irregular stellar heartbeats than we can imagine yet.”
Here’s a link to and a citation for the paper,
A Second Case of Outbursts in a Pulsating White Dwarf Observed by Kepler by J. J. Hermes, M. H. Montgomery, Keaton J. Bell, P. Chote, B. T. Gänsicke, Steven D. Kawaler, J. C. Clemens, Bart H. Dunlap, D. E. Winget, and D. J. Armstrong.
2015 ApJ 810 L5 (The Astrophysical Journal Letters Volume 810 Number 1). doi:10.1088/2041-8205/810/1/L5
Published 24 August 2015.
© 2015. The American Astronomical Society. All rights reserved.
This paper is behind a paywall but there is an earlier open access version available at arXiv.org,
A second case of outbursts in a pulsating white dwarf observed by Kepler by J. J. Hermes, M. H. Montgomery, Keaton J. Bell, P. Chote, B. T. Gaensicke, Steven D. Kawaler, J. C. Clemens, B. H. Dunlap, D. E. Winget, D. J. Armstrong. arXiv.org > astro-ph > arXiv:1507.06319
In an attempt to find some live heart beats to illustrate this piece, I found this video from Wake Forest University’s body-on-a-chip program,
The video was released in an April 14, 2015 article by Joe Bargmann for Popular Mechanics,
A groundbreaking program has converted human skin cells into a network of functioning heart cells, and also fused them with lab-grown liver cells using a specialized 3D printer. Researchers at the Wake Forest Baptist Medical Center’s Institute for Regenerative Medicine provided Popular Mechanics with both still and moving images of the cells for a fascinating first look.
“The heart organoid beats because it contains specialized cardiac cells and because those cells are receiving the correct environmental cues,” says Ivy Mead, a Wake Forest graduate student and member of the research team. “We give them a special medium and keep them at the same temperature as the human body, and that makes them beat. We can also stimulate the miniature organ with electrical or chemical cues to alter the beating patterns. Also, when we grow them in three-dimensions it allows for them to interact with each other more easily, as they would in the human body.”
If you’re interested in body-on-a-chip projects, I have several stories here (suggestion: use body-on-a-chip as your search term in the blog search engine) and I encourage you to read Bargmann’s story in its entirety (the video no longer seems to be embedded there).
One final comment, there seems to be some interest in relating large systems to smaller ones. For example, humans and other animals along with white dwarf stars have heartbeats (as in this story) and patterns in a gold nanoparticle of 133 atoms resemble the Milky Way (my April 14, 2015 posting titled: Nature’s patterns reflected in gold nanoparticles).