Chameleon Star Baffles Astronomers
- By Joshua E. Brown
Pulsars — tiny spinning stars, heavier than the sun and smaller than a city — have puzzled scientists since they were discovered in 1967.
Now, new observations by an international team, including University of Vermont astrophysicist Joanna Rankin, make these bizarre stars even more puzzling.
The scientists identified a pulsar that is able to dramatically change the way in which it shines. In just a few seconds, the star can quiet its radio waves while at the same time it makes its X-ray emissions much brighter.
The research “challenges all proposed pulsar emission theories,” the team writes in the Jan. 25 edition of the journal Science and reopens a decades-old debate about how these stars work.
Like the universe’s most powerful lighthouses, pulsars shine beams of radio waves and other radiation for trillions of miles. As these highly magnetized neutron stars rapidly rotate, a pair of beams sweeps by, appearing as flashes or pulses in telescopes on Earth.
Using a satellite X-ray telescope, coordinated with two radio telescopes on the ground, the team observed a pulsar that was previously known to flip on and off every few hours between strong (or “bright”) radio emissions and weak (or “quiet”) radio emissions.
Monitoring simultaneously in X-rays and radio waves, the team revealed that this pulsar exhibits the same behavior, but in reverse, when observed at X-ray wavelengths.
This is the first time that a switching X-ray emission has been detected from a pulsar.
Flipping between these two extreme states — one dominated by X-ray pulses, the other by a highly organized pattern of radio pulses — “was very surprising,” says Rankin.
“As well as brightening in the X-rays we discovered that the X-ray emission also shows pulses, something not seen when the radio emission is bright,” said Rankin, who spearheaded the radio observations. “This was completely unexpected.”
No current model of pulsars is able to explain this switching behavior. All theories to date suggest that X-ray emissions would follow radio emissions. Instead, the new observations show the opposite. “The basic physics of a pulsar have never been solved,” Rankin says.
Looking for the switch
The research was conceived by a small team then working at the University of Amsterdam, including UVM’s Rankin, who has studied this pulsar, known as PSR B0943+10, for more than a decade; Wim Hermsen from SRON, the Netherlands Institute for Space Research in Utrecht, and the lead author on the new paper; Ben Stappers from the University of Manchester, UK; and Geoff Wright from Sussex University, UK.
These researchers were joined by colleagues from institutions around the world to conduct simultaneous observations with the European Space Agency’s X-ray satellite, XMM-Newton, and two radio telescopes, the Giant Meter Wave Telescope (GMRT) in India and the Low Frequency Array (LOFAR) in the Netherlands, to reveal this pulsar’s so-far unique behavior.
“There is a general agreement about the origin of the radio emission from pulsars: it is caused by highly energetic electrons, positrons and ions moving along the field lines of the pulsar's magnetic field,” explains Wim Hermsen.
“How exactly the particles are stripped off the neutron star's surface and accelerated to such high energy, however, is still largely unclear,” he adds.
By studying the emission from the pulsar at different wavelengths, the team’s study had been designed to discover which of various possible physical processes take place in the vicinity of the magnetic poles of pulsars.
Instead of narrowing down the possible mechanisms suggested by theory, however, the results of the team’s observing campaign challenge all existing models for pulsar emission. Few astronomical objects are as baffling as pulsars, and despite nearly fifty years of study, they continue to defy theorists’ best efforts.
Hunting for gravity's wave
And understanding the basic physics of pulsars is important to one of the great science quests of this century: the hunt for gravitational waves.
First predicted by Albert Einstein in 1916 these waves ripple through the fabric of space and time, carrying information from the far edges of the universe. Astronomers hope that being able to measure gravitational waves will open a whole new spectrum of energy — gravitational energy — for observing the universe and will reveal cosmological mysteries such as the location of exotic “dark matter.”
But, so far, no one has been able to directly detect these gravitational waves — because they are so tiny.
This is where pulsars may help.
Because of their extreme density and enormous speed, pulsars turn out to be a nearly perfect flywheel, ticking along as the universe’s best clock. The arrival of pulses can be so regular that emissions from a group of pulsars is being studied by NANOGrav — an international consortium of scientists including Rankin — to distinguish the faint signal of passing gravitational waves from all the other noise of the universe.
Disturbances in the arrival time of pulsar pulses — i.e., deviations in the ticking of the clock — will show that a gravitational wave has passed by the Earth.
But pulsars, as this new research makes clear, have strange glitches, mysteries, and disturbances of their own.
“The NANOGrav effort and others are pushing the (pulsar) clock so hard that it is becoming clear that if we don’t understand the clock better,” Rankin says. “it may not work as a tool as well as it could.”
“We need to understand the complexities of pulsars,” Rankin says, “we need to see them as more than just a clock in the sky.”
Erratic star power
Of the more than 2,000 pulsars discovered to date, a number of them have erratic behavior, with emissions that can become weak or disappear in a matter of seconds but then suddenly return minutes or hours later.
B0943+10 is one of these erratic stars. Discovered at Pushchino Radio Astronomical Observatory near Moscow, “this star has two very different personalities,” that were uncovered by Svetlana Suleymanova in the 1980s, says Rankin.
“But we’re still in the dark about what causes this, and other pulsars, to switch modes,” Rankin says. “We just don’t know.”
“But the fact that the pulsar keeps memory of its previous state and goes back to it,” says Hermsen, “suggests that it must be something fundamental."
These new observations “strongly suggest that a temporary ‘hotspot’ appears close to the pulsar’s magnetic pole which switches on and off with the change of state,” says Geoff Wright, one of the team’s astronomers from the University of Sussex.
But the new results also suggest that something in the pulsar's whole magnetosphere is changing suddenly and not just at the poles or other hotspots. “Something is happening globally,” Rankin says, across the whole star.
In order for the radio emission to vary so radically on the short timescales observed, the pulsar's global environment must undergo a very rapid – and reversible – transformation.
“If that is true, it means the entire magnetosphere is alive and connected in very important ways,” Rankin says, allowing a change in the pulsar’s basic mode of shining in about one second, less time than it takes it to spin once on its axis.
“Since the switch between a pulsar's bright and quiet states links phenomena that occur on local and global scales, a thorough understanding of this process could clarify several aspects of pulsar physics,” says Hermsen. “Unfortunately, we have not yet been able to explain it.”
In the second half of 2013, the team plans to repeat the same study for another pulsar, PSR B1822-09, which exhibits similar radio emission properties but with a different geometry.
In the meantime, these observations will keep theoretical astrophysicists busy investigating possible physical mechanisms that could cause the sudden and drastic changes to the pulsar's entire magnetosphere and result in such a curious flip in how they shine.