A strange, pulsing star has revealed a powerful magnetic field around the giant black hole at the heart of Earth's Milky Way galaxy, scientists say.
The finding may help shed light on how the galaxy's supermassive black hole devours matter around it and spits out powerful jets of superhot matter, the researchers added.
The center of virtually every large galaxy is suspected to host a supermassive black hole with a mass that can range from millions to billions of times the mass of the sun. Astronomers think the Milky Way's core is home to the monster black hole called Sagittarius A* - pronounced "Sagittarius A-star" - that is about 4 million times the mass of Earth's sun. [No Escape: How Black Holes Work (Infographic)]
Scientists want to learn more about how black holes distort the universe around them, hoping to see if the leading theory regarding black holes, Einstein's theory of general relativity, holds up or if new concepts might be necessary. One way to see how black holes warp space and time is by looking at clocks near them. Cosmic versions of clocks are known as pulsars - rapidly spinning neutron stars that regularly give off pulses of radio waves.
Artist's impression of PSR J1745-2900, a pulsar with a very high magnetic field ("magnetar") potentially just less than half a light year from the supermassive black hole at the center of the Milky Way galaxy. The pulsar helped reveal the magnetic field around the Milky Way's supermassive black hole. Image released Aug. 14, 2013. Credit: Ralph Eatough/MPIfR
Pulsar tells the tale
Astronomers have been searching for pulsars near Sagittarius A* for the past 20 years.
Earlier this year, NASA's NuSTAR telescope helped confirm the existence of such a pulsar apparently less than half a light-year away from the black hole, one that pulsates radio signals every 3.76 seconds. Scientists quickly analyzed the pulsar using the Effelsberg Radio Observatory of the Max Planck Institute for Radio Astronomy in Bonn, Germany.
"On our first attempt, the pulsar was not clearly visible, but some pulsars are stubborn and require a few observations to be detected," said study lead author Ralph Eatough, an astrophysicist at the Max Planck Institute for Radio Astronomy in Bonn, Germany. "The second time we looked, the pulsar had become very active in the radio band and was very bright. I could hardly believe that we had finally detected a pulsar in the galactic center." [See a video of the pulsar and zoom in on the Milky Way's black hole]
Additional observations were performed in parallel and subsequently with other radio telescopes around the world. "We were too excited to sleep in between observations," said study co-author Evan Keane from the Jodrell Bank Observatory in England.
The newfound pulsar, named PSR J1745-2900, belongs to a rare kind of pulsars known as magnetars, which only make up about 1 out of every 500 pulsars found to date. Magnetars possess extremely powerful magnetic fields, ones about 1,000 times stronger than the magnetic fields of ordinary neutron stars, or 100 trillion times the Earth's magnetic field.
The radio pulses from magnetars are highly polarized, meaning these signals oscillate along one plane in space. This fact helped the researchers detect a magnetic field surrounding Sagittarius A*.
This image shows the Effelsberg radio telescope during regular observations of the Galactic Center region for unidentified pulsars. The Galactic Center is in the Sagittarius constellation and is only visible for approximately 2 hours and 25 minutes every day. Image released Aug. 14, 2013. Credit: MPIfR/Ralph Eatough
Black hole magnetic field revealed
Black holes swallow their surroundings, mainly hot ionized gas, in a process of accretion. Magnetic fields threading within this accretion flow can influence how this infalling gas is structured and behaves.
"The magnetic field we measure around the black hole can regulate the amount of matter the black hole eats and could even cause it to spit matter out in so-called jets," Eatough told SPACE.com. "These measurements are therefore of great importance in understanding how supermassive black holes feed, a process that can affect galaxy formation and evolution."
As radio signals traverse the magnetized gas around black holes, the way they are polarized gets twisted depending on the strength of the magnetic fields. By analyzing radio waves from the magnetar, the researchers discovered a relatively strong, large-scale magnetic field pervades the area surrounding Sagittarius A*.
In the area around the pulsar, the magnetic field is about 100 times weaker than Earth's magnetic field. However, "the field very close to the black hole should be much stronger - a few hundred times the Earth's magnetic field," Eatough said.
If the magnetic field generated by the infalling gas is accreted down to the event horizon of the black hole - its point of no return - that could help explain the radio and X-ray glow long associated with Sagittarius A*, researchers added.
"It is amazing how much information we can extract from this single object," said study co-author Adam Deller at the Netherlands Institute for Radio Astronomy in Dwingeloo.
Astronomers predict there should be thousands of pulsars around the center of the Milky Way. Despite that, PSR J1745-2900 is the first pulsar discovered there. "Astronomers have searched for decades for a pulsar around the central black hole in our galaxy, without success. This discovery is an enormous breakthrough, but it remains a mystery why it has taken so long to find a pulsar there," said study co-author Heino Falcke at Radboud Universiteit Nijmegen in the Netherlands.
"It could be the environment is very dense and patchy, making it difficult to see other pulsars," Eatough added.
The researchers cannot test the leading theory regarding black holes using PSR J1745-2900 - they cannot measure the way it warps space-time accurately enough, since the pulsar is slightly too far away from Sagittarius A* and, being relatively young, its spin is too variable. The researchers suggest pulsars that are closer to the black hole and are older with less variable spins could help test the theory.
"If there is a young pulsar, there should also be many older ones. We just have to find them," said study co-author Michael Kramer, director of the Max Planck Institute for Radio Astronomy.
The scientists detailed their findings online Aug. 14 in the journal Nature.
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