the tree of knowledge-eureka

Black hole at heart of our galaxy erupted 2 million years ago

WASHINGTON: Scientists have for the first time found that a dormant volcano - a supermassive black hole - lying at the heart of our Milky Way galaxy last erupted two million years ago.

Astronomers have long suspected such an outburst occurred, but this is the first time it has been dated.

The evidence comes from a lacy filament of gas, mostly hydrogen, called the Magellanic Stream. This trails behind our galaxy's two small companion galaxies, the Large and Small Magellanic Clouds.

"For twenty years we've seen this odd glow from the Magellanic Stream," said lead researcher professor Joss Bland-Hawthorn at the University of Sydney, Australia, and a Fellow at the Australian Astronomical Observatory.

"We didn't understand the cause. Then suddenly we realised it must be the mark, the fossil record, of a huge outburst of energy from the centre of our galaxy," he said.
"It's been long suspected that our galactic centre might have sporadically flared up in the past. These observations are a highly suggestive 'smoking gun'," said Martin Rees, Astronomer Royal, who was one of the first people to suggest that black holes generate the power seen coming from quasars and galaxies with 'active' centres.

The galaxy's supermassive black hole is orbited by a swarm of stars whose paths help measure the black hole's mass: four million times the mass of the Sun, 'phys.org' reported.

The region around the black hole, called Sagittarius A, pours out radio waves, infrared, X-rays and gamma rays.

Infrared and X-ray satellites have seen a powerful 'wind' (outflow) of material from this central region. Antimatter boiling out has left its signature. And there are the 'Fermi bubbles' - two huge hot bubbles of gas billowing out from the galactic centre, seen in gamma-rays and radio waves.

"All this points to a huge explosion at the centre of our galaxy. What astronomers call a Seyfert flare," said team member Dr Philip Maloney of the University of Colorado in Boulder, US.

At a workshop at Stanford University in California earlier this year, researchers realised the Stream could be holding the memory of the galactic centre's past.

Struck by the fiery breath of Sagittarius A, the Stream is emitting light, much as particles from the Sun hit our atmosphere and trigger the coloured glows of the aurorae - the Northern and Southern Lights.

The brightest glow in the Stream comes from the region nearest the galactic centre.

"Geometry, the amount of energy from the original flare from Sagittarius A, the time the flare would take to travel to the Magellanic Stream, the rate at which the Stream would have cooled over time - it all fits together, it all adds up," said team member Dr Greg Madsen of the University of Cambridge in UK.

Did songbirds ‘borrow’ DNA to fuel migration?


TORONTO: A common songbird may have acquired genes from fellow migrating birds in order to travel greater distances, according to a new study.


While most birds either migrate or remain resident in one region, the Audubon's warbler, with habitat ranging from the Pacific Northwest to Mexico, exhibits different behaviours in different locations.

The northern populations breed and migrate south for the winter, while southern populations have a tendency to stay put all year long.

Evolutionary biologists have long been puzzled by research that indicates some Audubon's warblers share the same mitochondrial DNA (mtDNA) with myrtle warblers — a different species of songbird that migrates annually to the southeastern US, Central America and the Caribbean — even though they look dramatically different.

"Mitochondria are only passed down from mothers to their offspring," said David Toews, a PhD candidate in the University of British Columbia's department of zoology.

"So it's a very useful marker for differentiating species. In this case, finding two species of songbirds sharing the same mtDNA is very surprising, so we set out to find out why," Towes said.

driven by very different physics

How unusual ring of radiation is formed in space

WASHINGTON: Scientists have explained the unprecedented behaviour of a previously unknown third radiation ring that made a brief appearance between the inner and outer rings of Van Allen radiation belts in September 2012 and persisted for a month.

In the new research, UCLA space scientists have revealed that the extremely energetic particles that made up the third ring, known as ultra-relativistic electrons, are driven by very different physics than typically observed Van Allen radiation belt particles.

The region the belts occupy -- ranging from about 1,000 to 50,000 kilometers above the Earth's surface -- is filled with electrons so energetic they move close to the speed of light.

Yuri Shprits, a research geophysicist with the UCLA Department of Earth and Space Sciences, said that in the past, scientists thought that all the electrons in the radiation belts around the Earth obeyed the same physics, but the recent study shows that radiation belts consist of different populations that are driven by very different physical processes.

"The velocity of ultra-relativistic electrons, which made up the third ring and are present in both the outer and inner belts, is very close to the speed of light, and the energy of their motion is several times larger than the energy contained in their mass when they are at rest," Adam Kellerman, a staff research associate in Shprits' group, said.

Kellerman asserted that the distinction between the behavior of the ultra-relativistic electrons and those at lower energies was key to the study.

Shprits and his team found that on September 1, 2012, plasma waves produced by ions that do not typically affect energetic electrons "whipped out ultra-relativistic electrons in the outer belt almost down to the inner edge of the outer belt."

Only a narrow ring of ultra-relativistic electrons survived this storm. This remnant formed the third ring.

After the storm, a cold bubble of plasma around the Earth expanded to protect the particles in the narrow ring from ion waves, allowing the ring to persist.

Shprits' group also found that very low-frequency electromagnetic pulsations that were thought to be dominant in accelerating and losing radiation belt electrons did not influence the ultra-relativistic electrons.

Shprits, who was honored by President Obama last July with a Presidential Early Career Award for Scientists and Engineers, asserted that the Van Allen radiation belts can no longer be considered as one consistent mass of electrons since they behave according to their energies and react in various ways to the disturbances in space.

The study was published in the journal Nature Physics.