Ocean eddies are similar to black holes

Ocean eddies are similar to black holes
WASHINGTON: Some of the largest ocean eddies on Earth are mathematically equivalent to the mysterious black holes of space, scientists say.

These eddies are so tightly shielded by circular water paths that nothing caught up in them escapes.

George Haller, Professor of Nonlinear Dynamics at ETH Zurich, and Francisco Beron-Vera, Research Professor of Oceanography at the University of Miami, have developed a new mathematical technique to find water-transporting eddies with coherent boundaries.

The challenge in finding such eddies is to pinpoint coherent water islands in a turbulent ocean. The rotating and drifting fluid motion appears chaotic to the observer both inside and outside an eddy.

Haller and Beron-Vera were able to restore order in this chaos by isolating coherent water islands from a sequence of satellite observations. To their surprise, such coherent eddies turned out to be mathematically equivalent to black holes.

Black holes are objects in space with a mass so great that they attract everything that comes within a certain distance of them. Nothing that comes too close can escape, not even light.

But at a critical distance, a light beam no longer spirals into the black hole. Rather, it dramatically bends and comes back to its original position, forming a circular orbit.

Haller and Beron-Vera discovered similar closed barriers around select ocean eddies. In these barriers, fluid particles move around in closed loops ? similar to the path of light in a photon sphere. And as in a black hole, nothing can escape from the inside of these loops, not even water.

It is these barriers that help to identify coherent ocean eddies in the vast amount of observational data available. The very fact that such coherent water orbits exist amidst complex ocean currents is surprising, researchers said.

Because black-hole-type ocean eddies are stable, they function in the same way as a transportation vehicle - not only for micro-organisms such as plankton or foreign bodies like plastic waste or oil, but also for water with a heat and salt content that can differ from the surrounding water.

Haller and Beron-Vera have verified this observation for the Agulhas Rings, a group of ocean eddies that emerge regularly in the Southern Ocean off the southern tip of Africa and transport warm, salty water northwest.

The researchers identified seven Agulhas Rings of the black-hole type, which transported the same body of water without leaking for almost a year.

Haller points out that similar coherent vortices exist in other complex flows outside of the ocean. In this sense, many whirlwinds are likely to be similar to black holes as well.

The study was published in the Journal of Fluid Mechanics.

Spinning CDs to clean sewage water

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WASHINGTON:Wondering what to do with your obsolete audio CDs? Researchers have come up with a practical application: they can be used to break down sewage.

"Optical disks are cheap, readily available, and very commonly used," said Din Ping Tsai, a physicist at National Taiwan University. Close to 20 billion disks are already manufactured annually, the researchers noted.

Tsai and his colleagues used the large surface area of optical disks as a platform to grow tiny, upright zinc oxide nanorods about a thousandth the width of a human hair. Zinc oxide is an inexpensive semiconductor that can function as a photocatalyst, breaking apart organic molecules like the pollutants in sewage when illuminated with UV light.

As the disks are durable and able to spin quickly, contaminated water that drips onto the device spreads out in a thin film that light can easily pass through, speeding up the degradation. The team's complete water treatment device is approximately one cubic foot in volume. The device also consists of a UV light source and a system that recirculates the water to further break down the pollutants.

The team tested the reactor with a solution of methyl orange dye. After treating a half-litre solution for 60 minutes, they found that over 95% of the contaminants had been broken down.

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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.