Institute of Astronomy

Dating our galaxy's dormant volcano

Published on 23/09/2013 

An artist's conception of a black hole generating a jet. Two million years ago the supermassive black hole at the centre of our Galaxy was 100 million times more powerful than it is today. Credit: NASA/Dana Berry/SkyWorks Digital

A dormant volcano — a supermassive black hole — lies at the heart of our Galaxy. Fresh evidence suggests that it last erupted two million years ago.

Astronomers have long suspected such an outburst occurred, but this is the first time they've been able to date it.

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 Professor Joss Bland-Hawthorn, an ARC Federation Fellow at the University of Sydney, Australia, and a Fellow at the Australian Astronomical Observatory, who led a team studying this problem. "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."

"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 team gives its arguments in a paper accepted for publication in The Astrophysical Journal.

The Galaxy's supermassive black hole has been known for decades. It's orbited by a swarm of stars whose paths let us measure the black hole's mass: four million times the mass of the Sun. The region around the black hole, called Sagittarius A* ["A-star"], pours out radio waves, infrared, X-rays and gamma rays. Flickers of radiation rise up when small clouds of gas fall onto the hot disk of matter that swirls around the black hole.

But evidence has been building of a real cataclysm in the past. 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," said team member Dr Philip Maloney of the University of Colorado in Boulder, USA. "What astronomers call a Seyfert flare."

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.

In the Stream, ultraviolet light splits hydrogen atoms into protons and electrons. When those components recombine, the electrons give off  'H-alpha' emission — a specific wavelength of light. 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," says team member Dr Greg Madsen of the University of Cambridge in the UK.

The Galaxy's stars don't produce enough ultraviolet to account for the glow. Nor could they have in the past, says Professor Bland-Hawthorn. "The Galactic Centre never formed stars at a high enough rate."

Will such an explosion happen again?

"There are lots of stars and gas clouds that could fall onto the hot disk around the black hole," says Professor Bland-Hawthorn.

"There's a gas cloud called G2 that we think will fall in next year. It's small, but we're looking forward to the fireworks!"

Link to movie showing a simulation of a black hole's jet.  Credits: Simulation: McKinney (UMD), Tchekhovskoy (Princeton) and Blandford (KIPAC);  Visualization: Kaehler (KIPAC)

Local (IoA) press contact:

Dr Greg Madsen, University of Cambridge, UK
T: +44 (0) 1223 765 846

J. Bland-Hawthorn, Philip R. Maloney, Ralph S. Sutherland, G.J. Madsen. "Fossil Imprint of a Powerful Flare at the Galactic Centre Along the Magellanic Stream." Accepted for publication in The Astrophysical Journal.


Page last updated: 23 September 2013 at 10:57