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The Last Cry of Matter from a Black Hole

Posted on: Friday, 28 November 2003, 06:00 CST

European Space Agency -- ‘Black holes’ are truly black. When an object gets within a certain distance from a black hole, it will get swallowed forever with no chance to escape. That includes light, which means that black holes do not shine.

How do astronomers detect black holes if they are unable to see them? Well, to be precise, astronomers do not detect black holes. But they do detect the phenomena that can only be explained by the existence nearby of objects that match the description of black holes!

The strong gravitational attraction of a black hole affects the motion of nearby objects. When astronomers see a star circling around something, but they cannot see what that something is, they may suspect it is a black hole, or a neutron star - the ultra-dense ‘corpse’ of a star.

Astronomers can even infer the mass of a black hole by measuring the mass of the star and its speed. The same kind of calculation can be done whith supermassive black holes that lurk at the centre of many galaxies, including our own galaxy, the Milky Way.

In the Milky Way, observations have revealed the existence of stars and gas moving very fast near the centre, a behaviour that can only be explained if a mass of several million times that of the Sun is at the centre of the galaxy.

Such mass has to be concentrated within a radius of only 10 light-days - roughly 40 times times the distance from the Sun to Pluto - and is most likely to be a black hole.

In fact, at the very centre of our galaxy, radio and X-ray telescopes have detected a powerful source called ‘Sagittarius A’, identified as the candidate to be this massive black hole.

This idea has recently received strong support, with the measurement for the first time of the orbit of a star that approaches this mysterious object to within 17 light-hours - only three times the distance between the Sun and Pluto - while travelling at speeds of than 5000 kilometres per second!

Shining to death

Another piece of evidence in favour of the idea of supermassive black holes in the centre of galaxies is the existence of quasars, discovered in 1967. Quasars are very distant and very luminous at the same time - the most luminous objects in the Universe.

To explain the incredible amount of energy they must release, astronomers also need black holes: just before disappearing into a black hole, the matter being swallowed heats up and emits great amounts of energy - its ‘last cry’. So quasars are believed to be caused by black holes with masses of one million to several billion times the mass of the Sun.

The ‘last cry’ of matter about to be swallowed is best detected with x-ray and gamma-ray telescopes, because the energy released is given off in the form of hard x-rays. In fact, ESA’s orbiting observatories XMM-Newton and Integral have already shown their skills in studying black holes in several discoveries.

For example, XMM Newton has recently discovered a small black hole whirling in our galaxy, in the Ara constellation of the southern sky.

Integral has detected what could be the first significant hard x-ray emission from the black hole in the centre of our galaxy.

Graphical depiction of gas swirling around a black hole before falling into it. Credits: ESA

Artist's rendition of the XMM-Newton spacecraft. Credit: ESA

The task of Integral, ESA's International Gamma-Ray Astrophysics Laboratory, is to gather the most energetic radiation that comes from space. Credits: ESA. Illustration by D. Ducros

About INTEGRAL

The task of INTEGRAL, ESA's International Gamma-Ray Astrophysics Laboratory, is to gather some of the most energetic radiation that comes from space. The spacecraft was launched on 17 October 2002 and it may help to solve some of the biggest mysteries in astronomy.

INTEGRAL is a truly international mission with the participation of all member states of ESA plus the United States, Russia, Czech Republic, and Poland. ESA appointed Alenia Spazio, Italy, as industrial prime contractor, responsible for the design, integration and testing of the satellite. On board, four instruments from teams led by scientists in Italy, France, Germany, Denmark, and Spain are today gathering and analysing the gamma-rays from space.

About XMM-Newton

After launch from Kourou, French Guiana on 10 December 1999, the European Space Agency's X-ray Multi-Mirror satellite is the most powerful X-ray telescope ever placed in orbit. Scientists are sure the mission will help solve many cosmic mysteries, ranging from enigmatic black holes to the formation of galaxies.

Many celestial objects generate X-rays in extremely violent processes. But Earth's atmosphere blocks out these X-rays, messengers of what occurred in the distant past when stars were born or died, and clues to our future. Only by placing X-ray detectors in space can such sources be detected, pinpointed and studied in detail. XMM-Newton, the largest science satellite ever built in Europe, has an unprecedented sensitivity.

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On the Net:

INTEGRAL Mission Home Page

XMM-Newton Mission Home Page

Black Holes -- learn more

European Space Agency

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