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A stellar black hole
A stellar black hole can be seen when it rips a companion star to pieces
The densest objects in the Universe
 
When a massive star explodes, not all the material is ejected into space. Some of it collapses into an extremely compact object known as a neutron star, inside which gravitational forces crush protons and electrons together, turning them into particles known as neutrons.
 
A neutron star contains a few solar masses of material squeezed into a radius of only 20 km. This means the matter is so compressed that a thimble full of it would weigh millions of tonnes on Earth. Fast-spinning neutron stars, whose radio emissions seem to pulse on and off, are called pulsars.

Beyond the mass limit of a neutron star - about three solar masses - gravity becomes overwhelming and collapses the star even further, creating a black hole. These are perhaps the strangest objects in the Universe because nothing, not even light, can escape from inside a black hole. So, the presence of a black hole can only be inferred by its effect on surrounding celestial objects and other interstellar material.  
 
A neutron star
A neutron star
Virtually all types of compact objects are significant sources of high-energy emission because of the enormous gravitational fields they tend to generate. Gravitational fields can accelerate particles in the vicinity to extreme velocities, which then emit gamma rays and X-rays.

Integral will capture images of the high-energy emission from such compact objects with unprecedented detail, allowing astronomers a clearer look than ever before at these enigmatic objects.
 
 
Last update: 15 October 2002

 


ESA's gamma-ray astronomy missionArtist's view of Integral
Observations: Seeing in the gamma-ray wavelengthsObservations: Seeing in X-ray wavelengths
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The densest objects in the Universe
 
 
 
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