A fraction of a second after the Big Bang, all the primordial soup of matter in the Universe was ‘broken’ into its most fundamental constituents. It was thought to have disappeared forever. However scientists strongly suspect that the exotic soup of dissolved matter can still be found in today’s Universe, in the core of certain very dense objects called neutron stars.
With ESA’s space telescope XMM-Newton, they are now closer to test this idea. For the first time, XMM-Newton has been able to measure the influence of the gravitational field of a neutron star on the light it emits. This measurement provides much better insight into these objects.
Neutron stars are among the densest objects in the Universe. They pack the mass of the sun inside a sphere 10 kilometres across. A sugar cube-sized piece of neutron star weighs over a billion tonnes. Neutron stars are the remnants of exploding stars up to eight times more massive than our Sun. They end their life in a supernovae explosion and then collapse under their own gravity. Their interior may therefore contain a very exotic form of matter.
Scientists believe that in a neutron star, the density and the temperatures are similar to those existing a fraction of a second after the Big Bang. They assume that when matter is tightly packed as it is in a neutron star, it goes through important changes. Protons, electrons, and neutrons – the components of atoms – fuse together. It is possible that even the building-blocks of protons and neutrons, the so-called quarks, get crushed together, giving rise to a kind of exotic plasma of ‘dissolved’ matter.
How to find out? Scientists have spent the last decades trying to identify the nature of matter in neutron stars. To do this, they need to know some important parameters, very precisely. If you know a star’s mass and radius, or the relationship between them, you can obtain its ‘compactness’. However, no instrument was advanced enough to perform the measurements needed, until now. Thanks to ESA’s XMM-Newton observatory, for the first time, astronomers have been able to measure the mass-to-radius ratio of a neutron star and acquire the first clues about its composition. These clues suggest that the neutron star contains normal, non-exotic matter, although they are not conclusive. The authors say this is a ‘key first step’ and that they will keep on with the search.
The way they got this measurement is a first in astronomical observation and it is considered a huge achievement. The method consists of determining the compactness of the neutron star in an indirect way. The gravitational pull of a neutron star is immense – thousands of million times stronger than the Earth’s. This makes the light particles emitted by the neutron star lose energy. This energy loss is called a gravitational ‘red shift’. The measurement of this red shift by XMM-Newton indicated the strength of the gravitational pull, and revealed the star’s compactness.
“This is a highly precise measurement that could not have been done without both the high sensitivity of XMM-Newton and its ability to distinguish details.” says Fred Jansen, ESA’s XMM-Newton Project Scientist.
According to the main author of the discovery, Jean Cottam of NASA Goddard Space Flight Center (Greenbelt, United States), “attempts to measure the gravitational red shift were made right after Einstein published the General Theory of relativity, but no one had ever been able to measure the effect in a neutron star, where it was supposed to be huge. This has now been confirmed.”
Note to editors
The result was obtained by observations of the neutron star EXO 0748-676. XMM-Newton detected the light in the form of X-rays. In particular, thanks to the analysis of this X-ray radiation, the astronomers were able to identify some chemical elements, namely iron, present in the material surrounding the neutron star. They then compared the distorted signal emitted by the iron atoms in the neutron star with the one produced by iron atoms in the laboratory. In this way, they could measure the actual degree of distortion due to the gravity of EXO 0748-676.
The result has been published in the 7 November 2002 issue of Nature. The lead author is Jean Cottam, of NASA Goddard Space Flight Center (Greenbelt, United States). Other authors are Mariano Mendez, of the National Institute for Space Research , SRON (The Netherlands); and Frits Paerels of Columbia University (New York, United States).
For more information please contact:
ESA Communication Department
Media Relations Office
Paris, France
Tel: +33 (0)1 53 69 7155
Fax: +33 (0)1 53 69 7690
Dr Fred Jansen
ESA XMM-Newton Project Scientist
Tel: +31 (0)71 565 4426
E-mail: fjansen@rssd.esa.int
Dr Jean Cottam
NASA Goddard Space Flight Center
Laboratory for High Energy Astrophysics
United States
Tel: +1 301 286 1586
E-mail: jcottam@milkyway.gsfc.nasa.gov
