Stardust discovered in far-off planetary systems

Sep 29, 2011
Astronomers from Jena University found a stardust belt around the stars TrES-2 in the Draco constellation and XO-5 in the Lynx constellation. Credit: WISE Image Service

Searching for extra-solar planets -- which are planets outside of our solar system -- is very popular these days. About 700 planets are known at the moment, a number that is continuously rising due to refined observational techniques. Professor Alexander Krivov and his team of astronomers of the Friedrich Schiller University Jena (Germany) just made a remarkable discovery: the scientists from the Astrophysical Institute were able to establish proof of so-called debris discs around two stars.

The debris discs are remnants of the formation of the planets. "We are dealing with enormous accumulations of chunks of matter which create dust when they collide", Alexander Krivov says. This dust is of greatest importance for the astronomers, because it helps to draw conclusions about the . There are even two debris discs in our solar system, the and the amongst whose bodies the dwarf planet Pluto belongs.

What makes the Jena discovery so special is the tremendous distance from our to the stars with the debris discs. "These stars are hundreds of light years away from the Earth", according to Krivov. The particular focus is on TrES-2 in the Draco constellation and XO-5 in the Lynx constellation. Planets orbiting these stars can only be detected with the help of the transit method. It sounds like a simple principle: The is photographed in regular intervals. Special software then checks the brightness of the stars on the images. If, in regular intervals, there are differences in brightness it is likely that a planet passes between the star and its observers.

The astronomers found evidence for the stardust with the help of photometric analysis. At first the characteristics of the stars can be analysed with it. If there are irregularities in the invisible , they point to the existence of stardust. Krivov says: "The dust is warmed up by the star and radiates heat. We see that radiation curve is above the radiation curve of the star as a clear sign of the existence of stardust."

Professor Krivov draws an impressive comparison for the search of debris discs in the vastness of the universe: it is as if you would detect an ice-cream cooled down to minus 130 degrees with a heat detector in a 5,000 kilometer distance from Jena.

Explore further: A spectacular landscape of star formation

More information: Alexander Krivov's team of scientists concentrated its search for debris disc candidates on about 100 known extra-solar systems with transiting planets. Of these systems, they found 52 in the observational results of the US-American space telescope WISE published in April this year. The Jena scientists got lucky with two systems. As early as June 1 Alexander Krivov, Martin Reidemeister, Simone Fiedler, Dr. Torsten Löhne und Professor Ralph Neuhäuser submitted their paper to the science magazine 'Monthly Notices of the Royal Astronomical Society' for publication in the 'Letters' section. Meanwhile the paper has been published under the title 'Debris disc candidates in systems with transiting planets' doi:10.1111/j.1745-3933.2011.01133.x

Provided by Friedrich-Schiller-Universitaet Jena

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1 / 5 (6) Sep 29, 2011
scientists were able to establish proof of so-called debris discs around two stars.


First-formed dust in the solar system was poorly-mixed stellar debris!

Here are a few of the experimental data:

Here are a few of the conclusions:

1. "Elemental and isotopic inhomogeneities in noble gases: The case for local synthesis of the chemical elements", Trans MO Acad Sci 9, 104-122 (1975)

2. "Strange xenon, extinct super-heavy elements, and the solar neutrino puzzle", Science 195, 208-209 (1977)

3. "Isotopes of tellurium, xenon and krypton in the Allende meteorite retain record of nucleosynthesis", Nature 277, 615-620 (1979)

Oliver K. Manuel