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A&A press release: Meteorites record past solar activity (26 September 2006)

A&A press release

Released on September 26th, 2006

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Meteorites record past solar activity

 

 

Based on the article “Long-term solar activity reconstructions: Direct test by cosmogenic 44Ti in meteorites” by Usoskin et al.

(To be published in Astronomy & Astrophysics Letters, volume 457-3, p. L25)



Original A&A article


Ilya Usoskin (Sodankylä Geophysical Observatory, University of Oulu, Finland) and his colleagues have investigated the solar activity over the past centuries. Their study is to be published this week in Astronomy & Astrophysics Letters. They compare the amount of Titanium 44 in nineteen meteorites that have fallen to the Earth over the past 240 years. Their work confirms that the solar activity has increased strongly during the 20th century. They also find that the Sun has been particularly active in the past few decades.

I. Usoksin and his colleagues have used meteorites to reconstruct past solar activity. Studying the earlier activity of our Sun is one of the oldest astrophysical projects, as astronomers began recording the number of sunspots to trace the Sun's magnetic activity four hundred years ago.

 Image

Fig. 1 - A sunspot the size of the Earth. Sunspots result from the solar magnetic activity.
Credit: Max Planck Institute for Solar System Research, Dr. Vasily Zakharov. Image taken with the Swedish Solar Telescope on the island of La Palma.
 
The international team examined a set of nineteen meteorites whose dates of fall are precisely known, and measured the amount of radioactive isotope Titanium 44 in these meteorites. Titanium 44 is produced by the cosmic rays in the meteorites while they are outside the Earth’s atmosphere. After the meteorite has fallen, it stops producing this isotope. By measuring the Titanium 44 in these meteorites, they are able to determine the level of solar activity at the time the meteorite fell.

Past solar activity is reconstructed with this technique in an independent way, that is, one not affected by terrestrial effects. How high the solar activity was at a given epoch was previously known from measuring the concentration of cosmogenic isotopes produced at that time. But most of the isotopes found on the Earth – in Greenland and Antarctic ice sheets or in tree rings, for instance – are also affected by terrestrial processes, in these examples related to the Earth’s magnetic field and climate. Until now, reconstructing past solar activity was thus very uncertain. This is shown by how various reconstructions that were previously published differ from one other. In the new study to be published this week in Astronomy & Astrophysics Letters, the team shows that the Sun is currently particularly active compared to earlier centuries.

[1] The team includes N. Bhandary (Basic Sciences Research Institute, Ahmedabad, India), G.A. Kovaltsov (Ioffe Physical-technical Institute, St. Petersburg, Russia), S.K. Solanki (Max-Planck Institute for Solar System Research, Katlenburg-Lindau, Germany), C. Taricco (Dipartimento di Fisica Generale, University of Torino, Italy) and I.G. Usoskin (University of Oulu, Finland).
 


Long-term solar activity reconstructions: Direct test by cosmogenic 44Ti in meteorites by I.G. Usoskin, S.K. Solanki, C. Taricco, N. Bhandari, G.A. Kovaltsov.
To be published in Astronomy & Astrophysics (A&A 2006, 457-3, p. L25)
Full article available in PDF format  

Contact persons:

  • Science:

Dr. Ilya Usoskin
Sodankyla Geophysical Observatory (Oulu unit)
P.O. Box 3000, FIN-90014 University of Oulu, Finland
Phone: +358-8-553 1377 - Email: ilya.usoskin (at) oulu.fi

  • Press office:

Dr. Jennifer Martin
Journal Astronomy & Astrophysics
61, avenue de l'Observatoire
75014 Paris, France
Phone: +33 1 43 29 05 41 - Email: aanda.paris (at) obspm.fr

© Astronomy & Astrophysics 2006

 

Editor-in-Chief: T. Forveille
Letters Editor-in-Chief: J. Alves
Managing Editor: C. Bertout

ISSN: 0004-6361 ; e-ISSN: 1432-0746
Frequency: 12 volumes per year
Published by: EDP Sciences

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