RECONS Mission Statement

The purpose of RECONS is to understand the nature of the Sun's nearest stellar neighbors, both individually and as a population. Our current primary goals are to discover ``missing'' members of the sample of stars within 10 parsecs (32.6 light years), and to characterize all stars within that distance limit. New members are found via astrometric, photometric, and spectroscopic techniques, or through companionship studies at small and large separations. Characterization includes photometry and spectroscopy at both optical and infrared wavelengths, as well as determinations of the luminosity function, mass function, and multiplicity fraction of the nearby stars. In the future, the RECONS effort will expand to further distances.

We request that if you use data from this website, please acknowledge RECONS.

Current support for RECONS comes from the National Science Foundation under grant AST-0507711. Our primary observing programs are carried out via the SMARTS Consortium, which operates four telescopes in the Chilean Andes under the auspices of National Optical Astronomy Observatory and the National Science Foundation.


NOTE THAT YOU CAN NOW REACH THIS RECONS HOMEPAGE FROM recons.org


RECONS Resources RECONS Latest Results RECONS Team


about the logo

The RECONS logo image is an infrared picture of the Alpha Centauri system taken while observing at the Cerro Tololo Inter-american Observatory near La Serena, Chile. The mirror cover at the 1.5m telescope, which has segments much like flower petals, was partially closed, causing the diffraction effects seen for each of the two stars, Alpha Centauri A and B. These two stars and Proxima Centauri (beyond the field of view) comprise the nearest stellar system to the Sun, which is, in fact, a triple star system.



 

 

 
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