Three examples of a new family of planets, which orbit a pair of stars rather than a single one, have been discovered. The Milky Way may contain millions of these circumbinary planets. See Letter p.475
This is a preview of subscription content, access via your institution
Access options
Subscribe to this journal
Receive 51 print issues and online access
$199.00 per year
only $3.90 per issue
Buy this article
- Purchase on Springer Link
- Instant access to full article PDF
Prices may be subject to local taxes which are calculated during checkout
Notes
*This article and the paper2 under discussion were published online on 11 January 2012.
References
Doyle, L. R. et al. Science 333, 1602–1606 (2011).
Welsh, W. F. et al. Nature 481, 475–479 (2012).
Mayor, M. & Queloz, D. Nature 378, 355–359 (1995).
Bakos, G. Á., Lázár, J., Papp, I., Sári, P. & Green, E. M. Publ. Astron. Soc. Pacif. 114, 974–987 (2002).
Pollacco, D. L. et al. Publ. Astron. Soc. Pacif. 118, 1407–1418 (2006).
Anderson, D. R. et al. Astrophys. J. 709, 159–167 (2010).
Hellier, C. et al. Nature 460, 1098–1100 (2009).
Author information
Authors and Affiliations
Corresponding author
Rights and permissions
About this article
Cite this article
Southworth, J. A new class of planet. Nature 481, 448–449 (2012). https://doi.org/10.1038/nature10818
Published:
Issue Date:
DOI: https://doi.org/10.1038/nature10818
