Hostname: page-component-8448b6f56d-mp689 Total loading time: 0 Render date: 2024-04-18T22:27:51.269Z Has data issue: false hasContentIssue false
  • English
  • Français

The MEarth project: searching for transiting habitable super-Earths around nearby M dwarfs

Published online by Cambridge University Press:  01 May 2008

Jonathan Irwin ,
David Charbonneau ,
Philip Nutzman  and
Emilio Falco
Jonathan Irwin
Affiliation:
Harvard-Smithsonian Center for Astrophysics, 60 Garden Street, Cambridge, MA 02138, USA email: jirwin@cfa.harvard.edu
David Charbonneau
Affiliation:
Harvard-Smithsonian Center for Astrophysics, 60 Garden Street, Cambridge, MA 02138, USA email: jirwin@cfa.harvard.edu
Philip Nutzman
Affiliation:
Harvard-Smithsonian Center for Astrophysics, 60 Garden Street, Cambridge, MA 02138, USA email: jirwin@cfa.harvard.edu
Emilio Falco
Affiliation:
Harvard-Smithsonian Center for Astrophysics, 60 Garden Street, Cambridge, MA 02138, USA email: jirwin@cfa.harvard.edu
Rights & Permissions [Opens in a new window]

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

Due to their small radii, M dwarfs are very promising targets to search for transiting super-Earths, with a planet of 2 Earth radii orbiting an M5 dwarf in the habitable zone giving rise to a 0.5% photometric signal, with a period of two weeks. This can be detected from the ground using modest-aperture telescopes by targeting samples of nearby M dwarfs. Such planets would be very amenable to follow-up studies due to the brightness of the parent stars, and the favourable planet-star flux ratio. MEarth is such a transit survey of ~2000 nearby M dwarfs. Since the targets are distributed over the entire (Northern) sky, it is necessary to observe them individually, which will be done by using 8 independent 0.4m robotic telescopes, two of which have been in operation since December 2007 at the Fred Lawrence Whipple Observatory (FLWO) located on Mount Hopkins, Arizona. We discuss the survey design and hardware, and report on the current status of the survey, and preliminary results obtained from the commissioning data.

Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 4 , Symposium S253: Transiting Planets , May 2008 , pp. 37 - 43
Copyright
Copyright © International Astronomical Union 2009

References

Andersen, J. 1991 A&ARv, 3, 91Google Scholar
Blake, C. H., Charbonneau, D., White, R. J., Marley, M. S., & Saumon, D. 2007 ApJ, 666, 1198CrossRefGoogle Scholar
Blake, C. H., Charbonneau, D., White, R. J., Torres, G., Marley, M. S., & Saumon, D. 2008 ApJ, 678, 125Google Scholar
Charbonneau, D. & Deming, D. 2007, The Dynamics-Based Approach to Studying Terrestrial Exoplanets, submitted to the Exoplanet Task Force (AAAC), 2 April 2007, arXiv:0706.1047Google Scholar
Etzel, P. B. 1981, in Carling, E. B., Kopal, Z., eds, Photometric and Spectroscopic Binary Systems, NATO ASI Ser. C., 69. Kluwer, Dordrecht, p. 111CrossRefGoogle Scholar
Fukugita, M., Ichikawa, T., Gunn, J. E., Doi, M., Shimasaku, K., & Schneider, D. P. 1996, AJ, 111, 1748CrossRefGoogle Scholar
Irwin, J., Irwin, M., Aigrain, S., Hodgkin, S., Hebb, L., & Moraux, E. 2007, MNRAS, 375, 1449Google Scholar
Lépine, S. 2008, AJ, 130, 1680CrossRefGoogle Scholar
Lépine, S. & Shara, P. 2008, AJ, 129, 1483Google Scholar
Nutzman, P. & Charbonneau, D. 2008, PASP, 120, 317Google Scholar
Popper, D. M. & Etzel, P. B. 1981, AJ, 86, 102CrossRefGoogle Scholar
Ribas, I. 2006 Ap&SS, 304, 89Google Scholar
Southworth, J., Maxted, P. F. L., & Smalley, B. 2004a, MNRAS, 351, 1277Google Scholar
Southworth, J., Zucker, S., Maxted, P. F. L., & Smalley, B. 2004b, MNRAS, 355, 986CrossRefGoogle Scholar
Skrutskie, M. F., et al. 2006, AJ, 131, 1163CrossRefGoogle Scholar
Young, A. T. 1967, AJ, 72, 747CrossRefGoogle Scholar