Exoplanet detection. Stellar activity masquerading as planets in the habitable zone of the M dwarf Gliese 581

doi:10.1126/science.1253253

. 2014 Jul 25;345(6195):440-4.

doi: 10.1126/science.1253253. Epub 2014 Jul 3.

Exoplanet detection. Stellar activity masquerading as planets in the habitable zone of the M dwarf Gliese 581

Paul Robertson¹, Suvrath Mahadevan², Michael Endl³, Arpita Roy²

Affiliations

¹ Department of Astronomy and Astrophysics, The Pennsylvania State University, University Park, PA 16802, USA. Center for Exoplanets and Habitable Worlds, The Pennsylvania State University, University Park, PA 16802, USA. pmr19@psu.edu.
² Department of Astronomy and Astrophysics, The Pennsylvania State University, University Park, PA 16802, USA. Center for Exoplanets and Habitable Worlds, The Pennsylvania State University, University Park, PA 16802, USA. The Penn State Astrobiology Research Center, The Pennsylvania State University, University Park, PA 16802, USA.
³ McDonald Observatory, The University of Texas at Austin, Austin, TX 78712-1206, USA.

PMID: 24993348
DOI: 10.1126/science.1253253

Exoplanet detection. Stellar activity masquerading as planets in the habitable zone of the M dwarf Gliese 581

Paul Robertson et al. Science. 2014.

. 2014 Jul 25;345(6195):440-4.

doi: 10.1126/science.1253253. Epub 2014 Jul 3.

Authors

Paul Robertson¹, Suvrath Mahadevan², Michael Endl³, Arpita Roy²

Affiliations

¹ Department of Astronomy and Astrophysics, The Pennsylvania State University, University Park, PA 16802, USA. Center for Exoplanets and Habitable Worlds, The Pennsylvania State University, University Park, PA 16802, USA. pmr19@psu.edu.
² Department of Astronomy and Astrophysics, The Pennsylvania State University, University Park, PA 16802, USA. Center for Exoplanets and Habitable Worlds, The Pennsylvania State University, University Park, PA 16802, USA. The Penn State Astrobiology Research Center, The Pennsylvania State University, University Park, PA 16802, USA.
³ McDonald Observatory, The University of Texas at Austin, Austin, TX 78712-1206, USA.

PMID: 24993348
DOI: 10.1126/science.1253253

Abstract

The M dwarf star Gliese 581 is believed to host four planets, including one (GJ 581d) near the habitable zone that could possibly support liquid water on its surface if it is a rocky planet. The detection of another habitable-zone planet--GJ 581g--is disputed, as its significance depends on the eccentricity assumed for d. Analyzing stellar activity using the Hα line, we measure a stellar rotation period of 130 ± 2 days and a correlation for Hα modulation with radial velocity. Correcting for activity greatly diminishes the signal of GJ 581d (to 1.5 standard deviations) while significantly boosting the signals of the other known super-Earth planets. GJ 581d does not exist, but is an artifact of stellar activity which, when incompletely corrected, causes the false detection of planet g.

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Exoplanet detection. Comment on "Stellar activity masquerading as planets in the habitable zone of the M dwarf Gliese 581".
Anglada-Escudé G, Tuomi M. Anglada-Escudé G, et al. Science. 2015 Mar 6;347(6226):1080. doi: 10.1126/science.1260796. Science. 2015. PMID: 25745156
Exoplanet detection. Response to Comment on "Stellar activity masquerading as planets in the habitable zone of the M dwarf Gliese 581".
Robertson P, Mahadevan S, Endl M, Roy A. Robertson P, et al. Science. 2015 Mar 6;347(6226):1080. doi: 10.1126/science.1260974. Science. 2015. PMID: 25745157

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Exoplanet detection. Stellar activity masquerading as planets in the habitable zone of the M dwarf Gliese 581

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Exoplanet detection. Stellar activity masquerading as planets in the habitable zone of the M dwarf Gliese 581

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