An Earth-sized planet with an Earth-like density

Francesco Pepe, Andrew Collier Cameron, David W. Latham, Emilio Molinari, Stéphane Udry, Aldo S. Bonomo, Lars A. Buchhave, David Charbonneau, Rosario Cosentino, Courtney D. Dressing, Xavier Dumusque, Pedro Figueira, Aldo F. M. Fiorenzano, Sara Gettel, Avet Harutyunyan, Raphaëlle D. Haywood, Keith Horne, Mercedes Lopez-Morales, Christophe Lovis, Luca MalavoltaMichel Mayor, Giusi Micela, Fatemeh Motalebi, Valerio Nascimbeni, David Phillips, Giampaolo Piotto, Don Pollacco, Didier Queloz, Ken Rice, Dimitar Sasselov, Damien Segransan, Alessandro Sozzetti, Andrew Szentgyorgyi, Christopher A. Watson

    143 Citationer (Scopus)

    Abstract

    cent analyses 1, 2, 3, 4 of data from the NASA Kepler spacecraft5 have established that planets with radii within 25 per cent of the Earth’s ( ) are commonplace throughout the Galaxy, orbiting at least 16.5 per cent of Sun-like stars1. Because these studies were sensitive to the sizes of the planets but not their masses, the question remains whether these Earth-sized planets are indeed similar to the Earth in bulk composition. The smallest planets for which masses have been accurately determined6, 7 are Kepler-10b (1.42 ) and Kepler-36b (1.49 ), which are both significantly larger than the Earth. Recently, the planet Kepler-78b was discovered8 and found to have a radius of only 1.16 . Here we report that the mass of this planet is 1.86 Earth masses. The resulting mean density of the planet is 5.57 g cm−3, which is similar to that of the Earth and implies a composition of iron and rock.
    OriginalsprogEngelsk
    TidsskriftNature
    Vol/bind503
    Udgave nummer7476
    Sider (fra-til)377-380
    Antal sider4
    ISSN0028-0836
    DOI
    StatusUdgivet - 21 nov. 2013

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