A&A 594, A92 (2016) Astronomy DOI: 10.1051/0004-6361/201628918 & c ESO 2016 Astrophysics A solar twin in the eclipsing binary LL Aquarii D. Graczyk1; 2; 3, R. Smolec3, K. Pavlovski4, J. Southworth5, G. Pietrzynski´ 3; 2, P. F. L. Maxted5, P. Konorski6, W. Gieren2; 1, B. Pilecki3, M. Taormina3, K. Suchomska6, P. Karczmarek6, M. Górski1; 2, P. Wielgórski3, and R. I. Anderson7; 8;? 1 Millenium Institute of Astrophysics, Santiago, Chile e-mail:
[email protected] 2 Universidad de Concepción, Departamento de Astronomía, Casilla 160-C, Concepción, Chile 3 Nicolaus Copernicus Astronomical Center, Polish Academy of Sciences, ul. Bartycka 18, 00-716 Warszawa, Poland 4 Department of Physics, University of Zagreb, Bijenicka´ cesta 32, 10000 Zagreb, Croatia 5 Astrophysics Group, Keele University, Keele, Staffordshire, ST5 5BG, UK 6 Warsaw University Observatory, Al. Ujazdowskie 4, 00-478 Warsaw, Poland 7 Physics and Astronomy Department, The Johns Hopkins University, 3400 North Charles St, Baltimore, MD 21202, USA 8 Département d’Astronomie, Université de Genève, 51 Ch. des Maillettes, 1290 Sauverny, Switzerland Received 13 May 2016 / Accepted 23 June 2016 ABSTRACT Aims. In the course of a project to study eclipsing binary stars in vinicity of the Sun, we found that the cooler component of LL Aqr is a solar twin candidate. This is the first known star with properties of a solar twin existing in a non-interacting eclipsing binary, offering an excellent opportunity to fully characterise its physical properties with very high precision. Methods. We used extensive multi-band, archival photometry and the Super-WASP project and high-resolution spectroscopy obtained from the HARPS and CORALIE spectrographs.