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LIBRIS Formathandbok  (Information om MARC21)
FältnamnIndikatorerMetadata
00009301naa a2201177 4500
001oai:research.chalmers.se:47f060b1-f00a-4b45-bd6b-592c81a2d6bb
003SwePub
008210115s2021 | |||||||||||000 ||eng|
024a https://doi.org/10.1051/0004-6361/2020394552 DOI
024a https://research.chalmers.se/publication/5218932 URI
040 a (SwePub)cth
041 a engb eng
042 9 SwePub
072 7a art2 swepub-publicationtype
072 7a ref2 swepub-contenttype
100a Luque, R.u Instituto de Astrofísica de Canarias,Universidad de la Laguna,University of La Laguna4 aut
2451 0a A planetary system with two transiting mini-Neptunes near the radius valley transition around the bright M dwarf TOI-776
264 c 2021-01-05
264 1b EDP Sciences,c 2021
520 a We report the discovery and characterization of two transiting planets around the bright M1 V star LP 961-53 (TOI-776, J = 8.5 mag, M = 0.54 ± 0.03 M⊙) detected during Sector 10 observations of the Transiting Exoplanet Survey Satellite (TESS). Combining the TESS photometry with HARPS radial velocities, as well as ground-based follow-up transit observations from the MEarth and LCOGT telescopes, for the inner planet, TOI-776 b, we measured a period of Pb = 8.25 d, a radius of Rb = 1.85 ± 0.13 R⊙, and a mass of Mb = 4.0 ± 0.9 M⊙; and for the outer planet, TOI-776 c, a period of Pc = 15.66 d, a radius of Rc = 2.02 ± 0.14 R⊙, and a mass of Mc = 5.3 ± 1.8 M⊙. The Doppler data shows one additional signal, with a period of ~34 d, associated with the rotational period of the star. The analysis of fifteen years of ground-based photometric monitoring data and the inspection of different spectral line indicators confirm this assumption. The bulk densities of TOI-776 b and c allow for a wide range of possible interior and atmospheric compositions. However, both planets have retained a significant atmosphere, with slightly different envelope mass fractions. Thanks to their location near the radius gap for M dwarfs, we can start to explore the mechanism(s) responsible for the radius valley emergence around low-mass stars as compared to solar-like stars. While a larger sample of well-characterized planets in this parameter space is still needed to draw firm conclusions, we tentatively estimate that the stellar mass below which thermally-driven mass loss is no longer the main formation pathway for sculpting the radius valley is between 0.63 and 0.54 M⊙. Due to the brightness of the star, the TOI-776 system is also an excellent target for the James Webb Space Telescope, providing a remarkable laboratory in which to break the degeneracy in planetary interior models and to test formation and evolution theories of small planets around low-mass stars.
650 7a NATURVETENSKAPx Geovetenskap och miljövetenskapx Meteorologi och atmosfärforskning0 (SwePub)105082 hsv//swe
650 7a NATURAL SCIENCESx Earth and Related Environmental Sciencesx Meteorology and Atmospheric Sciences0 (SwePub)105082 hsv//eng
650 7a NATURVETENSKAPx Fysikx Astronomi, astrofysik och kosmologi0 (SwePub)103052 hsv//swe
650 7a NATURAL SCIENCESx Physical Sciencesx Astronomy, Astrophysics and Cosmology0 (SwePub)103052 hsv//eng
650 7a NATURVETENSKAPx Geovetenskap och miljövetenskapx Geofysik0 (SwePub)105052 hsv//swe
650 7a NATURAL SCIENCESx Earth and Related Environmental Sciencesx Geophysics0 (SwePub)105052 hsv//eng
653 a Stars: individual: LP 961-53
653 a Planetary systems
653 a Stars: low-mass
653 a Techniques: radial velocities
653 a Techniques: photometric
700a Serrano, L. M.u Universita degli Studi di Torino,University of Turin4 aut
700a Molaverdikhani, K.u Max Planck Gesellschaft zur Förderung der Wissenschaften e.V. (MPG),Max Planck Society for the Advancement of Science (MPG)4 aut
700a Nixon, M. C.u University Of Cambridge4 aut
700a Livingston, J. H.u University of Tokyo, Japan4 aut
700a Guenther, E. W.u Thüringer Landessternwarte Tautenburg4 aut
700a Palle, E.u Instituto de Astrofísica de Canarias,Universidad de la Laguna,University of La Laguna4 aut
700a Madhusudhan, N.u University Of Cambridge4 aut
700a Nowak, G.u Universidad de la Laguna,University of La Laguna,Instituto de Astrofísica de Canarias4 aut
700a Korth, Judithu Universität zu Köln,University of Cologne4 aut
700a Cochran, W. D.u The University of Texas at Austin, USA4 aut
700a Hirano, T.u Tokyo Institute of Technology4 aut
700a Chaturvedi, Priyankau Thüringer Landessternwarte Tautenburg4 aut
700a Goffo, E.u Universita degli Studi di Torino,University of Turin4 aut
700a Albrecht, S.u Århus Universitet,Aarhus University4 aut
700a Barragán, O.u University Of Oxford4 aut
700a Briceño, C.4 aut
700a Cabrera, J.u Deutsches Zentrums für Luft- und Raumfahrt (DLR),German Aerospace Center (DLR)4 aut
700a Charbonneau, D.u Harvard-Smithsonian Center for Astrophysics4 aut
700a Cloutier, R.u Harvard-Smithsonian Center for Astrophysics4 aut
700a Collins, K. A.u Harvard-Smithsonian Center for Astrophysics4 aut
700a Collins, Kevin I.u George Mason University4 aut
700a Colón, K. D.u NASA Goddard Space Flight Center4 aut
700a Crossfield, I. J.M.u University of Kansas4 aut
700a Csizmadia, Szilardu Deutsches Zentrums für Luft- und Raumfahrt (DLR),German Aerospace Center (DLR)4 aut
700a Dai, Feiu California Institute of Technology (Caltech)4 aut
700a Deeg, H. J.u Instituto de Astrofísica de Canarias,Universidad de la Laguna,University of La Laguna4 aut
700a Esposito, M.u Thüringer Landessternwarte Tautenburg4 aut
700a Fridlund, Malcolm,d 1952u Chalmers tekniska högskola,Chalmers University of Technology,Universiteit Leiden (UL),Leiden University (UL)4 aut0 (Swepub:cth)malfri
700a Gandolfi, D.u Universita degli Studi di Torino,University of Turin4 aut
700a Georgieva, Iskra,d 1987u Chalmers tekniska högskola,Chalmers University of Technology4 aut0 (Swepub:cth)iskrag
700a Glidden, Anau Massachusetts Institute of Technology (MIT)4 aut
700a Goeke, Robertu Massachusetts Institute of Technology (MIT)4 aut
700a Grziwa, S.u Universität zu Köln,University of Cologne4 aut
700a Hatzes, A.u Thüringer Landessternwarte Tautenburg4 aut
700a Henze, C. E.u NASA Ames Research Center4 aut
700a Howell, S. B.u NASA Ames Research Center4 aut
700a Irwin, J.u Harvard-Smithsonian Center for Astrophysics4 aut
700a Jenkins, J. M.u NASA Ames Research Center4 aut
700a Jensen, E. L.N.u Swarthmore College4 aut
700a Kabath, Petru Czech Academy of Sciences4 aut
700a Kidwell, R. C.u Space Telescope Science Institute (STScI)4 aut
700a Kielkopf, J. F.u University of Louisville4 aut
700a Knudstrup, E.u Århus Universitet,Aarhus University4 aut
700a Lam, K. W.F.u Technische Universität Berlin4 aut
700a Latham, D. W.u Harvard-Smithsonian Center for Astrophysics4 aut
700a Lissauer, Jack J.u NASA Ames Research Center4 aut
700a Mann, A. W.u The University of North Carolina System4 aut
700a Matthews, Elisabethu Massachusetts Institute of Technology (MIT)4 aut
700a Mireles, Ismaelu Massachusetts Institute of Technology (MIT)4 aut
700a Narita, N.u University of Tokyo, Japan,National Institutes of Natural Sciences (NINS),Instituto de Astrofísica de Canarias,Japan Science and Technology Agency (JST)4 aut
700a Paegert, M.u Harvard-Smithsonian Center for Astrophysics4 aut
700a Persson, Carina,d 1964u Chalmers tekniska högskola,Chalmers University of Technology4 aut0 (Swepub:cth)carina64
700a Redfield, S.u Wesleyan University4 aut
700a Ricker, George R.u Massachusetts Institute of Technology (MIT)4 aut
700a Rodler, F.u European Southern Observatory Santiago4 aut
700a Schlieder, Joshua E.u NASA Goddard Space Flight Center4 aut
700a Scott, N. J.u NASA Ames Research Center4 aut
700a Seager, S.u Massachusetts Institute of Technology (MIT)4 aut
700a Šubjak, J.u Czech Academy of Sciences4 aut
700a Tan, T. G.4 aut
700a Ting, Eric B.u NASA Ames Research Center4 aut
700a Vanderspek, Roland K.u Massachusetts Institute of Technology (MIT)4 aut
700a Van Eylen, Vincentu University College London (UCL)4 aut
700a Winn, J. N.u Princeton University4 aut
700a Ziegler, C.u University of Toronto4 aut
710a Instituto de Astrofísica de Canariasb Universidad de la Laguna4 org
773t Astronomy and Astrophysicsd : EDP Sciencesg 645q 645x 0004-6361x 1432-0746
856u https://authors.library.caltech.edu/107510/1/aa39455-20.pdf
8564 8u https://doi.org/10.1051/0004-6361/202039455
8564 8u https://research.chalmers.se/publication/521893

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