中文
相关论文

相关论文: Transit Timing Variations in the three-planet syst…

200 篇论文

The Transiting Exoplanet Survey Satellite, TESS, is currently carrying out an all-sky search for small planets transiting bright stars. In the first year of the TESS survey, steady progress was made in achieving the mission's primary…

Transit Timing Variations (TTVs) can provide useful information on compact multi-planetary systems observed by transits, by putting constraints on the masses and eccentricities of the observed planets. This is especially helpful when the…

地球与行星天体物理 · 物理学 2024-05-24 A. Leleu , J. -B. Delisle , S. Udry , R. Mardling , M. Turbet , J. A. Egger , Y. Alibert , G. Chatel , P. Eggenberger , M. Stalport

Transiting exoplanets in multi-planet systems exhibit non-Keplerian orbits as a result of the gravitational influence from companions which can cause the times and durations of transits to vary. The amplitude and periodicity of the transit…

地球与行星天体物理 · 物理学 2019-12-24 Kyle A. Pearson

Multi-planet systems are valuable arenas for investigating exoplanet architectures and comparing planetary siblings. TOI-1246 is one such system, with a moderately bright K dwarf ($\rm{V=11.6,~K=9.9}$) and four transiting sub-Neptunes…

K2-19 is a star, slightly smaller than the Sun, that hosts three transiting planets. Two of these, K2-19 b and c, are between the size of Neptune and Saturn and have orbital periods near a 3:2 commensurability, and exhibit strong…

地球与行星天体物理 · 物理学 2025-09-23 Paige M. Entrican , Erik A. Petigura , Antoine C. Petit , Gregory J. Gilbert , Kento Masuda

We present the characterization of the TOI-6041 system, a bright ($V = 9.84 \pm 0.03$) G7-type star hosting at least two planets. The inner planet, TOI-6041b, is a warm Neptune with a radius of $4.55^{+0.18}_{-0.17}\,R_\oplus$, initially…

AU Mic is a very active M dwarf with an edge-on debris disk and two transiting sub-Neptunes with a possible third planetary companion. The two transiting planets exhibit significant transit-timing variations (TTVs) that are caused by the…

Exoplanetary systems with multiple giant planets present an opportunity to understand planet formation, migration processes, and long-term system-wide dynamical interactions. In particular, they provide constraints to distinguish between…

Determining the architecture of multi-planetary systems is one of the cornerstones of understanding planet formation and evolution. Resonant systems are especially important as the fragility of their orbital configuration ensures that no…

地球与行星天体物理 · 物理学 2021-01-25 A. Leleu , Y. Alibert , N. C. Hara , M. J. Hooton , T. G. Wilson , P. Robutel , J. -B. Delisle , J. Laskar , S. Hoyer , C. Lovis , E. M. Bryant , E. Ducrot , J. Cabrera , L. Delrez , J. S. Acton , V. Adibekyan , R. Allart , C. Allende Prieto , R. Alonso , D. Alves , D. R. Anderson , D. Angerhausen , G. Anglada Escudé , J. Asquier , D. Barrado , S. C. C. Barros , W. Baumjohann , D. Bayliss , M. Beck , T. Beck , A. Bekkelien , W. Benz , N. Billot , A. Bonfanti , X. Bonfils , F. Bouchy , V. Bourrier , G. Boué , A. Brandeker , C. Broeg , M. Buder , A. Burdanov , M. R. Burleigh , T. Bárczy , A. C. Cameron , S. Chamberlain , S. Charnoz , B. F. Cooke , C. Corral Van Damme , A. C. M. Correia , S. Cristiani , M. Damasso , M. B. Davies , M. Deleuil , O. D. S. Demangeon , B. -O. Demory , P. Di Marcantonio , G. Di Persio , X. Dumusque , D. Ehrenreich , A. Erikson , P. Figueira , A. Fortier , L. Fossati , M. Fridlund , D. Futyan , D. Gandolfi , A. García Muñoz , L. J. Garcia , S. Gill , E. Gillen , M. Gillon , M. R. Goad , J. I. González Hernández , M. Guedel , M. N. Günther , J. Haldemann , B. Henderson , K. Heng , A. E. Hogan , K. Isaak , E. Jehin , J. S. Jenkins , A. Jordán , L. Kiss , M. H. Kristiansen , K. Lam , B. Lavie , A. Lecavelier des Etangs , M. Lendl , J. Lillo-Box , G. Lo Curto , D. Magrin , C. J. A. P. Martins , P. F. L. Maxted , J. McCormac , A. Mehner , G. Micela , P. Molaro , M. Moyano , C. A. Murray , V. Nascimbeni , N. J. Nunes , G. Olofsson , H. P. Osborn , M. Oshagh , R. Ottensamer , I. Pagano , E. Pallé , P. P. Pedersen , F. A. Pepe , C. M. Persson , G. Peter , G. Piotto , G. Polenta , D. Pollacco , E. Poretti , F. J. Pozuelos , D. Queloz , R. Ragazzoni , N. Rando , F. Ratti , H. Rauer , L. Raynard , R. Rebolo , C. Reimers , I. Ribas , N. C. Santos , G. Scandariato , J. Schneider , D. Sebastian , M. Sestovic , A. E. Simon , A. M. S. Smith , S. G. Sousa , A. Sozzetti , M. Steller , A. Suárez Mascareño , Gy. M. Szabó , D. Ségransan , N. Thomas , S. Thompson , R. H. Tilbrook , A. Triaud , O. Turner , S. Udry , V. Van Grootel , H. Venus , F. Verrecchia , J. I. Vines , N. A. Walton , R. G. West , P. J. Wheatley , D. Wolter , M. R. Zapatero Osorio

In transiting planetary systems, where planetary sizes are accurately determined from transit observations, the presence of transit timing variations (TTVs), especially when combined with radial velocity (RV) data, provides powerful…