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相关论文: Three Temperate Neptunes Orbiting Nearby Stars

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Planets intermediate in size between the Earth and Neptune, and orbiting closer to their host stars than Mercury does the Sun, are the most common type of planet revealed by exoplanet surveys over the last quarter century. Results from…

地球与行星天体物理 · 物理学 2021-02-10 Jacob L. Bean , Sean N. Raymond , James E. Owen

Radial velocity searches for extrasolar planets have recently detected several very low mass (7-20M_Earth) planets in close orbits with periods <10 days. We consider the prospects for detecting the analogs of these planets in Galactic open…

天体物理学 · 物理学 2007-05-23 Joshua Pepper , B. Scott Gaudi

The NASA Exoplanet Archive was searched for planets with an equilibrium temperature below 600 K, mass uncertainty less than 27 percent, and radius uncertainty less than 8 percent. This search produced 93 planets with mass from 0.3 to 1680…

地球与行星天体物理 · 物理学 2023-03-14 David G. Russell

Although the formation and the properties of hot Jupiters (with orbital periods $P<10\,$d) have attracted a great deal of attention, the origins of warm Jupiters ($10<P<100\,$d) are less well-studied. Using a transit timing analysis, we…

地球与行星天体物理 · 物理学 2018-08-22 Dong-Hong Wu , Songhu Wang , Ji-Lin Zhou , Jason H. Steffen , Gregory Laughlin

The angle between the spin of a star and its planets' orbital planes traces the history of the planetary system. Exoplanets orbiting close to cool stars are expected to be on circular, aligned orbits because of strong tidal interactions…

We report the detection of two planetary mass companions to the solar-type star HD 155358. The two planets have orbital periods of 195.0 and 530.3 days, with eccentricities of 0.11 and 0.18. The minimum masses for these planets are 0.89 and…

天体物理学 · 物理学 2009-06-23 William D. Cochran , Michael Endl , Robert A. Wittenmyer , Jacob L. Bean

We report the discovery of two transiting extrasolar planets by the HATSouth survey. HATS-9b orbits an old (10.8 $\pm$ 1.5 Gyr) V=13.3 G dwarf star, with a period P = 1.9153 d. The host star has a mass of 1.03 M$_{\odot}$, radius of 1.503…

The loneliness of hot Jupiters supports the high-eccentricity migration as a primary path leading to the formation of systems with those planets stripped of any close-in planetary companions. Here we present the null results of searches for…

We report the discovery of a Neptune-like planet (LP 714-47 b, P = 4.05204 d, m_b = 30.8 +/- 1.5 M_earth , R_b = 4.7 +/- 0.3 R_earth ) located in the 'hot Neptune desert'. Confirmation of the TESS Object of Interest (TOI 442.01) was…

地球与行星天体物理 · 物理学 2021-01-04 S. Dreizler , I. , J. , M. Crossfield , D. Kossakowski , P. Plavchan , S. , V. Jeffers , J. Kemmer , R. Luque , N. Espinoza , E. Pallé , K. Stassun , E. Matthews , B. Cale , J. , A. Caballero , M. Schlecker , J. Lillo-Box , M. Zechmeister , S. Lalitha , A. Reiners , A. Soubkiou , B. Bitsch , M. , R. Zapatero Osorio , P. Chaturvedi , A. , P. Hatzes , G. Ricker , R. Vanderspek , D. , W. Latham , S. Seager , J. Winn , J. M. Jenkins , J. Aceituno , P. , J. Amado , K. Barkaoui , M. Barbieri , N. , M. Batalha , F. , F. Bauer , B. Benneke , Z. Benkhaldoun , C , Beichman , J. Berberian , J. Burt , R. , P. Butler , D. , A. Caldwell , A. Chintada , A. Chontos , J. , L. Christiansen , D. R. Ciardi , C. Cifuentes , K. , A. Collins , K. , I. Collins , D. Combs , M. Cortés-Contreras , J. , D. Crane , T. Daylan , D. Dragomir , E. Esparza-Borges , P. Evans , F. Feng , E. , E. Flowers , A. Fukui , B. Fulton , E. Furlan , E. Gaidos , C. Geneser , S. Giacalone , M. Gillon , E. Gonzales , V. Gorjian , C. Hellier , D. Hidalgo , A. , W. Howard , S. Howell , D. Huber , H. Isaacson , E. Jehin , E. , L. , N. Jensen , A. Kaminski , S. , R. Kane , K. Kawauchi , J. , F. Kielkopf , H. Klahr , M. , R. Kosiarek , L. Kreidberg , M. , Kürster , M. Lafarga , J. Livingston , D. Louie , A. Mann , A. Madrigal-Aguado , R. , A. Matson , T. Mocnik , J. , C. Morales , P. , S. Muirhead , F. Murgas , S. Nandakumar , N. Narita , G. Nowak , M. Oshagh , H. Parviainen , V. , M. Passegger , D. Pollacco , F. , J. Pozuelos , A. Quirrenbach , M. Reefe , I. Ribas , P. Robertson , C. Rodríguez-López , M. , E. Rose , A. Roy , A. Schweitzer , J. Schlieder , S. Shectman , A. Tanner , H. , V. Şenavcı , J. Teske , J. , D. Twicken , J. Villasenor , S. X. Wang , L. , M. Weiss , J. Wittrock , M. Yılmaz , F. Zohrabi

Terrestrial planets have been found orbiting Sun-like stars with extremely short periods --- some as short as 4 hours. These "ultra-short-period planets" or "hot Earths" are so strongly irradiated that any initial H/He atmosphere has…

地球与行星天体物理 · 物理学 2019-10-02 Fei Dai , Kento Masuda , Joshua N. Winn , Li Zeng

We report three newly discovered exoplanets from the SuperWASP survey. WASP-127b is a heavily inflated super-Neptune of mass 0.18 +/- 0.02 M_J and radius 1.37 +/- 0.04 R_J. This is one of the least massive planets discovered by the WASP…

We present the discovery of two mini Neptunes near a 2:1 orbital resonance configuration orbiting the K0 star TOI-1803. We describe their orbital architecture in detail and suggest some possible formation and evolution scenarios. Using…

地球与行星天体物理 · 物理学 2025-04-02 T. Zingales , L. Malavolta , L. Borsato , D. Turrini , A. Bonfanti , D. Polychroni , G. Mantovan , D. Nardiello , V. Nascimbeni , A. F. Lanza , A. Bekkelien , A. Sozzetti , C. Broeg , L. Naponiello , M. Lendl , A. S. Bonomo , A. E. Simon , S. Desidera , G. Piotto , L. Mancini , M. J. Hooton , A. Bignamini , J. A. Egger , A. Maggio , Y. Alibert , D. Locci , L. Delrez , F. Biassoni , L. Fossati , L. Cabona , G. Lacedelli , I. Carleo , P. Leonardi , G. Andreuzzi , A. Brandeker , R. Cosentino , A. C. M. Correia , R. Claudi , R. Alonso , M. Damasso , T. G. Wilson , T. Bàrczy , M. Pinamonti , D. Baker , K. Barkaoui , D. Barrado Navascues , S. C. C. Barros , W. Baumjohann , T. Beck , C. Beichman , W. Benz , A. Bieryla , N. Billot , P. Bosch-Cabot , L. G. Bouma , D. R. Ciardi , A. Collier Cameron , K. A. Collins , Ian J. M. Crossfield , Sz. Csizmadia , P. E. Cubillos , M. B. Davies , M. Deleuil , A. Deline , O. D. S. Demangeon , B. O. Demory , A. Derekas , D. Dragomir , B. Edwards , D. Ehrenreich , A. Erikson , B. Falk , A. Fortier , M. Fridlund , A. Fukui , D. Gandolfi , K. Gazeas , M. Gillon , E. Gonzales , M. Gudel , P. Guerra , M. N. Guunther , A. Heitzmann , Ch. Helling , S. B. Howell , K. G. Isaak , J. Jenkins , L. L. Kiss , J. Korth , K. W. F. Lam , J. Laskar , A. Lecavelier des Etangs , D. Magrin , R. Matson , E. C. Matthews , P. F. L. Maxted , S. McDermott , M. Munari , C. Mordasini , N. Narita , G. Olofsson , R. Ottensamer , I. Pagano , E. Pallè , G. Peter , D. Pollacco , D. Queloz , R. Ragazzoni , N. Rando , F. Ratti , H. Rauer , I. Ribas , S. Salmon , N. C. Santos , G. Scandariato , S. Seager , D. Sègransan , A. M. S. Smith , J. Schlieder , R. P. Schwarz , A. Shporer , S. G. Sousa , M. Stalport , M. Steinberger , S. Sulis , Gy. M. Szabò , J. D. Twicken , S. Udry , V. Van Grootel , J. Venturini , E. Villaver , N. A. Walton , J. N. Winn

In circumstellar disks around young stars, the gravitational influence of nascent planets produces telltale patterns in density, temperature, and kinematics. To better understand these signatures, we first performed 3D hydrodynamical…

地球与行星天体物理 · 物理学 2024-07-17 Dhruv Muley , Julio David Melon Fuksman , Hubert Klahr

We present radial-velocity measurements obtained in a programs underway to search for extrasolar planets with the spectrograph SOPHIE at the 1.93-m telescope of the Haute-Provence Observatory. Targets were selected from catalogs observed…

We report the detection of four new extra-solar planets from the Anglo-Australian Planet Search orbiting the somewhat metal-enriched stars HD73526, HD76700, HD30177 and HD2039. The planetary companion of HD 76700 has a circular orbit with a…

Surveys of nearby field stars indicate that stellar binaries are common, yet little is known about the effects that these companions may have on planet formation and evolution. The Friends of Hot Jupiters project uses three complementary…

Based on recently-taken and archival HARPS, FEROS and HIRES radial velocities (RVs), we present evidence for a new planet orbiting the first ascent red giant star HD33142 (with an improved mass estimate of 1.52$\pm$0.03 M$_\odot$), already…

The hot Neptune orbiting around GJ 436 is a unique example of an intermediate mass planet. Its close-in orbit suggests that the planet has undergone migration and its study is fundamental to understanding planet formation and evolution. As…

地球与行星天体物理 · 物理学 2010-11-02 P. Figueira , F. Pont , C. Mordasini , Y. Alibert , C. Georgy , W. Benz
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