Article
Astronomy & Astrophysics
Eric Agol, David M. Hernandez, Zachary Langford
Summary: This article discusses fitting N-body models to astronomical data and optimization techniques, introducing a general purpose symplectic integrator for arbitrary orbital architectures, and a method for computing derivatives using the chain rule. The algorithm has been implemented in the Julia language.
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
(2021)
Article
Astronomy & Astrophysics
Adrian Rodriguez, N. Callegari
Summary: This work examines the orbital evolution and dynamical stability near the small Saturnian moons Aegaeon, Methone, Anthe, and Pallene. Results show that for massless small moons, orbiting particles remain stable for at least 10(4) yr, while massive bodies cause significant perturbations and destabilization of particle orbits. Initial arcs around the moons are eroded within hundreds of years, providing insights into gravitational forces' time-scales for removing particles.
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
(2021)
Article
Astronomy & Astrophysics
A. S. Bonomo, X. Dumusque, A. Massa, A. Mortier, R. Bongiolatti, L. Malavolta, A. Sozzetti, L. A. Buchhave, M. Damasso, R. D. Haywood, A. Morbidelli, D. W. Latham, E. Molinari, F. Pepe, E. Poretti, S. Udry, L. Affer, W. Boschin, D. Charbonneau, R. Cosentino, M. Cretignier, A. Ghedina, E. Lega, M. Lopez-Morales, M. Margini, A. F. Martinez Fiorenzano, M. Mayor, G. Micela, M. Pedani, M. Pinamonti, K. Rice, D. Sasselov, R. Tronsgaard, A. Vanderburg
Summary: This article studies the exoplanet population around sun-like stars and finds that Jupiter may be one of the reasons for the absence of small planets and cold Jupiters in our solar system. Based on the data collected, there is no significant anti-correlation between small planets and cold Jupiters.
ASTRONOMY & ASTROPHYSICS
(2023)
Article
Astronomy & Astrophysics
Alysa Obertas, Daniel Tamayo, Norm Murray
Summary: Current planet formation theories suggest that the orbital architectures of observed exoplanet systems have been shaped by chaotic dynamics, instabilities, and giant impacts. This study shows that a significant number of Kepler multiplanet systems exhibit strong dynamical packing, indicating the importance of this metric in planet formation modeling and the search for unseen planets.
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
(2023)
Article
Astronomy & Astrophysics
Marco A. Munoz-Gutierrez, A. P. Granados Contreras, Gustavo Madeira, Joseph A. A'Hearn, Silvia Giuliatti Winter
Summary: The Saturnian small satellites Aegaeon, Methone, Anthe, and Pallene provide a unique study system for understanding the evolution of co-orbital dusty rings/arcs. This work explores the long-term evolution of Pallene and its ring through numerical simulations and analysis. The results show the current dynamical state of Pallene and its resonant behavior with Saturn's major moons. The study also investigates the dynamical evolution of micrometric particles in the ring and their effects on the ring's stability.
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
(2022)
Article
Astronomy & Astrophysics
H. Garzon, Adrian Rodriguez, G. C. de Elia
Summary: This study investigates the efficiency of different high-eccentricity mechanisms in producing Hot Jupiter candidates and finds that the E1 mechanism is the most efficient, followed by the Kozai-Lidov and E2 mechanisms. Furthermore, the study reveals that the Kozai-Lidov mechanism has the highest probability of significantly exciting the orbital inclinations of the Hot Jupiter candidates.
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
(2022)
Article
Astronomy & Astrophysics
Vera Wolthoff, Sabine Reffert, Andreas Quirrenbach, Matias Jones, Robert A. Wittenmyer, James S. Jenkins
Summary: The study investigates the occurrence rate of giant planets around evolved stars and examines its dependence on stellar mass, metallicity, and orbital period. By combining data from multiple radial velocity surveys, the authors find a positive correlation between planet occurrence and metallicity for evolved stars. The occurrence rate also peaks at a slightly smaller stellar mass compared to main-sequence stars, and the dependence on orbital period follows a broken power-law or log-normal distribution.
ASTRONOMY & ASTROPHYSICS
(2022)
Article
Astronomy & Astrophysics
Hanlun Lei, Jian Li
Summary: In this study, retrograde mean motion resonances (MMRs) are investigated using analytical and numerical methods, leading to the proposal of a new resonant angle to describe retrograde MMRs. The analytical model is validated through non-perturbative analysis using Poincare surfaces of section, showing excellent correspondence with numerical results. Additionally, seven retrograde asteroids are found within the resonant zones of retrograde MMRs with Jupiter, suggesting potential implications for understanding the dynamical evolution of asteroids in retrograde MMRs.
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
(2021)
Article
Astronomy & Astrophysics
A. -M. Lagrange, F. Philipot, P. Rubini, N. Meunier, F. Kiefer, P. Kervella, P. Delorme, H. Beust
Summary: This article investigates the population statistics and the impact of giant planets on the formation of planetary systems. By reanalyzing previous survey results, it is found that the conclusions about the distribution of giant planets beyond (5-8 astronomical units) are not reliable.
ASTRONOMY & ASTROPHYSICS
(2023)
Article
Astronomy & Astrophysics
V Bourrier, A. Deline, A. Krenn, J. A. Egger, A. C. Petit, L. Malavolta, M. Cretignier, N. Billot, C. Broeg, H-G Floren, D. Queloz, Y. Alibert, A. Bonfanti, A. S. Bonomo, J-B Delisle, O. D. S. Demangeon, B-O Demory, X. Dumusque, D. Ehrenreich, R. D. Haywood, S. B. Howell, M. Lendl, A. Mortier, G. Nigro, S. Salmon, S. G. Sousa, T. G. Wilson, V Adibekyan, R. Alonso, G. Anglada, T. Barczy, D. Barrado y Navascues, S. C. C. Barros, W. Baumjohann, M. Beck, W. Benz, F. Biondi, X. Bonfils, A. Brandeker, J. Cabrera, S. Charnoz, Sz Csizmadia, A. Collier Cameron, M. Damasso, M. B. Davies, M. Deleuil, L. Delrez, L. Di Fabrizio, A. Erikson, A. Fortier, L. Fossati, M. Fridlund, D. Gandolfi, M. Gillon, M. Guedel, K. Heng, S. Hoyer, K. G. Isaak, L. L. Kiss, J. Laskar, A. Lecavelier des Etangs, V Lorenzi, C. Lovis, D. Magrin, A. Massa, P. F. L. Maxted, V Nascimbeni, G. Olofsson, R. Ottensamer, I Pagano, E. Palle, G. Peter, G. Piotto, D. Pollacco, R. Ragazzoni, N. Rando, H. Rauer, I Ribas, N. C. Santos, G. Scandariato, D. Segransan, A. E. Simon, A. M. S. Smith, M. Steller, Gy M. Szabo, N. Thomas, S. Udry, V. Van Grootel, F. Verrecchia, N. Walton, T. Beck, M. Buder, F. Ratti, B. Ulmer, V. Viotto
Summary: Much is still unknown about exoplanets smaller than Neptune, particularly those in compact multi-planet systems. The study of the HD 3167 system, with its peculiar architecture and multiple planets, has provided insights into the dynamics and atmospheric evolution processes of such planets. The research has improved our understanding of planetary properties and has highlighted the contrasting characteristics of different planets within the system.
ASTRONOMY & ASTROPHYSICS
(2022)
Article
Astronomy & Astrophysics
Giacomo Lari, Melaine Saillenfest, Clara Grassi
Summary: The dynamics of the Galilean satellites are determined by Laplace resonance and strong tidal dissipation, causing variations of their semimajor axes. The compatibility of Callisto's fast migration with the current orbital configuration is investigated. Simulations show that Callisto can cross the 2:1 resonance with Ganymede without being captured, but is mostly captured despite its divergent migration. Eventually, Callisto can escape by crossing a high-order resonance with Ganymede and the system can relax to its current configuration.
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
(2023)
Article
Astronomy & Astrophysics
Jean-Loup Bertaux, Anastasiia Ivanova
Summary: The study utilizes the radial velocity method to detect 909 exoplanets and analyzes the observed distribution and true distribution to reveal the sub-Saturn desert and a statistically significant gap of planets near Uranus.
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
(2022)
Article
Astronomy & Astrophysics
E. L. Rickman, E. Matthews, W. Ceva, D. Segransan, G. M. Brandt, H. Zhang, T. D. Brandt, T. Forveille, J. Hagelberg, S. Udry
Summary: Using long-term precise Doppler measurements and combining multiple exoplanet detection techniques, including radial velocities, astrometric accelerations, and direct imaging, this study reveals the existence of companions on long-period orbits with model-independent and precise dynamical masses. The discovery of new companions, as well as the update of dynamical masses of previously imaged companions, provides valuable insights for testing mass-luminosity relations and advancing high-contrast imaging of exoplanets and brown dwarfs.
ASTRONOMY & ASTROPHYSICS
(2022)
Article
Astronomy & Astrophysics
Alexander J. Mustill, Melvyn B. Davies, Sarah Blunt, Andrew Howard
Summary: In this paper, the authors explore scenarios for the excitation of the eccentricity of the recently discovered giant exoplanet IIR5183b. They find that planet-planet scattering or Lidov-Kozai cycles from a binary companion can potentially explain the observed high eccentricity of the planet. The best case is when planet-planet scattering is combined with the Kozai cycles from the binary, resulting in a success rate of 14.5% for currently observing e >= 0.84.
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
(2022)
Article
Astronomy & Astrophysics
Apostolos A. Christou, Nikolaos Georgakarakos
Summary: Earth's co-orbital asteroids can survive for more than 50% of the age of the Solar system on near-circular, near-planar orbits, with horseshoe particles being more likely to survive. There may be several planetesimal-sized objects originally in co-orbital libration, and the Yarkovsky effect can cause asteroids to escape.
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
(2021)
Article
Astronomy & Astrophysics
Ben W. P. Lew, Daniel Apai, Yifan Zhou, Mark Marley, L. C. Mayorga, Xianyu Tan, Vivien Parmentier, Sarah Casewell, Siyi Xu
Summary: Brown dwarfs on ultrashort-period orbits around white dwarf hosts provide an ideal opportunity to study atmospheric response under strong irradiation and fast rotation. This study presents high-precision observational constraints on the atmospheric structures of an irradiated brown dwarf at different orbital phases.
ASTRONOMICAL JOURNAL
(2022)
Article
Astronomy & Astrophysics
Nestor Espinoza, Enric Palle, Jonas Kemmer, Rafael Luque, Jose A. Caballero, Carlos Cifuentes, Enrique Herrero, Victor J. Sanchez Bejar, Stephan Stock, Karan Molaverdikhani, Giuseppe Morello, Diana Kossakowski, Martin Schlecker, Pedro J. Amado, Paz Bluhm, Miriam Cortes-Contreras, Thomas Henning, Laura Kreidberg, Martin Kurster, Marina Lafarga, Nicolas Lodieu, Juan Carlos Morales, Mahmoudreza Oshagh, Vera M. Passegger, Alexey Pavlov, Andreas Quirrenbach, Sabine Reffert, Ansgar Reiners, Ignasi Ribas, Eloy Rodriguez, Cristina Rodriguez Lopez, Andreas Schweitzer, Trifon Trifonov, Priyanka Chaturvedi, Stefan Dreizler, Sandra Jeffers, Adrian Kaminski, Maria Jose Lopez-Gonzalez, Jorge Lillo-Box, David Montes, Grzegorz Nowak, Santos Pedraz, Siegfried Vanaverbeke, Maria R. Zapatero Osorio, Mathias Zechmeister, Karen A. Collins, Eric Girardin, Pere Guerra, Ramon Naves, Ian J. M. Crossfield, Elisabeth C. Matthews, Steve B. Howell, David R. Ciardi, Erica Gonzales, Rachel A. Matson, Charles A. Beichman, Joshua E. Schlieder, Thomas Barclay, Michael Vezie, Jesus Noel Villasenor, Tansu Daylan, Ismael Mireies, Diana Dragomir, Joseph D. Twicken, Jon Jenkins, Joshua N. Winn, David Latham, George Ricker, Sara Seager
Summary: We report the discovery and characterization of TOI-1759 b, a sub-Neptune-sized exoplanet with a moderate temperature orbiting the M dwarf TOI-1759. The actual period, radius, and mass of TOI-1759 b were determined through joint analysis of photometry and radial velocity measurements. This planet shows potential for transmission spectroscopy studies and is among the top exoplanets with the highest transmission spectroscopic metric (TSM) value. Additionally, two additional signals in the radial velocities indicate possible stellar activity and further investigation is needed to determine their nature.
ASTRONOMICAL JOURNAL
(2022)
Article
Astronomy & Astrophysics
Yifan Zhou, Daniel Apai, Xianyu Tan, Joshua D. Lothringer, Ben W. P. Lew, Sarah L. Casewell, Vivien Parmentier, Mark S. Marley, Siyi Xu, L. C. Mayorga
Summary: Studying the properties of atmospheres around brown dwarfs in close-in orbits around white dwarfs, phase-resolved observations and spectral analysis reveal rotational modulations, hot spots, and day/night heat transfer limitations in the irradiated objects.
ASTRONOMICAL JOURNAL
(2022)
Article
Astronomy & Astrophysics
E. Gonzalez-Alvarez, M. R. Zapatero Osorio, J. Sanz-Forcada, J. A. Caballero, S. Reffert, V. J. S. Bejar, A. P. Hatzes, E. Herrero, S. Jeffers, J. Kemmer, M. J. Lopez-Gonzalez, R. Luque, K. Molaverdikhani, G. Morello, E. Nagel, A. Quirrenbach, E. Rodriguez, C. Rodriguez-Lopez, M. Schlecker, A. Schweitzer, S. Stock, V. M. Passegger, T. Trifonov, P. J. Amado, D. Baker, P. T. Boyd, C. Cadieux, D. Charbonneau, K. A. Collins, R. Doyon, S. Dreizler, N. Espinoza, G. Furesz, E. Furlan, K. Hesse, S. B. Howell, J. M. Jenkins, R. C. Kidwell, D. W. Latham, K. K. McLeod, D. Montes, J. C. Morales, T. O'Dwyer, E. Palle, S. Pedraz, A. Reiners, I Ribas, S. N. Quinn, C. Schnaible, S. Seager, B. Skinner, J. C. Smith, R. P. Schwarz, A. Shporer, R. Vanderspek, J. N. Winn
Summary: The discovery of two super-Earth candidates orbiting the nearby dwarf star TOI-1238 was confirmed using combined photometric and spectroscopic analysis. The planets have unique properties and characteristics that contribute to our understanding of planetary systems and their formation and evolution.
ASTRONOMY & ASTROPHYSICS
(2022)
Article
Astronomy & Astrophysics
K. R. Sreenivas, V Perdelwitz, L. Tal-Or, T. Trifonov, S. Zucker, T. Mazeh
Summary: Using fifteen years of radial velocity data, this study identified two Jupiter analogs orbiting around F8V star HD 103891 and Solar-like star HD 105779. The study highlights the importance of long-term radial velocity surveys in studying planetary occurrence beyond the snow line of Solar-like stars.
ASTRONOMY & ASTROPHYSICS
(2022)
Article
Astronomy & Astrophysics
J. Kemmer, S. Dreizler, D. Kossakowski, S. Stock, A. Quirrenbach, J. A. Caballero, P. J. Amado, K. A. Collins, N. Espinoza, E. Herrero, J. M. Jenkins, D. W. Latham, J. Lillo-Box, N. Narita, E. Palle, A. Reiners, I Ribas, G. Ricker, E. Rodriguez, S. Seager, R. Vanderspek, R. Wells, J. Winn, F. J. Aceituno, V. J. S. Bejar, T. Barclay, P. Bluhm, P. Chaturvedi, C. Cifuentes, K. Collins, M. Cortes-Contreras, B-O Demory, M. M. Fausnaugh, A. Fukui, Y. Gomez Maqueo Chew, D. Galadi-Enriquez, T. Gan, M. Gillon, A. Golovin, A. P. Hatzes, Th Henning, C. Huang, S. Jeffers, A. Kaminski, M. Kunimoto, M. Kurster, M. J. Lopez-Gonzalez, M. Lafarga, R. Luque, J. McCormac, K. Molaverdikhani, D. Montes, J. C. Morales, V. M. Passegger, S. Reffert, L. Sabin, P. Schofer, N. Schanche, M. Schlecker, U. Schroffenegger, R. P. Schwarz, A. Schweitzer, A. Sota, P. Tenenbaum, T. Trifonov, S. Vanaverbeke, M. Zechmeister
Summary: We report the discovery of GJ 3929 b, a hot Earth-sized planet orbiting the nearby star GJ 3929. By analyzing photometric, spectroscopic, and transit observations, the important parameters of this planet were determined, and another planet candidate was found.
ASTRONOMY & ASTROPHYSICS
(2022)
Article
Astronomy & Astrophysics
Xianyu Tan
Summary: Observations of brown dwarfs and young extrasolar giant planets have provided valuable insights into atmospheric dynamics. This study focuses on the formation of zonal jets, the vertical mixing of tracers, and the inhomogeneity of cloud decks. The results show that small-scale thermal perturbations can drive zonal jet streams, and robust zonal jets with speeds up to a few hundred m s(-1) are typical outcomes. The study also highlights the impact of radiative and frictional dissipation on jet formation and the transport of passive tracers.
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
(2022)
Article
Astronomy & Astrophysics
Jan Eberhardt, Trifon Trifonov, Martin Kuerster, Stephan Stock, Thomas Henning, Anna Wollbold, Sabine Reffert, Man Hoi Lee, Mathias Zechmeister, Florian Rodler, Olga Zakhozhay, Paul Heeren, Davide Gandolfi, Oscar Barragan, Marcelo Tala Pinto, Vera Wolthoff, Paula Sarkis, Stefan S. Brems
Summary: The study provides an independent Doppler validation and dynamical orbital analysis of the two-planet system HD 107148, confirming the presence of a Saturn-mass planet and a eccentric Neptune-mass exoplanet. The system exhibits long-term stability, with large secular osculations in eccentricity but no particular mean motion resonance configuration.
ASTRONOMICAL JOURNAL
(2022)
Article
Astronomy & Astrophysics
A. Quirrenbach, V. M. Passegger, T. Trifonov, P. J. Amado, J. A. Caballero, A. Reiners, I Ribas, J. Aceituno, V. J. S. Bejar, P. Chaturvedi, L. Gonzalez-Cuesta, T. Henning, E. Herrero, A. Kaminski, M. Kuerster, S. Lalitha, N. Lodieu, M. J. Lopez-Gonzalez, D. Montes, E. Palle, M. Perger, D. Pollacco, S. Reffert, E. Rodriguez, C. Rodriguez Lopez, Y. Shan, L. Tal-Or, M. R. Zapatero Osorio, M. Zechmeister
Summary: This article reports two Saturn-mass planets orbiting M dwarfs and provides their characteristics data and related analysis conclusions. It also summarizes the situation of giant planets in the CARMENES sample, and proposes some hypotheses about the formation of these orbital planets.
ASTRONOMY & ASTROPHYSICS
(2022)
Article
Astronomy & Astrophysics
Luisa Maria Serrano, Davide Gandolfi, Alexander J. Mustill, Oscar Barragan, Judith Korth, Fei Dai, Seth Redfield, Malcolm Fridlund, Kristine W. F. Lam, Matias R. Diaz, Sascha Grziwa, Karen A. Collins, John H. Livingston, William D. Cochran, Coel Hellier, Salvatore E. Bellomo, Trifon Trifonov, Florian Rodler, Javier Alarcon, Jon M. Jenkins, David W. Latham, George Ricker, Sara Seager, Roland Vanderspeck, Joshua N. Winn, Simon Albrecht, Kevin Collins, Szilard Csizmadia, Tansu Daylan, Hans J. Deeg, Massimiliano Esposito, Michael Fausnaugh, Iskra Georgieva, Elisa Goffo, Eike Guenther, Artie P. Hatzes, Steve B. Howell, Eric L. N. Jensen, Rafael Luque, Andrew W. Mann, Felipe Murgas, Hannah L. M. Osborne, Enric Palle, Carina M. Persson, Pam Rowden, Alexander Rudat, Alexis M. S. Smith, Joseph D. Twicken, Vincent Van Eylen, Carl Ziegler
Summary: Researchers discovered a four-planet system orbiting the bright star TOI-500, including an Earth-sized ultra-short-period planet and three outer planets. Through simulations, they found that the system's architecture can be explained by a non-violent migration scenario.
Article
Astronomy & Astrophysics
R. Luque, B. J. Fulton, M. Kunimoto, P. J. Amado, P. Gorrini, S. Dreizler, C. Hellier, G. W. Henry, K. Molaverdikhani, G. Morello, L. Pena-Monino, M. Perez-Torres, F. J. Pozuelos, Y. Shan, G. Anglada-Escude, V. J. S. Bejar, G. Bergond, A. W. Boyle, J. A. Caballero, D. Charbonneau, D. R. Ciardi, S. Dufoer, N. Espinoza, M. Everett, D. Fischer, A. P. Hatzes, Th Henning, K. Hesse, A. W. Howard, S. B. Howell, H. Isaacson, S. Jeffers, J. M. Jenkins, S. R. Kane, J. Kemmer, S. Khalafinejad, R. C. Kidwell, D. Kossakowski, D. W. Latham, J. Lillo-Box, J. J. Lissauer, D. Montes, J. Orell-Miquel, E. Palle, D. Pollacco, A. Quirrenbach, S. Reffert, A. Reiners, I Ribas, G. R. Ricker, L. A. Rogers, J. Sanz-Forcada, M. Schlecker, A. Schweitzer, S. Seager, A. Shporer, K. G. Stassun, S. Stock, L. Tal-Or, E. B. Ting, T. Trifonov, S. Vanaverbeke, R. Vanderspek, J. Villasenor, J. N. Winn, J. G. Winters, M. R. Zapatero Osorio
Summary: This study reports the discovery of a multiplanetary system transiting the M0 V dwarf HD 260655. The system consists of at least two transiting planets, HD 260655 b and HD 260655 c. Both planets have been detected in transit by the TESS mission and confirmed independently with radial velocity measurements. The system is notable for being relatively close to Earth and having a bright host star, making it ideal for atmospheric studies with the James Webb Space Telescope.
ASTRONOMY & ASTROPHYSICS
(2022)
Article
Astronomy & Astrophysics
S. Ulmer-Moll, M. Lendl, S. Gill, S. Villanueva, M. J. Hobson, F. Bouchy, R. Brahm, D. Dragomir, N. Grieves, C. Mordasini, D. R. Anderson, J. S. Acton, D. Bayliss, A. Bieryla, M. R. Burleigh, S. L. Casewell, G. Chaverot, P. Eigmueller, D. Feliz, B. S. Gaudi, E. Gillen, M. R. Goad, A. F. Gupta, M. N. Gunther, B. A. Henderson, T. Henning, J. S. Jenkins, M. Jones, A. Jordan, A. Kendall, D. W. Latham, I Mireles, M. Moyano, J. Nadol, H. P. Osborn, J. Pepper, M. T. Pinto, A. Psaridi, D. Queloz, S. Quinn, F. Rojas, P. Sarkis, M. Schlecker, R. H. Tilbrook, P. Torres, T. Trifonov, S. Udry, J. Vines, R. West, P. Wheatley, X. Yao, Y. Zhao, G. Zhou
Summary: Through spectroscopic and photometric follow-up observations of the TESS data, two massive warm Jupiter-size exoplanets were confirmed to orbit the F8-type star TOI-5153 and the G1-type star NGTS-20 (=TOI-5152). These planets are valuable targets for further studies on planetary atmosphere and measurement of the spin-orbit angle of the system.
ASTRONOMY & ASTROPHYSICS
(2022)
Article
Astronomy & Astrophysics
Rafael Brahm, Solene Ulmer-Moll, Melissa J. Hobson, Andres Jordan, Thomas Henning, Trifon Trifonov, Matias I. Jones, Martin Schlecker, Nestor Espinoza, Felipe I. Rojas, Pascal Torres, Paula Sarkis, Marcelo Tala, Jan Eberhardt, Diana Kossakowski, Diego J. Munoz, Joel D. Hartman, Gavin Boyle, Vincent Suc, Francois Bouchy, Adrien Deline, Guillaume Chaverot, Nolan Grieves, Monika Lendl, Olga Suarez, Tristan Guillot, Amaury H. M. J. Triaud, Nicolas Crouzet, Georgina Dransfield, Ryan Cloutier, Khalid Barkaoui, Rick P. Schwarz, Chris Stockdale, Mallory Harris, Ismael Mireles, Phil Evans, Andrew W. Mann, Carl Ziegler, Diana Dragomir, Steven Villanueva, Christoph Mordasini, George Ricker, Roland Vanderspek, David W. Latham, Sara Seager, Joshua N. Winn, Jon M. Jenkins, Michael Vezie, Allison Youngblood, Tansu Daylan, Karen A. Collins, Douglas A. Caldwell, David R. Ciardi, Enric Palle, Felipe Murgas
Summary: We have discovered and characterized three new warm giant planets with transiting properties. These planets were initially detected through single-transit events in the light curves generated by the Transiting Exoplanet Survey Satellite. Further measurements and analysis confirmed their orbital periods and planetary nature. The planets orbit stars with slightly higher metal content. TOI 4406b has a low eccentricity orbit with a period of 30.08364 days, TOI 2338b has a highly eccentric orbit with a period of 22.65398 days, and TOI 2589b has an eccentric orbit with a period of 61.6277 days. TOI 4406b and TOI 2338b exhibit metal enrichment compared to their host stars, while TOI 2589b is consistent with having similar metal enrichment.
ASTRONOMICAL JOURNAL
(2023)
Article
Astronomy & Astrophysics
Trifon Trifonov, Rafael Brahm, Andres Jordan, Christian Hartogh, Thomas Henning, Melissa J. Hobson, Martin Schlecker, Saburo Howard, Finja Reichardt, Nestor Espinoza, Man Hoi Lee, David Nesvorny, Felipe I. Rojas, Khalid Barkaoui, Diana Kossakowski, Gavin Boyle, Stefan Dreizler, Martin Kuerster, Rene Heller, Tristan Guillot, Amaury H. M. J. Triaud, Lyu Abe, Abdelkrim Agabi, Philippe Bendjoya, Nicolas Crouzet, Georgina Dransfield, Thomas Gasparetto, Maximilian N. Guenther, Wenceslas Marie-Sainte, Djamel Mekarnia, Olga Suarez, Johanna Teske, R. Paul Butler, Jeffrey D. Crane, Stephen Shectman, George R. Ricker, Avi Shporer, Roland Vanderspek, Jon M. Jenkins, Bill Wohler, Karen A. Collins, Kevin I. Collins, David R. Ciardi, Thomas Barclay, Ismael Mireles, Sara Seager, Joshua N. Winn
Summary: The K-type star TOI-2525 has two companions, similar to Neptune and Jupiter, with measured masses, radii, and orbital periods. This discovery is important for understanding planet formation and evolution.
ASTRONOMICAL JOURNAL
(2023)
Article
Astronomy & Astrophysics
Vladimir Bozhilov, Desislava Antonova, Melissa J. Hobson, Rafael Brahm, Andres Jordan, Thomas Henning, Jan Eberhardt, Felipe I. Rojas, Konstantin Batygin, Pascal Torres-Miranda, Keivan G. Stassun, Sarah C. Millholland, Denitza Stoeva, Milen Minev, Nestor Espinoza, George R. Ricker, David W. Latham, Diana Dragomir, Michelle Kunimoto, Jon M. Jenkins, Eric B. Ting, Sara Seager, Joshua N. Winn, Jesus Noel Villasenor, Luke G. Bouma, Jennifer Medina, Trifon Trifonov
Summary: We discovered a super-Jovian 2:1 mean-motion resonance (MMR) pair around the G-type star TIC 279401253, which provides a benchmark for studying planet formation and orbital evolution. The discovery was made through a single-transit event recorded by the Transiting Exoplanet Survey Satellite mission, indicating the presence of a Jupiter-sized companion with uncertain orbital parameters. To learn more, we conducted ground-based radial velocity monitoring with HARPS and FEROS, revealing the existence of two massive planets with periods of 76.80 and 155.3 days, respectively. The system shows a rare example of a strong first-order, eccentricity-type 2:1 MMR, suggesting disk-induced planet migration.
ASTROPHYSICAL JOURNAL LETTERS
(2023)