Results 61 to 70 of about 53,007 (245)

WASP-189b: an ultra-hot Jupiter transiting the bright A star HR 5599 in a polar orbit [PDF]

, 2018
We report the discovery of WASP-189b: an ultra-hot Jupiter in a 2.72-d transiting orbit around the $V = 6.6$ A star WASP-189 (HR 5599). We detected periodic dimmings in the star's lightcurve, first with the WASP-South survey facility then with the ...
Anderson, D. R., Bouchy, F., Brown, D. J. A., Burdanov, A., Cameron, A. Collier, Gillon, M., Hellier, C., Jehin, E., Maxted, P. F. L., Nielsen, L. D., Pepe, F., Pollacco, D., Pozuelos, F. J., Queloz, D., Smalley, B., Ségransan, D., Temple, L. Y., Triaud, A. H. M. J., Turner, O. D., Udry, S., West, R. G.   +20 more
core  

A Secular Resonant Origin for the Loneliness of Hot Jupiters [PDF]

, 2017
Despite decades of inquiry, the origin of giant planets residing within a few tenths of an astronomical unit from their host stars remains unclear. Traditionally, these objects are thought to have formed further out before subsequently migrating inwards.
Batygin, Konstantin, Spalding, Christopher   +1 more
core   +3 more sources

Three-dimensional Orbital Architectures and Detectability of Adjacent Companions to Hot Jupiters

The Astrophysical Journal
The orbital properties of the (as yet) small population of hot Jupiters with nearby planetary companions provide valuable constraints on the past migration processes of these systems.
Thomas MacLean, Juliette Becker
doaj   +1 more source

Enhancement of the Plant‐Accessible Phosphate Fraction in Sewage Sludge Ashes by Na+ or K+ Addition Prior to Combustion

ChemSusChem, Volume 18, Issue 6, March 15, 2025.
The addition of Na2CO3 or K2CO3 to sewage sludge prior to combustion leads to the production of ashes containing phosphate in the form of buchwaldite‐like phases (Ca(Na/K)PO4). Compared to conventional sewage sludge mono‐ashes, such Na‐ or K‐ashes show greatly increased P‐solubilities and proved to be potent P‐fertiliser materials in greenhouse ...
Lorenz Bier‐Schorr, Viktoria Gräser, Michael Scherer‐Lorenzen, Peter Hajek, Philipp Kurz   +4 more
wiley   +1 more source

Ohmic Dissipation in the Atmospheres of Hot Jupiters

, 2010
Hot Jupiter atmospheres exhibit fast, weakly-ionized winds. The interaction of these winds with the planetary magnetic field generates drag on the winds and leads to ohmic dissipation of the induced electric currents.
Baraffe, Batygin, Burrows, Burrows, Charbonneau, Cooper, Dobbs-Dixon, Emily Rauscher, Gu, Hansen, Ibgui, Iro, Kristen Menou, Laine, Liu, Perna, Rauscher, Rosalba Perna, Sanchez-Lavega, Showman, Showman   +20 more
core   +1 more source

Toward Eclipse Mapping of Hot Jupiters [PDF]

, 2006
Recent Spitzer infrared measurements of hot Jupiter eclipses suggest that eclipse mapping techniques could be used to spatially resolve the day-side photospheric emission of these planets using partial occultations.
Bobinger A., Bradley M. S. Hansen, Drake Deming, Emily Rauscher, Horne K., James Y.‐K. Cho, Kristen Menou, Perryman M. A. C., Sara Seager, Spruit H. C., Valenti J. A., Warner B.   +11 more
core   +3 more sources

The TESS Grand Unified Hot Jupiter Survey. II. Twenty New Giant Planets

The Astrophysical Journal Supplement Series, 2023
NASA’s Transiting Exoplanet Survey Satellite (TESS) mission promises to improve our understanding of hot Jupiters by providing an all-sky, magnitude-limited sample of transiting hot Jupiters suitable for population studies.
Samuel W. Yee, Joshua N. Winn, Joel D. Hartman, Luke G. Bouma, George Zhou, Samuel N. Quinn, David W. Latham, Allyson Bieryla, Joseph E. Rodriguez, Karen A. Collins, Owen Alfaro, Khalid Barkaoui, Corey Beard, Alexander A. Belinski, Zouhair Benkhaldoun, Paul Benni, Krzysztof Bernacki, Andrew W. Boyle, R. Paul Butler, Douglas A. Caldwell, Ashley Chontos, Jessie L. Christiansen, David R. Ciardi, Kevin I. Collins, Dennis M. Conti, Jeffrey D. Crane, Tansu Daylan, Courtney D. Dressing, Jason D. Eastman, Zahra Essack, Phil Evans, Mark E. Everett, Sergio Fajardo-Acosta, Raquel Forés-Toribio, Elise Furlan, Mourad Ghachoui, Michaël Gillon, Coel Hellier, Ian Helm, Andrew W. Howard, Steve B. Howell, Howard Isaacson, Emmanuel Jehin, Jon M. Jenkins, Eric L. N. Jensen, John F. Kielkopf, Didier Laloum, Naunet Leonhardes-Barboza, Pablo Lewin, Sarah E. Logsdon, Jack Lubin, Michael B. Lund, Mason G. MacDougall, Andrew W. Mann, Natalia A. Maslennikova, Bob Massey, Kim K. McLeod, Jose A. Muñoz, Patrick Newman, Valeri Orlov, Peter Plavchan, Adam Popowicz, Francisco J. Pozuelos, Tyler A. Pritchard, Don J. Radford, Michael Reefe, George R. Ricker, Alexander Rudat, Boris S. Safonov, Richard P. Schwarz, Heidi Schweiker, Nicholas J. Scott, S. Seager, Stephen A. Shectman, Chris Stockdale, Thiam-Guan Tan, Johanna K. Teske, Neil B. Thomas, Mathilde Timmermans, Roland Vanderspek, David Vermilion, David Watanabe, Lauren M. Weiss, Richard G. West, Judah Van Zandt, Michal Zejmo, Carl Ziegler   +86 more
doaj   +1 more source

TWO HOT JUPITERS FROM K2 CAMPAIGN 4 [PDF]

The Astronomical Journal, 2016
ABSTRACT We confirm the planetary nature of two transiting hot Jupiters discovered by the Kepler  spacecraft’s K2 extended mission in its Campaign 4, using precise radial velocity measurements from FIES@NOT, HARPS-N@TNG, and the coudé spectrograph on the McDonald Observatory 2.7 m telescope.
Marshall C. Johnson, Davide Gandolfi, Malcolm Fridlund, Szilard Csizmadia, Michael Endl, Juan Cabrera, William D. Cochran, Hans J. Deeg, Sascha Grziwa, Ivan Ramírez, Artie P. Hatzes, Philipp Eigmüller, Oscar Barragán, Anders Erikson, Eike W. Guenther, Judith Korth, Teet Kuutma, David Nespral, Martin Pätzold, Enric Palle, Jorge Prieto-Arranz, Heike Rauer, Joonas Saario   +22 more
openaire   +5 more sources

Evidence From Microscopy and U–Pb Geochronology as a Clue to the Influence of the Cretaceous Magmatism in the Diagenesis of Pre‐Salt Carbonate Reservoirs in the Santos Basin (Brazil)

Geological Journal, EarlyView.
Carbonates from Santos Basin revealed U–Pb ages correlated with basalt ages (A), suggesting that they were formed during magmatic events. These events placed hot CO2 in the reservoir, which, when mixed with carbonate‐rich cold water (B), led to thermal convection, enabling the formation of the U contained in the carbonates.
Marco António Ruivo de Castro e Brito, Cristiano Leite Sombra, Davy Raeder Brandão, Cleverson Guizan Silva, Sidney Luiz de Matos Mello, Eugênio Vaz dos Santos Neto, Rui Jorge Fernandes Baptista, Ramsés Capilla, Luiz Antônio Pierantoni Gambôa   +8 more
wiley   +1 more source

Elliptical instability in hot Jupiter systems

, 2013
Several studies have already considered the influence of tides on the evolution of systems composed of a star and a close-in companion to tentatively explain different observations such as the spin-up of some stars with hot Jupiters, the radius anomaly ...
Bars, Michael Le, Cébron, David, Gal, Patrice Le, Leconte, J., Moutou, Claire, Sauret, Alban   +5 more
core   +1 more source