Results 161 to 170 of about 13,254 (205)

Astrovirology and terrestrial life survival. [PDF]

Bioinformation
Shapshak P, Zandi M, Somboonwit C, T Sinnott J.   +3 more
europepmc   +1 more source

A qualitative assessment of limits of active flight in low density atmospheres. [PDF]

Sci Rep
Pajusalu M, Seager S, Huang J, Petkowski JJ.   +3 more
europepmc   +1 more source

PEPSI Investigation, Retrieval, and Atlas of Numerous Giant Atmospheres (PIRANGA). IV. High-resolution Phased-resolved Spectroscopy of the Ultra-hot-Jupiter KELT-20 b. [PDF]

Astron J
Bonidie V, Johnson MC, Wang J, Petz S, Kamen J, Lenhart C, Duck A, Badenes C, Strassmeier K, Ilyin I.   +9 more
europepmc   +1 more source

The erosion of large primary atmospheres typically leaves behind substantial secondary atmospheres on temperate rocky planets. [PDF]

Nat Commun
Krissansen-Totton J, Wogan N, Thompson M, Fortney JJ.   +3 more
europepmc   +1 more source

A transiting giant planet in orbit around a 0.2-solar-mass host star. [PDF]

Nat Astron
Bryant EM, Jordán A, Hartman JD, Bayliss D, Sedaghati E, Barkaoui K, Chouqar J, Pozuelos FJ, Thorngren DP, Timmermans M, Almenara JM, Chilingarian IV, Collins KA, Gan T, Howell SB, Narita N, Palle E, Rackham BV, Triaud AHMJ, Bakos GÁ, Brahm R, Hobson MJ, Van Eylen V, Amado PJ, Arnold L, Bonfils X, Burdanov A, Cadieux C, Caldwell DA, Casanova V, Charbonneau D, Clark CA, Collins KI, Daylan T, Dransfield G, Demory BO, Ducrot E, Fernández-Rodríguez G, Fukuda I, Fukui A, Gillon M, Gore R, Hooton MJ, Ikuta K, Jehin E, Jenkins JM, Levine AM, Littlefield C, Murgas F, Nguyen K, Parviainen H, Queloz D, Seager S, Sebastian D, Srdoc G, Vanderspek R, Winn JN, de Wit J, Zúñiga-Fernández S.   +58 more
europepmc   +1 more source

Precise Masses Reveal that TOI-700 c is Low Density and TOI-700 d is Rocky

Gilbert E, Burt J, Barragán O, Siegel J, Mascareño AS, Silva A, Luque R, Rogers J, Lee E, Lopez E, Vanderburg A, Clement M, Youngblood A, Mamajek E, Sousa S, Cameron AC, Rodriguez J, Martin D, Arney G, Barclay T, Becker J, Colon K, Eisner N, Halverson S, Hord B, Kane S, Kreidberg L, Morley C, Mortier A, Nielsen L, Quintana E, Schlieder J, Suissa G, Triaud A, Trifonov T, Eylen VV.   +35 more
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Understanding Exoplanet Atmospheres

2022
The study of exoplanet atmospheres is a blossoming field. Over the past two decades, dozens of hot gas giant atmospheres have been observed using a variety of techniques with both space and ground telescopes, revealing the presence of water, the ubiquity of clouds, the presence of equatorial jets, the existence of photoevaporation, and much more. For
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Atmospheres of Exoplanets

2017
Atmospheres of exoplanets are our only window into the physical and chemical processes occurring in these distant worlds. These processes are important tracers of the origins and evolution of planetary systems, including our Solar System. In this broader context, we could better understand how common (or unique) are the conditions leading to the ...
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Exoplanet atmosphere. Thermal structure of an exoplanet atmosphere from phase-resolved emission spectroscopy.

Science (New York, N.Y.), 2014
Exoplanets that orbit close to their host stars are much more highly irradiated than their solar system counterparts. Understanding the thermal structures and appearances of these planets requires investigating how their atmospheres respond to such extreme stellar forcing.
Kevin B, Stevenson, Jean-Michel, Désert, Michael R, Line, Jacob L, Bean, Jonathan J, Fortney, Adam P, Showman, Tiffany, Kataria, Laura, Kreidberg, Peter R, McCullough, Gregory W, Henry, David, Charbonneau, Adam, Burrows, Sara, Seager, Nikku, Madhusudhan, Michael H, Williamson, Derek, Homeier   +15 more
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Exoplanet Atmosphere Modeler

American Scientist, 2022
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