Results 251 to 260 of about 4,316 (299)

Gas detection-assisted deep-space and deep-sea exploration. [PDF]

open access: yesInnovation (Camb)
Wang Q, Cao N, Hu M, Li X, Kan R.
europepmc   +1 more source

Convective dynamics in mantle of tidally-locked exoplanets. [PDF]

open access: yesNat Commun
Noto D   +4 more
europepmc   +1 more source

The evolution of Gaia(s). [PDF]

open access: yesPhilos Trans R Soc Lond B Biol Sci
Lenton TM.
europepmc   +1 more source

The rainout of formaldehyde favors a formose-based origin of life in shallow ponds

open access: yes
Scherf M   +10 more
europepmc   +1 more source

The Sizes of Habitable Planets

Publications of the Astronomical Society of the Pacific, 1960
Size requirements for habitable planets, discussing relationship between surface area and biological ...
Su-Shu Huang
exaly   +2 more sources

Survival of habitable planets in unstable planetary systems

open access: yesMonthly Notices of the Royal Astronomical Society, 2016
Many observed giant planets lie on eccentric orbits. Such orbits could be the result of strong scatterings with other giant planets. The same dynamical instability that produces giant planet scatterings can also alter the orbits of terrestrial planets ...
Daniel Carrera   +2 more
exaly   +3 more sources

Habitable Moist Atmospheres on Terrestrial Planets near the Inner Edge of the Habitable Zone around M Dwarfs [PDF]

open access: yesAstrophysical Journal, 2017
Terrestrial planets in the habitable zones (HZs) of low-mass stars and cool dwarfs have received significant scrutiny recently. Transit spectroscopy of such planets with the James Webb Space Telescope (JWST) represents our best shot at obtaining the ...
Ravi Kumar Kopparapu   +2 more
exaly   +2 more sources

Habitable Planets with High Obliquities

Icarus, 1997
Earth's obliquity would vary chaotically from 0 degrees to 85 degrees were it not for the presence of the Moon (J. Laskar, F. Joutel, and P. Robutel, 1993, Nature 361, 615-617). The Moon itself is thought to be an accident of accretion, formed by a glancing blow from a Mars-sized planetesimal.
D M, Williams, J F, Kasting
openaire   +2 more sources

Habitable Planet, Characterization

2011
The spectrum of a planet can contain signatures of atmospheric species, which create its spectral fingerprint. The presence and abundance of atmospheric species, in the context of the properties of the star and the planet, can elucidate the underlying physics and characterize a planetary environment.
Lisa Kaltenegger, Franck Selsis
openaire   +1 more source

Evolution of a Habitable Planet

Annual Review of Astronomy and Astrophysics, 2003
▪ Abstract  Giant planets have now been discovered around other stars, and it is only a matter of time until Earth-sized planets are detected. Whether any of these planets are suitable for life depends on their volatile abundances, especially water, and on their climates.
Kasting, JF, Catling, DC
openaire   +2 more sources

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