News & Views |
Featured
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Article |
The future lifespan of Earth’s oxygenated atmosphere
Earth’s oxygen-rich atmosphere will probably persist for only one billion more years before it sharply deoxygenates to low-level oxygen similar to those of the Archaean, according to a combined biogeochemistry and climate model.
- Kazumi Ozaki
- & Christopher T. Reinhard
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Article |
Implications of the iron oxide phase transition on the interiors of rocky exoplanets
The interior structure and rheology of large terrestrial exoplanets is strongly affected by the phase transition of iron-oxide, according to dynamic compression and X-ray diffraction FeO experiments up to 700 GPa and calculation of the binary MgO–FeO phase diagram.
- F. Coppari
- , R. F. Smith
- & T. S. Duffy
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Article |
Efficient cooling of rocky planets by intrusive magmatism
Rocky planets dominated by intrusive magmatism can cool more efficiently than those dominated by extrusive volcanism, according to numerical simulations of mantle convection.
- Diogo L. Lourenço
- , Antoine B. Rozel
- & Paul J. Tackley
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Article |
Continuous reorientation of synchronous terrestrial planets due to mantle convection
Mantle convection in rocky planets in a synchronous orbit around their host stars can induce continuous reorientation, according to an analysis of the efficiency of true polar wander for synchronous exoplanets.
- Jérémy Leconte
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Comment |
Atmospheric science looks to Venus
Making sense of exoplanet observations requires better understanding of terrestrial atmospheres in our solar system, especially for Venus. We need to not just intermittently explore, but continuously monitor these atmospheres — like we do for Earth.
- Kevin McGouldrick
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News & Views |
Bypassing the habitable zone
In our own solar system, Venus is too hot, Mars is too cold and Earth is just right. Simulations show that making an icy planet habitable is not as simple as melting its ice: many icy bodies swing from too cold to too hot, bypassing just right.
- Andrew P. Ingersoll
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Article |
Abrupt climate transition of icy worlds from snowball to moist or runaway greenhouse
Icy planets and moons could become habitable as their host stars brighten and their ice melts. Climate simulations instead show a rapid transition from a snowball to an inhospitable greenhouse climate with significant water loss.
- Jun Yang
- , Feng Ding
- & Yonggang Liu
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Letter |
Water contents of Earth-mass planets around M dwarfs
Faint M dwarf stars are the focus of searches for habitable planets. Numerical models suggest that changes in stellar luminosity lead to planets that are either too dry or too wet to be habitable in M dwarf systems.
- Feng Tian
- & Shigeru Ida
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Editorial |
Expanding spheres of interest
Extrasolar planet research is booming. We welcome submissions with links to the geosciences.
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Commentary |
Strange news from other stars
The dawn of exoplanet discovery has unearthed a rich tapestry of planets different from anything encountered in the Solar System. Geoscientists can and should be in the vanguard of investigating what is out there in the Universe.
- Raymond T. Pierrehumbert