habitable exoplanet tagged posts

Exploring late accretion’s role in terrestrial planet evolution


Media Title
High-energy Venus Impacts

Southwest Research Institute has collaborated with Yale University to summarize the scientific community’s notable progress in advancing the understanding of the formation and evolution of the inner rocky planets, the so-called terrestrial planets. Their paper focuses on late accretion’s role in the long-term evolution of terrestrial planets, including their distinct geophysical and chemical properties as well as their potential habitability.

The Review paper is published in the journal Nature.

Solar systems form when clouds of gas and dust begin to coalesce. Gravity pulls these elements together, forming a central star, like our sun, surrounded by a flattened disk of consolidating materials...

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Possible Atmospheric Destruction of a potentially Habitable Exoplanet

Astrophysicists studying a popular exoplanet in its star’s habitable zone have found that electric currents in the planet’s upper atmosphere could create sufficient heating to expand the atmosphere enough that it leaves the planet, likely leaving the planet uninhabitable.

Until now, planetary scientists have thought that a habitable planet needs a strong magnetic field surrounding it to act as a shield, directing ionized particles, X-rays and ultraviolet radiation in the stellar wind around and away from its atmosphere.
That’s what happens on Earth, preventing dangerous radiation from reaching life on the surface, and what does not occur on Mars, which now lacks a global magnetic field, meaning any initial inhabitants of the red planet will probably need to live in underground caves...

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A Planet 1,200 light-yrs away is a good Prospect for a Habitable World

An artist's conception of Kepler-62f, a planet in the 'habitable zone' of a star located about 1,200 light-years from Earth. Credit: NASA Ames/JPL-Caltech/T. Pyle

An artist’s conception of Kepler-62f, a planet in the ‘habitable zone’ of a star located about 1,200 light-years from Earth. Credit: NASA Ames/JPL-Caltech/T. Pyle

Combined climate, orbit models show Kepler-62f might be able to sustain life. The planet, in the direction of constellation Lyra, is ~40% larger than Earth. At that size, Kepler-62f is within the range of planets that are likely to be rocky and possibly could have oceans. NASA’s Kepler mission discovered the planetary system that includes Kepler-62f in 2013, and it identified Kepler-62f, the outermost of 5 planets orbiting a star that is smaller and cooler than the sun. but there was no composition, atmosphere or orbit data.

To determine whether the planet could sustain life, the team came up with possible scenarios about what it...

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