Established in 2006 by the International Astronomical Union, the current definition specifies that to qualify as a planet, a celestial body must orbit the Sun within our Solar System. But…
Within the uncertainties of involved astronomical and biological parameters, the Drake equation typically predicts that there should be many exoplanets (< 100 to millions) in our Milky Way Galaxy hosting active,…
Ocean worlds are planetary bodies that have a liquid ocean, often under an icy shell or within the rocky interior. In our own Solar System, several moons of Jupiter and…
Fully understanding how a rocky planet becomes habitable and remains so is a fundamental challenge for planetary scientists and astrobiologists, given the diversity and complexity of intrinsic and extrinsic processes…
The NASA/ESA/CSA James Webb Space Telescope has begun its scientific mission, which includes the atmospheric characterization of transiting exoplanets. Some of the first exoplanets to be observed by Webb have…
The search for definitive biosignatures — unambiguous markers of past or present life — is a central goal of paleobiology and astrobiology. A team of researchers led by the Carnegie…
Plate tectonics is a fundamental factor in the sustained habitability of Earth, but its time of onset is unknown, with ages ranging from the Hadean to Proterozoic eon. University of…
Astronomers recently announced the discovery of TOI-700e, a habitable-zone, Earth-sized planet some 102 light-years away in the southern constellation of Dorado. Could this new discovery lead to humans one day…
The timing and locations of formation of planetesimals — the building blocks of planets — are crucial to the understanding of planet formation. If we are to form larger planets…