Tag

Habitability

All articles tagged with #habitability

A 0.8 Earth-Radius Threshold Signals When Tiny Planets Lose Their Atmospheres
space13 days ago

A 0.8 Earth-Radius Threshold Signals When Tiny Planets Lose Their Atmospheres

A new model called STEHM finds that planets smaller than about 0.8 Earth radii struggle to hold onto atmospheres due to weaker gravity and faster interior cooling, which suppresses outgassing; under common CO2 conditions, 0.6–0.5 R⊕ worlds can lose atmospheres in tens to hundreds of millions of years, while planets at or above 0.8 R⊕ retain thick atmospheres for billions of years. Exceptions exist for unusually high initial carbon, minimal core radius, or a cold start delaying outgassing. The study suggests using 0.8 R⊕ as a practical filter in planning future exoplanet observations and prioritizing targets for atmospheric characterization.

Desert Exoplanets in the Habitable Zone May Not Harbor Life
science27 days ago

Desert Exoplanets in the Habitable Zone May Not Harbor Life

A University of Washington study finds that an Earth-sized planet needs a substantial surface water inventory—about 20–50% of Earth’s ocean volume—to maintain long-term habitability. On very dry worlds, the carbon cycle can break down, allowing CO2 to build up and heat the planet, potentially rendering it uninhabitable despite being in the habitable zone. Venus serves as a nearby analog, illustrating how small water differences can dramatically impact climate. The work suggests many desert-like exoplanets thought promising for life may actually be poor candidates and informs future observations and Venus missions.

Curiosity detects diverse organics on Mars, hinting at ancient habitability
science-space1 month ago

Curiosity detects diverse organics on Mars, hinting at ancient habitability

NASA’s Curiosity rover, via a wet-chemistry experiment on a Mary Anning rock at Gale Crater, uncovered 21 carbon-containing molecules, including seven not previously detected on Mars. The organics could be preserved for about 3.5 billion years, reinforcing the idea that ancient Mars was habitable, though the findings do not prove life. Researchers say definitive answers require returning samples to Earth, and future missions with similar chemistry experiments (e.g., ExoMars Rosalind Franklin, Dragonfly) will continue probing Mars’ organic past.

Rogue planets' moons may host billions of years of habitability
space2 months ago

Rogue planets' moons may host billions of years of habitability

Astronomers propose that moons orbiting free-floating, starless rogue planets could stay warm enough for liquid water for billions of years thanks to tidal heating and hydrogen-dominated atmospheres that trap heat via collision-induced absorption (CIA). Using radiative-transfer (HELIOS) and chemistry (GGchem) codes, the study shows such exomoons could maintain long-term habitability even without a sun, though the models rely on simplifications (e.g., dry atmospheres, constant gravity) and future work will add clouds and water-vapor effects. This expands the search for life beyond traditional, star‑dependent habitable zones.

Dark-world oceans: moons around sunless rogue planets could harbor life for billions of years
space-exploration2 months ago

Dark-world oceans: moons around sunless rogue planets could harbor life for billions of years

New simulations suggest Earth-sized moons orbiting free-floating, starless rogue planets could remain warm enough to keep liquid water on their surfaces for up to 4.3 billion years, thanks to tidal heating and insulating hydrogen atmospheres, potentially expanding habitable environments beyond traditional stellar zones.

NASA’s SPARCS CubeSat Captures First Ultraviolet Images of Common Milky Way Stars
space2 months ago

NASA’s SPARCS CubeSat Captures First Ultraviolet Images of Common Milky Way Stars

NASA's Star-Planet Activity Research CubeSat (SPARCS), launched in January 2026, has delivered the first ultraviolet images of nearby low-mass stars, confirming its UV-sensitive detectors and readiness for science operations. Over about a year it will monitor around 20 stars to study how their flares and UV activity affect orbiting exoplanets, a key step in understanding planetary atmospheres and habitability.

Inside-Out Exoplanet System Upends Formation Theory
world3 months ago

Inside-Out Exoplanet System Upends Formation Theory

CHEOPS observations reveal four planets orbiting the red dwarf LHS 1903 far closer to their star than Mercury is to the Sun: two rocky super-Earths and two gaseous mini-Neptunes. The outermost planet, surprisingly rocky, challenges standard models that predict rocky worlds close in and gas giants farther out, suggesting an 'inside-out' assembly in which gas was depleted by inner planets or the atmosphere was stripped after formation. With a mass of about 5.8 Earth masses and a surface temperature around 60°C, it could be marginally habitable, and future JWST studies could probe its atmosphere.

Europa’s Ice Shell Is Much Thicker Than We Thought, New Juno Data Show
space-and-spaceflight3 months ago

Europa’s Ice Shell Is Much Thicker Than We Thought, New Juno Data Show

A 2022 Juno flyby analysis estimates Europa’s ice shell in the observed region to be about 29 kilometers (18 miles) thick on average. If a warmer, convective inner layer exists, the total thickness could be greater; the presence of dissolved salt could reduce thickness by roughly 4.8 kilometers. Near-surface “scatterers” (cracks/pores) are likely small and not major pathways for exchange with the ocean. These findings help constrain how the subsurface ocean might connect to the surface and inform upcoming Europa Clipper and Juice missions in assessing the moon’s habitability.

Juno Estimates Europa’s Ice Shell at 29 Kilometers, Hinting at a Deeper Ocean
space3 months ago

Juno Estimates Europa’s Ice Shell at 29 Kilometers, Hinting at a Deeper Ocean

NASA’s Juno used its Microwave Radiometer to measure Europa’s near-surface ice shell during a 2022 flyby, finding an average thickness of about 29 km (18 miles) in the observed region and favoring thicker-shell models; if a salty layer exists, thickness could be reduced by about 3 miles. The data also reveal small near-surface scatterers—cracks and pores—not likely to provide major nutrient pathways to the subsurface ocean, with implications for future Europa Clipper and Juice missions.

Basal magma oceans could power magnetic shields on super-Earths, boosting habitability
space3 months ago

Basal magma oceans could power magnetic shields on super-Earths, boosting habitability

A Nature Astronomy study suggests that some super-Earths (about 3–6 times Earth's mass) may sustain long‑lived magnetic fields not from a core dynamo but from a basal magma ocean layer between the core and mantle, potentially protecting atmospheres and improving habitability; while detecting such fields remains challenging, future observations could test this BMO‑driven dynamo scenario.