Proxima Centauri b Archives - Astrobiology

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“Proxima Centauri b”

How Airports Could Help Aliens Spot Earth

SETI & Technosignatures

How Airports Could Help Aliens Spot Earth

Simulating The Detectability Of A Range Of Molecules For High-contrast, High-resolution Observations Of Non-transiting Terrestrial Exoplanets

Astrochemistry

Simulating The Detectability Of A Range Of Molecules For High-contrast, High-resolution Observations Of Non-transiting Terrestrial Exoplanets

Bioverse: GMT and ELT Direct Imaging and High-Resolution Spectroscopy Assessment – Surveying Exo-Earth O2 and Testing the Habitable Zone Oxygen Hypothesis

Biosignatures & Paleobiology

Bioverse: GMT and ELT Direct Imaging and High-Resolution Spectroscopy Assessment – Surveying Exo-Earth O2 and Testing the Habitable Zone Oxygen Hypothesis

Migration Of Bodies In The Proxima Centauri and Trappist 1 Planetary Systems

Exoplanets, -moons, -comets

Migration Of Bodies In The Proxima Centauri and Trappist 1 Planetary Systems

Earth-like Exoplanets In Spin-orbit Resonances: Climate Dynamics, 3D Atmospheric Chemistry, and Observational Signatures

Proxima Centauri

Earth-like Exoplanets In Spin-orbit Resonances: Climate Dynamics, 3D Atmospheric Chemistry, and Observational Signatures

RISTRETTO: A VLT XAO Design To Reach Proxima Cen b In The Visible

Proxima Centauri

RISTRETTO: A VLT XAO Design To Reach Proxima Cen b In The Visible

Detectability Simulations of a NIR Surface Biosignature on Proxima Centauri b with Future Space Observatories

Proxima Centauri

Detectability Simulations of a NIR Surface Biosignature on Proxima Centauri b with Future Space Observatories

Exoplanets In Reflected Starlight With Dual-field Interferometry: A Case For Shorter Wavelengths And A Fifth Unit Telescope At VLTI/Paranal

Astronomy & Telescopes

Exoplanets In Reflected Starlight With Dual-field Interferometry: A Case For Shorter Wavelengths And A Fifth Unit Telescope At VLTI/Paranal

Lethal Surface Ozone Concentrations Are Possible On Habitable Zone Exoplanets

Habitable Zones

Lethal Surface Ozone Concentrations Are Possible On Habitable Zone Exoplanets

Swarming Proxima Centauri: Coherent Picospacecraft Swarms Over Interstellar Distances

Interstellar

Swarming Proxima Centauri: Coherent Picospacecraft Swarms Over Interstellar Distances

The Impact Of Ozone On Earth-like Exoplanet Climate Dynamics: The Case Of Proxima Centauri b

Proxima Centauri

The Impact Of Ozone On Earth-like Exoplanet Climate Dynamics: The Case Of Proxima Centauri b

Water Vapour Transit Ambiguities for Habitable M-Earths

Exoplanets, -moons, -comets

Water Vapour Transit Ambiguities for Habitable M-Earths

Biosignatures: Looking For Signs Of Life Among Exoplanet Atmospheres

Biosignatures & Paleobiology

Biosignatures: Looking For Signs Of Life Among Exoplanet Atmospheres

Orbital Stability And Secular Dynamics Of The Proxima Centauri Planetary System

Proxima Centauri

Orbital Stability And Secular Dynamics Of The Proxima Centauri Planetary System

Swarming Proxima Centauri: Optical Communication Over Interstellar Distances

Proxima Centauri

Swarming Proxima Centauri: Optical Communication Over Interstellar Distances

Water Content Of Rocky Exoplanets In The Habitable Zone

Water/Hycean Worlds & Oceanography

Water Content Of Rocky Exoplanets In The Habitable Zone

Visible Extreme Adaptive Optics On Extremely Large Telescopes: Towards Detecting Oxygen In Proxima Centauri b And Analog

Proxima Centauri

Visible Extreme Adaptive Optics On Extremely Large Telescopes: Towards Detecting Oxygen In Proxima Centauri b And Analog

New Models of Reflection Spectra for Terrestrial Exoplanets: Present and Prebiotic Earth Orbiting Around Stars of Different Spectral Types

Imaging & Spectroscopy

New Models of Reflection Spectra for Terrestrial Exoplanets: Present and Prebiotic Earth Orbiting Around Stars of Different Spectral Types

Revisiting The Space Weather Environment Of Proxima Centauri b

Proxima Centauri

Revisiting The Space Weather Environment Of Proxima Centauri b

Traveling Planetary-scale Waves Cause Cloud Variability On Tidally Locked Aquaplanets

Exoplanets, -moons, -comets

Traveling Planetary-scale Waves Cause Cloud Variability On Tidally Locked Aquaplanets