February 2015 - Astrobiology

ARCHIVE

Month: February 2015

Environment Around Black Hole Protects Organic Chemicals

Astrochemistry

Environment Around Black Hole Protects Organic Chemicals

Complex Organics in the Inner Regions of Solar-type Protostars

Astrochemistry

Complex Organics in the Inner Regions of Solar-type Protostars

Oxygen Enrichment in Carbon-rich Planetary Nebulae

Astrochemistry

Oxygen Enrichment in Carbon-rich Planetary Nebulae

Shielding From The Solar Wind: Implications for Habitability

Habitable Zones & Global Climate

Shielding From The Solar Wind: Implications for Habitability

Linking Europa's Plume Activity to Tides, Tectonics, and Liquid Water

Europa

Linking Europa's Plume Activity to Tides, Tectonics, and Liquid Water

Shedding Light on the Formation of the Pre-biotic Molecule Formamide with ASAI

Astrochemistry

Shedding Light on the Formation of the Pre-biotic Molecule Formamide with ASAI

Collisions of Small ice Particles Under Microgravity Conditions

Astrochemistry

Collisions of Small ice Particles Under Microgravity Conditions

A New Chemical Scheme to Study Carbon-rich Exoplanet Atmospheres

Astrochemistry

A New Chemical Scheme to Study Carbon-rich Exoplanet Atmospheres

Does Dark Matter Cause Mass Extinctions and Geologic Upheavals?

Astrobiology (general)

Does Dark Matter Cause Mass Extinctions and Geologic Upheavals?

Determining Interior Structure of Rocky Exoplanets From Mass and Radius Measurements

Astrogeology

Determining Interior Structure of Rocky Exoplanets From Mass and Radius Measurements

Plants Survive Better Through Mass Extinctions Than Animals

Impact events

Plants Survive Better Through Mass Extinctions Than Animals

New Data on Chemical Gardens, Whose Formation is a Mystery for Science

Biogeochemical Cycles & Geobiology

New Data on Chemical Gardens, Whose Formation is a Mystery for Science

Earth-like Planets More Likely to Orbit Sun-like stars – Not Lower-mass Stars

Exoplanets & Exomoons

Earth-like Planets More Likely to Orbit Sun-like stars – Not Lower-mass Stars

Ancient Rocks Show Life Could Have Flourished on Earth 3.2 Billion Years Ago

Fossils & Paleontology

Ancient Rocks Show Life Could Have Flourished on Earth 3.2 Billion Years Ago

Antifreeze in the Hot Core of Orion: First Detection of Ethylene Glycol in Orion-KL

Astrochemistry

Antifreeze in the Hot Core of Orion: First Detection of Ethylene Glycol in Orion-KL

Earth and Terrestrial Planet Formation

Exoplanets & Exomoons

Earth and Terrestrial Planet Formation

Life on Other Planets: Alternative Chemistries of Life

Astrochemistry

Life on Other Planets: Alternative Chemistries of Life

Hydrogenation at Low Temperatures Does Not Always Lead to Saturation: The Case of HNCO

Astrochemistry

Hydrogenation at Low Temperatures Does Not Always Lead to Saturation: The Case of HNCO

Colliding Winds in Low-Mass Binary Star Systems: Implications for Habitable Planets

Exoplanets & Exomoons

Colliding Winds in Low-Mass Binary Star Systems: Implications for Habitable Planets

In-situ Measurements of the Radiation Stability of Amino Acids at 15-140 K

Astrochemistry

In-situ Measurements of the Radiation Stability of Amino Acids at 15-140 K