Mélisse Bonfand Mélisse Bonfand

K2-18 b: A Carbon-Rich Planet with a Methane-Dominated Atmosphere

About 124 light-years away from Earth lies the planet K2-18 b. This exoplanet orbits its star in the “habitable zone,” where temperatures could allow liquid water to exist. Orbiting a red dwarf star, K2-18 b is larger than Earth but smaller than Neptune, with average temperatures around 300K, or 80 °F. It is often referred to as a “sub-Neptune” These planets are among the most common in our galaxy, yet their nature remains poorly understood. As a potentially life-friendly world, the James Webb Space Telescope(JWST) Cycle 1 GO Program 2722 lead by  personal investigator Nikku Madhusudhan, brought K2-18 b back into the spotlight, bringing better insight into the actual composition and structure.

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Brielle Shope Brielle Shope

A Lonely Massive Star Reveals Secrets of Stellar Chemistry

Led by Dr. Prasanta Gorai, a team of astrochemists studied an isolated massive star and uncovered a remarkably rich and complex chemical environment. Using observations from a powerful radio telescope in the Atacama Desert in Chile, researchers uncovered a mix of molecules and used them as “chemical fingerprints” to learn more about how the star is growing.

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Samantha Scibelli Samantha Scibelli

Unraveling Cosmic Chemistry: New Insights into Formaldehyde Formation

Imagine peering into the cold, dark corners of space, where stars are just beginning to flicker into existence. It is in these cosmic nurseries where key chemical species formaldehyde (H₂CO) and methanol (CH₃OH) are forged. These precursor molecules are vital ingredients for brewing the more complex organic molecules that are essential to understanding how life might have originated on Earth or, perhaps, elsewhere in the universe.

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Drew Christianson Drew Christianson

Unveiling the Origins of Sulfur in Comets

A team of astrophysicists led by Duncan V. Mifsud from the University of Kent, UK, has conducted an experimental study to investigate the origin of sulfur-bearing molecules in cometary ices.

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