Tag Archive for 'Glycine'

An artist’s rendering of the surface of Saturn’s largest moon, Titan. Image credit: Benjamin de Bivort, debivort.org / CC BY-SA 3.0.

Titan May Be Able to Support Only Minuscule Amount of Biomass, New Modeling Study Suggests

Apr 8, 2025 by News Staff

A team of biologists from the United States, Canada, the United Kingdom and France has developed a scenario of what life on Titan, Saturn’s largest moon,...

Titan Most Likely Non-Habitable, Astrobiologists Say

Feb 20, 2024 by News Staff

Saturn’s moon Titan has an organic-rich atmosphere and surface with a subsurface ocean that may represent a habitable environment. In a new study, astrobiologists...

PAH molecules overlaid on the Taurus Molecular Cloud, a large blue-white cloud made of gas and dust with large and small stars of varying luminosities interspersed throughout. Aromatic molecule structures shown in order from left to right: 1-cyanonaphthalene, 1-cyano-cyclopentadiene, HC11N, 2-cyanonaphthalene, vinylcyanoacetylene, 2-cyano-cyclopentadiene, benzonitrile, E-cyanovinylacetylene, HC4NC, propargylcyanide. Image credit: M. Weiss / Harvard & Smithsonian Center for Astrophysics.

Meteoritic Polymers of Glycine Shed Light on Pre-Solar Space Chemistry

Jun 30, 2021 by News Staff

Asteroid material in chondritic Vigarano class alteration type 3 (CV3) meteorites provide a good record of complex chemistry present when or before our...

An artist’s impression of glycine together with dark interstellar clouds in the lab. Image credit: Harold Linnartz.

Amino Acids Can Form Long Before Stars and Planets: Study

Nov 16, 2020 by News Staff

Glycine and other amino acids form in dense interstellar clouds well before they transform into new stars and planets, suggests a new study led by researchers...

This SEM image shows a polished thin section of Asuka 12236. The section is about 1 cm (a third of an inch) across. Most of the bright grains in the image are iron-nickel-metal and/or iron-sulfide. The gray is mostly silicate, with the darker gray areas more magnesium-rich, while the lighter gray areas are more iron-rich. The roundish objects, and some fragments of them, that tend to contain most of the small, bright metal grains are called chondrules, which formed as molten droplets. They are set in a very fine-grained matrix, which is where the organic compounds and presolar grains are found. Image credit: Carnegie Institution for Science / Conel M. O’D. Alexander.

Researchers Find Extraterrestrial Amino Acids in Antarctic Meteorite

Aug 31, 2020 by News Staff

A team of astrobiologists from NASA’s Goddard Space Flight Center and the Carnegie Institution for Science has found a wide diversity of amino acids...

Model of the hemolithin molecule: space-filling mode (top), ball and stick (center), enlarged view of iron, oxygen and lithium termination (bottom). White = H; orange = Li; gray = C; blue = N; red = O and green = Fe. Hydrogen bonds are shown by dotted lines. Image credit: McGeoch et al, arXiv: 2002.11688.

Researchers Find Extraterrestrial Protein in Meteorite Acfer 086

Mar 26, 2020 by Sergio Prostak

A research team led by Harvard University scientist Julie McGeoch has found a never-before-seen protein inside a meteorite called Acfer 086. A sample of...

The Rosetta spacecraft has detected ingredients considered important for life as we know it on Earth, in the atmosphere of Comet 67P/Churyumov-Gerasimenko. Image credit: ESA / ATG Medialab / Rosetta / NavCam / CC BY-SA IGO 3.0 / Kathrin Altwegg et al.

Rosetta Detects Two Ingredients for Life on 67P/Churyumov-Gerasimenko

May 27, 2016 by News Staff

ESA’s Rosetta orbiter has detected volatile glycine and phosphorus in the fuzzy atmosphere of Comet 67P/Churyumov-Gerasimenko. The Rosetta spacecraft...