Category
page 1Astrochemistry
interstellar medium
matter and radiation in the space between the star systems in a galaxy
cosmic dust
dust floating in space

astrochemistry
thumb|Infographic showing the theorized origin of the chemical elements that make up the human body
Astrochemistry is the interdisciplinary scientific study of the abundance and reactions of molecules in space and their interaction with radiation. The discipline overlaps with astronomy and chemistry. The term may refer to studies within both the Solar System and the interstellar medium. The investigation of elemental abundances and isotope ratios in Solar System materials, such as meteorites, is known as cosmochemistry, while the study of interstellar atoms and molecules and their interaction
Fraunhofer lines
spectral lines of the Sun
polycyclic aromatic hydrocarbons
hydrocarbons composed of multiple aromatic rings

tholin
thumb|Neverland Regio, a dark region on Charon's north pole. The region is stained a dark brown by deposits of tholins
Tholins (after the Greek ('''') "hazy" or "muddy"; from the ancient Greek word meaning "sepia ink") are a wide variety of organic compounds formed by solar ultraviolet or cosmic ray irradiation of simple carbon-containing compounds such as carbon dioxide (), methane () or ethane (), often in combination with nitrogen () or water (). Tholins are disordered polymer-like materials made of repeating chains of linked subunits and complex combinations of functional groups, typically

cosmochemistry
thumb|Meteorites are often studied as part of cosmochemistry.
hydrogen line
spectral line of hydrogen state transitions
absorption spectroscopy
spectroscopic techniques that measure the absorption of radiation
abundance of the chemical elements
any of several measures of the occurrence of different chemical elements

biosignature
A biosignature is a phenomenon that can be explained by biological processes where all possible abiotic causes of this phenomenon have been eliminated. This term is mainly used in the field of astrobiology in the search for past or present extraterrestrial life, from planets and moons in the Solar System to exoplanets. Candidate biosignatures strongly indicate some of the earliest known life forms, aid studies of the origin of life on Earth as well as the possibility of life on Mars, Venus and elsewhere in the universe.

cumulene
thumb|Butatriene, the simplest cumulene
Goldschmidt classification
geochemical classification grouping the chemical elements according to their preferred host phases
Local Void
Empty region of space adjacent to the Local Group of galaxies.
trihydrogen cation
chemical compound
list of interstellar and circumstellar molecules
Wikimedia list article
dicarbon
chemical compound
polyyne
thumb|right|Diacetylene, the simplest polyyne
astrophysical maser
naturally occurring source of stimulated spectral line emission, typically in the microwave portion of the electromagnetic spectrum

Cryochemistry
Cryochemistry is the study of chemical interactions at temperatures below . It is derived from the Greek word cryos, meaning 'cold'. It overlaps with many other sciences, including chemistry, cryobiology, condensed matter physics, and even astrochemistry.
tricarbon
Tricarbon (systematically named 1λ2,3λ2-propadiene and '''catena-tricarbon''') is an inorganic compound with the chemical formula (also written [C(μ-C)C] or ). It is a colourless gas that only persists in dilution or solution as an adduct. It is one of the simplest unsaturated carbenes. Tricarbon can be found in interstellar space and can be produced in the laboratory by a process called laser ablation.
equivalent width
measure of spectral lines

isobutyronitrile
Isobutyronitrile is a complex organic molecule that has recently been found in several meteorites arrived from space. The singularity of this chemical is due to the fact that it is the only one among the molecules arriving from the universe that has a branched, rather than straight, carbon backbone. The backbone is also larger than usual, in comparison with others.
Swan band
Emission spectra characteristic of burning hydrocarbon fuels
photoelectrochemical process
electrochemical processes involving photons and the emission or absorption of light
diffuse interstellar band
absorption features in the spectra of astronomical objects in the Milky Way and other galaxies
Atomic and molecular astrophysics
field of study on atomic and molecular particles in space
hydroxyaluminium(I)
chemical compound
methyl
radical
Interstellar ice
ice that forms in the interstellar medium
propynylidyne
Propynylidyne is a chemical compound that has been identified in interstellar space.
molecules in stars
space chemistry