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AsteriaStar
Dataset

Astrochemistry & the Molecular Universe Dataset

The chemistry of space — the interstellar environments, the interstellar molecules (water, CO, ammonia, methanol, PAHs, prebiotic precursors), and the astrochemical processes that build and destroy them.

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Generated from the canonical knowledge graph. Open, machine-readable, and free to reuse under CC BY-SA 4.0.

Version
1.0.0
Entities
20
Last generated
2026-06-29
License
CC BY-SA 4.0
Checksum
(published at release)

Sample (20 of 20)

NameType
Amino-Acid PrecursorsInterstellar molecule
AmmoniaInterstellar molecule
Carbon DioxideInterstellar molecule
Carbon MonoxideInterstellar molecule
Cometary & Meteoritic ChemistryAstrochemical process
Gas-Phase ChemistryAstrochemical process
Grain-Surface ChemistryAstrochemical process
Hydrogen CyanideInterstellar molecule
Interstellar DustInterstellar environment
MethanolInterstellar molecule
Molecular CloudsInterstellar environment
PhotochemistryAstrochemical process
Planet-Formation ChemistryAstrochemical process
Polycyclic Aromatic HydrocarbonsInterstellar molecule
Prebiotic ChemistryAstrochemical process
Protoplanetary DisksInterstellar environment
Shock ChemistryAstrochemical process
Star-Forming RegionsInterstellar environment
The Diffuse Interstellar MediumInterstellar environment
WaterInterstellar molecule

Source references

The primary and reference sources this topic draws on.

  • NASANational Aeronautics and Space Administration

    Mission data, planetary science, space telescopes, and public-domain imagery.

    Most NASA-produced imagery is in the public domain; individual items are checked for usage terms before publication.

  • ESOEuropean Southern Observatory

    Southern-hemisphere observatory data and imagery (VLT, ALMA partner).