The term "HD 179079 b" does not correspond to a widely recognized or established concept in publicly available, reliable encyclopedic sources as of the current knowledge base. It appears to follow a naming convention used in astronomy for exoplanets, where "HD" refers to entries in the Henry Draper Catalogue, a stellar catalog, and the suffix "b" typically denotes the first discovered planet orbiting the star HD 179079.
However, no confirmed exoplanet designated HD 179079 b is listed in major astronomical databases such as the NASA Exoplanet Archive or the Extrasolar Planets Encyclopaedia. The parent star, HD 179079, may exist in stellar catalogs, but definitive data on a planetary companion labeled "b" is not verifiable through authoritative sources.
Etymologically, the name breaks down as:
- "HD": Abbreviation for the Henry Draper Catalogue.
- "179079": The star's identifier within that catalog.
- "b": Standard suffix indicating the first detected exoplanet in orbit around the star.
Accurate information regarding characteristics such as mass, orbital period, discovery method, or physical properties is not confirmed. The term may represent a candidate or unconfirmed object that has not been validated or published in peer-reviewed literature.
Related Topics:
- HD 179079 (if cataloged)
- Exoplanet nomenclature
- Henry Draper Catalogue
- Extrasolar planets
Due to the lack of verification, HD 179079 b cannot be described as an established astronomical entity.