Population II
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English
Alternative forms
Etymology
Proposed by astronomer Walter Baade in 1944.
Proper noun
- (astrophysics, usually attributively) A population or group of stars formed early in the history of the Universe, characterized by having a low metallicity.
- Coordinate terms: Population I, Population III
- 2019 December 11, Brian Koberlein, “The Stars In Our Galaxy Are More Varied Than We Thought”, in Forbes, archived from the original on 2022-09-15:
- While the thick disk is largely composed of Population II stars, they found it contains two stellar populations.
- 2021 May 21, Tom Metcalfe, “An ancient star casts new light on the birth of the universe”, in NBC News, archived from the original on 2022-07-06:
- Those heavy elements were created by fusion within Population II stars that exploded as supernovas and seeded them into interstellar clouds.
- 2022 December 6, Jonathan O'Callaghan, “Astronomers Grapple with JWST’s Discovery of Early Galaxies”, in Scientific American, archived from the original on 2022-12-09:
- The brightness of these galaxies could be attributed to such stars, which would be much hotter and brighter than subsequent Population II stars and Population I stars, such as our sun, both of which fill our modern-day universe.
Derived terms
- Pop II (abbreviation)