Population I

• population I

Proposed by astronomer Walter Baade in 1944.

Population I

1. (astrophysics, usually attributively) A population or group of stars formed relatively late in the history of the Universe, characterized by having a high metallicity.

   Coordinate terms: Population II, 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:

     We generally place stars into one of three populations based on their metallicity. Population I stars like the Sun are metal heavy. They are younger stars and tend to be found in the spiral arms of the Milky Way.

   • 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:

     Most stars, such as the sun, are third-generation "Population I" stars that contain relatively heavy elements such as iron, nickel, carbon and oxygen.

   • 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.

• Pop I (abbreviation)