Spite plateau

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The Spite plateau (or Spite lithium plateau) is a baseline in the abundance of lithium found in old stars orbiting the galactic halo. It was named after the astronomers François and Monique Spite, who published the discovery in 1982.[1]

The element lithium was first produced during the Big Bang that created the observable universe. The cosmic abundance of lithium is of interest because it provides several constraints to the various Big Bang models.[2] Those models that fail to satisfy these constraints are therefore subject to rejection or correction by the scientific community.

Lithium is readily consumed by fusion with protons at temperatures above 2 × 106 K, such as is found in the cores of stars. Thus, if the convection zone of a main sequence star carries lithium to the core region, the abundance of lithium in the star can decrease. Likewise, lithium can be produced in interstellar matter by spallation collisions with cosmic rays, or by the evolution of stars of moderate mass.[2]

To obtain a good estimate of the primordial abundance of lithium, astronomers François and Monique Spite measured the abundance of lithium in old, population II stars (or old halo stars). Such stars were formed early in the universe out of material that had not been significantly modified by other processes. Their results showed that the curve on a graph of the abundance of lithium versus effective surface temperature formed a plateau among old halo stars for effective temperatures below about:

log Teff ~ 3.75

or roughly 5,600 K. This suggested that the plateau represented the primordial abundance level of lithium in the Milky Way, and thus they were able to estimate that the abundance of lithium at the beginning of the galaxy was:

NLi = (11.2 ± 3.8) × 10−11 NH

where NH is the abundance of hydrogen.[2]

The current estimates for the primordial abundance of lithium, as measured by this technique, are in tension with the predictions of the standard model of Big Bang nucleosynthesis, a discrepancy known as the Lithium Problem.[3]


  1. ^ Coc, Alain; Vangioni, Elisabeth (May 23–27, 2005). "Lithium and Big-Bang Nucleosynthesis". In Hill, V.; François, P.; Primas. From Lithium to Uranium: Elemental Tracers of Early Cosmic Evolution, IAU Symposium Proceedings of the international Astronomical Union 228. Paris, France: Cambridge University Press. pp. 13–22. Bibcode:2005IAUS..228...13C. doi:10.1017/S1743921305005156. 
  2. ^ a b c Spite, F.; Spite, M. (November 1982). "Abundance of lithium in unevolved halo stars and old disk stars - Interpretation and consequences". Astronomy and Astrophysics. 115 (2): 357–366. Bibcode:1982A&A...115..357S. 
  3. ^ Fields, Brian D. (2012). "The Primordial Lithium Problem". Annual Review of Nuclear and Particle Science. 61: 47–68. arXiv:1203.3551Freely accessible. Bibcode:2011ARNPS..61...47F. doi:10.1146/annurev-nucl-102010-130445.