lithium
(Li)
(metal, Li, atomic number 3)
Lithium (Li ) is the
element with atomic number 3, symbol Li.
The most abundant isotope , with mass number 7,
is stable, as is that with mass number 6.
Lithium burns at a temperature less than that of hydrogen burning ,
suggesting that main sequence stars quickly deplete themselves of it,
faster than would brown dwarfs , and its presence has been used
to identify the latter.
Lithium is thought to have been formed in the Big Bang ,
but though observed hydrogen and helium abundances
reflect current models of relic abundances , the abundance of lithium does not.
The discrepancy between the expected abundance and that
indicated by observation is termed the lithium problem .
The Sun shows a low abundance, seemingly inconsistent with
the much larger abundance found in meteorites , this discrepancy
termed the solar lithium problem . Both these problems retain
research interest.
Lithium in stars is detected through a spectral feature , a
spectral line at 6708 Å .
(element,metal,chemistry )
Further reading:
https://en.wikipedia.org/wiki/Lithium
https://en.wikipedia.org/wiki/Nucleosynthesis
https://en.wikipedia.org/wiki/Cosmological_lithium_problem
https://en.wikipedia.org/wiki/Standard_solar_model#Lithium_depletion_at_the_solar_surface
http://hyperphysics.phy-astr.gsu.edu/hbase/pertab/li.html
https://dictionary.obspm.fr/terms/lithium/
https://www.rsc.org/periodic-table/element/3/lithium
https://physics.nist.gov/PhysRefData/Handbook/Tables/lithiumtable1.htm
https://pubchem.ncbi.nlm.nih.gov/element/Lithium
https://ui.adsabs.harvard.edu/abs/2017A%26A...598A..64T/abstract
https://ui.adsabs.harvard.edu/abs/2025A%26A...701A.164M/abstract
Referenced by pages:
abundances
Big Bang nucleosynthesis (BBN)
brown dwarf (BD)
element
J1407
lithium burning
lithium depletion boundary (LDB)
lithium problem
refractory material
relic
spectral type
surface abundance
T-Tauri star (TTS)
thermal runaway
V339 Delphini (V339 Del)
Notes to myself regarding this page
Index