Astrophysics (Index)About

metal

(in astrophysics, any element more massive than helium)

In astrophysics, the term metal is used for any element other than hydrogen or helium. Metallicity is a measure of the amount of such elements in an astronomical body such as a star. Such metal was nearly non-existent in the early universe, and has since been produced within stars as well as supernovae and other cataclysmic events. Its abundance relative to hydrogen and helium is still low in universe, stars, and clouds, but it is key to the occurrence of rocky planets.


The common meaning of metal is a particular class of substances that are hard, opaque, transmit heat and electricity, and can be heated to the point of malleability. Science (outside astrophysics) refines the term to mean elements in which the electrons in the outer orbit are easily removed, which is the basis of the electrical and heat conductivity. Under very high pressure (millions of atm), hydrogen and helium are theorized to have a metal-like phase that conducts electricity, called metallic hydrogen (or conductive hydrogen) and metallic helium, which are believed to be present within Jupiter and Saturn.


(atoms)
Further reading:
http://en.wikipedia.org/wiki/Metallicity
http://en.wikipedia.org/wiki/Metal
http://en.wikipedia.org/wiki/Metallic_hydrogen
http://astronomy.swin.edu.au/cosmos/M/Metals

Referenced by pages:
alpha process
Am star
Ap star
bolometer
carbon star (C)
chemically peculiar star (CP star)
electron screening
first galaxies
G-type star (G)
globular cluster (GC)
habitability
helium (He)
K-type star (K)
L-type star (L)
line blanketing
mass fraction
mass ratio (μ)
metallicity (Z)
Milky Way
Milky Way chemical evolution
planet formation
solar energetic particle (SEP)
spectral class
stellar age determination
stellar population
Sun
super-Earth
Tillotson equation
weak-line star
white dwarf (WD)

Index