Astrophysics (index)

Helium

(He)
(non-metallic element, He, atomic number 2.)

Helium (He) is the element with atomic number 2, symbol He. Its most common isotope and has atomic weight 4, but atomic weight 3 is also stable.

It is the second most common element, about 24% of the observable universe by mass.

Most helium is from the Big Bang but some is the result of nuclear fusion of Hydrogen (H) in stars.

Helium has a Metastable State of Excitation with one electron excited and of opposite the typical spin. It can remain in this state for a couple of hours and on relaxing, produces an Emission Line of about 80830 Angstroms (Å).


(element,non-metal,chemistry)
http://en.wikipedia.org/wiki/Helium

Referenced by:
Asymptotic Giant Branch (AGB)
Alpha Process
Bose-Einstein Statistics
Carbon Star
CNO Cycle
Energetic Neutral Atom (ENA)
Gas Giant
Giant Planet
Horizontal Branch (HB)
Helium Flash
Helium Runaway Shell
HI Region (HI)
Ice Giant
Intracluster Medium (ICM)
Low Mass Star
Main Sequence Star
Metal
Metallicity (Z)
Metastable
Nucleosynthesis
Planetary Nebula (PN)
Proton-Proton Chain
Protogalaxy
Solar Energetic Particle (SEP)
Supernova (SN)
Spitzer Space Telescope (SST)
Stellar Age Determination
Sun
Thermal Pulse
Triple Alpha Process
White Dwarf
Wolf-Rayet Star

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