Helios Helium
This image of the active Sun
was
made using ultraviolet light emitted by ionized
Helium
atoms in
the
Solar chromosphere.
Helium was first discovered in
the
Sun in 1868,
its name fittingly derived from from the Greek word Helios, meaning
Sun.
Credit for the discovery goes to astronomer
Joseph Norman Lockyer (born May 17, 1836).
Lockyer relied on a then recently developed
technique of spectroscopy,
dissecting sunlight into a spectrum,
and the idea that each element produces a characteristic spectral pattern
of bright lines.
He noticed a yellow line in a solar spectrum made during an eclipse
which could not be accounted for by elements known on Earth.
Almost 27 years later terrestrial
Helium was finally discovered when the
spectrum of a
Helium bearing mineral of Uranium
provided an exact match to the
previously detected element of the Sun.
Helium is now known to be
the second most abundant element
(after Hydrogen) in the Universe.