Credit & Copyright: Amir H. Abolfath
Explanation:
The many spectacular colors of the
Rho Ophiuchi
(oh'-fee-yu-kee) clouds highlight the many processes that occur there.
The blue regions shine primarily by reflected light.
Blue light from the
Rho Ophiuchi star system
and nearby stars reflects
more efficiently off this portion of the nebula than red light.
The Earth's
daytime sky appears blue for the same reason.
The red and yellow regions shine primarily because of
emission from
the nebula's atomic and molecular gas.
Light from nearby blue stars - more energetic than the bright star
Antares - knocks
electrons
away from the gas, which then shines when the electrons
recombine with the gas.
The dark brown regions are caused by
dust grains - born in young stellar atmospheres -
which effectively block light emitted behind them.
The Rho Ophiuchi star clouds,
well in front of the
globular
cluster
M4 visible
here
on the upper right, are even more colorful than
humans can see - the clouds emits light in every
wavelength band from the
radio
to the
gamma-ray.
Astrophysicists:
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Publikacii s klyuchevymi slovami:
Rho Ophiuchi - Zmeenosec - otrazhatel'nye tumannosti - emissionnaya tumannost'
Publikacii so slovami: Rho Ophiuchi - Zmeenosec - otrazhatel'nye tumannosti - emissionnaya tumannost' | |
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