Astronomy Picture of the Day |
APOD: 2005 April 24 - M16: Stars from the Eagle's EGGs
Explanation:
Newborn stars are forming in the Eagle Nebula.
This image, taken with the Hubble Space Telescope in 1995, shows
evaporating gaseous globules (EGGs)
emerging from pillars of molecular
hydrogen gas and
dust.
The giant pillars are
light years in length
and are so dense that interior gas contracts gravitationally to form stars.
At each pillars' end,
the intense radiation of bright young stars
causes low density material to boil away,
leaving stellar nurseries of dense EGGs exposed.
The
Eagle Nebula, associated with the
open star cluster
M16, lies about 7000
light years away.
APOD: 1999 June 4 - NGC 3603: From Beginning To End
Explanation:
>From beginning to end, different stages of a star's life appear in
this exciting Hubble Space Telescope picture of the environs
of galactic emission nebula
NGC 3603.
For the beginning, eye-catching "pillars" of glowing
hydrogen at the right signal
newborn stars emerging
from their dense, gaseous, nurseries.
Less noticeable,
dark clouds
or "Bok globules" at the top
right corner are likely part of a still earlier stage, prior to their
collapse to form stars.
At picture center lies a cluster of bright
hot blue stars whose strong
winds and ultraviolet radiation have cleared away nearby material.
Massive and young, they will soon exhaust their nuclear fuel.
Nearing the end of its life, the bright supergiant
star Sher 25 is
seen above and left of the cluster, surrounded by a glowing ring and flanked
by ejected blobs of gas.
The ring structure is reminiscent of
Supernova 1987a and Sher 25
itself may be only a few thousand years from its
own devastating finale.
But what about planets?
Check out the two
teardrop-shaped objects below the cluster
toward the bottom of the picture.
Although larger, these emission nebulae are similar to suspected
proto-planetary disks (proplyds) encompassing stars in the Orion Nebula.
APOD: 2004 July 13 - Orion Nebula in Oxygen, Hydrogen, and Sulfur
Explanation:
The Great Nebula in Orion, an
immense, nearby starbirth region,
is arguably the most famous of all astronomical nebulae.
The
Orion Nebula,
also known as M42, is
shown above through
ultraviolet
and blue filters augmented with three exact colors specifically emitted by
hydrogen,
oxygen, and
sulfur.
In addition to housing a bright open cluster of stars known as the
Trapezium, the
Orion Nebula contains many
stellar nurseries.
These nurseries contain glowing gas, hot young stars,
proplyds, and
stellar jets spewing material at high speeds.
Many of the filamentary structures visible in
this image are actually
shock waves - fronts where fast moving material encounters slow moving gas.
The Orion Nebula spans about 40 light years and is located about 1500 light years away in the same
spiral arm of our Galaxy as the Sun.
Authors & editors:
Robert Nemiroff
(MTU) &
Jerry Bonnell
(USRA)
NASA Web Site Statements, Warnings, and
Disclaimers
NASA Official: Jay Norris.
Specific rights apply.
A service of:
EUD at
NASA /
GSFC
& Michigan Tech. U.