MessageToEagle.com - The Trifid Nebula (M20) is home to thousands of massive newborn stars and one of the most prominent
nebulae in the night sky. There is so much happening in this cosmic object and a well-known open cluster.
This is a rare combination of three nebulae types that reveal the fury of freshly formed stars and point to more star
birth in the future.
This massive star factory is so named for the dark dust bands that trisect its glowing heart, and is a rare combination of
three nebula types, revealing the fury of freshly formed stars and presaging more star birth.
Dust lanes radiating from the center appear to divide the nebula into three parts.
This large luminous cloud of ionized hydrogen is located at distance of ˜1.7 kpc in the Sagittarius (the Archer)
spiral arm and about 8 light-years away from the nebula's central star.
The Trifid is approximately 9,000 light-years from Earth .
The Trifid nebula (M20) is a well-known prominent, optical HII region of starbirth, which is strong in UV
radiation and very hot (around ~10,000K). It shows many similarities to M42 but the Trifid is thought to be significantly
younger than the Orion Nebula (~ 105 yr rather than ~ 106 yr).
It presents a compelling portrait of the early stages of a star's life, from gestation to first light.
Click on image to enlarge
The Trifid Nebula, aka M20, is easy to find with a small telescope and a well-known stop in the nebula rich
constellation Sagittarius. But where visible light pictures show the nebula divided into three parts by dark, obscuring
dust lanes, this penetrating infrared image reveals filaments of luminous gas and newborn stars.
This spectacular false-color view is courtesy of the Spitzer Space Telescope. Astronomers have used the Spitzer
infrared image data to count newborn and embryonic stars that otherwise lie hidden in the natal dust and glowing
clouds of this intriguing stellar nursery. Image credit: NASA, JPL-Caltech, J. Rho (SSC/Caltech)
The heat and "winds" of newly ignited, volatile stars stir the Trifid's gas and dust-filled cauldron; in time, the dark
tendrils of matter strewn throughout the area will themselves collapse and form new stars.
Dust pillars are like interstellar mountains. Visible in the above picture is the end of a huge gas and dust pillar
in the Trifid Nebula, punctuated by a smaller pillar pointing up and an unusual jet pointing to the left.
Trifid Pillars & Jets. Credit: J. Hester (Arizona St. U) et al., WFPC2, HST, NASA
The pink dots are newly formed low-mass stars.
A star near the small pillar's end is slowly being stripped of its accreting gas by radiation from a tremendously
brighter and powerful star situated off the above picture to the upper right.
The jet extends nearly a light-year and would not be visible without external illumination. As gas and dust
evaporate from the pillars, the hidden stellar source of this jet will likely be uncovered, possibly over the next 20,000 years.
Closeup of Jet in Trifid Nebula. Credit: NASA, ESA, and The Hubble Heritage Team (AURA/STScI)
A prominent jet is being lit up by radiation from the massive, luminous star that powers the Trifid Nebula.
The jet and a long finger-like object, a "stalk" with a possible young stellar object are emerging from the wall of a
cloud, toward the star that powers the Trifid Nebula. This stalk is a prominent example of the evaporating gaseous globules,
or "EGGs".
Hubble astronomers are believe that the jet as the last gasp from a star that was cut off from its supply lines 100,000 years ago.
The French astronomer Charles Messier first observed the Trifid Nebula in June 1764, recording the hazy, glowing object
as entry number 20 in his renowned catalogue.
Observations made about 60 years later by John Herschel of the dust lanes that appear to divide the cosmic cloud into
three lobes inspired the English astronomer to coin the name "Trifid".
The massive star factory (image above) known as the Trifid Nebula in Sagittarius, the Archer, was captured in all its glory with the
Wide-Field Imager camera attached to the MPG/ESO 2.2-metre telescope at ESO's La Silla Observatory in northern Chile.
Named for the dark dust bands that trisect its glowing heart, the Trifid Nebula is a rare combination of three nebulae
types that reveal the fury of freshly formed stars and point to more star birth in the future. Credit: ESO/S. Guisard
(www.eso.org/~sguisard) and A. Fujii. Music by John Dyson from the CD darklight
The Trifid Nebula can be observed through a small telescope and is a popular deep sky object among amateur astronomers.
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Cosmic Robbers: Black Hole Jets May Cause
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Armchair explorers of the cosmos can now have at their fingertips the nearly 2,000 distant planetary systems discovered by NASA's Kepler Mission.
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Galaxy With A Voracious Appetite
Observations by the two of the European Space Agency's space observatories have provided a multi-wavelength view of
the mysterious galaxy Centaurus A.
The new images, from the Herschel Space Observatory and the XMM-Newton x-ray satellite, are revealing further hints about
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New Kepler Explorer:
View The 1,790 Distant Planetary Systems - For Free!
Armchair explorers of the cosmos can now have at their fingertips the nearly 2,000 distant planetary systems discovered by NASA's Kepler Mission.
Now available for free from the iTunes App Store, Kepler Explorer was developed through the OpenLab initiative at UC Santa Cruz,
which brought together faculty and students in astrophysics, art, and technology for a summer institute last year.
Dwarf Irregular Galaxy
That Forces Scientists To Re-Evaluate Old Theory
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The dwarf galaxy I Zw 18 is, one of the poorest in heavy elements, located only 59 million light years away.
It's among those that have strong star forming activity.
Though the universe is filled with billions upon billions of stars, the discovery of a single variable star in 1923 altered the
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It's a very important discovery!
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