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NS 3324 leads C93 across the international bridge into Fort Erie, ON, while CN L531 waits in the south to head over to Buffalo, NY.
NGC 3324
Outer part of the
Eta Carina Nebula
Image taken using the
Telescope Live CHI-1 telescope.
El Sauce Observatory, Chile.
Planewave CDK 24" f/6.5
CCD Camera: FLI ProLine PL9000 3056 x 3056
1.62 arcsec / px (bin 2x2)
Narrowband image using 3nm Astrodon filters.
Ha: 6 x 10m
OIII: 6 x 10m
SII: 8 x 10m
Processed with PixInsight and Photoshop CC2020
Acquired at Deep Sky West Chile
Takahashi TOA
FLI MicroLine ML16200
PixInsight 1.8 and Photoshop CC
Description at www.billionsandbillions.com
NGC 3324
Nebulosa Gabriela Mistral
HaRGB
120 - 8 - 4 - 4 (minutos
Total: 136 minutos
TS 115/800
ZWO ASI 1600 Mono Cooled
What looks much like craggy mountains on a moonlit evening is actually the edge of a nearby, young, star-forming region NGC 3324 in the Carina Nebula. Captured in infrared light by the Near-Infrared Camera (NIRCam) on NASA’s James Webb Space Telescope, this image reveals previously obscured areas of star birth.
Called the Cosmic Cliffs, the region is actually the edge of a gigantic, gaseous cavity within NGC 3324, roughly 7,600 light-years away. The cavernous area has been carved from the nebula by the intense ultraviolet radiation and stellar winds from extremely massive, hot, young stars located in the center of the bubble, above the area shown in this image. The high-energy radiation from these stars is sculpting the nebula’s wall by slowly eroding it away.
NIRCam – with its crisp resolution and unparalleled sensitivity – unveils hundreds of previously hidden stars, and even numerous background galaxies. Several prominent features in this image are described below.
•The “steam” that appears to rise from the celestial “mountains” is actually hot, ionized gas and hot dust streaming away from the nebula due to intense, ultraviolet radiation.
•Dramatic pillars rise above the glowing wall of gas, resisting the blistering ultraviolet radiation from the young stars.
•Bubbles and cavities are being blown by the intense radiation and stellar winds of newborn stars.
•Protostellar jets and outflows, which appear in gold, shoot from dust-enshrouded, nascent stars.
•A “blow-out” erupts at the top-center of the ridge, spewing gas and dust into the interstellar medium.
•An unusual “arch” appears, looking like a bent-over cylinder.
This period of very early star formation is difficult to capture because, for an individual star, it lasts only about 50,000 to 100,000 years – but Webb’s extreme sensitivity and exquisite spatial resolution have chronicled this rare event.
Located roughly 7,600 light-years away, NGC 3324 was first catalogued by James Dunlop in 1826. Visible from the Southern Hemisphere, it is located at the northwest corner of the Carina Nebula (NGC 3372), which resides in the constellation Carina. The Carina Nebula is home to the Keyhole Nebula and the active, unstable supergiant star called Eta Carinae.
NIRCam was built by a team at the University of Arizona and Lockheed Martin’s Advanced Technology Center.
Image acquired using the Telescope Live remote imaging platform.
Telescope: ASA 500N Newtonian. 500mm aperture, focal length 1900mm, f/3.8
CCD Camera: Finger Lake Instruments FLI 16803.
Equatorial Mount: ASA DDM85 direct drive.
Astrodon H-alpha, OIII and RGB filters.
H-alpha: 8 x 10m
OIII: 7 x 10m
SII: 10 x 10m
Processed with PixInsight and Affinity Photo.
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