Click image for detailed view
The Propeller Nebula, also known as NGC 7822, is a region of active star formation located in the constellation Cepheus, approximately 3,000 light-years from Earth. It’s a bright emission nebula, a region where gas and dust are illuminated by the ultraviolet light of young, hot stars, causing the surrounding gas to emit light.
The “propeller” shape comes from the complex structure of gas and dust in the nebula. The name originates from the distinct, somewhat symmetrical appearance of the nebula, which can resemble a propeller or a pair of wings when viewed through telescopes.
The Propeller Nebula is a stellar nursery, a place where new stars are being born. The dense molecular clouds in the nebula collapse under gravity to form stars. These newborn stars release energetic radiation that ionizes the surrounding gas, causing it to glow brightly.
The nebula spans about 6,000 light-years in diameter, and contains a significant number of young, hot stars. The nebula was first cataloged by John Herschel in the 19th century, but its most notable features were revealed through detailed observations in the 20th and 21st centuries. The nebula has been studied in various wavelengths, from visible light to radio and infrared, allowing astronomers to observe both the glowing gas and the cooler dust clouds.
Within the nebula, there are areas where the light from the young stars reflects off surrounding dust, creating reflection nebulae. In other parts, the intense ultraviolet radiation from these stars ionizes the surrounding hydrogen gas, leading to regions of emission nebulae.
The Propeller Nebula is a great laboratory for studying the processes involved in star formation. Its relatively close distance to Earth and its rich structure make it an excellent object for both amateur and professional astronomers. Its relatively active star-forming environment also provides insights into the lifecycle of stars and the dynamics of molecular clouds.
While the Propeller Nebula itself may not be as well-known as other nebulae like the Orion Nebula or the Eagle Nebula, its dramatic shape and active star-forming activity make it a popular target for astrophotographers, adding it to the roster of visually spectacular deep-sky objects.
Object | Propeller Nebula (NGC 6914) |
Link | https://www.shetzers.com/propeller-nebula-ngc-6914/ |
Wiki Link | https://en.wikipedia.org/wiki/NGC_6914 |
Hemisphere | Northern |
Constellation | Cygnus |
Other Names contained in image | NGC 6914 |
Imaging telescopes or lenses | Takahashi TOA-130NFB |
Imaging cameras | QHY268M |
Mounts | Software Bisque Paramount MYT |
Focal reducers | None |
Software | Software Bisque The Sky X, N.I.N.A., PHD Lab PHD2, Viking, PixInsight, Photoshop, Lightroom |
Filters | Astrodon LRGB Gen2 E-Series Tru-Balance 36mm unmounted. Chroma Technology Narrowband 3nm Ha, SII, OIII – 36mm Unmounted |
Accessories | Moonlite NightCrawler 35 focuser, Maxdome II, Digital Loggers Pro Switch, Sky Alert Weather Station, Pegagsus Ultimate Powerbox v2, QHY 7-slot filter wheel. |
Guiding Telescope or Lenses | Orion 60mm Guide Scope |
Guiding Camera | ZWO ASI290MM Mini |
Imaging Dates | 6/22/23, 6/23/23, 6/24/23, 6/25/23, 6/26/23, 6/27/23, 6/28/23, 6/29/23, 6/30/23 |
Frames | Ha: 59×600″ (9.8h) Gain 56, High Gain Mode, Temp -10C, Bin 1×1 OII: 21×600″ (3.5h) Gain 56, High Gain Mode, Temp -10C, Bin 1×1 SIII: 33×600″ (5.5h) Gain 56, High Gain Mode, Temp -10C, Bin 1×1 Red: 7×180″ (0.4h) Gain 26, Photographic Mode, Temp -10C, Bin 1×1 Green: 7×180″ (0.4h) Gain 26, Photographic Mode, Temp -10C, Bin 1×1 Blue :7×180″ (0.4h) Gain 26, Photographic Mode, Temp -10C, Bin 1×1 |
Integration | 20h |
Darks | 50 |
Flats | 20 per Filter |
Flat Darks | 40 |
Bortle Dark-Sky Scale: | 2 |
RA center | 303.99949 |
DEC center | 43.64452 |
Pixel scale | 3.76 |
Resolution | 6280 x 4210 |
Locations | Sirus 3.5m Observatory, Carbondale Colorado |
Data source | Backyard |
Seeing | Average |
Post Processing Techniques | PixInsight to Photoshop to Lightroom |
Type | SHO with RGB stars |