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Photographer : Syed Redwan Haque
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Conatct : +88 01777 686715
© Elegant Frames
some of my frames from sundays show. size 8x12 SOLD. shot out to I_like_to_bench_fr8s for the inspiration. shoot me your info and i got you on a print of this one player.
4 January 2024, 00:20 UT; Stuart, Florida USA (Bortle 7).
Celestron CPC Deluxe 1100 HD at f/10. QHY294M Pro camera, bin 2, exposure 15s , Mono16, gain 1600, stacked 98 frames (total 25 min), Optolong UHC filter, no guiding, dark/bias/flat calibration frames, sensor 0°C. Processed in Pixinsight and Photoshop.
Appearance: very small, faint planetary nebula, starlike core surrounded by a darker ring then a bright lanceolate ring within a dimmer disc. Boundary distinct from background rich starfield
from Stellarium:
Azimuth: 106°
Altitude: 46°
Magnitude: 11.6
Apparent size: 0.5 arcmin
Moon illuminated: 49%
Clouds: partly cloudy
Transparency: 2
Seeing: G
from Wikipedia
NGC 2022 is a planetary nebula in the equatorial constellation of Orion, located at a distance of 8.21 kilolight-years from the Sun. It was first observed by William Herschel on December 28, 1785, who described it as: considerably bright, nearly round, like a star with a large diameter, like an ill-defined planetary nebula. In medium-sized amateur telescopes it looks like a small grayish patch of light. It is not very bright but it is still easy to spot it in the eyepiece. Even in a telescope as small as 80mm it can just be seen using a narrowband filter such as an OIII filter as a 'fuzzy' star. The object has the shape of a prolate spheroid with a major to minor axis ratio of 1.2, an apparent size of 28″, and a halo extending out to 40″, which is about the angular diameter of Jupiter as seen from Earth.
This is a double-shell planetary nebula with a wind-compressed inner shell and a more nebulous second shell. The linear radius of the inner shell is estimated at 0.326 ± 0.039 ly. It is expanding with a velocity of 28±2 km/s. The second shell is nearly circular and is expanding more slowly than the inner. The mass of the ionized elements in the planetary nebula is 0.19 M☉, or 19% of the Sun's mass. A faint outer halo consists of the remains of material ejected during the central star's asymptotic giant branch stage.
NGC 2022 lies 11° away from the Galactic Plane, which position suggests it was formed from a low-mass star. The elemental abundances are similar to those in the Sun, although carbon is about 50% higher and sulfur is a factor of two lower. The central star of this nebula has a visual magnitude of 15.92, a temperature of 122,000 K, and is radiating 852 times the luminosity of the Sun from a photosphere that has only 6.55% of the Sun's radius.
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Today, Tuesday 29th, Brett and Luke are straightening the wall, bracing them ready for the roof trusses next week.
Photographer : Syed Redwan Haque
Facebook - fb.com/elegantframesbd
Conatct : +88 01777 686715
© Elegant Frames