My new image of Betelgeuse and Pickett's Bell
The Star Betelgeuse And Pickett's Bell, RGB 12-19-2023
Good Everything Everyone... I hope all of you having a good day...
Finally I was able to finish my RGB... I never thought photographing Betelgeuse with a 100mm lens would be so beautiful in this area of Orion... The star colors are just insane.... I think it's due to those long 30 minute exposures that I take....
In this shot Betelgeuse looks as if it's inside a bubble of dust and gas...
As they say "Orion just keeps on giving" lol ?? ??????????
I hope all of you like it.... :-)
I plan to add more time to this image with some H-Alpha and OIII but it will have to be in a few weeks when the Moon is down and the cold cloudy weather has cleared up...
Have a good day Everyone and go safely.
The Details
Betelgeuse is a red supergiant star of spectral type M1-2 and one of the largest visible to the naked eye. It is usually the tenth-brightest star in the night sky and, after Rigel, the second-brightest in the constellation of Orion. It is a distinctly reddish, semiregular variable star whose apparent magnitude, varying between +0.0 and +1.6, has the widest range displayed by any first-magnitude star. At near-infrared wavelengths, Betelgeuse is the brightest star in the night sky. Its Bayer designation is a Orionis, Latinised to Alpha Orionis and abbreviated Alpha Ori or a Ori.
If it were at the center of our Solar System, its surface would lie beyond the asteroid belt and it would engulf the orbits of Mercury, Venus, Earth, and Mars. Calculations of Betelgeuse's mass range from slightly under ten to a little over twenty times that of the Sun. For various reasons, its distance has been quite difficult to measure; current best estimates are of the order of 500–600 light-years from the Sun – a comparatively wide uncertainty for a relatively nearby star. Its absolute magnitude is about -6. Less than 10 million years old, Betelgeuse has evolved rapidly because of its large mass and is expected to end its evolution with a supernova explosion, most likely within 100,000 years. When Betelgeuse explodes, it will shine as bright as the half-Moon for more than three months; life on Earth will be unharmed. Having been ejected from its birthplace in the Orion OB1 association – which includes the stars in Orion's Belt – this runaway star has been observed to be moving through the interstellar medium at a speed of 30 km/s, creating a bow shock over four light-years wide.
In 1920, Betelgeuse became the first extrasolar star whose photosphere's angular size was measured. Subsequent studies have reported an angular diameter (i.e., apparent size) ranging from 0.042 to 0.056 arcseconds; that range of determinations is ascribed to non-sphericity, limb darkening, pulsations and varying appearance at different wavelengths. It is also surrounded by a complex, asymmetric envelope, roughly 250 times the size of the star, caused by mass loss from the star itself. The Earth-observed angular diameter of Betelgeuse is exceeded only by those of R Doradus and the Sun.
Starting in October 2019, Betelgeuse began to dim noticeably, and by mid-February 2020 its brightness had dropped by a factor of approximately 3, from magnitude 0.5 to 1.7. It then returned to a more normal brightness range, reaching a peak of 0.0 visual and 0.1 V-band magnitude in April 2023. Infrared observations found no significant change in luminosity over the last 50 years, suggesting that the dimming was due to a change in extinction around the star rather than a more fundamental change. A study using the Hubble Space Telescope suggests that occluding dust was created by a surface mass ejection; this material was cast millions of miles from the star, and then cooled to form the dust that caused the dimming.
Equipment Details
Scope/Lens: Canon EF 100mm F2.8 Macro USM Set At F 5.6
Reducer: Non
Camera ZWO ASI 1600MM Pro Mono w/Filter Wheel
Filter Wheel: ZWO 8 Position Filter Wheel
Filters Used: Astronomik 1.25 Red, Green, Blue
Mount: Takahashi EM-200 Temma 2M
Guide Scope: William Optics M-G50RIII + M-GRIIIRD Guide Scope
Guide Camera: ZWO ATI 120MM Mono
Guide Software: PHD2 v2.6.9dev5
Goto Software: Stellarium v0.21.0
Imaging Software: APT Astro Photography Tool v4.01 For ZWO 1600MM Camera
Stacking Software: DeepSkyStacker 64 bit v4.2.6 Beta
Processing Software: Photoshop CS6 And Adobe Camera Raw
Photoshop CS6 Plugins
AstroFlat Pro
Astronomy Tools Actions
Annie’s Astro Actions
ASCOM: Platform 6
Exposure Details
Exposure: Red 30 Minutes Each (15hrs Total Exposure Time.)
Gain Set To: 0
Offset: 0
Temp: -5c
Bin: 1x1
Filters: Astronomik 1.25 Red
Number of Stacked Images: 30
Number of Dark Frames: 30
Number of Bias Frames: 30
Number of Flat Frames: 0
Number of Dark Flat Frames: 0
Exposure: Green 30 Minutes Each (15hrs Total Exposure Time.)
Gain Set To: 0
Offset: 0
Temp: -5c
Bin: 1x1
Filters: Astronomik 1.25 Green
Number of Stacked Images: 30
Number of Dark Frames: 30
Number of Bias Frames: 30
Number of Flat Frames: 0
Number of Dark Flat Frames: 0
Exposure: Blue 30 Minutes Each (15hrs Total Exposure Time.)
Gain Set To: 0
Offset: 0
Temp: -5c
Bin: 1x1
Filters: Astronomik 1.25 Blue
Number of Stacked Images: 30
Number of Dark Frames: 30
Number of Bias Frames: 30
Number of Flat Frames: 0
Number of Dark Flat Frames: 0