The Herschel 400 Astronomical League Project is underway
It’s not too late to join. We are about 30 objects into the Herschel 400. Hope to get another session in soon. Please subscribe to the YouTube channel so you get notifications on LIVE STREAMS.
Angels in Monoceros: The Monoceros M2 Complex
The Monoceros R2 molecular complex (often shortened to Mon R2) is a massive giant molecular cloud and one of the nearest active star-forming regions to Earth. It's a dynamic stellar nursery embedded in dense gas and dust, where new stars—particularly massive ones—are actively being born.
Key Facts
Location: Southwestern part of the constellation Monoceros (the Unicorn), near the border with Orion. It's part of the larger Orion-Monoceros cloud complex.
Distance: Approximately 2,400–2,700 light-years (around 830 parsecs).
Size and Structure: The main dense core is relatively compact (a few light-years across), but the overall molecular cloud and associated nebulae span a wide area—reflection nebulae alone stretch up to about 2° in the sky. It's situated well below the galactic plane, which makes it stand out in certain observations.
Age and Activity: Star formation here began roughly 6–10 million years ago. It hosts an OB association (young, hot, massive B- and A-type stars) that illuminates surrounding dust, creating prominent reflection nebulae with bluish hues. There's also significant emission from ionized gas (red glows) and dark nebulae that appear as shadowy silhouettes blocking background light.
Notable Features:
A central hub of massive star formation with embedded clusters, molecular outflows, and HII regions.
Infrared observations (like those from VISTA or 2MASS) penetrate the dust to reveal hidden young stars and protoplanetary disks.
It's a key site for studying early stellar evolution, variability in young stellar objects (YSOs), and the interplay between massive stars and their natal clouds.
The most famous and photogenic part of Mon R2 is the region around NGC 2170 (the Angel Nebula), a striking reflection nebula with wing-like dust structures, glowing blue from scattered starlight, mixed with red emission and dark lanes. Wider views of the complex reveal a richer tapestry of colorful gas, dust filaments, and star clusters.
Credit: GROK 2/28/26
Click on image for larger view.
New Astro Camera: OM-3
Join me for a LIVE conversation about this new astro camera coming to the market. Is this the best option for you? How does it compare to other options? https://www.earthandskyphoto.com Correction: when discussing Bulb mode with Canon, I incorrectly said it had a limit of 30”. I meant to say manual exposure has a max of 30”. In bulb, you need to use a remote control or app for exposure time control. The problem is you can’t set exposure time for stills in the camera menu. I was made aware that Olympus no longer owns the OM system. It is owned by Japanese industrial Partners, a private equity firm. For content on the OM-3 for astrophotography, please see Ben Chapell’s Narrow Band channel. https://youtube.com/@TheNarrowbandChannel?si=GcWY-BM9skG9LPhY
Rosette Nebula from Winter Star Party
The Rosette Nebula (please click on image for larger presentation) is approximately 5500 light years from Earth and spans over 1 degree in the sky which is more than 5 full moons. The nebula itself has different NGC designations including 2223, 2238, 2239, and 2246. The open star cluster in the middle of the nebula is designated as NGC 2244. The nebula is located in the constellation Monoceros.
This image is another in my continuing experimentation with using Adobe Light Room and Photoshop exclusively in post-processing. I actually selected only 11 of the best images I had for this object taken during the Winter Star Party in February 2009. The 11 images were each 3.5 minutes in exposure at ISO 1600 for a total exposure time of 40 minutes. ISO 1600 was used as a compromise to maximize exposure time due to the sporadic cloudiness that was present. The telescope used was a Tom Back 92mm signature series refractor at approximately f4 and a focal length of about 400mm. The camera used was a modified Canon 450D. So far, I am very happy with the results of the Adobe processing work flow. The only question that I have is how well with this process work on hydrogen alpha images. I hope to do some experimentation with this in the coming weeks. I hope you enjoy the image and please drop me a line if you get a chance.
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