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.

Link for image acquisition details at Astrobin

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

Astrophotography, Video Jeff Ball Astrophotography, Video Jeff Ball

Comet Lulin video


Comet Lulin graced North American skies in the winter of 2009. Fortunately, the closest approach was during the Winter Star Party in February. Comet Lulin proved to be much more interesting than I had previously been inclined to believe. The comet brightened dramatically over the week of February 24 and sported a beautiful ion blue tail. I slewed to the comet with the scope and began my initial exposures and was surprised by the views on the LCD screen. The blue ion tail was crumpled and extending away from the comet nucleus in a beautiful fashion. So this object became the main target object during the 2-4 a.m. imaging window on most nights.

This video is a time-lapse sequence of 9 3.5 minute exposures taken on February 21, 2009 from the Winter Star Party in the Florida Keys. Each image was optimized in Adobe Light Room and the video was compiled with Windows Movie Maker. The video loops several times so that the viewer can pick up the subtle changes in the blue ion tail. Geostationary satellites are common in this area of sky and pass through the field as through they were moving airplanes, but in fact it is the telescope and camera moving to compensate for the Earth's rotation.

You can download a wmv file from my Vimeo site which is a much larger and higher quality presentation.

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Jeff Ball Jeff Ball

Comet Lulin


Comet Lulin graced North American skies in the winter of 2009. Fortunately, the closest approach was during the Winter Star Party in February. Comet Lulin proved to be much more interesting than I had previously been inclined to believe. The comet brightened dramatically over the week of February 24 and sported a beautiful ion blue tail. I slewed to the comet with the scope and began my initial exposures and was surprised by the views on the LCD screen. The blue ion tail was crumpled and extending away from the comet nucleus in a beautiful fashion. So this object became the main target object during the 2-4 a.m. imaging window on most nights. More information on the comet can be found by clicking on the title of the blog at NASA's website. You may also click on the image for a larger presentation.

This particular image was taken during the 2 a.m. hour of February 21, 2009. It is a composite of 9 exposures of 3.5 minutes each at ISO 1600 on the Canon 450D through the TMB 92SS refractor. Comet imaging poses additional challenges when the comet is fast moving such as Comet Lulin. The imager must combine several short exposures for the background sky as well as for the comet. So two iterations of stacking are needed since the comet is moving relative to the fixed star field. This is quite challenging in processing, but we do have techniques that allow us to accomplish this with nice results.

All of the processing was accomplished with Adobe Light Room 2.0 and PS3 with some Noise Ninja for noise reduction. Images were aligned and stacked with Images Plus. A Sigma median combine was used on the comet nucleus to achieve a reduction in star trails and isolate the comet nucleus and tail in the combination. The total exposure time is approximately 30 minutes. I am also going to present a movie which depicts the comet moving relative to the star field. I hope you enjoy the image and please check out the NASA link for more information on the comet.

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