Sharpless-Osterbrock 15, Stromlo (Gum) 73, Sharpless 2-27
Zeta Ophuchi Nebula
Ophiuchus
Shockwave Emission Nebula
RA 16:37:10
DEC -10:34:02
Mag --
Size 9°
(Note: Paul Alsing let me go a week early to alleviate a personal scheduling conflict)
I first learned of Sh 2-27’s existence quite a few years ago probably the way most of you did – some excellent, extremely wide-field image of the Sgr, Sco, Oph region. But I’ve never heard of any observations of it until I somehow stumbled upon Dr. Jiri Gardavsky’s last year.
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In January of 1952, while working together at the Yerkes Observatory, two young Northerners – Stewart L. Sharpless (age 25) and Donald E. Osterbrock (age 27) – got their The Nearest H II Regions paper published. In it, they presented the results of their short Ha survey with the Greenstein-Henyey wide-angle camera, of which included some of the largest emission nebulae in the sky. Using a red filter and a Ha interference filter, they cataloged 16 nebulae, with all of them having been discovered previously…except for one. And that “one”, with an angular diameter of nearly 10°, is one of the largest emission nebulae in the sky. They found that it was nearly perfectly centered on Zeta Ophiuchi and in their paper, undertook a quick comparison of it to that of the Lambda Orionis, which they had also photographed.
The next paper published about it, titled A Description of Certain Galactic Nebulosities, was submitted for review in late 1954 by Morgan, Strömgren, and Johnson. Working at Yerkes but in conjunction with McDonald, they had photographed several regions of the sky in H II that they were interested in investigation further. They found the dimensions of the Zeta Oph Nebula to be approximately 7° x 10°, and included a surprisingly detailed image of it on both page 5 and 6.
In the first half of the 1950s, Colin S. Gum, working from Australia, created a catalog of southern H II nebula that he had managed to photograph. A Survey of Southern H II Regions was published in 1955 and included the Zeta Oph Nebula as Stromlo #73 (hereafter Gum 73). Four years later, in late 1959, Sharpless included the Zeta Oph Nebula in his second and final catalog. There it was cataloged as the 27 object (hereafter Sh 2-27).
At a distance of about 365 light-years, Zeta Oph (the third-brightest star in Ophiuchus) is a single, rapidly-rotating hot O-type star. It’s also a runaway or exile star (at least 25% of massive stars are ejected from their parent cluster) because it was actually born in the Scorpius OB2 association (Sco-Cen), which is the nearest OB association to the Sun and is composed of three subgroups (Upper Sco, Upper Cen-Lup, and Lower Cen-Cru). While Zeta Oph is only about 3 million years old, it’s been theorized that for the first half of its life it had a more massive companion. But then the “primary” was destroyed in a Type II supernova, possibly pushing Zeta Oph on its current course.
Zeta Oph wArrow.jpg
In the image above (which I got from https://stellarscenes.net/object_e/zeta_oph.htm), you can see that the nebula is structured while there are dark nebulae in front of it (the white arrow indicates the direction Zeta Oph is traveling). Because of how much energy Zeta Oph is putting out, it’s ionizing a density-bound H II region around itself. Along with that, kinetic energy is generated in the surrounding Interstellar Medium (ISM) from the H II region’s expansion at a rate comparable to the mechanical luminosity of the stellar wind from Zeta Oph. The reason the H II region around it has remained quite spherical is because it’s always dynamically young, in contrast to the often-complex shapes of old H II regions around static stars. In the infrared wavelength, a distinct and impressive 1/2°-long bow shock is visible due to how fast the star is moving the dust-rich environment above the galactic plane.
Interestingly, against the odds, astrophotographer Mathew Ludgate managed to get the bow shock to show up in an image he posted last year on AstroBin. He coaxed it out by focusing his efforts on the feeble amount of O III emissions produced in the bow shock.
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On the morning of March 20th of this year, I attempted to tackle this humongous nebula with best instrument for the job – a 6-inch f/5 reflector. With that and my Explore Scientific 30/82, I was able to operate at 26x and grab nearly 3.2° of sky. None of the nebula was visible, however, until I added a H-Beta filter and concentrated on the area northwest of Zeta. Then I got a great look at the largest, brightest streak and a smaller one farther above it. What was really exciting was when I was able to see the brightest little piece (LBN 35) with no filter by using an eyepiece yielding 59x and encompassing 1.5° of sky. I looked at it all again on May 1st and found that while both H-Beta and NPB showed the “wave” or “hotdog streak” of nebula NW of Zeta, I felt my eye caught site of it better with the NPB…something about the contrast boost.
Now I'd like to see it in binoculars like Gardavsky did!
Until then,
“Give it a go and let us know!”
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Originally Posted by j.gardavsky
