Howard B
December 5th, 2021, 10:01 PM
Orion
Herbig-Haro objects
RA: 5 36 22.8
Dec: -06 46 03
4544
Mount Lemmon SkyCenter Schulman Telescope / Adam Block
First, a refresher on what HH (Herbig – Haro) objects are: ( https://tinyurl.com/uwm5tm46 ) and HH 1/2 in particular: ( https://en.wikipedia.org/wiki/HH_1/2 )
I’ve been looking forward to writing his OOTW since early September when I had the completely unexpected pleasure of stumbling across HH 1/2 while observing NGC 1999 from my backyard. In the hour before dawn on September 9, 2021, NGC 1999 had risen high enough in the east so I’d have a decent chance of seeing it fairly well. I was in the final stages of writing an article about 1999 and wanted to get an observation or two from my backyard even though it would be located low in the most heavily light polluted part of my sky. The forecast called for above average transparent skies so I gave it go.
The view of 1999 was fairly dim, and I couldn’t make out its dark cavity, but my eye kept catching on a faint streak of nebulosity nearby. I thought I was imagining it at first, but then the entire area to the southwest of 1999 seemed to filled with faint, lumpy nebulosity! After dawn I came back in the house to confirm the position and orientation of HH 1/2 relative to NGC 1999, and sure enough my sketch lined up with reality.
4545 4546
I was astonished – this was in the brightest part of my sky with a SQM in the low 19’s. Perhaps the most incredible part is that I was observing with my 8-inch f/4 scope. Evidently, the transparency forecast was a spectacular understatement.
Two mornings later, again just before dawn, I repeated this observation with my 28-inch f/4 scope under an even more remarkably transparent sky, and had an awesome view of both NGC 1999 and HH 1/2. NGC 1999 looked like a photograph, and HH 1/2 were easy, direct vision objects that even showed a little structure. My observing notes:
“The best view of HH1/2 was also at 408x and 545x. 408x showed the greatest extant of nebulosity, while 545x revealed a bit of detail. Pretty awesome! The 408x field of view nicely framed 1999 along with HH1/2 which is why I spent the most time at this magnification. Steady seeing, even at this low elevation (about 20 degrees) made the view even more enjoyable.
I don’t think the atmosphere can get much clearer than it is this morning – just exceptional transparency! The early sunrise colors confirm how clear the air is. (19.94 SQM toward the east, 20.71 straight up)”
4547 4548
Nebula filters didn’t improve the view at all, and my observations were made without them.
These two observations, and remarkably transparent skies, were exceptional in my experience and have given me food for thought on how darkness, transparency and steady seeing effect views of deep sky objects. These early morning observations are the two best views I’ve had of HH 1/2, and considering how well I saw them with the 28-inch, and that I could see them at all with my 8-inch so low in a light polluted sky, has changed my thinking. It seems to me that transparency is the most important factor in seeing faint deep sky objects – or at least for HH1/2 and NGC 1999.
I’m very interested to read your experiences of observing HH 1/2, and how you think of the interplay between darkness, transparency and seeing.
Give it go, and let us know!
Herbig-Haro objects
RA: 5 36 22.8
Dec: -06 46 03
4544
Mount Lemmon SkyCenter Schulman Telescope / Adam Block
First, a refresher on what HH (Herbig – Haro) objects are: ( https://tinyurl.com/uwm5tm46 ) and HH 1/2 in particular: ( https://en.wikipedia.org/wiki/HH_1/2 )
I’ve been looking forward to writing his OOTW since early September when I had the completely unexpected pleasure of stumbling across HH 1/2 while observing NGC 1999 from my backyard. In the hour before dawn on September 9, 2021, NGC 1999 had risen high enough in the east so I’d have a decent chance of seeing it fairly well. I was in the final stages of writing an article about 1999 and wanted to get an observation or two from my backyard even though it would be located low in the most heavily light polluted part of my sky. The forecast called for above average transparent skies so I gave it go.
The view of 1999 was fairly dim, and I couldn’t make out its dark cavity, but my eye kept catching on a faint streak of nebulosity nearby. I thought I was imagining it at first, but then the entire area to the southwest of 1999 seemed to filled with faint, lumpy nebulosity! After dawn I came back in the house to confirm the position and orientation of HH 1/2 relative to NGC 1999, and sure enough my sketch lined up with reality.
4545 4546
I was astonished – this was in the brightest part of my sky with a SQM in the low 19’s. Perhaps the most incredible part is that I was observing with my 8-inch f/4 scope. Evidently, the transparency forecast was a spectacular understatement.
Two mornings later, again just before dawn, I repeated this observation with my 28-inch f/4 scope under an even more remarkably transparent sky, and had an awesome view of both NGC 1999 and HH 1/2. NGC 1999 looked like a photograph, and HH 1/2 were easy, direct vision objects that even showed a little structure. My observing notes:
“The best view of HH1/2 was also at 408x and 545x. 408x showed the greatest extant of nebulosity, while 545x revealed a bit of detail. Pretty awesome! The 408x field of view nicely framed 1999 along with HH1/2 which is why I spent the most time at this magnification. Steady seeing, even at this low elevation (about 20 degrees) made the view even more enjoyable.
I don’t think the atmosphere can get much clearer than it is this morning – just exceptional transparency! The early sunrise colors confirm how clear the air is. (19.94 SQM toward the east, 20.71 straight up)”
4547 4548
Nebula filters didn’t improve the view at all, and my observations were made without them.
These two observations, and remarkably transparent skies, were exceptional in my experience and have given me food for thought on how darkness, transparency and steady seeing effect views of deep sky objects. These early morning observations are the two best views I’ve had of HH 1/2, and considering how well I saw them with the 28-inch, and that I could see them at all with my 8-inch so low in a light polluted sky, has changed my thinking. It seems to me that transparency is the most important factor in seeing faint deep sky objects – or at least for HH1/2 and NGC 1999.
I’m very interested to read your experiences of observing HH 1/2, and how you think of the interplay between darkness, transparency and seeing.
Give it go, and let us know!