At a recent (January new moon) BAS star party in south India, I happened to look at the NGC 1999 and HH1 / HH2 field in Orion through a 16" dob.
(2024-01-11) After carefully studying the field, I could hold HH2 about 70% of the time. It seemed slightly shifted west from the location seen on the POSSII. I was unable to detect HH 1, and I did not push very hard as it was a shared telescope.
Coming back to my notes, I see that I have two previous log entries for these objects. At Okie-Tex Star Party in 2021 October, I had somewhat similar results.
(2021-10-06) I seeing HH2 about 50% with averted vision. HH1 was way fainter, a threshold object which yielded ~4 flashes.
But previously in 2016 from Ft. Griffin in Texas, I had the opposite result:
(2016-01-10) I logged HH2 as more stellar and more faint, held about 10% of the time with averted vision. Of HH1, I wrote, "Diffuse, irregular and brighter. Held nearly 50% of the time, appeared much bigger [than HH2], seemed irregular and somewhat elongated in shape, axis of elongation roughly E-W.
I notice that in 2020, Scott Harrington reports HH2 as being brighter. (https://www.cloudyni...g-haro-objects/)
Uwe Glahn's observation sometime in 2006 reports HH2 brighter again.
I compared my 2016 sketch with the POSSII image, and the sketch checks out...
Now this is not absurd per se because Herbig-Haro objects can show variability in position, shape and brightness over the course of days or weeks. But I'm wondering if anyone else has noticed such substantial variation in the relative brightness of HH1 and HH2.
Clear Skies
Akarsh