Speaking of challenges, the two objects arrowed in this image (MAC 2-123 and MAC 2-203) are perhaps the two brightest (in the V band) member stars of M31. Although I have observed a single known star in M33, I’ve never attempted ones in M31. Using a line drawn between two nearby mag 12.3 and 13.1 stars, I was able to positively identify these mag 16.5 stars and showed them the Rick Linden and Alan Agrawal. Rick followed up by tracking these down with his 32” (no problem). These stars are A-type supergiants and confirmed members of M31, at a distance of 2.5 million l.y.!
I also tracked down three *very* distant galaxies that hit the 1 billion light year mark. All were very small fuzzball, quite dim, with no special appeal — except their light had been speeding through space for the past 1 billion years!
Hickson Compact Groups are scattered across the Fall skies and I looked at HCG 86, 87, 88, 89, 93 and 97.
HCG 87 in Capricorn was captured in this fan favorite HST image. A, B and C were seen, but not D.
HCG 88 consists of a quartet of spirals in Aquarius. Three of these are relatively easy NGCs in a line — NGC 6978, 6977, 6976 — and one very tough galaxy, HCG 88D = PGC 65612.
Hickson 93 is a quintet of NGCs in Pegasus and includes the distorted spiral NGC 7549 — also known as Arp 99. I caught just a hint of the spiral arms as brighter arcs on the outside of the central region, but nothing of the thin stretched extensions. I’ve looked at HCG 93 a total of 7 times since 1989 and it’s one of the easier (relatively) quintets.
Finally, HCG 97 is another quintet — all with IC designations — and a range of magnitudes from 13.0 to 15.6. Hickson 97 was discovered by one visual observer — E.E. Barnard. He found it on 28 October 1889, while an astronomer at Lick Observatory. While observing Brooks Comet (1889V) through the 36-inch Clark refractor, he stumbled across the entire quintet nearby! I previously had seen the brightest 4 galaxies through my 18”, but this was my first successful sighting of HCG 97E.