Welcome to the Galaxies Section of the Webb Deep-Sky Society. Our role is to promote visual observation and scientific imaging of galaxies by amateur astronomers.
Galaxy of the Month
Below is our current Galaxy of the Month. These are galaxies that we feel are particular worthy of your precious observing time. We have an archive of these articles that stretch back to the beginning of 2011. You can browse them, or search for specific objects and constellations in the Galaxy of the Month archives.
Your observations (sketches, images or observing notes) of any of these objects are very welcome.
For those that use observation planning software
We have plans available for all the Galaxy of the Month pieces from 2011 onwards to make it easier to find the galaxies we have covered so far.
- For Skytools (updated for March 2019)
- For Deep Sky Planner (use right mouse click and Save Link As)
- For AstroPlanner
These will be updated as new GOM’s are added.
NGC 1888 and Arp 123 in Lepus
December 2019 - Galaxy of the Month
The galaxy pair NGC1888/1889 in Lepus was first discovered by William Herschel in 1785, although he only saw one of the pair, NGC 1888. It took Bindon Stoney using Lord Rosse's 72" in 1851 to discover the smaller galaxy in the pair which became NGC 1889.
Arp catalogued the pair as Arp 123 in his group of "Ellipticals close to and perturbing spirals". NGC 1888 does look as it is being distorted by an encounter with extended spiral arms. The galaxy does have a spiral arm on the opposite side to NGC 1889 which contains lots of young blue stars. Vorontsov-Velyaminov also included it in his extended catalogue of interacting galaxies as VV 1138. The pair also hosted the Type Ia supernova SN 2018yu.
The galaxies lie at a distance of perhaps 110 million light years from us.
Close by and in the same high power field is the edge on galaxy MCG-2-14-15, also known as RFGC 973, which at magnitude 14.5 should be visible in larger telescopes. For those with very large telescopes there is a third edge on galaxy called LEDA 147414 (PGC 147414), but at mag 16.5 this is likely to require very large telescopes from high dark sites to find.
Unfortunately for UK observers Arp 123 never rises that high, barely reaching the 1 airmass line at 30 degrees. Nevertheless it was visible in my 15” telescope and in an 18” at the October 2019 Haw Wood star party in Suffolk at the high altitude of maybe 70m. The MCG galaxy was not seen but the night was not the most transparent. The group did make the DeepSkyForum (DSF) Object of the Week in 2012.
NGC 1888 is classified as SB(s)c pec and NGC 1889 as cD pec. Arp gave them different classifications as Sc and E0. The pair are almost certainly in the early throws of a merger. MCG -2-14-15 is well in the background and not associated with the main pair.
Perhaps surprisingly given this is an Arp pair there is not much in the literature on them. The pair makes both the Night Sky Observer's Guide (NSOG) Volume 1 and the Webb Society Deep-Sky Observer's Handbook (WSDSOH) Volume 4, which suggests that a 16” is good whereas the NSOG suggests that a 30cm telescope will show the pair. Both suggest high power is needed to split them.
Owen Brazell - Galaxy Section Director