A group of us had a nice session last Saturday night at the Cherry Road site. After M31 had gained enough altitude, I went after some of its globular clusters with my 18-inch scope, typically using 275x. The East Valley Astronomy Club has 25 of the brightest globular clusters in M31 ( http://evaconline.org/m31globs.html ) as one of its observing programs, so I worked from that list. A good "finder chart" is Rob Gendler's annotated image of M31 ( http://www.robgendlerastropics.com/M31NMmosaicglobs.html ). And to give you one more reference, probably the best set of notes is Steve Gottlieb's notes for 37 M31 globulars ( http://astronomy-mall.com/Adventures.In.Deep.Space/gcm31.htm ). I managed to observe eight globulars before my attention was diverted to observing in a more neighborly fashion. It was enjoyable, and surprisingly easy to determine the location of the globulars with Gendler's large-scale photo and Megastar. Some of the globulars I went after have magnitudes in the mid-15's, which made them a challenge to hold steady. I found a number of them to at least appear "gray" compared to stars of similar magnitude. The background, be it a dark lane or of the bright core of the galaxy, has a big effect on visibility. I made my size estimates mostly from memory of the apparent size of the disc of Jupiter's moon Ganymede, which is typically in the 1.5" to 2" range. G1: This is the brightest of the globulars, and it's located fully 2 1/2 degrees away from the center of the Andromeda Galaxy. It is involved in a tiny equilateral triangle with two comparison stars. I saw G1 as only 5" across at most, with a bright core. G33: This one is paired with a 15th-magnitude star less than 10" to the east. G33 appears hazier than that star, and roughly as bright. G35: I could just barely hold this one steady; it appeared very slightly nebulous. Only 5' to the south I could see a strip of brightening of the field that is the stellar association A122. G52: Another faint one, due to placement against a bright background. In this case, it's the edge of NGC 206, the galaxy's most prominent star cloud. It appeared nearly 4" across. G58: Close to the southern end of NGC 205. Faint, but easily held steady, barely non-stellar with a bright center. G78: As M31's globulars go, this one is bright and non-stellar, 5" in diameter. It is seen against a brighter background. It's the acute corner of a 30-60 triangle with two 12th magnitude stars to the west. G72: 5' north of G78. Faint, just barely non-stellar, as disc appears gray. G64: Similar to G72 in brightness, may be showing a very small, uniform disc during moments of good seeing. -- See message header for info on list archives or unsubscribing, and please send personal replies to the author, not the list.