M2

Messier 2 is a magnificent celestial metropolis hanging in the autumn sky, located about 5° north of Beta Aquarii in the constellation of Aquarius the Water Bearer. Shining at a bright magnitude 6.3, this ancient globular cluster is one of the grandest of its kind, packing roughly 150,000 stellar citizens into a tight, buzzing ball of light. Discovered by Jean-Dominique Maraldi in 1746 and later cataloged by Charles Messier, it sits approximately 37,000 light-years away, offering backyard astronomers a stunning glimpse into the deep galactic past.

Sweeping the area with 7x50 binoculars easily reveals M2 as a prominent, fuzzy un-stellar blob that stands out clearly against a sparse background field. Through a 4-inch refractor at low power, the cluster transforms into a beautiful, circular glow with a strikingly bright, dense core that tapers off into a soft, misty border. The view is remarkably intense, showcasing a compressed center that refuses to yield individual stars easily, keeping its secrets guarded like a classic, unresolved cosmic snowball.

To truly unlock this deep-sky masterpiece, slide a high-power eyepiece into a 8-inch or larger telescope on a night of steady, transparent air. At 150x, the smooth outer halo shatters into a glittering spray of tiny, pinpoint diamonds, while a few rogue stars can be seen glinting across its brilliant face. Larger instruments will reveal the cluster's slightly oval shape and a fascinating, dark dust lane cutting across its northeastern edge, adding a touch of mystery to this stellar city.

M1

Messier 1, the Crab Nebula, is a haunting celestial ghost drifting in the winter sky just 1° northwest of Zeta Tauri, the southern horn of Taurus the Bull. For backyard astronomers, this 8.4-magnitude supernova remnant represents a rare chance to gaze directly at the shredded remains of a dying star—an explosion witnessed by earthbound stargazers in the year 1054. While astrophotographs reveal an intricate web of colorful filaments, the visual view through a modest eyepiece is delightfully subtle, demanding careful attention and a dark sky.

Chasing this cosmic crustacean requires a bit of patience and a star-hop to the bull’s horn. At low power in a 4-inch refractor, M1 appears as a smooth, ghostly oval smudge, looking remarkably like a faint, tail-less comet—the exact illusion that prompted Charles Messier to start his famous catalog. Stepping up to a 6- or 8-inch telescope begins to peel back the layers, revealing an asymmetrical, pear-shaped silhouette that brightens gently toward the center before melting softly into the dark background.

To coax the absolute best out of this deep-sky classic, push the magnification to medium-high levels on a night of steady, transparent air. Under a truly dark sky, a 12-inch or larger instrument transforms the smooth wash of gray light into a complex, mottled tapestry. With careful averted vision, the nebula's borders turn delightfully ragged, hinting at the violent, expanding tendrils of stellar guts that continue to rush outward into the interstellar void.

NGC 6217

Barred spiral galaxy. Distance 70 Mly. Size 3'. Magnitude 11. Ursa Minor. 2025-08-24, Williamsville. 12" SCT, F/3.3, 40 s exposure. Bar dominates. Bright nucleus. Faint star embedded in the bar next to the nucleus. Bar brighter opposite the star, where it curves into an arm away from the nearest field star. This arm segment almost connects to an arc running through the opposite end of the bar.

Late Fall Herschels

October 8, 2024. Spruce Knob, T 3/5, S 1/5, SQM 21.24 (diffuse aurora). 20" F/4. Late fall Herschels.

NGC 772, GX, Ari. 8 mm. Small, slightly elongated, brighter in the middle to a nucleus. Thin arm points between two stars. Much smaller galaxy near.

NGC 752, OC, And. This cluster fills the field of the 26 mm 100-deg. Bright stars, no concentration.

NGC 891, GX, And. 26 mm. Very greatly extended, brighter to the middle, tapering ends. Bisected in the middle by a dark lane.

M33 (NGC 598, HV-17). GX, Tri. 26 mm. Very large, just framed. Overall slightly elongated. Relatively small bright core. Two arms dominate. One ends in two knots, the other extends symmetrically like an "S" and ends in a broad patch. Two more arms are found between these two. One of these ends in an enhanced patch and points at a widely separated compact cloud. The second short arm has two knots.

NGC 404, GX, And. Next to a very bright star. Small, relatively bright, compact.

NGC 908, GX, Cet. 8 mm. Elongated, little brighter in the middle to a nonstellar nucleus. Arm runs on one end inwards of a star. The opposite arm is brighter and has a sharp outer edge near the core, which faces a bright star pair.

NGC 1055, GX, Cet. 8 mm. Greatly elongated. Tapering ends, gradually brighter to the middle. The edge facing the star is straight and sharp. There is a faint extended patch of light next to the star.

NGC 936, GX, Cet. 8 mm. Small round core, bright nucleus, thin extensions of the core. Traces of an off-round halo with an enhanced edge that is extended in a different direction from the core.

NGC 1022, GX, Cet. 8 mm. Round core, gradually brighter to the middle. Short arm emerges CW from the core opposite a star that is near. A fainter star is embedded in the halo.

NGC 1052, GX, Cet. 8 mm. Elongated overall. Small bright core with a nucleus. Faint extensions. A triangle of faint stars near.

NGC 1084, GX, Eri. 8 mm. Elongated, little brighter in the middle. Fine mottling. Short CW arm points S, another points N.

NGC 488, GX, Psc. 8 mm. Slightly elongated. Small core with a nucleus. Extensive halo is brighter away from the star.

NGC 524, GX, Psc. 8 mm. Considerably small and faint. Much brighter in the middle to a nonstellar nucleus. Edges diffuse.