U 339
17:52 to 18:24
-17° to -28°
Sgr

FEATURED OBJECTS: NGC 6469, Cz 37, UKS 1, NGC 6494, LDN 305, Ru 136, Ru 169, NGC 6507, NGC 6506, Ru 137, Ru 138, Ru 139, Terzan 9, Boch 14, NGC 6514, LDN 97, NGC 6520, Terzan 10, NGC 6526, NGC 6531, NGC 6523, NGC 6530, NGC 6533, IC 1271, NGC 6537, NGC 6540, LDN 122, IC 4678, NGC 6544, NGC 6546, LDN 306, vdB 113, LDN 216, IC 4684, NGC 6554, IC 4681, LDN 212, IC 4685, NGC 6553 (Ben 105), IC 1274, NGC 6559, IC 1275, NGC 6556, LDN 228, Terzan 12, Terzan 11, NGC 6568, NGC 6567, NGC 6573, Biur 5, LDN 326, NGC 6583, LDN 198, Cr 469, NGC 6578, NGC 6589, NGC 6590, LDN 330, NGC 6595, IC 1283, LDN 275, NGC 6603 (Ben 107a), AL 4, LDN 338, NGC 6613, NGC 6620.

NGC 6469
Mel 182, Cr 353, Rb 124
RA 17:52:53
Dec -22°20.0'
Open cluster

h: "a pretty rich insulated milky way cluster; place of a course double star in it. The milky way hereabouts is very poor."

Cz 37
ESO521-SC003
RA 17:53:16
Dec -27°22.4'
Open cluster

UKS 1
C1751-241
RA 17:54:26
Dec -24°09.0'
Globular cluster

NGC 6494
Messier 23, Mel 184, Cr 356, Rb 126
RA 17:57:04
Dec -18°59.1'
Open cluster

Discovered by Messier in June of 1764, he described it as a cluster 15' in diameter with stars "very close to one another."

In the Appendix to the 1912 'Scientific Papers of Sir William Herschel' this object is described as "1784, June 18, 20 feet telescope, a cluster of beautifully scattered, large stars, nearly of equal magnitude (visible in my finder), it extends much further than the field of the telescope will take in, and in the finder seems to be a nebula of a lengthened form extending to about half a degree."

Burnham notes that the stars are scattered more or less evenly across the whole field, with very little concentration toward the centre. A number of the stars, however, appear to be arranged in curving arcs and chains, "which to the imaginative observers may suggest the outline of a Chinese temple, or perhaps some bit of oriental calligraphy." Flammarion saw near the centre a circle of six stars, with "nine stars in an arc" in the north-east portion of the cluster. K G Jones points out that "three or more" of the star chains appear to be potions of concentric arcs which are seemingly focused toward the bright 8th mag star on the north-east side of the cluster. Admiral Smythe described M23 as "A loose cluster, an elegant sprinkling of telescopic stars over the whole field under moderate magnification. The most clustering portion is oblique in a direction Sp. and N.f." C E Barns writes of the cluster as "a blazing wilderness of starry jewels." Burnham comments on a chain of faint stars running from the cluster out to a bright mag 6.5 white star in the northwest, some 18' from the cluster centre. He adds that the most pleasing views can be obtained with a 10" f/6 reflector working at 45 power.

Harrington notes that it "might just be visible to the naked eye on clear nights as a slightly brighter spot along the Milky Way. Through binoculars it appears as a nebulous glow spanning about half a degree. With low-power telescopes M23 is a beautiful sight. Some observers see the group as fan-shaped, though the allusion has always escaped me. In all, about 120 suns as bright as 9th mag reside in the group.

Steve Coe, observing with a 13" f/5.6, notes: "(M 23) Bright, large and not compressed. At 100X it has chains of stars that form a pattern like the seats of a sports arena. Rose Bowl Cluster?"

11x80: "Wonderful open cluster, a large haze of many pinpricks of light, accompanied by a bright star to the northwest. Very noticeable even when sweeping. Although not nearly as luminous as nearby M7, this M23 has a different charm and is as interesting as its bright neighbour." On a second occasion: "Spectacular cluster. Irregularly round. Bright star nearby. Uncountable swarm, random scatter of stars, no concentration. Looks like M44 with the naked eye." [AS]

LDN 305
Barnard 84A
RA 17:57:29
Dec -17°40.3'
Dark nebula

Barnard (Astrophysical Journal, January 1919) writes in his 'Notes on the Catalogue' that BD -19°9457 (mag 9.5) lies in the centre of this dark nebula.

Ru 136
ESO521-SC004
RA 17:59:16
Dec -24°41.7'
Open cluster

Ru 169
ESO521-SC005
RA 17:59:21
Dec -24°46.4'
Open cluster

NGC 6507
Cr 358
RA 17:59:35
Dec -17°23.0'
Open cluster

Discovered in 1786 by William Herschel (H VIII-053) "a cluster of scattered small stars, 8' diameter, not very rich."

11x80: "The smallest of little puffs of light. To the east of a 9th mag star. Not a very positive sighting." On a second occasion, I noted: "Quite faint, irregular glow. Looks quite large, but very little light." [AS]

NGC 6506
ESO521-SC006, OCL-16
RA 17:59:53
Dec -24°40.8'
Open cluster

h: "a very loose but very rich cluster, which fills many fields. Stars small."

The RNGC (Sulentic and Tifft 1973) notes that this is a nonexistent object. Their coded description reads NOCL S.

Ru 137

RA 17:59:53
Dec -25°10.0'
Open cluster

Ru 138

RA 17:59:53
Dec -24°40.0'
Open cluster

Ru 139
ESO521-SC010
RA 18:01:01
Dec -23°32.0'
Open cluster

Terzan 9
ESO521-SC011, C1758-268
RA 18:01:38
Dec -26°50.3'
Globular cluster

Boch 14

RA 18:01:58
Dec -23°41.0'
Open cluster

NGC 6514
Trifid, Messier 20, Cr 360, Boch 14
RA 18:02:16
Dec -23°01.0'
Open cluster

Better known as the Trifid nebula, M 20 was probably first seen by LeGentil in 1747 and discovered by Messier in June 1764. Messier saw it as a cluster of faint stars.”

Recorded as IV.41 on May 26, 1786 by William Herschel with an 18.7-inch f/13 speculum telescope. He called it “a double star with extensive nebulosity of different intensity. About the double star is a black opening resembling the neb. in Orion in miniature.” In the Appendix to the 1912 'Scientific Papers of Sir William Herschel' this object is described as “1783, May 3, 20 feet telescope, two nebulae close together, both resolvable into stars; the preceding however leaves some doubt, though I suppose a higher power and more light would confirm the conjecture. 10 feet telescope, power 350; the instrument will not bear a higher power in this low altitude.”
He also noted it as “three nebulae, faintly joined, form a triangle. In the middle is a double star, vF, and of great extent.”

Admiral Smythe found its presence “indicated only by a peculiar glow [which surrounded] the delicate triple star in the centre of its opening, the nebulous matter resisted light of my telescope...” Sir William Herschel found the nebulosity conspicuously divided by a curious pattern of dark lanes, and catalogued the brightest portions as four separate objects. John Herschel was probably the first to call it the “Trifid” nebula, and described it as “consisting of three bright and irregularly formed nebulous masses, graduating away insensibly externally, but coming up to a great intensity of light at their interior edges where they enclose and surround a sort of 3-forked rift or vacant area, abruptly and uncouthly crooked and quite void of nebulous light... A beautiful triple star is situated precisely on the edge of one of these nebulous masses just where the interior vacancy forks into two channels. “This multiple star, GC 24537, which is also the illuminating star in the nebula, has six components which were discovered by S.W. Burnham using the 36” Lick refractor:
Components Magnitudes Separation PA
A - B 7 10.6 5.4” 23
A - C 7 8.8 10.6” 212
A - F 7 13.8 22.1” 106
C - D 8.8 10.5 2.2” 282
C - E 8.8 12.4 6.2” 191

h: “triple star in the trifid nebula.” On a second occassion he called it “one of the most remarkable nebulae, and must bve very carefully delineated. It is very large and has many outlying portions and sinuses. See fig 2, Plate II.”

Hartung notes that a 4” will show three of the companions, whilst an 8” is needed to see the fourth. C E Barns described the Trifid as “a dark night revelation even in modest apertures... Bulbous image trisected with dark rifts of interposing opaque cosmic dustclouds...” Burnham comments that the trifid appearance should be easy in a good 8-inch at moderate power, while Hartung says that the lanes “may be seen with 10.5cm [4”]”. The lanes are about 45” across, the east and west lane merging into the surrounding blackness of the night sky on the edges of the nebula, whereas the southern lane is blocked by a bright feature.

David Neilson (Oakland, California, USA), writes in the The Webb Society Nebulae and Clusters Section Report No. 10, July 1992: “Not seen to advantage. Bright, close pair at centre of mistiness. Closer inspection shows the tripartite division of the mist. Seven or eight fainter stars involved (12.8-inch).”

It is a member of the Sagittarius OB 1 Association. Beverly Lynds (Astrophysical Journal Supplement, No 105, 1965) in her Catalogue of Bright Nebulae, notes that its maximum size is 20' x 20' and that it is brighter on the red POSS plate.
The dark lanes are also known as Barnard 85.

Donald J. Ware:”The Trifid Nebula. Only a short distance north of M-8, this object is rather easily found, but is considerably fainter than that object. A double star is seen surrounded by a mostly circular patch of light. This patch of light is divided into three separate regions by dark lanes which intersect near its center. On a good night, a fainter region of reflection nebulosity of almost equal size as the main portion can be seen to the north.”

Steve Coe, observing with a 13” f/5.6, notes: “(M20) Very bright, very large, irregularly round, approximately 40 stars involved in a nebula that is criss-crossed by dark lanes at 135X. The Trifid is naked eye from even a moderately dark site. The UHC filter enhanced the nebulosity, but I like the view of this object better without the filter. The triple star in the center of the brightest section is HN 40, it is split at 165X and it two yellow and one light blue star embedded within the Trifid nebulosity.”

LDN 97
Barnard 86
RA 18:02:43
Dec -27°49.9'
Dark nebula

Somewhat north of the centre of the Sagittarius Cloud lies this dark nebula, one of the most prominent in the sky. It rims the west edge of the compact little open cluster NGC 6520, and appears as a distinct inky spot against the surrounding star-shimmer. Burnham comments that "this is one of the few dark nebulae that may be appreciated in amateur telescopes."

Barnard writes of this object in his article "On the Dark Markings of the Sky", (Astrophysical Journal, January 1919) as follows: "This black spot, known to me in my early days of comet seeking [with a 5" refractor], is very sharply defined on its east edge, but less definite on the west. There is a 12th magnitude star near the middle." and adds "It was found in my comet-seeking in the early eighties. On account of its extreme blackness it was one of the most impressive objects in the Milky Way. I examined it with the 36-inch refractor of the Lick Observatory with a power of 350 and a field of 6', on August 18, 1895. It nearly filled the field of view. The western half was fairly well defined, while the eastern half was more diffused. Considerable nebulosity seemed to be connected with it. A photograph on July 11, 1917, with the Crossley reflector, kindly sent me by Dr. H.D. Curtis, shows this black spot to be very remarkable, having considerable nebulosity connected with it. On his photograph, its southwest side is very sharply defined,... Its east side...is more or less diffused. The star CD-27°12302 (mag 7.4) is on the northwest border, while CD -27°12310 (mag 9.0) is close east of the spot. The beautiful cluster of small bright stars, NGC 6520, is also close east."

As an aside, after Barnard swept up this object, he announced its discovery in 1884 in the Astronomische Nachrichten, where it is described as "a small triangular hole in the Milky Way. Perfectly black, some 2' diameter, much like a jet black nebula."

Note that when Barnard observed it with a 5-inch telescope, he reported its diameter as 2 arc minutes, but in his catalogue he calls it: "Diameter 5'; several small stars in it."

The following article, authored by H E Houghton, appeared in MNASSA Vol 1, p 107, Feb. 1942 titled "Sir William Herschel's 'Hole in the Sky'." "When Sir John Herschel was leaving for the Cape in 1834, his aunt, Miss Caroline Herschel, wrote to him as folows: 'Dear Nephew. As soon as your instrument is erected I wish you would see if there is not something remarkable in the lower part of the Scorpion to be found, for I remember your Father returned several nights and years to the same spot, but could not satisfy himself about the uncommon appearance of that part of the heavens. It was something more than a total absence of stars (I believe)'. Soon after his arrival at the Cape, Sir John wrote in reply: "I have not been unmindful of your hint about Scorpio. I am now rummaging the recesses of that constellation and find it full of beautiful globular clusters.' Miss Herschel was not satsified and replied to her nephew: "It is not the Clusters of Stars I want you to discover in the body of the Scorpion (or thereabouts) for that does not answer my expectation, remembering having once heard your Father, after a long awful silennce, exclaim `Hier ist wahrhaftig ein Loch im Himmel` and as I said before, stopping afterwards at the same spot but leaving it unsatisfied. . . . It is now generally thought to be a dark nebula reported by Secchi in RA 17h 54.6m and Decl. -27° 53'. . . Father Hagen holds that Sir William Herschel did not consider the appearance to be anything but a starless spce, but it seems from Miss Herschel's first letter quoted above that her brother had some doubt about this object and that he saw something in the nature of a faint nebulous appearance. This provides anbother example of his visual acuteness, by the detection of such a faint nebulous appearance in an object which culminated at an altitude of only about ten degrees abive his horizon."

Steve Coe, observing with a 13” f/5.6, notes: “is a DARK Barnard Nebula right next to NGC 6520. It has an hourglass shape and is about 5 minutes in size. There is a lovely orange star in the field. Don't miss this very nice area.”

NGC 6520
Mel 187, Cr 361, Rb 127
RA 18:03:16
Dec -27°53.2'
Open cluster

Discovered in 1785 by William Herschel (H VII-007) “a considerably rich but pretty compressed, scattered cluster if stars, a little more compressed in the middle.”

h: “a pretty compact cluster class VII of stars 9..13m; irregularly scattered, diam 4'.”

Harrington writes: “With persistence, NGC 6520 can be seen as a faint smudge through 7x binoculars. Although a 4-inch telescope at low magnification shows a little more, higher powers and larger apertures are needed to unveil the cluster's true nature - a rich school of faint stars swarming in the stream of the Milky Way. In all, tiny NGC 6520 holds 60 stars within a 6' area.”

Tom Lorenzin: “9M; 5' diameter; small and dense; 25-plus 9 thru 12M members; DK NEB B-86 on W edge; cluster N6540 is 30' due E.”

Terzan 10
ESO521-SC016, C1800-260
RA 18:03:37
Dec -26°05.1'
Globular cluster

NGC 6526
ESO521-*N018, Gum 74B, RCW 145
RA 18:03:54
Dec -23°21.9'
Bright nebula

Discovered in 1784 by William Herschel (H V-9) “Large, extended, broad, milky, faint.” In the Philosophical Transactions, 1811, Herschel describes it as “a large, extended, broad, faint nebula; its nebulosity, like that of the preceding one (which is de la Caille's last but one in the Catalogue des Nebuleuses du Ciel Austral) [NGC 6523] is of the milky kind.”

NGC 6531
Messier 21, Mel 188, Cr 363, Rb 128
RA 18:04:13
Dec -22°29.4'
Open cluster

NGC 6523
Lagoon Nebula
, Messier 8, LBN 25
RA 18:04:15
Dec -24°19.3'
Bright nebula

Also known as the Lagoon Nebula, it is plainly visible to the naked eye as a glowing patch just off the main stream of the Sagittarius Milky Way. Burnham notes that the discovery of M8 is often credited to Le Gentil in 1747, who described it as “a small nebulosity like the tail of a comet with numerous stars... like the more transparent and whitish localities of the Milky Way.” Burnham further writes that “it seems that it was recorded by Flamsteed as a “nebulosum” preceding the “Bow of Sagittarius” as early as 1680; de Cheseaux in 1746 also refers to a “cluster in Sagittarius' bow.”

Lacaille included it in his 1755 catalogue as Class III No. 13. In his half-an-inch 8x telescope he saw it as “three stars in nebulosity parallel to the Equator.”

Messier observed it in 1764, describing at as “a cluster which looks like a nebula in an ordinary telescope of three feet but in a good instrument one observes only a large number of small stars... A fairly bright star nearby is surrounded with a very faint glow; this is 9 Sagittarii, 7 mag. The cluster appears elongated NE-SW. Diam 30'.”

Sir William Herschel described it as “an extensive milky nebulosity divided into two parts; the north part being the strongest. Its extended exceeds 15'; the southern part is followed by a parcel of stars.” In the Appendix to the 1912 'Scientific Papers of Sir William Herschel' this object is described as “1784, May 22. Large, extended, pretty bright, broad. The nebulosity of the milky kind, there are some pB stars in it, but they seem to have no connection with it, being of very different sizes and colours and resembling the other stars that are everywhere scattered about in this neighbourhood. This is probably the star surrounded with nebulosity mentioned by Messier. There is indeed one of the stars which are in the nebula that is somewhat larger than the rest and may be the only one he saw.”

Sir John Herschel saw it as “a collection of nebulous folds and matter surrounding and including a number of dark, oval vacancies and in one place coming to so great a degree of brightness as to offer the appearance of an elongated nucleus. Superimposed on this nebula and extending in one direction beyond its area, is a fine and rich cluster of scattered stars which seems to have no connection with it as the nebula does not, as in the region of Orion, show any tendency to congregate about the stars..” At the Cape of Good Hope, he observed it with an 18-inch f/13 speculum telescope. He recorded it as “A noble nebula; to be monographed. The star taken is = 9 Sagittarii 7m. It is followed by a great cluster VI.13, of which with the nebula fills many fields.” On a second occassion he called it “a superb nebula... See plate 1, fig 1.”

Webb called it “a splendid galaxy object, visible to naked eye. In a large field we find a bright coarse triple star, followed by a resolvable luminous mass, including two stars, or starry centres, and then by a loose and bright cluster enclosed by several stars; a very fine combination...”

C E Barns wrote of it as “myriads of low-mag stars and a few brighter units resembling somewhat the Pleiades, involved in wide wastes of incandescent hydrogen and helium, overflung with dark absorbing patches..”

Hartung notes that “this fine nebula needs a large field and shows very extensive luminosity of varying brightness, involving two bright stars, with irregular lanes and followed by a bright open cluster... The whole field is wonderfully fine and varied, and small apertures show it well.”

Burnham notes that the western half of M8 “is dominated by two bright stars just 3' apart; the southern star is 9 Sagittarii... Just 3' WSW from 9 Sagittarii lies the brightest segment of the nebulosity, a 'figure 8' shaped knot about 30” in size and often called from its shape “The Hourglass”...”

David Neilson (Oakland, California, USA), writes in the The Webb Society Nebulae and Clusters Section Report No. 10, July 1992: “Roughly bar-shaped, misty nebula surrounding four stars (mag 10-11). Due east, the dark rift is very distinct and is followed by a large, indistinct region of nebulosity (8-inch).”

John Bortle (Webb Society Quarterly Journal, January 1976) using 10x50 binoculars, estimates the visual magnitude of NGC 6523+6530 as 3.7.

Beverly Lynds (Astrophysical Journal Supplement, No 105, 1965) in her Catalogue of Bright Nebulae, notes that its maximum size is 45' x 30'.

Tom Lorenzin: “5M; 80' x 40' extent! easily found with naked eye or binoculars; dark lane winds thru SW to NE; in E segment lies 1' diameter “HOURGLASS”, 3' WSW of 9 SGR, illumination source; dark void surrounds 12M star just W of Hourglass's constriction; use high-x; cluster N6530 (10' diameter; 25-plus 7M and dimmer members) in N part of E segment; N-filter aids greatly; called “LAGOON”; one more of the best!.”

Donald J. Ware:”The Lagoon Nebula. With the possible exception of the Great Orion Nebula (M-42), this is probably the finest cluster and nebula combination in the heavens. A large and loosely scattered open cluster is seen in juxtaposition with a large and swirling mist of nebulosity. Many dark regions can be seen in looping patterns which are highlighted by the brighter regions. This object is easily seen in finder scopes, binoculars, and with the naked eye.”

Steve Coe, observing with a 13” f/5.6, notes: “(M 8) Very bright, very, very large, somewhat compressed cluster with lots of nebulosity. With the 2" eyepiece that gives a one degree field with the 13", the entire field is nebulous and the dark lane that gives the Lagoon its' name is obvious. I counted 40 stars included within the cluster and there are another 50 stars among the outer parts of the nebula and 10 of the stars are within the dark lane. Going to 100X shows the west side of the nebulosity is brightest and adding the UHC makes the nebula grow 1.5 times in size. I don't like the view with the UHC filter because it dims the stars involved and that is a large part of the beauty of this area of the sky. The Lagoon is an obvious naked eye spot in the Milky Way, even on a mediocre evening. In the finder or 10X50 binoculars this area in spectacular, the Lagoon and Trifid fit in the same field with star chains and dark lanes winding their way through the entire field of view. This part of Sagittarius will be a favorite as long as people construct telescopes.”

NGC 6530
Cr 362
RA 18:04:30
Dec -24°21.6'
Open cluster

h: “cluster large and bright, just fills field, a double star taken. The cluster follows M8.” On a second occassion he called it “a bright, pretty rich irregularly round cluster, place that of a double star in the following part of the cluster, which is itself in the great nebula M8.”

Trumpler (Lick Obs Bul, Vol 14, No. 420) gives the diameter as 14' and the class as 2 2 mN.

NGC 6533

RA 18:05:05
Dec -24°53.0'
Nonexistent

William Herschel observed it in 1784 (H V-013) “an extensive milky Nebulosity divided into two parts; the most north being the strongest. Its extent exceeds 15'; the southern part is followed by a parcel of stars.” and also “. . . the most north, above 15'. the most south, followed by stars.”

The RNGC (Sulentic and Tifft 1973) notes that this is a nonexistent object. Their coded description reads NF S.

IC 1271
ESO521-*N022
RA 18:05:09
Dec -24°23.9'
Bright nebula

NGC 6537
ESO590-PN001, PK010+00.01
RA 18:05:11
Dec -19°02.0'
Planetary nebula

The RNGC (Sulentic and Tifft 1973) notes that this is a 12.5 mag planetary nebula.

Steve Coe, observing with a 13” f/5.6, notes: “Pretty bright, very small, not brighter in the middle, round, about twice the size of the Airy disk at 220X.”

NGC 6540
Cr 364
RA 18:06:07
Dec -27°45.8'
Open cluster

Discovered in 1784 by William Herschel (H II-198) “Pretty faint, not large, crookedly extended, easily resolvable.”

Harrington notes that this open cluster is “all but ignored by casual deepsky observers. You'll probably need an 8-inch telescope just to find it, and larger instruments are required to see any inner detail. My 13.1-inch f/4.5 Newtonian at 214x discloses only an arc of a half dozen faint stars amid the subtle glow of unresolved suns - not exactly an outstanding sight!”

Tom Lorenzin: “11M; 0.7' diameter! 10-plus 14M and dimmer members; another toughie! great in larger scopes; 30' due W is cluster N6520.”

LDN 122
Barnard 299
RA 18:06:24
Dec -27°24.6'
Dark nebula

IC 4678
ESO521-N*026
RA 18:06:32
Dec -23°57.5'
Bright nebula

NGC 6544
ESO521-SC028, GCL-87
RA 18:07:17
Dec -25°00.0'
Globular cluster

Discovered in 1784 by William Herschel (H II-197) “pB, pL, iR, r.”

Described in the NGC as considerably faint, pretty large and of irregular form with mottled appearance, the compact globular cluster lies “in a beautiful field sown profusely with stars”, according to Hartung.

Tom Lorenzin: “9M; 1' diameter; faint and small; 50' off SE edge of M-8.”

8-inch f/6.7 Newtonian, 9.7mm Super Plossl: “Very faint. Requires medium to high power.” (suburban skies) [GG]

12-inch Meade, 40mm eyepiece, 53’ fov: Similar in appearance to NGC 6528. Small faintly starlike, roundish with no stars and lanes. Small stars scattered around in a medium starfield. [MS]

NGC 6546
Cr 365
RA 18:07:21
Dec -23°17.8'
Open cluster

h: “the middle of a great and rich cluster in the milky way.”

Tom Lorenzin: “8M; 13' diameter; large and scattered; 80-plus 11M and dimmer members.”

LDN 306
Barnard 304/301/297
RA 18:07:55
Dec -18°59.5'
Dark nebula

vdB 113

RA 18:08:36
Dec -21°26.0'
Open cluster

LDN 216
Barnard 302
RA 18:09:02
Dec -24°00.4'
Dark nebula

IC 4684
vdB 115, Bernes 8
RA 18:09:05
Dec -23°25.0'
Bright nebula

NGC 6554

RA 18:09:05
Dec -18°26.0'
UNK

The RNGC (Sulentic and Tifft 1973) notes that this is a nonexistent object. Their coded description reads NOCL S.

IC 4681
LBN 31
RA 18:09:08
Dec -23°26.1'
Bright nebula

LDN 212
Barnard 303
RA 18:09:08
Dec -24°07.4'
Dark nebula

IC 4685
ESO521-*N037, Bernes 7
RA 18:09:16
Dec -23°59.2'
Bright nebula

NGC 6553
ESO521-SC036, GCL-88
RA 18:09:17
Dec -25°54.0'
Globular cluster

Discovered in 1785 by William Herschel (H IV-012) “F, L, iR, inclining to meridian, 3 or 4' diameter, like a brush to a N.p. star but probably unconnected.”

h: “globular, vF, a little oval, vglbM, barely resolvable, stars 20m, one star 14m, diam in RA = 7.5 seconds.”

Burnham notes that this globular cluster “is one of the most difficult globulars to resolve, as the obscuration in the region appears to exceed 6 magnitudes!”

Hartung notes that “it appears as a rather faint haze just resolvable on occasion with a 12”. There is little central condensation and it is markedly elliptical, about 2' by 1.5', in a field sprinkled with stars.

Tom Lorenzin: “10M; 2' diameter; faint, small and elongated”

8-inch f/6.7 Newtonian, 9.7mm Plossl: “Very faint. It contains a star in the nnp border.” [GG]

12-inch Meade, 40mm eyepiece, 53’ fov.: “Eliptical globular cluster, just a patch hazy light of medium size with fringed edges. I could not make out any stars or lanes, just a faint star towards the edges of this globular cluster.” [MS]

IC 1274
LBN 33, Bernes 7
RA 18:09:28
Dec -23°44.0'
Bright nebula

NGC 6559
LBN 29, Bernes 7, RCW 146
RA 18:09:56
Dec -24°06.6'
Bright nebula

h: “vF, L, oblong, 5' long, 3' broad, place of a double star involved, 6 other stars near. Query, if involved.”

Gerd Bahr-Vollrath (Noosa Heads, Queensland, Australia) observing with an 8-inch f/12 SCT, writes in the The Webb Society Nebulae and Clusters Section Report No. 10, July 1992: “ [NGC 6559, IC 1274, IC 1275, IC 4684, IC 4685] This complex of faint nebulosity lies about one degree east of M8, and deep photographs reveal that it seems connected to its more prominent neighbour. Low magnifications and a UHC filter were necessary to see indistinct faint patches of nebulosity, most of which seem associated with groups of stars.”

Beverly Lynds (Astrophysical Journal Supplement, No 105, 1965) in her Catalogue of Bright Nebulae, notes that this nebula is bright, more promiment on the red POSS plate, and has a maximum size of 15' x 10'.

IC 1275
ESO521-N*041, Bernes 7
RA 18:09:58
Dec -23°50.0'
Bright nebula

NGC 6556

RA 18:09:58
Dec -27°31.0'
Nonexistent

h: “Cluster VI An oval patch comprised within limits of the field, barely resolvable into infinitely minute points, but which, without attention, appears as a great neb 15' long, 12' broad; hardly bM.”

The RNGC (Sulentic and Tifft 1973) notes that this is a nonexistent object. Their coded description reads NF S.

LDN 228
Barnard 90
RA 18:10:01
Dec -23°39.4'
Dark nebula

Terzan 12
ESO522-SC001
RA 18:12:13
Dec -22°44.7'
Globular cluster

Terzan 11
C1809-227
RA 18:12:30
Dec -22°44.9'
Globular cluster

NGC 6568
Cr 369
RA 18:12:44
Dec -21°37.7'
Open cluster

Discovered in 1786 by William Herschel (H VII-030) “a cluster of pS scattered stars, above 15' diameter.”

h: “cluster VIII, loose, scattered, fills field, is decidedly richer than any part of the milky way that has occured to-night.”

Tom Lorenzin: “8.5M; 13' diameter; 50-plus members; large, scattered group 35' SSW of 4M Mu SGR”

Steve Coe, observing with a 13” f/5.6, notes: “Pretty bright, large, pretty rich, somewhat compressed, 33 stars within 10 arcmin at 100X, a nice globular of pretty faint stars.”

NGC 6567
ESO590-PN008, PK011-00.02
RA 18:13:44
Dec -19°09.9'
Planetary nebula

Steve Coe, observing with a 13” f/5.6, notes: “Faint, very small, round at 220X. This small planetary could be seen at 150X, but higher powers made it stand out better. There is a 13th mag star about 1 arcmin east of the nebula.”

Tom Lorenzin: “11.5M; 11” x 7” extent; small smudge with diffuse edges.”

NGC 6573

RA 18:13:48
Dec -22°10.0'
Nonexistent

The RNGC (Sulentic and Tifft 1973) notes that this is a nonexistent object. Their coded description reads NOCL S.

Biur 5
ESO590-SC009, Markarian 38
RA 18:15:16
Dec -18°59.9'
Open cluster

LDN 326
Barnard 92
RA 18:15:30
Dec -18°11.0'
Dark nebula

This dark nebula is also known as Lynds 323, and lies in the Sagittarius Milky Way, about 0°.7 west and 0°.2 north of the bright open cluster Messier 24, within the Small Sagittarius Starcloud. To best view this nebula, choose a dark night when the Milky Way is very prominent, and use a RFT or large binoculars. Barnard describes it as a black spot extending 15' north-south and 9' east-west. Describing it as a fine example of a black spot, he writes: "Visual observations actually show, however, that the object is really feebly luminous." Barnard remarks that the nebula "was examined with the 40-inch telescope in July 1913" and very much resembles Barnard 133 in that both are black only by contrast.

Harrington notes that the Small Sagittarius Cloud "acts as a dazzling backdrop for two visually distinct patches of absorption nebulosity [B92 and B93]. B92 is the more prominent. Rated as opacity 6, it strikes most observers as an oval hole measuring 12' by 6'. Most amateur telescopes will reveal a lone 10th mag star in front of the cloud." He adds that it has sharp edges that clearly delineate it.

Steve Coe, observing with a 13” f/5.6, notes: “Large, prominent dark nebula on the NW edge of the Small Sagittarius Star Cloud. It can easily be seen in 10X50 binoculars.”

11x80: Round dark patch, on edge of M24 cloud. Readily seen. (suburban skies) [AS]

NGC 6583
Cr 370
RA 18:15:48
Dec -22°08.3'
Open cluster

Discovered in 1786 by William Herschel (H VII-031) “a cluster of vS and pretty compressed stars, considerably rich, 2' or 3' diameter.”

h: “oblong cluster, not v rich nor v comp, but well insulated, stars 12m, 5' long, 4' broad.”

Tom Lorenzin: “10M; 2' diameter; 35-plus 10M and dimmer members; small and condensed; looks like small, distant, poor GLOB; 1 degree SSE of 4M Mu SGR.”

The RNGC (Sulentic and Tifft 1973) notes that this is a 12.0 mag open cluster.

11x80: Although looking at the exact position, nothing resembling a small cluster here. Instead, a _vast_ starcloud at least two degrees across, nothing seperately condensed and outlined I would call an open cluster. (dark exurban skies) [AS]

LDN 198
Barnard 306
RA 18:15:52
Dec -25°44.0'
Dark nebula

Cr 469
ESO590-SC013
RA 18:16:14
Dec -18°15.8'
Open cluster

NGC 6578
ESO590-PN012, PK010-01.01
RA 18:16:16
Dec -20°12.2'
Planetary nebula

William P. Clarke (San Diego, California, USA) writes in the The Webb Society Nebulae and Clusters Section Report No. 10, July 1992: “Small, faint and just non-stellar. Some contrast enhancement with an O III filter. No central star seen (21-inch f/20, x140, x350).”

Steve Coe, observing with a 13” f/5.6, notes: “Faint, small, round, no central star even at 320X. This greenish planetary was recognized at 100X, it is about three times the size of the Airy disk. This observation was on a night I rated 8/10 for seeing and 10/10 for transparency.”

NGC 6589
LBN 46
RA 18:16:50
Dec -19°46.7'
Bright nebula

Beverly Lynds (Astrophysical Journal Supplement, No 105, 1965) in her Catalogue of Bright Nebulae notes that this nebula is bright, more prominent on the blue POSS plate and has a maximum size of 4' x 3'.

NGC 6590
LBN 43
RA 18:16:50
Dec -19°46.7'
Bright nebula

Beverly Lynds (Astrophysical Journal Supplement, No 105, 1965) in her Catalogue of Bright Nebulae notes that this nebula is bright, more prominent on the blue POSS plate and has a maximum size of 4' x 3'.

LDN 330
Barnard 93
RA 18:16:54
Dec -18°03.9'
Dark nebula

Barnard (Astrophysical Journal, January 1919) writes in his 'Notes on the Catalogue' that this cometary object "has a sharply defined black head 2' in diameter with a diffused tail 15' long running south." It lies near the northern edge of M24, the Small Sagittarius Starcloud.

Harrington notes that the Small Sagittarius Cloud "acts as a dazzling backdrop for two visually distinct patches of absorption nebulosity [B92 and B93]. ... Although nearly equal is size to B92, B93 proves more difficult to spot because of its lower contrast with the background. Unlike B92, which has sharp edges that clearly delineate it, B93 diffuses outward.

NGC 6595
Cr 371
RA 18:17:03
Dec -19°52.0'
Open cluster

IC 1283
IC 1284, Gum 78, RCW 153, LBN 47
RA 18:17:38
Dec -19°40.3'
Bright nebula

LDN 275
Barnard 308
RA 18:17:59
Dec -22°08.8'
Dark nebula

NGC 6603
Bennett 107a
Messier 24, Cr 374, Rb 129
RA 18:18:25
Dec -18°24.3'
Open cluster

Donald J. Ware: “Has sometimes been erroneously identified as M- 24. This cluster is a small and tightly gathered grouping of stars which is best seen through a telescope.”

The RNGC (Sulentic and Tifft 1973) notes that this is a 11.5 mag open cluster.

Phil Harrington (Sky & Telescope, July, 1992) writes: “... NGC 6603 appears as a rich, albeit faint, glow measuring 5' across and accented with a few feeble points of 14th mag light. Although most definitely an open cluster, the misty appearance of NGC 6603 has led more than a few observers to believe it's a globular. Only after closer examination with higher magnifications and larger apertures will the true nature of NGC 6603 be revealed.”

12-inch Meade, 40mm eyepiece, 53’ fov: “Cluster easy visible with well condensed bright stars in an elongated haziness. Relatively rich and busy starfield.” [MS]

AL 4
ESO522-SC016
RA 18:19:05
Dec -27°07.8'
Open cluster

LDN 338
Barnard 307
RA 18:19:07
Dec -17°48.7'
Dark nebula

NGC 6613
Messier 18, Cr 376
RA 18:19:53
Dec -17°06.0'
Open cluster

This open cluster was discovered by Messier in June 1764, and he wrote of it as “a cluster of small stars, a little below M17; surrounded by a slight nebulosity, Easier to see than M16... Appears nebulous in a 3.5 foot telescope; with a better telescope the stars can be seen... diam 5'“

In the Appendix to the 1912 'Scientific Papers of Sir William Herschel' this object is described as “1783, July 31, 20 feet telescope, About 20 large and several small stars irregularly scattered. 1784, June 22. A cluster of coarsely scattered large stars, not rich.”

Burnham says that M 18 is “among the minor objects in Sagittarius... little more than a loose grouping of about a dozen stars, the brighter members arranged in several coarse pairs, on a background flecked with countless faint star-points. Admiral Smythe says the field contains “a long and straggling assemblage of stars... The whole vicinity is very rich and there are several splendid fields about a degree to the south.” This latter reference is to M24. Burnham notes that Messier's impression of nebulosity “was doubtless due to the unresolved background of faint stars.. photographs do show a faint nebulosity enveloping the cluster, but this cannot be detected visually...”

Tom Lorenzin: “8M; 7' diameter; small and sparse; 12-plus 9 thru 10M members; raspberries!.”

11x80: Looks like a round globular cluster with several stars; compact cluster, small but bright. Milky Way here very rich, especially M24 to the south. (suburban skies) [AS]

6-inch f/8.6 Newtonian: This cluster has about 20 stars in all, the three brightest lying in a short bow NE-SW. This row marks the edge of the cluster, the other, fainter members lying to the south and east. The surrounding field is very busy and has several 8-9th mag stars. The cluster is pB, pS, iF and I estimate the Trumpler class to be III 3 m. (suburban skies) [AS]

NGC 6620
ESO522-PN022, PK005-06.01
RA 18:22:52
Dec -26°18.2'
Planetary nebula

Tom Lorenzin: “14M; 5” diameter; small and very, very faint; much brighter core; like star with attendant fuzz; not as tough as M-estimate would lead one to believe; 12M star 2.5' to NNW.”

Steve Coe, observing with a 13” f/5.6, notes: “Faint, very, very small, not brighter in the middle and round at 220X. This tiny greenish disk is about 3 times the size of the seeing disk on a good night.”

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"Deepsky Observers Companion" (http://www.global.co.za/~auke) Copyright 1998 Auke Slotegraaf. All rights reserved. Uranometria 2000.0 copyright (c) 1987-1996 Willmann-Bell, Inc. Page last updated 1998 April 05