| 105 Finest Objects For The LX200 by Nigel Puttick | ||||||
| # | Object | Const | Keypad | (Mag)/[Sep] | Type of Object | Description |
| 1 | M81 | UMa | M81 | 8 | Spiral galaxy | M81's bright core and fainter outer parts can be seen in a 10-inch scope at 80x. 1. |
| 2 | M82 | UMa | M82 | 9 | Irregular galaxy | M82 is the nearby spindle-shaped companion of M81. Dark lanes are visible in a 10-inch. 2. |
| 3 | Gamma | Leo | *296 | (3,4)[4.5"] | Double star | Gamma Leonis is a beautiful yellow pair, 4.5-seconds apart, easily split in a 3-inch. 3. |
| 4 | NGC3242 | Hya | NGC3242 | 9 | Planetary nebula | NGC3243 is one of the brightest and easiest of all planetary nebulae. Visible as a blue disk in a 3-inch at 90x. |
| 5 | Xi | UMa | *297 | (4,5)[2.5"] | Double star | Xi Ursa Majoris forms a tight white pair (2.5-seconds) in a 6-inch. |
| 6 | Delta | Crv | *123 | (3,8)[24"] | Double star | Delta Corvi is a wide (24-second) pair, white and lilac, in colour. |
| 7 | 24 | Com | *302 | (5,7)[20"] | Double star | 24 Coma Berenices, a 20-second pair show orange and blue-green stars, vivid in larger scopes. |
| 8 | M104 | Vir | M104 | 9 | Spiral galaxy | M104, the Sombrero galaxy, shows the dark equatorial band in a 13-inch at 190x. Small instruments show only a hazy ellipse. |
| 9 | Gamma | Vir | *303 | (4,4)[5"] | Double star | Gamma Virginis, one of the best-known binary stars, has a white pair of nearly the same magnitude, nearly 5-seconds apart. |
| 10 | Gamma | CVn | SAO44317 | (5-7) | Red star | Y Canum Venaticorm has a deep orange colour, particularly intense in small apertures. |
| 11 | M94 | CVn | M94 | 8 | Spiral galaxy | M94 is a very bright galaxy, round and featureless in small instruments, but easy to see. |
| 12 | Alpha | CVn | *133 | (3,5)[20"] | Double star | Cor Caroli, a 20-second blue-white double, is one of the best for small scopes. |
| 13 | M64 | Com | M64 | 9 | Spiral galaxy | M64, the Blackeye galaxy, large and bright, needs a 6-inch to see the dark central patch which gives rise to its nickname. |
| 14 | Zeta | UMa | *305 | (2,4)[15"] | Double star | Mizar is a fine double, its components, both white, 15-seconds apart, while Alcor is 12-minutes away. Excellent for comparing what the naked eye can see with what the telescope reveals. |
| 15 | M51 | CVn | M51 | 8 | Spiral galaxy | M51, the Whirlpool galaxy, shows hints of its spiral structure in a 10-inch at 80x. Its closecompanion, NGC5195, gives the appearance of a double nebula in wider fields of view. |
| 16 | M3 | CVn | M3 | 6 | Globular cluster | M3 is the first bright globular cluster of the spring skies. It is partly resolved in a 6-inch and completely so in a 13-inch. |
| 17 | Epsilon | Boo | *311 | (3,5)[3.5"] | Double star | Epsilon Bootis, a 3.5-second pair, has yellow primary and a blue secondary. They can be split in good seeing with a 3-inch. |
| 18 | Xi | Boo | *312 | (5,7)[7"] | Double star | Xi Bootis, a yellow and red visual binary, (7-seconds) are easily split with modest instruments. |
| 19 | M5 | Ser | M5 | 6 | Globular cluster | M5, a marvelous object in a 10-inch, rivals M13. |
| 20 | Mu | Boo | *316 | (4,7,8)[2"] | Triple star | Mu Bootis is a fine triple star, being a wide double (108-seconds) whose fainter member is a close 2-second pair. |
| 21 | Delta | Ser | *317 | (4,5)[4"] | Double star | Delta Serpentis offers a fine white pair for a 3-inch. Separation is 4-seconds. |
| 22 | Zeta | CrB | *318 | (5,6)[6"] | Double star | Zeta Coronae Borealis a 6-second double consisting of nearly equally bright bluish and greenish stars. Colours definite in a 6-inch. |
| 23 | Xi | Sco | *319 | (-)[1,8,12"] | Quintuple star | Xi Scorpii is triple, part of a multiple system, a 1-second pair with another 8-seconds away. In the same field is the 12-second pair, Struve 1999. A 3-inch shows only four stars, a 6-inch at least is needed to split the close pair. |
| 24 | Beta | Sco | *172 | (3,5)[14"] | Double star | Beta Scorpii resembles Mizar, being a 14-second blue-white pair. It makes for an interesting colour comparison with Antares. |
| 25 | Nu | Sco | SAO159764 | (4,6,7,8) | Quadruple star | Nu Scorpii is a colourful double-double, a 2-second pair and a 1-second, 42-seconds apart. A 6-inch at least is needed to resolve all four stars. |
| 26 | M4 | Sco | M4 | 6 | Globular cluster | M4 is large and easily resolved, best seen in larger instruments. These show many faint stars in apparent chains, giving a feeling of dark lanes crossing the cluster. |
| 27 | Alpha | Sco | Antares | (1,6)[3.5"] | Double star | Antares is a beautiful, unequal double star, red and emerald green. Because it is only 3.5-seconds away and much fainter, the companion is difficult in 6 to 8-inch scopes. Even though it may not be resolved, the companion will show a green tinge to one si |
| 28 | 16-17 | Dra | SAO30012 | (6,6,7)[1.5'] | Triple star | 16 and 17 Draconis, 1.5-minutes apart form a triple, the brighter components are nearly equal, and the primary has a close companion. |
| 29 | M13 | Her | M13 | 6 | Globular cluster | M13, the finest northern globular cluster, hints at resolution in a 3-inch and resolves well in a 6-inch. |
| 30 | NGC6210 | Her | NGC6210 | 10 | Planetary nebula | NGC6210 is a small but bright planetary nebula showing a featureless blue disk in smaller scopes. |
| 31 | M12 | Oph | M12 | 7 | Globular cluster | M12 and |
| 32 | M10 | Oph | M10 | 7 | Globular cluster | M10 are similar globular clusters only a few degrees apart, the best of many in Ophiuchus. They appear granular in a 4-inch and can be resolved in a 10-inch. |
| 33 | Alpha | Her | *327 | (3,5)[4.5"] | Double star | Alpha Herculis consists of an intensely coloured orange and blue-green pair, 4.5 seconds apart. |
| 34 | Delta | Her | *191 | (3,9)[9"] | Double star | Delta Herculis, colours white and purple, is an optical 9-second pair. |
| 35 | M92 | Her | M92 | 6 | Globular cluster | M92 is a globular with a bright center. Often overlooked because of its neighbour, M13. Easily seen in a 3-inch. |
| 36 | Rho | Her | *328 | (5,5)[4"] | Double star | Rho Herculis, a 4-second double, is attractive even in small scopes. |
| 37 | Nu | Dra | SAO30447 | (5,5)[62"] | Double star | Nu Draconis. A pair of perfectly matched white stars of equal brightness separated by 62 seconds. |
| 38 | M6 | Sco | M6 | 5 | Open cluster | M6 is a large, bright cluster of scattered stars. This and the next two objects need a low-power, wide-field view of at least 0.5 degrees to be appreciated. |
| 39 | M7 | Sco | M7 | 3 | Open cluster | M7, a large, very bright open cluster, is easily resolved in a 3-inch at 45x. |
| 40 | M23 | Sgr | M23 | 7 | Open cluster | M23 is a large, uniform, and fairly rich open cluster, striking in an 8/10-inch at 150x. |
| 41 | NGC6543 | Dra | NGC6543 | 9 | Planetary nebula | NGC 6543, a bright blue-green ring, has an 11th-magnitude central star, just visible in a 3-inch. A fine object in an 8-inch or larger scope. |
| 42 | 95 | Her | *329 | (5,5)[6"] | Double star | 95 Herculis is a 6-second pair of bright stars, pale red and pale green in colour. |
| 43 | M8 | Sgr | M8 | (?) | Diffuse nebula | M8, the Lagoon nebula, appears as a nebulous patch traversed by a large dark lane and a scattered open cluster to one side. A 3-inch shows all but the dark lane, for which a larger scope is needed. |
| 44 | 70 | Oph | *331 | (4,6)[3"] | Double star | 70 Ophiuchi has a present separation of 3 seconds. The colours, yellow and red, are strong at 150x. |
| 45 | NGC6572 | Oph | NGC6572 | 10 | Planetary nebula | NGC 6572, a small, bright, blue planetary, looks like a star in a 4-inch. Colour is intense in larger scopes. |
| 46 | M17 | Sgr | M17 | (?) | Diffuse nebula | M17, the Swan or Omega nebula, can been easily seen in a 3-inch. The Milky Way background is quite rich here. |
| 47 | M22 | Sgr | M22 | 6 | Globular cluster | M22 is rated by the authors as the finest globular cluster in the northern hemisphere after M13. It is easily resolved to the center in a 10-inch. |
| 48 | Alpha | Lyr | Vega | (0,10?)[1'] | Double star | Vega is a dazzling blue-white diamond. About 1 minute of arc to the south lies a faint companion, difficult to see in less than a 6-inch. |
| 49 | Epsilon | Lyr | *334/5 | (5,5,5,6) | Quadruple star | Epsilon Lyrae, the famous double-double, is the finest multiple star in this list. Both close pairs, 2.3 and 2.6 seconds apart, can just be resolved in a 3-inch. |
| 50 | M11 | Sct | M11 | 6 | Open cluster | M11, the Wild Duck cluster, is the finest open cluster north of -40 degrees for large instruments, yet easily resolved in a 4-inch. Very rich and compact, it has a bright star near its center. |
| 51 | M57 | Lyr | M57 | 9 | Planetary nebula | M57, the famous Ring nebula, rates as the authors' finest planetary. Its central hole is seen at 100x in a 3-inch. The faint central star needs a large scope to be seen. |
| 52 | Theta | Ser | SAO124068 | (4,5)[23"] | Double star | Theta Serpentis is an easy pair of white stars, separated by 23 seconds. |
| 53 | Beta | Cyg | Albireo | (3,5)[35"] | Double star | Alberio is a beautiful 35-second pair, orange and blue. These colours are much more vivid in smaller scopes. |
| 54 | M55 | Sgr | M55 | (6?) | Globular cluster | M55 is a large, rich globular, but so far south that it reqires a first-class night for a good view. To be seen as more than a hazy patch needs a larger scope. |
| 55 | NGC6818 | Sgr | NGC6818 | 10 | Planetary nebula | NGC 6818 appears as a bright, uniform, blue disk in a 13-inch. In common with other planetaries, it is starlike in small scopes at low power. |
| 56 | Delta | Cyg | *224 | (3,6)[2"] | Double star | Delta Cygni offers a close (2-second) binary which needs a 6-inch in good seeing to be split. The primary is white, the companion blue-white. |
| 57 | NGC6826 | Cyg | NGC6826 | 9 | Planetary nebula | NGC 6826 is sometimes called the "blinking planetary." It consists of a pale blue disk with an 11th magnitude central star. Looking exactly at the star, the nebula disappears; while looking with averted vision causes the star to disappear in the nebulosit |
| 58 | M27 | Vul | M27 | 8 | Planetary nebula | M27, the Dumbell nebula, is large and bright, pinched near the middle in 4-inch at 40x. |
| 59 | Gamma | Del | *342 | (4,5)[10"] | Double star | Gamma Delphini, a 10-second pair, appears delicately coloured yellow and pale green. |
| 60 | NGC7009 | Aqr | NGC7009 | 8 | Planetary nebula | NGC 7009, the Saturn nebula, is a very bright, blue-green, featureless elliptical disk. The appendages that give rise to the name are not visible even in a 30-inch reflector. |
| 61 | 61 | Cyg | *346 | (6,6)[28"] | Double star | 61 Cygni, a famous long-period binary star, has orange components 28 seconds apart. |
| 62 | M15 | Peg | M15 | 6 | Globular cluster | M15. This bright and very compact globular is not completely resolved in a 13-inch refractor at 190x. |
| 63 | Beta | Cep | *236 | (3,8)[14"] | Double star | Beta Cephei offers an unequal 14-second double of blue-white stars. |
| 64 | M2 | Aqr | M2 | 6 | Globular cluster | M2, a very rich swarm, appears as a hazy patch in a 3-inch. |
| 65 | Mu | Cep | SAO33693 | (4-5) | Red star | Mu Cephei, long-famed as Herschel's garnet star, is a semi-regular, variable super giant. It is almost red in a 3-inch, deep orange in an 8-inch, and yellow-orange in a 13-inch. |
| 66 | Zeta | Aqr | *347 | (4,5)[1.4"] | Double star | Zeta Aquarii is a fine, 1.4-second binary. Both stars are white. |
| 67 | Delta | Cep | *348 | (4,8)[41"] | Double star | Delta Cephei, a 41-second pair, is easily split in a 3-inch. The colours are pale orange and white. |
| 68 | NGC7662 | And | NGC7662 | 9 | Planetary nebula | NGC 7662 is a small blue dot in a 6-inch and a bright blue perforated disk with a 13-inch. |
| 69 | 19 | Psc | SAO128374 | 5 | Red star | 19 (TX) Piscium has a very red colour, apparent in all apertures. |
| 70 | M31 | And | M31 | 5 | Spiral galaxy | M31. The great Andromeda galaxy is finest representative of its class. Scopes up to 6-inch show a bright, hazy, featureless ellipse. Some dark structure can be seen in a 13-inch and larger. |
| 71 | NGC253 | Scl | NGC253 | (9?) | Spiral galaxy | NGC 253 looks somewhat like M31, but smaller. |
| 72 | Eta | Cas | SAO21732 | (4,8)[10"] | Double star | Eta Cassiopeiae has yellow and reddish-purple components which are about 10-seconds apart. |
| 73 | Gamma | Ari | *264 | (5,5)[9"] | Double star | Gamma Arietis is a pair of equally bright white stars, 9 seconds apart. They are easily seen in a 3-inch. |
| 74 | Alpha | Psc | *265 | (4,5)[3"] | Double star | Alpha Piscium is a tight, white pair, 3 seconds apart. |
| 75 | Gamma | And | *266 | (2,5,6)[10"] | Triple star | Gamma Andromedae is one of the finest coloured doubles, orange and blue. At 10 seconds separation, it is visible in all apertures. |
| 76 | NGC869 | Per | NGC869 | 4 | Open cluster | NGC 869 and |
| 77 | NGC884 | Per | NGC884 | 5 | Open cluster | 884 make up the double cluster in Perseus. Rated as the finest open clusters for small telescopes, they are superb in many. Contrasting star colours are discernible in larger scopes. |
| 78 | Iota | Cas | *269 | (5,7,8)[3,7"] | Triple star | Iota Cassiopeiae is a fine triple, with blue-white companions 2.5 and 7 seconds from the yellowish primary. Scopes 6-inch and above are needed. |
| 79 | Gamma | Cet | *271 | (4,6)[3"] | Double star | Gamma Ceti. Atractive close (3-second) pair. |
| 80 | Theta | Eri | *21 | (3,4)[9"] | Double star | Theta Eridani, although very close to the horizon at our latitude, is a brilliant pair of white stars 9 seconds apart. |
| 81 | 32 | Eri | *277 | (5,6)[7"] | Double star | 32 Eridani's components are yellow and blue-green, separated by about 7 seconds. Colour contrast is vivid in medium to larger scopes. |
| 82 | NGC1535 | Eri | NGC1535 | 9 | Planetary nebula | NGC 1535 is a small, pale blue-green disk with a faint central star. A 6-inch at 100x shows it but not the star; a 13-inch reveals both. |
| 83 | Beta | Ori | Rigel | (0,7)[10"] | Double star | Rigel is a blue-white star with a white, much fainter companion 10 seconds away. It is just resolved in a 3-inch. |
| 84 | Eta | Ori | *43 | (4,5)[1.5"] | Double star | Eta Orionis, a bright white pair only 1.5 seconds apart, needs a 10-inch for separation. |
| 85 | Lambda | Ori | *285 | (4,6)[5.5"] | Double star | Lambda Orionis is a 5.5-second pair of white stars. |
| 86 | Theta | Ori | *286 | (-) | Multiple star | Theta Orionis. This beautiful multiple system is embedded in the Orion nebula. Six components are visible in a 4-inch. |
| 87 | M42 | Ori | M42 | (?) | Diffuse nebula | M42, the Orion nebula, is the finest difuse nebula in this survey- a magnificent sight! Even a 3-inch reveals darker areas and long filaments in this bright green nebulosity. |
| 88 | Iota | Ori | *49 | (3,7)[12"] | Double star | Iota Orionis, a 12-second pair, is a fainter version of Rigel, with a hint of dim nebulosity. In the same field is the double Struve 747. |
| 89 | Sigma | Ori | SAO132406 | (4,6,7,10) | Multiple star | Sigma Orionis is a multiple star, three components being easily seen in a 3-inch, four in a 6-inch. The bright star has a very difficult close (0.3 second) companion. |
| 90 | Zeta | Ori | *53 | (2,4,9)[2.5"] | Triple star | Zeta Orionis has a bright close (2.5 second) companion and a distant faint one, all three being blue-white. |
| 91 | M37 | Aur | M37 | 6 | Open cluster | M37 is the finest of the great open clusters in Auriga. It is rich and uniform, resolved in a 4-inch at 40x, and has an orange star near its center. |
| 92 | Theta | Aur | *58 | (3,8)[3"] | Double star | Theta Aurigae, a very unequal, close (3-second) pair; difficult in any scope much smaller than 10 inches. |
| 93 | M35 | Gem | M35 | 5 | Open cluster | M35, a large, uniform, and bright star cluster, needs at least a 30-minute field for a good view. |
| 94 | Beta | Mon | *287 | (5,5,6)[10"] | Triple star | Beta Monocerotis is the finest triple star in the list. The components, all yellow-white, form a triangle of 10-seconds greatest extent. Easy in a 6-inch. |
| 95 | UU | Aur | SAO59280 | (5-7) | Red star | UU Aurigae is a bright, very red carbon star, more vivid in an 8-inch than in a 13-inch. |
| 96 | 12 | Lyn | SAO25939 | (5,6,8) | Triple star | 12 Lyncis is a triple system, nice in a 6-inch. |
| 97 | Alpha | CMa | Sirius | (-1,9) | Double star | Sirius, the brightest star other than the sun, dazzles the eye with its blue-white brilliance. Under excellent conditions, the white dwarf companion can just be seen in an 8-inch at 280x. |
| 98 | Delta | Gem | SAO79294 | (4,8)[7"] | Double star | Delta Geminorum is a 7-second pair with yellow and reddish-purple components. |
| 99 | NGC2392 | Gem | NGC2392 | 8 | Planetary nebula | NGC 2392 is a vivid blue planetary nebula with a bright central star. It is easy with a 6-inch at 100x, and a 13-inch at 600x permits dark structures in the disk to be glimpsed with averted vision. |
| 100 | Alpha | Gem | Castor | (2,3,10)[1',2"] | Triple star | Castor. The two very bright, blue-white stars form a close binary whose separation is just under 2-seconds. The faint third star, a minute of arc away, is orange and just visible in a 3-inch at 150x. |
| 101 | Kappa | Pup | SAO174198 | (4,5)[10"] | Double star | Kappa Puppis, easy in a 3-inch, is a 10-second pair of white stars. |
| 102 | M46 | Pup | M46 | 9 | Open cluster | M46 is a uniform cluster of faint stars. On its northern edge is NGC 2438, a dim ring nebula visible in a 10-inch. |
| 103 | Zeta | Cnc | *293 | (6,6,6)[6"] | Triple star | Zeta Cancri is an attractive but difficult triple. A 4-inch shows only two components about 6 seconds apart. The three, all yellow, are well resolved in a 10-inch at 320x. |
| 104 | Iota | Cnc | SAO80416 | (4,7)[31"] | Double star | Iota Cancri is an orange star with a blue neighbour 31 seconds away. |
| 105 | M67 | Cnc | M67 | 6 | Open cluster | M67 is a rich swarm of rather faint stars, resolved in a 4-inch, is a fine sight in a 6-inch. |