This is a map of the universe within 500 million light years. It shows most of the major galaxy superclusters that surround the Virgo supercluster. These superclusters are not isolated in space but together with many other smaller concentrations of galaxies they form parts of extensive walls of galaxies surrounding large voids. Three of the biggest walls near us are marked on the map as well as several of the largest voids. There are several hundred thousand large galaxies within 500 million light years, so even on this scale our galaxy is a very insignificant object. There is a negative version of this map, which might be easier to print.
This is a list of the nearest rich clusters of galaxies listed in the Abell catalogue. These are clusters of galaxies which contain many tens or hundreds of large galaxies. I also added the Virgo cluster to this list - George Abell excluded it from his catalogue because it covered too large an area of the sky to appear on a single photographic plate.
The Nearest Abell Clusters ~~~~~~~~~~~~~~~~~~~~~~~~~~~~ 1 2 3 4 5 6 7 8 9 Abell Equatorial Supergalactic R Redshift Distance Supercluster Number Coordinates Coordinates Mly Membership RA Dec L° B° (H=70) Virgo 12 29.6 +11 49 103.3 -2.8 1 .0037 52 Virgo A3526 12 48.9 -41 18 156.4 -11.4 0 .0102 142 Centaurus A3565 13 36.7 -33 58 151.8 -0.4 1 .0111 154 Centaurus A1060 10 36.9 -27 32 139.4 -37.5 1 .0114 158 Hydra A3627 16 15.5 -60 54 188.1 +7.1 1 .0145 201 A3574 13 49.2 -30 18 149.2 +3.3 0 .0148 205 Centaurus A262 01 52.8 +36 09 335.0 -2.0 0 .0151 209 Perseus-Pisces A3742 21 06.7 -47 09 229.7 +20.5 0 .0152 211 Pavo-Indus A426 03 18.6 +41 31 347.7 -14.1 2 .0167 231 Perseus-Pisces A194 01 25.6 -01 30 297.1 -7.8 0 .0168 233 A347 02 25.8 +41 52 342.8 -5.5 0 .0172 238 Perseus-Pisces A3656 20 00.5 -38 32 221.8 +33.6 0 .0178 246 Pavo-Indus A3698 20 36.0 -25 17 237.8 +42.2 1 .0188 260 Pavo-Indus A569 07 09.2 +48 37 29.1 -25.6 0 .0189 262 A1367 11 44.5 +19 50 92.2 -10.5 2 .0208 288 Coma A779 09 19.8 +33 46 60.9 -29.7 0 .0217 300 A3581 14 07.5 -27 01 147.6 +8.3 0 .0218 301 Centaurus A1656 12 59.8 +27 59 89.6 +8.2 2 .0219 303 Coma A2870 01 07.7 -46 55 251.0 -13.5 0 .0225 311 Phoenix A400 02 57.6 +06 02 312.0 -27.4 1 .0232 320 A2877 01 09.8 -45 54 252.1 -13.8 0 .0235 324 Phoenix A634 08 14.6 +58 03 37.2 -14.4 0 .0253 349 A3389 06 21.8 -64 58 211.0 -40.4 0 .0255 352 A2666 23 50.9 +27 09 320.0 +21.1 0 .0260 358 A2806 00 40.2 -56 10 240.9 -11.0 0 .0265 365 Phoenix A539 05 16.6 +06 27 336.9 -57.1 1 .0272 375 A2199 16 28.6 +39 31 72.4 +50.2 2 .0287 395 Hercules(a) A2836 00 53.7 -47 37 249.9 -11.3 0 .0288 397 Phoenix A4038 23 47.7 -28 08 264.7 +6.8 2 .0288 397 A2197 16 28.2 +40 54 70.5 +49.5 1 .0296 407 Hercules(a) A3747 21 08.7 -43 30 232.3 +23.4 0 .0298 410 A2634 23 38.3 +27 02 319.5 +23.9 1 .0298 410 A2731 00 10.2 -56 59 239.1 -7.2 0 .0300 413 Phoenix A1177 11 09.5 +21 42 87.1 -17.3 0 .0304 418 Leo A2896 01 18.3 -37 06 261.3 -14.0 0 .0306 421 Phoenix A3537 13 01.0 -32 26 148.2 -7.1 0 .0308 424 A1016 10 27.0 +10 59 92.8 -31.1 0 .0310 426 Leo A2162 16 12.5 +29 32 88.9 +50.3 0 .0310 426 Hercules(a) A999 10 23.4 +12 51 90.4 -31.1 0 .0311 428 Leo A1185 11 10.8 +28 41 80.8 -13.9 1 .0313 430 Leo A397 02 57.0 +15 57 322.0 -23.3 0 .0315 433 A189 01 23.7 +01 39 300.0 -6.5 1 .0316 434 A496 04 33.6 -13 15 295.9 -55.7 1 .0317 436 A1267 11 27.9 +26 51 84.1 -11.3 0 .0317 436 Leo A3390 06 25.0 -37 21 222.1 -67.4 1 .0321 441 Columba A1314 11 34.8 +49 02 64.5 -0.7 0 .0323 444 A1257 11 26.1 +35 19 76.2 -8.1 0 .0332 456 Leo A1142 11 00.9 +10 33 97.1 -23.7 0 .0337 463 Leo A2052 15 16.8 +07 00 119.2 +36.0 0 .0338 464 Hercules(b) A2147 16 02.3 +15 54 110.0 +48.5 1 .0338 464 Hercules(b) A1228 11 21.5 +34 20 76.7 -9.3 1 .0340 467 Leo A2063 15 23.0 +08 38 117.7 +37.8 1 .0341 468 Hercules(b) A3193 03 58.2 -52 20 240.0 -39.5 0 .0345 474 A3381 06 09.9 -33 36 234.0 -69.4 1 .0347 476 Columba A260 01 51.9 +33 10 332.1 -2.9 1 .0351 482 A1836 14 01.7 -11 36 132.5 +12.5 0 .0351 482 A2151 16 05.2 +17 45 107.3 +49.4 2 .0354 486 Hercules(b) A3570 13 46.8 -37 55 156.2 +0.2 0 .0354 486 Shapley A3664 20 14.0 -80 39 209.6 -6.9 1 .0357 490 A2995 02 15.2 -24 50 275.9 -24.4 1 .0360 494 A3575 13 52.6 -32 53 151.9 +3.1 0 .0365 501 Shapley |
Column 1: The Abell catalogue number of the cluster. Column 2: The Right Ascension in hours and minutes for epoch 2000. Column 3: The declination in degrees and minutes for epoch 2000. Column 4: The supergalactic longitude. Column 5: The supergalactic latitude. Column 6: The 'richness class' of the cluster. Roughly, this is the number of the very brightest galaxies in the cluster: 0 = 30-49 galaxies, 1 = 50-79 galaxies, 2 = 80-129 galaxies. Column 7: The redshift of the cluster relative to the cosmic microwave background. Column 8: The distance to the cluster in millions of light years assuming that the Hubble constant is 70 km/s/Mpc. Column 9: The supercluster the cluster belongs to. References: Abell G, Corwin H, Olowin R, (1989), A catalogue of Rich Clusters of Galaxies, Astrophys J Supp, 70, 1. Struble M, Rood H, (1999), A compilation of redshifts and velocity dispersions for ACO clusters, Astrophys J, 125, 35.
The best introduction to the subject of superclusters is this book 'Large-Scale Structures in the Universe' by Anthony Fairall, (Wiley, 1998). It is an introductory textbook which explains both the history and the future of the entire subject and also contains many accurate (two-dimensional) maps of the distribution of galaxies in the nearby universe. Some examples of his galaxy plots can be seen in this paper written by him and five colleagues in 1990.
One useful aspect of Anthony Fairall's book is that he lists many of the major voids in the local universe. This is a list of voids adapted from his list. Some of these voids are labelled on the above map and most of the nearer voids are marked on the 200 million light years map.
1 2 3 4 5 6 7 8 Void Name Equatorial Supergal. Redshift Dist. Diam. Coordinates Coordinates z Mly Mly RA Dec L° B° Local Void 18.0 -10 178 +61 0.0050 70 140 Delphinus 20.0 +20 314 +74 0.0083 115 140 Eridanus 1.0 0 297 -1 0.0083 115 185 Corvus 12.0 -15 128 -17 0.0100 140 115 Gemini 6.0 +40 14 -33 0.0100 140 115 Virgo 13.5 +10 109 +11 0.0100 140 115 Cygnus 20.5 +25 323 +66 0.0117 165 115 Leo 10.5 +30 75 -21 0.0117 165 140 Taurus 3.5 +20 330 -28 0.0133 185 185 Aquila 22.0 0 282 +42 0.0150 210 140 Microscopium 18.0 -20 185 +52 0.0150 210 160 Canis Major 6.5 -20 260 -83 0.0167 235 230 Coma Berenices 13.5 +15 104 +12 0.0167 235 140 Hydra 12.0 -30 143 -19 0.0167 235 140 Corona Borealis 17.0 +35 74 +58 0.0173 240 185 Pegasus 22.0 +15 302 +45 0.0183 255 140 Sculptor 0.5 -35 261 -4 0.0183 255 275 Ursa Minor 19.0 +85 26 +21 0.0183 255 230 Ursa Major 9.0 +50 47 -19 0.0200 280 140 Columba 4.0 -30 269 -48 0.0217 305 230 Pisces 1.0 +15 311 +3 0.0233 325 140 Apus 20.0 -75 211 -1 0.0250 350 230 Fornax 2.0 -25 275 -21 0.0267 375 230 Capricornus 19.0 -35 208 +39 0.0284 395 230 |
Column 1: A name for the void. Column 2: The Right Ascension in hours for epoch 2000. Column 3: The declination in degrees for epoch 2000. Column 4: The supergalactic longitude. Column 5: The supergalactic latitude. Column 6: The approximate redshift of the centre of the void. Column 7: The distance to the centre of the void in millions of light years assuming that the Hubble constant is 70 km/s/Mpc. Column 8: The approximate diameter of the void in millions of light years.