Knowledge (XXG)

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890:
broadcast and a narrow-beam broadcast. If we tried to send a signal out (using our most powerful transmitter) in a tiny, narrow beam, aimed specifically at one particular star - then we could put out enough energy for the aliens to detect. However, our radio, TV, cellphone, etc traffic is spread all over the sky. Consider a 1 arc-second-wide narrow beam - it's something like 360x60x60x180x60x60x2 = 1,700,000,000,000...1.7 trillion times more powerful than an omnidirectional beam because all of the energy is focussed down that narrow 'slot'. But the trouble is that with a 1 arc-second beam - you could only talk to one reasonably close star at a time. Whilst we've been putting out omnidirectional signals for a long time - we've only tried sending such a narrow (and hence appropriately powerful) beam a few times. There has been no effort to try narrow-casting signals at nearby stars on a regular basis. Doing it for just a few seconds per star isn't really enough for the aliens to get a 'fix' on us - and it's not enough for use to transmit a useful amount of information. We would need a fairly major engineering program to set up enough narrow-field/high-power transmitters to transmit for long periods to all of the nearby stars.
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might produce), we have no hope...as I indicated. Assuming this is 'first contact', either we have to be able to pick up an omnidirectional broadcast from some unsuspecting alien - or he/she/it is going to have to pick up an omnidirectional broadcast from us. Once that initial detection is made - we could chat happily (but S-L-O-W-L-Y) via some kind of narrow-beam link. But if their (omnidirectional) transmitters are only as powerful as the best we can manage - or if their radio telescopes are no better than our best - then we're all going to be blissfully unaware of each other no matter how close we happen to be.
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theology - just because there is no intelligent life out there sending signals we can detect doesn't mean there isn't any intelligent life out there, they could just have better things to do with their time and energy than send out random signals. We aren't currently sending out any signals that we could detect if they had come from another star, so there is no reason to assume other civilisations will be. Things may improve as our search of
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diminished. All of this is because you know there actually was a Hoffa to begin with. You can't make any conclusions on the lack of SETI success—there's no way to distinguish the many possible reasons for that (there are no aliens; aliens can't communicate with us; they tried to and we didn't miss it; we're looking in the wrong place; we're looking in the wrong way; etc.). Which in my opinion is not encouraging. --
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on a universe-wide scale, that we are actively looking for them). This does not reflect, though, on whether there are extra-terrestrial intelligences out there—it just reflects on our limited means of detecting them. Personally I think there is very limited scientific justification for something like SETI, but that fact has no implications on science or theology in general. --
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Sorry, I don't buy it. I think the SETI money could be spent better elsewhere (for scientific research, even), and I think things like Seti@Home are a total waste of processing power that could otherwise be used for most practical projects (like protein folding). If we lived in a world where there were infinite resources, then sure. But we don't.
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has searched millions of radio channels over the entire sky, and has found no sign of any ETI life. Therefore, at least some of its original assumptions has been proven false. We know, for example, that ETI civilizations are not as prevalent as was once thought. This implies that either climates that
467:
I don't know that it seems probably it will continue to fail. It's a big sky and you need to be looking in just the right direction at just the right time - it could well be that we just haven't gotten lucky yet. Even if it continues to fail for the next 100 years, it doesn't mean much for science or
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Who assumed SETI would find what it was looking for in the first 48 years? Plenty of people may have hoped they would, but did anyone involved actually assume it? You've ignored the possibility of ETI that isn't blasting out powerful radio signals. If the SETI institute aren't looking any more, what
589:
The problem with SETI is that if you reframe it around activities that are not done by licensed scientists it sounds stupid. You might as well bring up perpetual motion machines as your example along with heavier-than-air—just because none of the plans have worked yet, and we have no reason to think
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The odds that SETI will ever detect anything is basically almost zero (we are looking for the tiniest needles in the biggest of haystacks, and needles that may have not even been put in a place where we could find them, have long since passed us by, or will not be around for the tiny window of time,
884:
It's certainly true that as our technology improves, our radio receivers get more sensitive and so there is no need to transmit with so much power. Hence the net output of our planet isn't increasing as much as you might hope. Worse still, we're adopting complex multiplexed digital signalling and
838:
Oh, we're transmitting locally all right, but as multiple people have pointed out above, our transmitters are barely up to the task of interstellar transmission, assuming anyone would even bother to set one up for such a purpose (which, I might add, was the point of my question). Do you know of any
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And you have to study each bit of sky at a wide range of wavelengths. And then there are stars that have currently been ruled out as very unlikely to harbour life, but ought to be checked at some point just in case. And then there are other galaxies that it might be worth having a look at (although
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However, that's limited only by 8bits-per-color computer graphics cards. Some fancy setups can do 10 bits or more per component. There are laser projectors that can do 16 bits per component. Those permit VASTLY more subtle colors - and pinks that are so amazingly subtly different from pure white
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continues - if we find some planets that look habitable by life as we know it then we can carefully listen to them (and maybe even beam signals to them) and might stand a chance of hearing something. Listening pretty much at random (there is some science to where they point the receivers, but it's
755:
Yes and no. That's only true because using the Arecibo telescope as a transmitter would produce a very narrow beam of radio waves - you'd pretty much have to aim it at a particular star and push all the energy down that narrow beam. For omnidirectional broadcasting (such as - say - a TV station
508:
There are lots of things which have not worked as yet, but that does not mean we abandon them. There were some rather long odds on other events which turned out to be quite real; people a century ago thought heavier-than-air flight was technologically impossible, and yet here we are today. SETI
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designed signalling system would sound like)...which makes it less and less likely that the aliens would realise we're sending intelligent signals at all. It's not like we're sending a bunch of prime numbers in morse code! But the key here is to note the difference between an omnidirectional
585:
Let me make an analogy. SETI, to me, is like making a giant bucket for your backyard—at some expense—in order to catch a meteorite in it. Would this be a reasonable endeavor? Operation Catch a Meteorite has so far been a failure... but that doesn't mean it won't succeed in the future, does it?
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make conclusions based on his lack of being found—even if they aren't specific ones. You can say, for example, that if someone killed him—as seems almost surely to be the case—they did a pretty good job of getting rid of him. You can also say that the ability of the FBI to find him is somewhat
343:
The complementary colour of a primary colour is a secondary colour. In the RGB system, the complement of blue is red+green=yellow. "Purple" isn't a primary or secondary colour, you probably mean magenta, which is red+blue, so its complement is green. Orange isn't a secondary colour, either, it
688:
The thing to bear in mind is this: If you took the most powerful radio transmitter than mankind has ever made - placed it in orbit around the nearest star to ours - then the most powerful radio telescope that humans have ever made would not be able to detect it. We have a LONG way to go.
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operates on a shoe-string budget, with meager resources, and it has a LOT of space to cover (well, ALL of it). I don't think its lack of data yet means much of anything. What fraction of known space has it analyzed? When that gets to 100%, then we can pronounce failure. --
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might be found from Pantone. Jarry1250 didn't quite get the numbers right: the lightest shade of pink you can display using an 8 bit per component computer graphics card is #FFFEFE (that's R:255, G:254, B:254)...but it's SO similar to pure white that you'd find it hard to
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to describe the ability to connect an iPod via a USB cable and use the stereo's controls to select music on the iPod. In other words, the iPod isn't just treated as a line in source; you can "control" the iPod from the head unit without using the iPod's controls.
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In the end, it's down to the ability of our eyes to distinguish it - and that's a question that varies between individuals, it varies depending on the ambient light levels and a bunch of other parameters. So there really isn't a single "correct" answer.
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much worse if we are relying on leakage of things like television signals; there we probably can't pull in stuff from anything but the few nearest stars, though I'd check that with someone who knows a lot more about the topic than I.
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But you don't need to build a big bucket to catch meteorites, you just need to wait for one to fall and then go and get it. You do need to build big radio telescopes and point them at distant stars if you want to find ETI.
733:-type radio telescope using our own Aricebo at distances exceeding 1000 light years. I expect that in the intervening three decades, both our detectors and our data crunching capabilities have improved substantially. 736:...Which is not to say that the problem is easy to solve — that assumes that the aliens have deliberately pointed their transmitter at us, and that we happen to watching at the moment that they did. The situation 387:
Yes, I just realised that and came back to clarify. The OP is talking about computer screens, though, which are additive. So Julia is right, but about the wrong thing. I'm right about the right thing, so I win! :)
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Your premise completely ignores the question why an ETI would bother blasting radio information into space. Does the fact that an ETS fails to send such radio waves render them unintelligent? Are
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Since the Search for Extra-Terrestrial Intelligence has failed so far, it seems probable that it will continue to fail. What are the consequences of this failure for science and for theology.
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Good plan - although the complementary color of blue is yellow - not pink - so your white box ought to be looking yellowish...but the Knowledge (XXG) logo and backdrop is grey - not blue.
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Yep, my error (I was typing off the top of my head, always a mistake), but actually if you look at the three boxes, then back, to the first one etc, it's very hard to tell (as you say). -
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Someone may correct me, but I don't think there's an authority for that. The colours above are simply accepted; they may be Pantone. But by my reckoning, surely R:256, G:255, B:255 (Hex
25: 867:) that Earth's radio output may be decreasing in favor of terrestrial transmission. It's not unreasonable to surmise that ETI wouldn't blast radio information. — 85:
The page you are currently viewing is an archive page. While you can leave answers for any questions shown below, please ask new questions on one of the
538:
Actually, we wouldn't even be able to declare failure then, because new civilizations might have sprung up in areas of space searched early on. Thanks,
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Getting back to my question, Assuming that SETI has found that the probability of finding ETI life approaches zero, what are the implications?
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they might work under our current understanding, doesn't mean we should give up on financing research into them, does it? Or maybe it does. --
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Thanks. I've decided to use white, as it actually looks pinkish when compared to the blue-tinted Knowledge (XXG) backdrop. Thanks once again,
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mostly guesswork) is never going to give a very high chance of success unless there is an enormous number of civilisations out there. --
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are a primary and the other two primary colours combined, so for blue it's actually orange; purple's complementary is yellow.
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notes that – using 1979 technology and a reasonable observing program – we could quite comfortably detect a signal from an
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employing 'spread spectrum' techniques. These make our signals look more and more like white noise (which is what a
86: 17: 944: 612:. We have no such positive reason w.r.t. SETI, so a comparison of SETI and PM is flawed in conception. Sorry. -- 1006: 841: 806: 790: 746: 457: 143: 675: 595: 495: 704:
I said that already... Your strategy of being the last to reply to questions does have its drawbacks! ;) --
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current projects attempting to beam radio waves into space in hopes of an ETI contact? –
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What is the meaning of USB DIRECT CONTROL available in in car audio systems now-a-days?
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The SETI Institute itself has abandoned the search, but SETI@Home is still going strong.
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support ETI life aren not very common, or ETI civilizations tend to self-destruct.
438:. Ok Tango, you win, you trag' you, ;) Julia (damn that logout) 4 March 2009 (UTC) 325:
On my screen the white box looks more light pink than the lightest pink. Btw, the
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it would require a very powerful civilisation to signal over such a distance). --
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The lightest shade of pink is not that difficult to calculate if you listen to "
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Yes we are, and have been for over a hundred years. Think television. -
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that it would take extremely subtle instruments to tell the difference.
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Welcome to the Knowledge (XXG) Miscellaneous Reference Desk Archives
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or the "light color" system. Sometimes, you both can be right! --
185:) is the lightest shade of pink (essentially the whitest red). - 994: 777: 445: 1001:, and the ideas expressed here have answered my questions. 362:
or the "pigment color" system. Tango's system works for
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was not found either, with equally profound results.
943:It seems you're right. SETI@home is run by the 604:We have positive reasons for not searching for 947:, which doesn't seem to be connected with the 911:numbers are the SETI@home people crunching? -- 8: 929:was ever related to the SETI@HOME project. 647:Absolutely none. Lack of news is not news. 608:machines, since they violate of the law of 49: 36: 65: 993:article combined with the articles on 725:Er, I don't think that's quite true. 43: 237:The lightest possible pink (#FFFEFE) 7: 163:What is the lightest shade of pink? 251:PINK (#FFEEEE) per User:Jarry1250 32: 863:We are, but some have suggested ( 344:contains more red than green. -- 247: 233: 219: 205: 104:What is direct wire USB control? 970:You might be interested in the 776:In the past forty eight years, 358:Julia Rossi's system works for 18:Knowledge (XXG):Reference desk 1: 665:Well, except with Hoffa, you 434:Thank you Jayron32. I was in 33: 804:sending such radio waves? – 925:It doesn't appear that the 1026: 194:The lightest shade with a 1011:03:16, 3 March 2009 (UTC) 984:23:23, 2 March 2009 (UTC) 961:13:35, 3 March 2009 (UTC) 945:Space Sciences Laboratory 939:04:29, 3 March 2009 (UTC) 921:23:24, 2 March 2009 (UTC) 900:19:16, 3 March 2009 (UTC) 872:20:51, 2 March 2009 (UTC) 851:21:26, 2 March 2009 (UTC) 834:19:55, 2 March 2009 (UTC) 816:19:15, 2 March 2009 (UTC) 795:19:08, 2 March 2009 (UTC) 751:15:05, 2 March 2009 (UTC) 714:12:13, 2 March 2009 (UTC) 699:03:56, 2 March 2009 (UTC) 680:01:34, 2 March 2009 (UTC) 661:20:28, 1 March 2009 (UTC) 635:12:13, 2 March 2009 (UTC) 620:01:36, 2 March 2009 (UTC) 600:01:29, 2 March 2009 (UTC) 569:20:27, 1 March 2009 (UTC) 554:19:37, 1 March 2009 (UTC) 526:19:26, 1 March 2009 (UTC) 500:19:22, 1 March 2009 (UTC) 483:19:00, 1 March 2009 (UTC) 462:18:44, 1 March 2009 (UTC) 430:18:16, 3 March 2009 (UTC) 398:13:55, 3 March 2009 (UTC) 383:13:49, 3 March 2009 (UTC) 354:13:43, 3 March 2009 (UTC) 339:22:03, 2 March 2009 (UTC) 315:04:07, 2 March 2009 (UTC) 301:17:43, 1 March 2009 (UTC) 288:17:38, 1 March 2009 (UTC) 279:17:05, 1 March 2009 (UTC) 190:16:48, 1 March 2009 (UTC) 176:16:36, 1 March 2009 (UTC) 153:13:00, 1 March 2009 (UTC) 129:11:06, 1 March 2009 (UTC) 610:conservation of energy 414:A Whiter Shade of Pale 87:current reference desk 999:Allen Telescope Array 327:complementary colours 989:Thank you all. The 731:Aricebo Observatory 418:rose-tinted glasses 136:USB Direct Control 865:one recent example 470:extrasolar planets 436:colour pencil mode 360:subtractive colors 38:Miscellaneous desk 832: 716: 523: 517: 380: 374: 255: 254: 241: 240: 227: 226: 213: 212: 132: 115:comment added by 93: 92: 73: 72: 1017: 849: 847: 845: 826: 814: 812: 810: 703: 606:perpetual motion 551: 549: 544: 521: 515: 416:" while wearing 378: 372: 296: 248: 234: 223:WHITE (#FFFFFF) 220: 206: 171: 151: 149: 147: 131: 109: 75: 34: 1025: 1024: 1020: 1019: 1018: 1016: 1015: 1014: 843: 842: 840: 808: 807: 805: 770: 547: 542: 540: 450: 364:additive colors 294: 256: 242: 228: 214: 209:PINK (#FF8080) 169: 161: 145: 144: 142: 110: 106: 101: 30: 29: 28: 12: 11: 5: 1023: 1021: 1003:Phil_burnstein 986: 968: 967: 966: 965: 964: 963: 949:SETI Institute 927:SETI Institute 907: 906: 905: 904: 903: 902: 877: 876: 875: 874: 858: 857: 856: 855: 854: 853: 787:Phil_burnstein 784: 782: 772: 769: 766: 764: 762: 761: 760: 759: 758: 757: 743:TenOfAllTrades 734: 720: 719: 718: 717: 685: 684: 683: 682: 644: 643: 642: 641: 640: 639: 638: 637: 622: 587: 578: 577: 576: 575: 574: 573: 572: 571: 531: 530: 529: 528: 503: 502: 486: 485: 454:Phil_burnstein 449: 443: 442: 441: 440: 439: 409: 408: 407: 406: 405: 404: 403: 402: 401: 400: 323: 322: 321: 320: 319: 318: 317: 266: 258: 253: 252: 246: 244: 239: 238: 232: 230: 225: 224: 218: 216: 211: 210: 204: 203: 202: 201: 200: 165:List of colors 160: 157: 156: 155: 105: 102: 100: 97: 95: 91: 90: 82: 81: 71: 70: 64: 48: 41: 40: 31: 15: 14: 13: 10: 9: 6: 4: 3: 2: 1022: 1013: 1012: 1008: 1004: 1000: 996: 992: 991:Fermi paradox 987: 985: 981: 977: 973: 972:Fermi paradox 962: 958: 954: 950: 946: 942: 941: 940: 936: 932: 928: 924: 923: 922: 918: 914: 909: 908: 901: 897: 893: 888: 883: 882: 881: 880: 879: 878: 873: 870: 866: 862: 861: 860: 859: 852: 848: 837: 836: 835: 830: 825: 824: 819: 818: 817: 813: 803: 799: 798: 797: 796: 792: 788: 779: 775: 767: 765: 754: 753: 752: 748: 744: 739: 735: 732: 728: 727:This proposal 724: 723: 722: 721: 715: 711: 707: 702: 701: 700: 696: 692: 687: 686: 681: 677: 673: 672:98.217.14.211 668: 664: 663: 662: 658: 654: 650: 646: 645: 636: 632: 628: 623: 621: 618: 615: 611: 607: 603: 602: 601: 597: 593: 592:98.217.14.211 588: 584: 583: 582: 581: 580: 579: 570: 566: 562: 557: 556: 555: 552: 550: 545: 537: 536: 535: 534: 533: 532: 527: 524: 518: 512: 507: 506: 505: 504: 501: 497: 493: 492:98.217.14.211 488: 487: 484: 480: 476: 471: 466: 465: 464: 463: 459: 455: 447: 444: 437: 433: 432: 431: 427: 423: 419: 415: 411: 410: 399: 395: 391: 386: 385: 384: 381: 375: 369: 365: 361: 357: 356: 355: 351: 347: 342: 341: 340: 336: 332: 328: 324: 316: 312: 308: 304: 303: 302: 299: 297: 291: 290: 289: 286: 282: 281: 280: 276: 272: 267: 263: 262: 261: 260: 259: 250: 249: 245: 236: 235: 231: 222: 221: 217: 208: 207: 197: 193: 192: 191: 188: 184: 183:close to this 180: 179: 178: 177: 174: 172: 166: 158: 154: 150: 139: 135: 134: 133: 130: 126: 122: 118: 114: 103: 98: 96: 88: 84: 83: 80: 77: 76: 68: 61: 57: 53: 47: 42: 39: 35: 27: 26:Miscellaneous 23: 19: 988: 969: 886: 821: 801: 773: 771: 763: 737: 666: 653:Clarityfiend 539: 451: 257: 243: 229: 215: 195: 167:baffles me. 162: 107: 94: 78: 974:article. -- 649:Jimmy Hoffa 614:Tagishsimon 331:Julia Rossi 111:—Preceding 46:February 28 976:JGGardiner 892:SteveBaker 691:SteveBaker 422:BrainyBabe 307:SteveBaker 271:SteveBaker 117:Akshun1991 887:perfectly 285:Jarry1250 187:Jarry1250 50:<< 931:Rmhermen 823:mattbuck 522:contribs 511:Jayron32 379:contribs 368:Jayron32 125:contribs 113:unsigned 24:‎ | 22:Archives 20:‎ | 448:failure 295:Queenie 170:Queenie 138:appears 99:March 1 89:pages. 67:March 2 997:, the 774:Update 768:Update 617:(talk) 543:Genius 953:Tango 913:Tango 706:Tango 627:Tango 561:Tango 475:Tango 390:Tango 346:Tango 199:tell: 69:: --> 63:: --> 62:: --> 56:March 44:< 16:< 1007:talk 995:SETI 980:talk 957:talk 935:talk 917:talk 896:talk 869:Lomn 829:Talk 791:talk 778:SETI 747:talk 710:talk 695:talk 676:talk 657:talk 631:talk 596:talk 565:talk 516:talk 496:talk 479:talk 458:talk 446:SETI 426:talk 394:talk 373:talk 350:talk 335:talk 311:talk 275:talk 196:name 159:Pink 121:talk 667:can 548:101 60:Apr 52:Feb 1009:) 982:) 959:) 937:) 919:) 898:) 802:we 793:) 749:) 738:is 712:) 697:) 678:) 659:) 633:) 625:-- 598:) 567:) 498:) 481:) 460:) 428:) 420:. 396:) 388:-- 352:) 337:) 313:) 277:) 141:– 127:) 123:• 58:| 54:| 1005:( 978:( 955:( 933:( 915:( 894:( 846:4 844:7 831:) 827:( 811:4 809:7 789:( 745:( 708:( 693:( 674:( 655:( 629:( 594:( 563:( 519:. 513:. 494:( 477:( 456:( 424:( 392:( 376:. 370:. 348:( 333:( 309:( 273:( 148:4 146:7 119:(

Index

Knowledge (XXG):Reference desk
Archives
Miscellaneous
Miscellaneous desk
February 28
Feb
March
Apr
March 2
current reference desk
unsigned
Akshun1991
talk
contribs
11:06, 1 March 2009 (UTC)
appears
74
13:00, 1 March 2009 (UTC)
List of colors
Queenie

16:36, 1 March 2009 (UTC)
close to this
Jarry1250
16:48, 1 March 2009 (UTC)
SteveBaker
talk
17:05, 1 March 2009 (UTC)
Jarry1250
17:38, 1 March 2009 (UTC)

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