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#1
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![]() A fellow here in the computer lab is askin and I thought of all the folk I converse with _this_ group would have a ready answer. Of course I'll be Googeling right afterI post this but its often wheatberries amoungst the chaff time with the search engine. In any case Thx in advance. TBerk |
#2
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TBerk wrote:
A fellow here in the computer lab is askin and I thought of all the folk I converse with _this_ group would have a ready answer. Of course I'll be Googeling right afterI post this but its often wheatberries amoungst the chaff time with the search engine. In any case Thx in advance. TBerk M31 aka Andromeda .. unless you count the Magellanic Clouds. Gee .. hope I got this right ![]() Phil |
#3
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TBerk wrote:
Of course I'll be Googeling right afterI post this but its often wheatberries amoungst the chaff time with the search engine. Y'mean, as compared with Usenet? ![]() See he http://antwrp.gsfc.nasa.gov/apod/ap031117.html -- St. John It's a good thing we don't get all the government we pay for. |
#4
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TBerk wrote:
A fellow here in the computer lab is askin and I thought of all the folk I converse with _this_ group would have a ready answer. See: http://www.astro.uu.se/~ns/images/local_group1.gif |
#5
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Sam Wormley wrote:
TBerk wrote: A fellow here in the computer lab is askin and I thought of all the folk I converse with _this_ group would have a ready answer. See: http://www.astro.uu.se/~ns/images/local_group1.gif Also from http://www.seds.org/messier/more/local.html looks like CMa dw galaxy is the closest at 25,000 light years. Local Group Member Galaxies Galaxy RA Dec Type m_v dim RV Dist WLM 00:02.0 -15:28 IB(s) IV-V 10.9 12 x 4 - 42 3400 IC 10 00:20.4 +59:18 KBm? 10.3 7.3 x 6.4 - 83 4200: Cet dw 00:26.1 -11:02 dSph/E4 14.4 2800 NGC 147 00:33.2 +48:31 dE5 pec 9.5 15.0 x 9.4 + 89 2400 And III 00:35.4 +36:31 dSph/E2 13.5p 4.5 x 3.0 2900: NGC 185 00:39.0 +84:20 dE3 pec 9.2 14.5 x 12.5 + 39 2300 M110 00:41.3 +41:41 E5 pec 8.5 19.5 x 12.5 - 1 2900 And VIII 00:42.3 +40:37 dSph pec 9.1 45 x 10 -250 2700: M 32 00:42.7 +40:52 E2 (cE2) 8.1 11.0 x 7.3 + 35 2900 M 31 00:42.7 +41:16 SA(s)b I-II 3.4 185.0 x 75.0 - 59 2900 And I 00:45.7 +38:00 dSph/E3 pec ? 13.2 2.5 x 2.5 2900: SMC 00:51.7 -73:14 SB(s)m pec 2.3 280 x 160 - 30 210 And IX 00:52.9 +43:12 dSph 16.2 5 2900: Scl dw 01:00.0 -33:42 dSph/E3 pec 10.5p +162 300: LGS 3 01:03.8 +21:53 Irr 15.4p 2 3000: IC 1613 01:05.1 +02:08 IAB(s)m V 9.2 20.0 x 18.5 -125 2900: And X 01:06.6 +44:48 dSph 16.1 7 2900: And V 01:10.3 +47:38 dSph 15.9 2900: And II 01:16.4 +33:27 dSph/E0 13.5 3.6 x 2.5 2900: M 33 01:33.9 +30:39 SA(s)cd II-III 5.7 67.0 x 41.5 + 3 3000 Phe dw 01:51.1 -44:27 Irr 13.1 4.9 x 4.1 1600: For dw 02:39.9 -34:32 dSph/E2 8.1 12.0 x 10.2 500 UGCA 92 04:32.0 +63:36 Irr ? S0 ? 13.8 2.0 x 1.0 + 66 4700 LMC 05:19.7 -68:57 SB(s)m 0.1 650 x 550 + 13 179 Car dw 06:14.6 -50:58 dSph/E3 20.9 23.5 x 15.5 360 CMa dw 07:15 -28 Irr 720 25 Leo A 09:59.4 +30:45 IBm V 12.9 5.1 x 3.1 2500 Sex B 10:00.0 +05:20 Ir+ IV-V 11.8 5.1 x 3.5 4700 NGC 3109 10:03.1 -26:09 Ir+ IV-V 10.4 16.0 x 2.9 +131 4500 Ant dw 10:04.1 -27:20 dSph/E3 14.8 2.0 x 1.5 4600 Leo I 10:08.5 +12:18 dE3 9.8 9.8 x 7.4 900 Sex A 10:11.1 -04:43 Ir+ V 11.9 5.9 x 5.0 5200 Sex dw 10:13.2 -01:37 dSph/E3 12. 320 Leo II 11:13.5 +22:10 dSph/E0 pec 12.6 12.0 x 11.0 750 GR 8 12:58.7 +14:13 Im V 14.5 1.2 x 1.1 +165 7900: UMi dw 15:08.8 +67:12 dSph/E4 10.9 41.0 x 26.0 240 Dra dw 17:20.1 +57:55 dSph/E0 pec 9.9 51.0 x 31.0 280 Milky Way 17:45.6 -28:56 SAB(s)bc I-II ? - 0 28 SagDEG 18:55 -30:30 dSph/E7 +168 88 SagDIG 19:30.1 -17:42 IB(s)m V 15.5 2.9 x 2.1 4200 NGC 6822 19:44.9 -14:49 IB(s)m IV-V 9.3 15.5 x 13.5 + 66 1800 Aqr dw 20:46.8 -12:51 Im V 13.9 2.3 x 1.2 3400 Tuc dw 22:41.7 -64:25 dSph/E5 15.7 2.9 x 1.2 3200 UKS2323-326 23:26.5 -32:23 Irr 13.9 1.5 x 1.2 4700 And VII 23:27.8 +50:35 dSph 2.5 x 2.0 2600 Peg dw 23:28.6 +14:45 Im V 13.2 5.0 x 2.7 3000: And VI 23:51.7 +24:36 dSph 11.2 3.5 x 3.5 2800 Possible further members: UGCA 86 03:59.9 +67:08 Irr ? S0 ? 13.5 0.8 x 0.7 +262 6200 Willman 1 10:49.4 +51:03 dSph? GC ? 15.3 1.75 147 IC 5152 22:06.1 -51:17 IAB(s)m IV 10.6 4.9 x 3.0 + 30 5800 Below we list some nearby but probably non-member field galaxies (which are also not members of one of the neighboring groups listed above), in the same format as above: |
#6
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There's the small ones that are in orbit around our galaxy, LMC/SMC/Sag.Df.
galaxy, outside of them and coming at us is M31. -- The Lone Sidewalk Astronomer of Rosamond Telescope Buyers FAQ http://home.inreach.com/starlord Sidewalk Astronomy www.sidewalkastronomy.info Astronomy Net Online Gift Shop http://www.cafepress.com/astronomy_net In Garden Online Gift Shop http://www.cafepress.com/ingarden Blast Off Online Gift Shop http://www.cafepress.com/starlords "TBerk" wrote in message ups.com... A fellow here in the computer lab is askin and I thought of all the folk I converse with _this_ group would have a ready answer. Of course I'll be Googeling right afterI post this but its often wheatberries amoungst the chaff time with the search engine. In any case Thx in advance. TBerk |
#7
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![]() Hmm, it looks like (for a long time) Andromeda was the goto answer. Now I'm finding out about a Dwarf Galaxy we (the milky Way) are cannibalizing, it seems to be in/ part of Canis Major. Well, Thx everybody. TBerk |
#8
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Sam Wormley wrote:
Sam Wormley wrote: TBerk wrote: A fellow here in the computer lab is askin and I thought of all the folk I converse with _this_ group would have a ready answer. TBerk - Just to add another reference - Powell's Atlas of the Universe Local Galaxy Groups Map http://anzwers.org/free/universe/localgr.html Local Galaxy Groups Table http://anzwers.org/free/universe/galaxies.html This excludes the partially cannibalized and graviationally captured dwarf galaxies mentioned in other posts in this thread. I typically assign those objects to the "Milky Way System" as opposed to the "Local Group" of galaxies. Powell's Atlas of the Universe The Satellite Galaxies [of the Milky Way] http://anzwers.org/free/universe/sattelit.html The picture in Powell's Atlas does not show the Canis Major Dwarf galaxy which is basically inside the Milky Way spiral arm structure and which is shown in the APOD picture posted by St. John Smythe in this thread. http://antwrp.gsfc.nasa.gov/apod/ap031117.html So, a fair answer to the top poster's question depends on how you define a "galaxy" and how you define what is the "Milky Way Galaxy." If you mean a dwarf galaxy and the "Milky Way" means only the spiral arm structure and Milky Way core - it's the Canius Major Dwarf at 12 kiloparsecs. If you mean, what lay people would call a "real galaxy" and the "Milky Way system," it's either Andromeda at about 735 kiloparsecs or a small dwarf outside the Milky Way System, like Leo II at 205 kiloparsecs. But IMHO you can fairly look at the answer both ways. - Canopus56 |
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