Glossary
The Local Group (of Galaxies)

The Local Group consists of approximately 30 galaxies laying within about 1 Mpc of the Galaxy. These galaxies are thought to be loosely gravtitationally bound. The most prominent members are our Galaxy (the "Milky Way"), M31 (the Andromeda galaxy), and M33 (the Triangulum galaxy). These are all spiral galaxies. The next most luminous are the so-called Large and Small Magellanic Clouds (LMC & SMC). These are irregular galaxies (with 11 others). The remaining galaxies are so-called dwarf Ellipticals/spheriods. (see also 2002 PHYS 316 Notes Lecture-5 and Lecture-14).

The exact membership of of Local Group (particularly on its outskirts) remains a matter of some debate. There appear to be two subgroups within the Local Group:

  • the Galaxy subgroup, consisting of our Galaxy and a dozen or so other galaxies (including the LMC & SMC)
  • the Andromeda subgroup, consisting of M31, M32, M33 and a handful of other galaxies.
From the observed dynamics of the galaxies, combined with estimates of the masses, the gravitational center of the Local Group can be estimated. Most estimates place this approximately 450 kpc away from the Sun in the direction of M31 (Gal coords 120, -21).

The Sun's motion relative to the Local Group can then be estimated. This calculation involves determining the vector for the Sun's motion within the Local Standard of Rest (~20 km/s), the orbit of the Local Standard of Rest around the Galactic Center (~220 km/s), and our Galaxy's motion with respect to the center of the Local Group. Most estimates agree that the Sun's motion wrt the Local Group is 308 km/s in a direction with Galactic Coordinates +100 deg, -4 deg.

Name Class v-helio
v-LG
(hcat)
v-CMB
(hcat)
Distance
(kpc)
D-LG
(kpc)
R C X
Milky Way Sbc I-II ... +308 +371 8 460 ... ... ...
SDG (Sagittarius) dSph(t) +142 30 460 ... 30 53
ESO056-115 (LMC) * Ir III-IV +275 +82 +355 60 480 ... ... ...
NGC0292 (SMC) Im IV-V +148 -7 +114 58 480 ... ... ...
DDO199 (Ursa Minor) dSph -247 -19 -170 60 430 no no no
DDO208 (Draco) dSph -293 -66 -316 80 430 5 no ?
ESO351-030 (Sculptor) dSph +110 +141 -108 90 440 ? no 13
7ZW828 (Sextans) dSph +226 ??? ??? 90 510 2 no no
ESO206-020A (Carina) dSph +223 -14 +339 100 510 9 no no
ESO356-004 (Fornax) dSph 53 -10 -127 140 450 11 no no
DDO 074 (Leo I) dSph +287 +97 +555 250 610 no no no
DDO 093 (Leo II) dSph +76 -83 +320 210 570 no no no
ESO245-007 (Phoenix) dIr/dSph +56 -16 -119 400 590 no no no
NGC6822 Ir IV-V -56 +8 -254 500 670 lot 28 no
NGC0185 Sph -202 +54 -491 660 220
NGC0147 Sph -193 +133 -415 660 220
IC 10 (UGC 192) Ir IV -344 -47 -553 660 270
DDO69 (Leo A) Ir V +24 -15 +292 690 880
Cassiopeia (AND VII.) dSph ... ... ... 690 290
[KK98a]011341.9+330920 (And. II) dSph ... ... ... 700 260
IC1613 Ir V -232 -62 -552 720 470
NGC0224 (M31) Sb I-II -301 -14 -576 760 300
NGC0221 (M32) E2 -205 +73 -490 760 310
NGC0205 (M110) Sph -244 +52 -511 760 310
PGC002121 (AND III.) dSph ... ... ... 760 310
DDO 216 (Pegasus) Ir V -182 +61 -539 760 440
NGC0598 (M33) Sc II-III -181 +68 -454 790 370
PGC002666 (AND I.) dSph ... ... ... 810 360
(AND V.) dSph ... ... ... 810 370
LGS3 (Pisces) dIr/dSph -286 -14 -576 810 420
Peg dSph (And VI.) dSph ... ... ... 830 430
DDO210 (Aquarius) ? IBm V -131 -32 -405 1020 1020
EQ 2238-646 (Tucana) ? dSph ... ... ... 870 1100
DD0221 (WLM) IBr IV-V -120 -7 -447 930 790
ESO594-4 (Sag DIG) ? Ir V -79 -36 -253 1400 1480