Spiral Galaxies
(page 1)
Spiral galaxies are rotating disk systems of stars, gas and dust. Due to their varying orientations in the sky, they may appear as face-on whirlpools, edge-on disks, or as something in between. Spirals are classified based on the tightness of their arms the size and shape of their nucleus. Those with an elongated bar-like center are called "barred spirals."
Arp 102 |
Arp 273 |
CG4 |
Helix |
![]() IC342 |
IC4182 |
IC4182 |
M31 |
M31 |
M31 |
M31 (bit) |
M31/M32 |
M31/Moon |
M33 |
M33 |
M33 |
M33 |
M33 |
M51 |
![]() M51 |
M51 |
M58 |
M61 |
M63 |
M64 |
M64 |
M65 |
M65/66, Leo Triplet |
M66 |
M74 |
M74 |
M77 |
M81 |
M81 |
M83 |
![]() M83, NGC5236 |
M88 |
M90 |
M91 |
M94 |
M94 |
M95 |
M95 |
M96 |
M98 |
M99 |
M100 |
M101 |
M101 |
M101 N |
M101 S |
M102 |
M104 |
M104 |
M106 |
M108 |
M109 |
![]() NGC55 |
NGC55 |
More Spiral Galaxies
| webmaster@noao.edu Last updated: Feb 28 2013 |
![[IC342]](/image_gallery/images/d2/ic342-th.jpg)
![[M51]](/image_gallery/images/d2/m51-th.jpg)
![[M83, NGC5236]](/image_gallery/images/d4/J1337-29_crop1-th.jpg)
![[NGC55]](/image_gallery/images/d6/ngc55-th.jpg)


