Al Bustan 
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IC5146 - Cocoon
M5 - NGC5904
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M16 - Eagle Nebula
M17_Swan
M20 - Trifid
M27 - Dumbbell
M31 - Andromeda
M33 - Pinwheel
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M51 - Whirlpool
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M63 - Sunflower
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M65 - NGC3623
M67 - NGC2682
M98 - NGC4192
M99 - Pinwheel
M100 - NGC4321
M101 - NGC5457
M104 - Sombrero
M105 - NGC3379
M106 - NGC4258
C/2004 Q2 - Machholz
NGC 891
NGC2024 - Flame
NGC2244 - Rosette
NGC6960 - Veil
The Mice - NGC4676

 

 

 

 

 

M99 in Coma Berenices, at 50 to 60 million light years away, is part of the Coma-Virgo galaxy cluster, together with M88, M91, M98, M100 and several other galaxies.

It is an inclined galaxy known for its strong one-armed structure. The south arm is filled with bright star-forming regions while the north arm is weak. This dichotomy is unexplained by optical observations, but radio images show clouds of neutrl hydrogen perturbing the the spiral from the south. The one armed appearance is evident in a 12" or large telescope, which shows a bright core 1" across with the prominent arm wraping from the east edge to the south. This spiral arm is mottled and ends at a stellar association. The northern arm is barely visible in a 12" aperture and does not wrap as tightly around the core.

M99 Observer´s Log

Spiral Galaxy
Pinwheel Nebula
M99
NGC4254
Dreyer description: Very remarkable! Bright, large, round, gradually brighter middle, resolvable, but mottled, 3-branched spiral; = M99.
Other ID: UGC7345
Other ID: MCG3-31-99
Other ID: MESS99
Other ID: PGC39578
Magnitude: 10.1
RA: 12h 18m 59.6s Dec: +14°24'04"
RA: 12h 18m 49.3s Dec: +14°25'07" (Epoch 2000)
Size: 5.4' x 4.8'

 

 

 

 
   

 

 

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This site was last updated 2006-04-22                                                                                                          Site created and maintained by Jorge Lázaro