NGC4826 Galaxy in Coma Berenices
DATE | 29 Mar 2014 |
TELESCOPE OPTICS | 508 mm mirror f.4 . effective f4.6 with paracorr2. ccd Kodak KAF8300 3326 x 2504px 5.4 x 5.4µm |
EXPOSURE | binning 1: composite image, 13min |
IMAGE SIZE (ARCMIN) | 25 |
LIGHT TRAVEL TIME (Derived Redshift. Millions Light Years) | NGC4826 2MASX J12572147+2140450 = 1,416 2MASX J12572893+2137370 = 974 2MASX J12561052+2148274 = 1,419 2MASX J12571196+2146234 = 2,066 SDSS J125648.92+213624.2 = 978 |
MAGNITUDE | NGC4826 = 9.36 2MASX J12572147+2140450 = 18.63 2MASX J12572893+2137370 = 18.1g 2MASX J12561052+2148274 = 17.5g 2MASX J12571196+2146234 = 18.6g SDSS J125648.92+213624.2 = 19.58 |
POSITION RA-DEC J2000 | NGC4826 = 12:56:43.60 +21:40:59.0 2MASX J12572147+2140450 = 12:57:21.40 +21:40:45.0 2MASX J12572893+2137370 = 12:57:28.90 +21:37:38.0 2MASX J12561052+2148274 = 12:56:10.50 +21:48:28.0 2MASX J12571196+2146234 = 12:57:12.00 +21:46:24.0 SDSS J125648.92+213624.2 = 12:56:48.90 +21:36:24.0 |
POSITION ANGLE: | 180 |
Rotation Velocity km/s | 160 |
Size (Light Years) | 53,000 (RC3 D_0 (blue)) |
DETAILS | NGC4826, also known as M64 or Blackeye galaxy is classed as a spiral with Seyfert 2 activity. It is unusual in as much as it has counter rotating gaseuos rings and a very heavy dust lane close to the centre. The rings are thought to be the result of a collision with a smaller galaxy that had a lot of gas. |