Cookie consent

AstroBin saves small pieces of text information (cookies) on your device in order to deliver better content and for statistical purposes. You can disable the usage of cookies by changing the settings of your browser. By browsing AstroBin without changing the browser settings, you grant us permission to store that information on your device.

I agree
Contains:  omega Cen, NGC 5139
Getting plate-solving status, please wait...
NGC5139 Omega Centauri, Centaurus, 


            Thomas V. Davis
NGC5139 Omega Centauri, Centaurus

NGC5139 Omega Centauri, Centaurus

Technical card

Resolution: 4050x4020 job: 2099070

RA center: 201.685 degrees

DEC center: -47.483 degrees

Pixel scale: 2.198 arcsec/pixel

Orientation: 10.516 degrees

Field radius: 1.742 degrees

Data source: Own remote observatory


NGC5139 Omega Centauri, Centaurus
Astro-Physics 155 EDF (155TCC) f/5.4 refractor
KAF-16803; FLI Proline
Total Exposure Time: 4.6+ hours; LRGB 115:55:55:55 minutes, unbinned
February 2009; RDO, Moorook, AU

Comments: This is the biggest of all globular clusters in our Milky Way galaxy. With its about 5 million solar masses, it is about 10 times as massive as other big globulars, and has about the same mass as the smallest whole galaxies. It is also the most luminous Milky Way globular, and the brightest globular cluster in the sky. In the Local Group, it is outshined only by the brightest globular cluster G1 in the Andromeda Galaxy M31. In 1999, a team led by Young-Wook Lee of Yonsei University, South Korea, obtained a color-magnitude diagram (CMD) for 50,000 member stars of Omega Centauri with the 0.9-m telescope of CTIO in Chile. Studies of this CMD indicate that the stars of this cluster did not all form at once but over a 2-billion-year period of time, with several starburst peaks. This was the first time that multiple populations were found in a globular cluster. The team who carried out this work speculates that this result may indicate that Omega Centauri might be the remnant of a nucleus of a small galaxy which has merged with our Milky Way .

Interestingly, there is faint dust or flux nebulosity in this region that I haven't seen before in any image. I suspect that it gets processed out. This dust is in the lower right portion of the image. It is very faint and can be seen if you look at the screen from the right side instead of directly in front. It really is there!

This image was NASA APOD March 1, 2009.



Thomas V. Davis
License: None (All rights reserved)

Sky plot

Sky plot


NGC5139 Omega Centauri, Centaurus, 


            Thomas V. Davis