esahubble_heic2409a July 10th, 2024
Credit: ESA/Hubble & NASA, M. Häberle (MPIA)
Omega Centauri is visible from Earth with the naked eye and is one of the favourite celestial objects for stargazers in the southern hemisphere. Although the cluster is 17 700 light-years away, lying just above the plane of the Milky Way, it appears almost as large as the full Moon when seen from a dark rural area. The exact classification of Omega Centauri has evolved through time, as our ability to study it has improved. It was first listed in Ptolemy's catalogue nearly two thousand years ago as a single star. Edmond Halley reported it as a nebula in 1677, and in the 1830s the English astronomer John Herschel was the first to recognise it as a globular cluster. Omega Centauri consists of roughly 10 million stars that are gravitationally bound. [Image Description: A globular cluster, appearing as a highly dense and numerous collection of shining stars. Some appear a bit larger and brighter than others, with the majority of stars appearing blue and orange. They are scattered mostly uniformly, but in the centre they crowd together more and more densely, and merge into a stronger glow at the cluster’s core.]
Provider: Hubble Space Telescope | ESA
Image Source: https://esahubble.org/images/heic2409a/
Curator: ESA/Hubble, Baltimore, MD, United States
Image Use Policy: Creative Commons Attribution 4.0 International License
| Telescope | Spectral Band | Wavelength | |
|---|---|---|---|
|
Hubble (WFC3) | Ultraviolet (UV) | 275.0 nm |
|
Hubble (WFC3) | Optical (U) | 336.0 nm |
|
Hubble (WFC3) | Optical (B) | 438.0 nm |
|
Hubble (WFC3) | Optical (V) | 606.0 nm |
|
Hubble (ACS) | Optical (V) | 606.0 nm |
|
Hubble (WFC3) | Optical (r) | 625.0 nm |
|
Hubble (WFC3) | Optical (I) | 814.0 nm |
|
Hubble (ACS) | Optical (I) | 814.0 nm |
|
Hubble (WFC3) | Optical (N II) | 658.0 nm |
|
Hubble (ACS) | Optical (B) | 435.0 nm |
Detailed color mapping information coming soon...
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