Central regions of 47 Tucanae seen in the ultraviolet
This NASA/ESA Hubble Space Telescope image shows the central region of a globular cluster known as NGC 104 — or, more commonly, 47 Tucanae, since it is part of the constellation of Tucana (The Toucan) — seen in ultraviolet light.
Using the ultraviolet capabilities of Hubble’s sharp-eyed Wide Field Camera 3, the astronomers traced populations of white dwarfs with a range of ages and positions. This made it possible, for the first time, to collect a census of young white dwarf stars beginning their migration from the crowded centre of an ancient star cluster to its less populated outskirts.
NASA, ESA, and H. Richer and J. Heyl (University of British Columbia, Vancouver)
About the Image
| Id: | heic1510c |
|---|---|
| Type: | Observation |
| Release date: | 14 May 2015, 19:00 |
| Related releases: | heic1510 |
| Size: | 800 x 800 px |
About the Object
| Name: | 47 Tucanae, NGC 104 |
|---|---|
| Type: | Milky Way : Star : Grouping : Cluster : Globular |
| Distance: | 15000 light years |
| Constellation: | Tucana |
| Category: | Star Clusters |
Classic Wallpapers
Coordinates
| Position (RA): | 0 24 6.56 |
|---|---|
| Position (Dec): | -72° 5' 4.01" |
| Field of view: | 0.53 x 0.53 arcminutes |
| Orientation: | North is 14.9° left of vertical |
Colours & filters
| Band | Wavelength | Telescope |
|---|---|---|
| Ultraviolet UV | 225 nm |
Hubble Space Telescope
WFC3 |
| Ultraviolet UV | 336 nm |
Hubble Space Telescope
WFC3 |

