NGC1850 as seen with the Very Large Telescope and Hubble
This image shows NGC1850, a cluster of thousands of stars roughly 160 000 light-years away in the Large Magellanic Cloud, a Milky Way neighbour. The reddish filaments surrounding the cluster, made of vast clouds of hydrogen, are believed to be the remnants of supernova explosions.
The image is an overlay of observations conducted in visible light with ESO’s Very Large Telescope (VLT) and NASA/ESA’s Hubble Space Telescope (HST). The VLT captured the wide field of the image and the filaments, while the central cluster was imaged by the HST.
Among many stars, this cluster is home to a black hole 11 times as massive as the Sun and to a five-solar-mass star orbiting it. By looking at the star’s orbit, a team of astronomers were able to infer the presence of the black hole, making it the first small black hole outside of our galaxy to be found this way. For this discovery, the team used the Multi Unit Spectroscopic Explorer (MUSE) instrument at the VLT.
Credit:ESO, NASA/ESA/R. Gilmozzi/S. Casertano, J. Schmidt
About the Image
Id: | eso2116b |
Type: | Observation |
Release date: | 11 November 2021, 13:00 |
Related releases: | eso2116 |
Size: | 3097 x 3093 px |
About the Object
Name: | NGC 1850 |
Type: | Local Universe : Nebula : Type : Supernova Remnant Local Universe : Star : Grouping : Cluster |
Constellation: | Dorado |
Category: | Star Clusters |
Wallpapers
Coordinates
Position (RA): | 5 8 46.19 |
Position (Dec): | -68° 45' 39.77" |
Field of view: | 6.80 x 6.79 arcminutes |
Orientation: | North is 33.2° right of vertical |
Colours & filters
Band | Wavelength | Telescope |
---|---|---|
Optical B | 440 nm | Very Large Telescope FORS1 |
Optical B | 439 nm | Hubble Space Telescope WFPC2 |
Optical V | 555 nm | Hubble Space Telescope WFPC2 |
Optical V | 557 nm | Very Large Telescope FORS1 |
Optical r | 675 nm | Hubble Space Telescope WFPC2 |
Optical v | 569 nm | Hubble Space Telescope WFPC2 |
Optical i | 791 nm | Hubble Space Telescope WFPC2 |
Optical H-alpha | 656 nm | Very Large Telescope FORS1 |
Optical H-alpha | 656 nm | Hubble Space Telescope WFPC2 |