EmissionNebula NGC6357, by NASA, ESA and Jesœs Maz Apellÿniz (Instituto de astrofísica de Andalucia, Spain). Acknowledgement: Davide De Martin…, 2006-12-19
Gallery mode Full size at the museum

Window mode follows your eyes with your camera, in this browser only: no picture or position leaves your device.

EmissionNebula NGC6357

NASA, ESA and Jesœs Maz Apellÿniz (Instituto de astrofísica de Andalucia, Spain). Acknowledgement: Davide De Martin…

2006-12-19

Classification
Photograph
Museum
Wikimedia Commons
Credit line
https://www.spacetelescope.org/images/heic0619a/ (TIFF image 36 MB)
Rights
Public domain, as the museum states it.
Who can see it
Teens profiles and older: its museum says too little about what it shows to place it for younger viewers. How works are placed

View at the Wikimedia Commons

About this work

The star cluster Pismis 24 lies in the core of the large emission nebula NGC 6357 that extends one degree on the sky in the direction of the Scorpius constellation. Part of the nebula is ionised by the youngest (bluest) heavy stars in Pismis 24. The intense ultraviolet radiation from the blazing stars heats the gas surrounding the cluster and creates a bubble in NGC 6357. The presence of these surrounding gas clouds makes probing into the region even harder.