This web page was created programmatically, to learn the article in its authentic location you possibly can go to the hyperlink bellow:
http://www.sciencedaily.com/releases/2025/09/250911073620.htm
and if you wish to take away this text from our website please contact us
This new NASA/ESA Hubble Space Telescope Picture of the Week includes a cloudy starscape from a powerful star cluster. This scene is positioned within the Large Magellanic Cloud, a dwarf galaxy located about 160,000 light-years away within the constellations Dorado and Mensa. With a mass equal to 10-20% of the mass of the Milky Way, the Large Magellanic Cloud is the biggest of the handfuls of small galaxies that orbit our galaxy.
The Large Magellanic Cloud is dwelling to a number of large stellar nurseries the place gasoline clouds, like these strewn throughout this picture, coalesce into new stars. Today’s picture depicts a portion of the galaxy’s second-largest star-forming area, which is named N11. (The most large and prolific star-forming area within the Large Magellanic Cloud, the Tarantula Nebula, is a frequent goal for Hubble.) We see vibrant, younger stars lighting up the gasoline clouds and sculpting clumps of mud with highly effective ultraviolet radiation.
This picture marries observations made roughly 20 years aside, a testomony to Hubble’s longevity. The first set of observations, which had been carried out in 2002-2003, capitalized on the beautiful sensitivity and backbone of the then-newly-installed Advanced Camera for Surveys. Astronomers turned Hubble towards the N11 star cluster to do one thing that had by no means been carried out earlier than on the time: catalogue all the celebrities in a younger cluster with plenty between 10% of the Sun’s mass and 100 instances the Sun’s mass.
The second set of observations got here from Hubble’s latest digicam, the Wide Field Camera 3. These pictures centered on the dusty clouds that suffuse the cluster, bringing a brand new perspective on cosmic mud.
This web page was created programmatically, to learn the article in its authentic location you possibly can go to the hyperlink bellow:
http://www.sciencedaily.com/releases/2025/09/250911073620.htm
and if you wish to take away this text from our website please contact us
