Many Faces in Doradus

NASA, ESA, D. Lennon and E. Sabbi (ESA/STScI), J. Anderson, S. E. de Mink, R. van der Marel, T. Sohn, and N. Walborn (STScI), N. Bastian (Excellence Cluster, Munich), L. Bedin (INAF, Padua), E. Bressert (ESO), P. Crowther (University of Sheffield), A. de Koter (University of Amsterdam), C. Evans (UKATC/STFC, Edinburgh), A. Herrero (IAC, Tenerife), N. Langer (AifA, Bonn), I. Platais (JHU), and H. Sana (University of Amsterdam)

Many faces hide around the star cluster NGC 2060 in this image from the NASA/ESA Hubble Space Telescope.

Explore the loose collection of stars and nebula. What stories or pictures do you see? Leave a note in the comments below.

The star cluster NGC 2060 is a family of stars that are drifting apart. These stellar siblings were born from the same star cloud but now they are no longer gravitationally bound. Within a few million years the grouping will cease to be as all the stars will have dispersed. The nebula is full of little gems besides young stars. Look just left of center in the image. A supernova, created when a massive hot star ended its short life after burning all of its nuclear fuel, exploded blowing a bubble within the cloud about 10,000 years ago. The dark area near the center of the image is a dense cloud of cold dust between Earth and the cloud. Other smaller dark globs of dust blot out the starlight from behind. Fierce stellar winds and blistering ultraviolet radiation from the young stars in this nebula push the glowing gas and dust into arcs and pillars

NGC 2060 is part of 30 Doradus, the brightest star-forming region that we know about 170,000 light-years from Earth in the Large Magellanic Cloud. The LMC is a dwarf galaxy near our Milky Way Galaxy. The massive nebula is home to some of the most massive stars in our cosmic neighborhood. It is so bright and close, that Hubble can see individual stars offering scientists information on how stars are born, evolve and die.

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