Six or seven billion years ago, most stars formed in super star clusters. That type of star formation has largely died out now. Astronomers know of two of these SSCs in the modern Milky Way and one in the Large Magellanic Cloud (LMC), and all three of them are millions of years old. <\/p>\n
New JWST observations have found another SSC forming in the LMC, and it\u2019s only 100,000 years old. What can astronomers learn from it?<\/p>\n
<\/p>\n SSCs are responsible for a lot of star formation, but billions of years have passed since their heyday. Finding a young one in a galaxy so close to us is a boon for astronomers. It gives them an opportunity to wind back the clock and see how SSCs are born.<\/p>\n New research published in The Astrophysical Journal presents the new findings. It\u2019s titled \u201cJWST Mid-infrared Spectroscopy Resolves Gas, Dust, and Ice in Young Stellar Objects in the Large Magellanic Cloud.\u201d The lead author is Omnarayani (Isha) Nayak from the Space Telescope Science Institute and NASA\u2019s Goddard Space Flight Center.<\/p>\n At about 160,000 light-years away, the LMC is close in terms of galactic neighbours. It\u2019s also face-on from our vantage point, making it easier to study. The N79 region in the LMC is a massive star-forming nebula about 1600 light-years across. The JWST used its Mid-Infrared Instrument (MIRI) and found 97 new young stellar objects (YSOs) in N79, where the newly discovered super star cluster, H72.97-69.39, is located.<\/p>\n Stellar metallicity increases over time as generations of stars are born and die. The LMC\u2019s metallic abundance is only half that of our Solar System, meaning the conditions in the new SSC are similar to when stars formed billions of years ago in the early Universe. This is another of those situations in astronomy where studying a particular object or region is akin to looking into the past. <\/p>\n \u201cStudying YSOs in the LMC gives astronomers a front-row seat to witness the birth of stars in a nearby galaxy. For the first time, we can observe individual low-mass protostars similar to the Sun forming in small clusters\u2014outside of our own Milky Way Galaxy,\u201d said Isha Nayak, lead author of this research. \u201cWe can see with unprecedented detail extragalactic star formation in an environment similar to how some of the first stars formed in the universe.\u201d<\/p>\n The YSOs near the SSC H72.97-69.39 (hereafter referred to as H72) are segregated by mass. The most massive YSOs are concentrated near H72, while the less massive are on the outskirts of N79. The JWST revealed that what astronomers used to think were single massive young stars are actually clusters of YSOs. These observations confirm for the first time that what appear to be individual YSOs are often small clusters of protostars.<\/p>\n This finding brings attention to the complex processes of early star formation. \u201cThe formation of massive stars plays a vital role in influencing the chemistry and structure of the interstellar medium (ISM),\u201d the authors write in their published research. \u201cStar formation takes place in clusters, with massive stars dominating the luminosity.\u201d<\/p>\n One of the five young stars is over 500,000 times more luminous than the Sun. As revealed by the JWST Near InfraRed Camera (NIRCam), it\u2019s surrounded by more than 1,550 young stars.<\/p>\n Previous Atacama Large Millimeter\/submillimeter Array (ALMA) observations hinted at what might contribute to the formation of SSCs. ALMA showed that colliding filaments of molecular gas at least one parsec long are in the region. These filaments could be behind H72\u2019s formation. <\/p>\n This work highlights JWST\u2019s power to resolve complex star formation locations in other galaxies. Not only did the JWST show us that what appeared to be individual YSOs are actually groups of stars, but it allowed the researchers to determine their mass accretion rates and chemical properties. The JWST\u2019s new data gives astronomers new insights into complex chemistry, including the presence of organic molecules, dust, and ice in star-forming regions. <\/p>\n![\"A](\"https:\/\/www.universetoday.com\/wp-content\/uploads\/2025\/01\/NIRCAM_composite-B187-BRP335-Y444-1024x464-2.jpg\")
![\"This](\"https:\/\/www.universetoday.com\/wp-content\/uploads\/2025\/01\/apjad18bcf1_hr.jpg\")
![\"This](\"https:\/\/www.universetoday.com\/wp-content\/uploads\/2025\/01\/apjab1b38f5_hr-1024x749.jpg\")
Like this:<\/h3>\n