A distant star far from Earth is displaying some remarkable activity. Thanks to the James Webb Space Telescope, we can see this massive star firing off powerful jets into space, forming a structure known as Sharpless 2-284, or Sh2-284 for short. These jets stretch across eight light-years and travel at incredible speeds—hundreds of thousands of miles per hour. Their existence gives us a peek into how the universe’s largest stars are born.
Jonathan Tan, an astrophysicist from the University of Virginia, states, “Once we found a massive star launching these jets, we realized we could use the Webb observations to test theories of massive star formation.” This highlights the importance of these discoveries as they contribute to our understanding of stellar birth.
Stellar jets are common among lower-mass stars, but for more massive stars—those that eventually go supernova—forming these jets happens in a chaotic way. The material falling into these stars creates a disk around the protostar, and excess material is ejected in jets, thanks to magnetic fields. Interestingly, the jets from Sh2-284 appear straight and stable, suggesting that the formation process was quite orderly.
Tan suggests that this star is around ten times the mass of our Sun and is still growing. The characteristics of the jets—such as their energy and shape—give astronomers clues about the environment where these stars form. Yu Cheng, who led the JWST observations, notes that such a significant outflow of hydrogen is rare in our galaxy, making this find even more exciting.
The location of Sh2-284 is also noteworthy. It sits about 15,000 light-years from us, in an area with low amounts of heavy elements, often referred to as “metals.” This is because heavy elements are typically created within stars, and star formation in this part of the galaxy hasn’t produced many. Studying a star in this low-metallicity environment is valuable to scientists, as it mimics conditions prevalent in the early universe.
Cheng emphasizes that this discovery helps illuminate how massive stars form in these unique environments, allowing us to better understand cosmic history. The jets of Sh2-284 are not static; they tell the story of the star’s life, with the oldest material found at the tips and younger material trailing behind.
As impressive as the jets and nebula are, they are temporary. Eventually, the star will emerge fully grown, possibly weighing several times more than our Sun. It will have a brief lifespan of a few million years before exploding in a supernova, enriching space with new heavy elements.
Observations of Sh2-284 were recently published in The Astrophysical Journal, providing exciting insights into the processes that shape our universe.