Stars are born in vast, chilly clouds of gas and dust that collapse under gravity. Recently, scientists uncovered a huge molecular cloud called Eos, located about 300 light-years from Earth. This cloud might be the closest of its kind to our solar system, and it offers a fantastic opportunity for astronomers to study how stars form.
Eos is remarkable not just for its size, but also because it helps us understand the star-making process. It resides in the Local Bubble, a region filled with hot plasma and surrounded by gas and dust. Scientists usually locate molecular clouds by observing dust emissions, but Eos was discovered by detecting the far-ultraviolet glow of hydrogen, which is challenging to see from Earth. According to Blakesley Burkhart, a professor at Rutgers University and the lead author of this discovery, “This is the first-ever molecular cloud discovered by looking for far ultraviolet emission of molecular hydrogen directly.”
Molecular hydrogen is crucial yet elusive, being the most common molecule in the universe. It glows in wavelengths that the Earth’s atmosphere absorbs, making it tough to observe. Burkhart explained, “The data showed glowing hydrogen molecules detected via fluorescence in the far ultraviolet. This cloud is literally glowing in the dark.”
The Eos cloud has a crescent shape and spans an area equivalent to 40 full Moons. Its mass is about 3,400 times that of the Sun. The method used to discover Eos could lead to the identification of more hidden clouds across the Milky Way galaxy.
Burkhart emphasized the significance of this discovery, stating, “When we look through our telescopes, we catch whole solar systems in the act of forming, but we don’t know in detail how that happens. Our discovery of Eos is exciting because we can now directly measure how molecular clouds are forming and how interstellar gas and dust transform into stars and planets.”
As our understanding of such molecular clouds grows, we may unlock more secrets about the universe’s evolution. Recent studies show that similar clouds could help scientists get insights into star formation rates and the lifecycle of galaxies. This could potentially lead to advancements in our grasp of cosmology.
For further reading on this fascinating topic, you can explore the complete findings in this Nature Astronomy paper.
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