When massive stars – many times larger than our Sun – are born, they shine hot and bright before eventually exploding as supernovas – in fact, they release so much energy that they can affect the evolution of galaxies.
But, unlike stars like our Sun, astronomers know much less about how these enormous stars form.
“Massive stars like this represent less than one percent of all stars, but they can affect the formation of their stellar siblings,” says Jim de Buizer, Universities Space Research Association senior scientist at the SOFIA Science Centre. “Stars like our Sun have much quieter and humbler origins, and because there are so many of them, we understand their birth properties more thoroughly.”
To learn more, researchers used the Stratospheric Observatory for Infrared Astronomy, or SOFIA, to study a giant celestial cloud, called W51. Located almost 17 000 light years away and made mostly of hydrogen, it’s a place where rare, gigantic stars are forming. But they are born deep inside the cloud, invisible to the light our eyes can see.
Using SOFIA’s airborne telescope and sensitive infrared camera, the research team peered inside the dense cloud. They captured a cosmic light show sparked by the forming stars, including many that have never been seen before.
The infrared camera, called Faint Object infraRed CAmera for the SOFIA Telescope, or FORCAST, has sensitive detectors and powerful magnification that let the researchers discover the enormous stars right after their birth. Learning how massive stars form in our Milky Way Galaxy helps scientists understand how these stars form in distant galaxies that are too far away to see in detail.
“This is the best resolution currently available using these wavelengths of infrared light,” said Wanggi Lim, Universities Space Research Association scientist at the SOFIA Science Centre. “Not only does this reveal areas that we could not see before, but it’s critical to understanding the physical properties and relative age of the stars and their parental clouds.”
Researchers combined the SOFIA data with data from NASA’s Spitzer Space Telescope and Herschel Space Observatory to analyze the stars. They found that while they are all young, some are more evolved, and others are the youngest, most recently-created stars in the cloud.
One may be exceptionally large – estimated to have the equivalent mass of 100 Suns. If future observations confirm it is indeed a single, colossal star, rather than multiple stellar siblings clustered together, it would be one of the most massive forming stars in our galaxy.
These are the first results from a survey that will reveal how young, massive stars are lighting up other parts of our Milky Way Galaxy.
Pictured: A cosmic light show sparked by the formation of massive stars in the stellar nursery, called W51, glows over on a star field image (white) from the Sloan Digital Sky Survey. The oldest and most evolved massive star is in the upper left of the image, shown at the middle of yellowish bubble. The youngest generations are typically found in areas near the center of this figure, near the brightest ball at the slight left from the middle. Massive stars like these emit so much energy that they play a critical role in the evolution of our galaxy.
Credits: NASA/SOFIA/Lim and De Buizer et al and Sloan Digital Sky Survey