Gotcha! 📸
For the first time, a phenomenon astronomers have long hoped to image directly has been captured by
@esawebb in a beautiful view that is revealing secrets about how stars are born!
In the Serpens Nebula, a young star-forming region, Webb’s captured a surprising discovery: jets of gas from newborn stars, all pointing in the same direction! Normally, these jets are chaotic, but here, they’re aligned like sleet in a storm.
So just how does the alignment of the stellar jets relate to the rotation of the star? As an interstellar gas cloud collapses in on itself to form a star, it spins more rapidly. The only way for the gas to continue moving inward is for some of the spin (known as angular momentum) to be removed. A disc of material forms around the young star to transport material down, like a whirlpool around a drain. The swirling magnetic fields in the inner disc launch some of the material into twin jets that shoot outward in opposite directions, perpendicular to the disc of material.
In the Webb image, these jets are identified by bright red clumpy streaks, which are shockwaves caused when the jet hits the surrounding gas and dust. Here, the red colour indicates the presence of molecular hydrogen and carbon monoxide. Webb can image these extremely young stars and their outflows, which were previously obstructed at optical wavelengths.
Astronomers say there are a few forces that potentially can shift the direction of the outflows during this period of a young star’s life. One way is when binary stars spin around each other and wobble in orientation, twisting the direction of the outflows over time.
Webb instrument will now analyze the gas and dust to understand how volatile chemicals survive star and planet formation.
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@NASA ,
@europeanspacagency ,
@canadianspaceagency ,
@space_telescopes , K. Pontoppidan (
@nasajpl ), J. Green (Space Telescope Science Institute)
📹 NASA, ESA, CSA, A. Pagan (STScI)
Acknowledgement: Akira Fujii, Digitized Sky Survey, Spitzer Space Telescope
📹 NASA, ESA, CSA, STScI, K. Pontoppidan (NASA’s Jet Propulsion Laboratory), J. Green (Space Telescope Science Institute), N. Bartmann (ESA/Webb)