Skip to main content

Starbreath

This article was published in Scientific American’s former blog network and reflects the views of the author, not necessarily those of Scientific American


Deserving of a quick post is a series of extraordinary time-lapse movies showing the complex motion of jets of matter expelled from baby-stars. Followed for more than ten years by the Hubble Space Telescope these systems are some 1,300 light years from us. These proto-stellar objects are just a few millions of years into their growth, surrounded by dense disks of gas and dust the rapidly spinning central stellar infants (not yet compressed enough to initiate full-blown hydrogen fusion in their cores) squirt out jets of matter moving at hundreds of thousands of kilometers and hour. These are most likely channeled and accelerated through magnetic fields generated by the inner disks and the forming stars.

Three examples of the structures produced as high velocity material in proto-stellar jets collides with surrounding interstellar matter, producing "bow-shocks" as the supersonic jets crash into their surroundings.

As the jets plow out into interstellar space the hot particles dump out their kinetic energy as photons of light. Colliding and smashing like water sloshing down a slide this hot matter also pushes into the surrounding nebula out of which the stars formed. It's an amazing phase in the life-cycle of stars, and coincides with the first steps towards the coagulation of planetary bodies in the rich disks of material surrounding them.


On supporting science journalism

If you're enjoying this article, consider supporting our award-winning journalism by subscribing. By purchasing a subscription you are helping to ensure the future of impactful stories about the discoveries and ideas shaping our world today.


Below is one of the time-lapse movies showing the jet from the proto-star Herbig-Haro 34, in Orion. This stitched together footage spans a total of thirteen years, from 1994 to 2007.

 

Loading player...

NASA, ESA, P. Hartigan (Rice University), G. Bacon (STScI)