How neighboring large stars form planetary techniques | EUROtoday

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La discovery that made the entrance web page of the journal Science this week sheds new mild on the formation of planetary techniques. Thanks to the James-Webb house telescope and the Atacama Large Millimeter Array (Alma), a global workforce of astronomers led by Frenchman Olivier Berné, CNRS researcher on the Toulouse Institute for Research in Astrophysics and Planetology (IRAP), seen that the highly effective ultraviolet radiation emitted by large stars within the Orion Nebula eradicated the fuel current within the protoplanetary disk of a younger neighboring star, named d203-506, inflicting it to quickly lose its mass.

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A phenomenon that has a reputation – photoevaporation – however has by no means been documented on this means. “The fact that massive stars play a role in planet formation is something we have seen with Hubble in the past. However, we were unable to precisely measure this effect,” explains Olivier Berné to Point.

Concretely, by heating the higher layers of a protoplanetary disk, ultraviolet rays improve the temperature of the fuel it accommodates and thus trigger it to flee from the system. “The reason is relatively simple: each temperature corresponds to a level of agitation of atoms and molecules. So the hotter the gas, the higher the average speed of the particles within it. However, when this speed becomes sufficiently high, the particles reach what we call the escape speed: that from which they can escape the gravitational attraction of the body around which it rotates,” explains the creator. of Destination Orion: journey aboard the James-Webb telescope*. A bit like a rocket manages to go away the Earth.

No fuel for a Jupiter!

In the case of the nascent planetary system studied by Olivier Berné and his colleagues, the speed at which its mass is lowering means that its disk may very well be emptied of fuel in simply one million years. This ought to lead to an incapacity to type fuel large sort planets like Jupiter. “At least, that leaves very little time to achieve this,” nuance Olivier Berné. It should be stated that, within the case of D203-506, the massive stars which warmth the fuel are ten occasions extra large than the Sun and 100 thousand occasions extra luminous, whereas the younger star on the heart of the disk is ten occasions extra much less large than our personal star. Suffice it to say that the battle between the results of the ultraviolet of the previous and the gravity of the latter is very unequal!

It follows that the function of those neighboring large stars is essential for the evolution of the planetary techniques which they contribute, to a sure extent, to shaping. Their affect is all of the extra necessary because the mass of the star on the heart of the system is low. This is a vital discovery insofar as, past this primary instance and even past the Orion Nebula, a lot of the low-mass stars round which planets type are born in clusters which, just like the well-known cosmic nursery, additionally shelter different very large stars.

“We also think that the solar system was also formed near massive stars. We have evidence of this in meteorites in the form of chemical traces. If Jupiter exists, it is very probably because our star had a gravitational field strong enough to retain the gas necessary for its formation,” notes Olivier Berné. This is sufficient to provide a brand new understanding of the historical past of our photo voltaic system in addition to all these fashioned round stars apart from ours.

* Destination Orion: journey aboard the James-Webb telescopeDunod editions, 2023.


https://www.lepoint.fr/astronomie/comment-les-etoiles-massives-voisines-faconnent-les-systemes-planetaires-29-02-2024-2553911_1925.php