Stellar Wind Kicks Up Dust ✎ express

Original: "JOYS: Launching and destruction of dust in protostellar jets. The case of BHR71-IRS1 with JWST/MIRI"
arXiv:2604.11904 · 2026-04-13 · arXiv non-exclusive · independent analysis · 1 min
The James Webb Telescope has for the first time seen a newborn star ejecting not just gas but also dust grains.

A newborn star is like a kitchen mixer: it whips up the surrounding cloud, and splatters fly in all directions. Only instead of batter, it's gas and dust. Previously, astronomers had only seen gas jets, and dust was considered too fragile: the shock wave should shatter dust grains into atoms.

The James Webb Space Telescope peered into the cloud BHR71, where a star is just beginning its life. The MIRI instrument split the jet's light into thousands of shades and found lines of iron, nickel, and cobalt — elements that make up dust grains. But some of these elements remained in the dust: it survived the shock and flew off with the gas. The dust is warm, 200–400 kelvins, like a heated skillet.

The star's jet strikes at 70 kilometers per second — faster than a bullet. Yet the dust grains withstand this impact.

This is the first time dust has been caught in the jet of such a young star. This means that stars, from the moment of birth, scatter the building material for future planets and even for new stars. The cloud BHR71 is like an invisible hand sowing dust across the galaxy.

The jet from star BHR71 moves 200 times faster than the speed of sound in air, yet the dust grains in it do not burn up but fly onward.

Scientists
Ludwig BoltzmannSubrahmanyan ChandrasekharEnrico FermiJames JeansCecilia Payne-GaposchkinMichael Faraday
Concepts
protoplanetary disk winds dust protoplanetary disk dust grain jet supernova jets star formation gas relativistic jets james webb space telescope snow line gas star formation regions first stars miri erg first stars nucleosynthesis crust young stellar object interstellar space millimeter emission