science & techESA/Hubble

Infant star’s artistic outburst

the gist

HH 34 is a Herbig-Haro object, a glowing patch of gas about 1,400 light-years away near the Orion Nebula. It is produced when a hot, blue jet of gas, launched by a very young star still wrapped in dust, crashes into slower material ahead of it. The jet is heated where it collides and glows visibly. The knots and ripples along the jet are thought to come from several outbursts from the star that have caught up with one another over time. Herbig-Haro objects last only a few thousands of years, which is brief on astronomical timescales. Hubble has been able to see changes in them across observations only a few years apart.

so what

Herbig-Haro objects are a direct record of how young stars shed material as they form. They show how stars push back against their surroundings during the earliest stage of their lives.

fun fact

Herbig-Haro objects are named after the astronomers George Herbig and Guillermo Haro, who studied them independently.

ESA/Hubble · CC BY 4.0

Image: ESA/Hubble & NASA