Scientists may have discovered a clue to how massive stars form in the Orion Nebula and a stellar birthplace.

An explosive outflow of molecular gas within the Orion Nebula
This composite, false-color image reveals an explosive outflow of molecular gas within the Orion Nebula. A new study explores another such explosion and examines how it relates to the birth of massive stars.
ALMA / ESO / NAOJ / NRAO / J. Bally / H. Drass et al.

There’s still much we don’t know about the birth of massive stars — stars with more than 8 times the mass of the Sun. A recent study reveals details of a thousand-year-old explosion that might provide clues about the formation of these giants.

An Unexpected Explosion

The Orion Nebula
The clouds of molecular gas in regions like the Orion nebula provide nurseries in which massive stars form and evolve.
ESO / G. Beccari

Several decades ago, astronomers discovered something odd. In a region inside the Orion Nebula where massive star formation is underway, scientists detected signs of an explosive outflow: dense molecular gas streaming outward from a central point at rapid speeds. Surprisingly, there was nothing at the center of this explosion.

This one-off discovery was intriguing. One could imagine a number of sudden, energy-liberating events that could occur in a massive star-forming environment — like the formation of a close massive stellar binary, or the merger of two young, massive protostars. And the discovery of several candidate runaway stars at the fringes of the explosion provided another hint to a dynamical origin.

Could this explosion help us understand the process of how massive stars form in their birth environments? Or was it just a fluke event? As years passed without astronomers finding evidence of another, similar outflow, these questions remained unanswered.

Two of a Kind

The star-forming region G5.89
This ALMA SiO map of the star-forming region G5.89 shows outflowing molecular gas surrounding an expanding, shell-like HII region (white contours). Two stars moving away from the origin are marked in magenta and cyan.
Adapted from Zapata et al. 2020

Forty years later, we now have proof of another such explosive outflow in a massive star-forming environment. In a recent publication led by Luis Zapata (UNAM Radio Astronomy and Astrophysics Institute, Mexico), a team of scientists has used the Atacama Large Millimeter/submillimeter Array (ALMA) to confirm the presence of streamers of molecular gas flowing isotropically outward from a central point in the massive stellar birthplace G5.89, which lies roughly 10,000 light-years away from us.

Zapata and collaborators measured 34 molecular filaments in this explosive outflow, finding that the streamers are accelerating as they expand outward. This is consistent with behavior of the Orion explosion and shows that the density of the ejecta is substantially larger than the surrounding medium.

As with the Orion explosive outflow, the point of origin of the filaments contains no source. Previous studies, however, have identified several young, massive stars in the periphery of the G5.89 explosion that are speeding away from the point of origin at roughly the right speed to have been at the center 1,000 years previously at the time of explosion.

Learning about Stellar Birth

A visualization of a protostar embedded in a disk of gas and dust
A protostar lies embedded in a disk of gas and dust in this visualization. The collision of two protostars could release enough energy to power an explosive molecular outflow — and produce a massive star.
NASA’s Goddard SFC

What does all this tell us about the origins of massive stars? Explosive outflows like this — caused by dynamical interactions during the birth of massive stars — may be more common than we previously thought!

The authors estimate a rate for such outflows based on our limited observations, finding that there should be one every ~100 years. The fact that this is very close to the rate of supernovae further solidifies the connection of explosive molecular outflows to massive star formation.

Dedicated, high-sensitivity searches for more such outflows in nearby massive star-forming regions will certainly go a long way toward confirming this theory. In the meantime, the authors argue, we should consider revising high-mass star formation models to include dynamical interactions, as these stellar explosions may prove to be regular occurrences!


Zapata et al. 2020

The animation below shows a different view of the authors’ ALMA-observed streamers, traced by CO gas. Two axes give the position of observations, while the third axis and the colors show the radial velocity at each point in the streamers, showing how the ejecta are accelerating as they expand outward. The star marks the origin of the explosive outflow.


“Confirming the Explosive Outflow in G5.89 with ALMA,” Luis A. Zapata et al 2020 ApJL 902 L47. doi:10.3847/2041-8213/abbd3f

This post originally appeared on AAS Nova, which features research highlights from the journals of the American Astronomical Society.


Image of Anthony Barreiro

Anthony Barreiro

February 25, 2021 at 9:37 pm

The ALMA map lacks the Right Ascension axis, so it's impossible to tell where G5.89 is in the sky. This report on has the same map, with RA:

G5.89 is in Sagittarius. It looks to me like it's in the Lagoon nebula.

Unlike professional astronomers, we amateurs want to know where things are in the sky.

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Image of Yaron Sheffer

Yaron Sheffer

March 3, 2021 at 12:51 pm

Good catch! Having both axes annotated is always helpful 🙂

Close but no cigar: this object is about half a width of M8 to the west of M8's western border (visually). But G5.89 is pretty much invisible, unless viewed in the Infrared. It is also about twice as far as M8 from here, and "suffering" higher interstellar extinction.

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