Alignment of bipolar jets confirms star formation theories

First of its kind detection made in striking new Webb image

Share

Follow us onFollow Tech Explorist on Google News

For the first time, a phenomenon astronomers have long hoped to image directly has been captured by the NASA/ESA/CSA James Webb Space Telescope’s Near-InfraRed Camera (NIRCam). In this stunning image of the Serpens Nebula, the discovery lies in the northern area of this young, nearby star-forming region.

The astronomers found an intriguing group of protostellar outflows, formed when jets of gas spewing from newborn stars collide with nearby gas and dust at high speeds. Typically these objects have a variety of orientations within one region. Here, however, they are all slanted in the same direction, to the same degree, like sleet pouring down during a storm.

The discovery of these aligned objects, made possible only by Webb’s exquisite spatial resolution and sensitivity at near-infrared wavelengths, is providing information about the fundamentals of how stars are born.

So just how does the alignment of the stellar jets relate to the rotation of the star? As an interstellar gas cloud collapses in on itself to form a star, it spins more rapidly. The only way for the gas to continue moving inward is for some of the spin (known as angular momentum) to be removed. A disc of material forms around the young star to transport material down, like a whirlpool around a drain. The swirling magnetic fields in the inner disc launch some of the material into twin jets that shoot outward in opposite directions, perpendicular to the disc of material.

In the Webb image, these jets are identified by bright red clumpy streaks, which are shockwaves caused when the jet hits the surrounding gas and dust. Here, the red colour indicates the presence of molecular hydrogen and carbon monoxide. Webb can image these extremely young stars and their outflows, which were previously obstructed at optical wavelengths.

Astronomers say there are a few forces that potentially can shift the direction of the outflows during this period of a young star’s life. One way is when binary stars spin around each other and wobble in orientation, twisting the direction of the outflows over time.

Stars of the Serpens Nebula

The Serpens Nebula is only one or two million years old, which is very young in cosmic terms. It’s also home to a particularly dense cluster of newly forming stars (around 100 000 years old) at the centre of this image, some of which will eventually grow to the mass of our Sun.

Serpens Nebula (NIRCam compass Image)
This image of the Serpens Nebula, captured by Webb’s Near-InfraRed Camera (NIRCam), shows compass arrows, a scale bar and a colour key for reference. The north and east compass arrows show the orientation of the image on the sky. Note that the relationship between north and east on the sky (as seen from below) is flipped relative to the direction of arrows on a map of the ground (as seen from above). The scale bar is labelled in light-years, which is the distance that light travels in one Earth-year. One light-year is equal to about 9.46 trillion kilometres, or 5.88 trillion miles. This image shows invisible near-infrared wavelengths of light that have been translated into visible-light colours. The colour key shows which NIRCam filters were used when collecting the light. The colour of each filter name is the visible light colour used to represent the infrared light that passes through that filter. [Image description: At the centre of the image is a nebula against the black background of space. A young star-forming region is filled with wispy orange, red, and blue layers of gas and dust. The upper left corner of the image is filled with mostly orange dust, and within that orange dust, there are several small red plumes of gas that extend from the top left to the bottom right, at the same angle. The centre of the image is filled with mostly blue gas. Small points of light are sprinkled across the field; the brightest sources in the field have the eight-pointed diffraction spikes characteristic of Webb images. At lower left, a white arrow pointing in the 8 o’clock direction is labelled N for north, while an arrow pointing in the 5 o‘clock direction is labelled E for east. At top right, a scale bar is labelled .25 light-years. At the bottom is a list of NIRCam filters in different colours, from left to right: F140M (blue), F210M (cyan), F360W (orange), F480M (red).] Credit: NASA, ESA, CSA, STScI, K. Pontoppidan (NASA’s Jet Propulsion Laboratory), J. Green (Space Telescope Science Institute)

Serpens is a reflection nebula, which means it’s a cloud of gas and dust that does not create its own light but instead shines by reflecting the light from stars close to or within the nebula.

So, throughout the region in this image, filaments and wisps of different hues represent reflected starlight from still-forming protostars within the cloud. In some areas there is dust in front of that reflection, which appears here in an orange, diffuse shade.

This region has been home to other coincidental discoveries, including the flapping ‘Bat Shadow’, which earned its name when 2020 data from the NASA/ESAHubble Space Space Telescope revealed it to flap, or shift. This feature is visible at the centre of the Webb image.

Future studies

The stunning image and the serendipitous discovery of the aligned objects are actually just the first step in this scientific programme. The team will now use Webb’s NIRSpec (Near-InfraRed Spectrograph) to investigate the chemical make-up of the cloud.

Astronomers are interested in determining how volatile chemicals survive star and planet formation. Volatiles are compounds that sublimate, or transition from a solid directly to a gas, at a relatively low temperature — including water and carbon monoxide. They’ll then compare their findings to the amounts found in protoplanetary discs of similar-type stars.

Here’s more reading you might find interesting:

These observations were made as part of the Webb General Observer programme 1611 (PI: K. Pontoppidan). The team’s initial results have been published in the Astrophysical Journal.

Journal Reference

  1. Joel D. Green, Klaus M. Pontoppidan, Megan Reiter, Dan M. Watson, Sachindev S. Shenoy, P. Manoj, and Mayank Narang. Why are (almost) all the protostellar outflows aligned in Serpens Main? Science Paper
University

Trending