Hubble Space Telescope captures the earliest stage of star formation

By Georgina Torbet November 20, 2022

This week’s image from the Hubble Space Telescope shows a beautiful cloud of dust and gas located in the constellation of Serpens. This cloud is a type of object called a dense core, with enough densely packed material that it could one day be the birthplace of a new star.

The object, called CB 130-3, makes an interesting companion to the protostar image recently shared from the James Webb Space Telescope. This Hubble image shows the earliest phase of star formation, in which dust and gas come together to form a core, while the Webb image shows the next phase of development in which the core is dense enough to attract more material via gravity and starts rotating and giving off jets.

A small, dense cloud of gas and dust called CB 130-3 blots out the center of this image from the NASA/ESA Hubble Space Telescope. CB 130-3 is an object known as a dense core, a compact agglomeration of gas and dust. This particular dense core is in the constellation Serpens and seems to billow across a field of background stars. — A small, dense cloud of gas and dust called CB 130-3 blots out the center of this image from the NASA/ESA Hubble Space Telescope. ESA/Hubble, NASA & STScI, C. Britt, T. Huard, A. Pagan

You can’t see the core itself in the Hubble image, as it is deep within the cloud, but you can see how the cloud is not a uniform sphere but rather has patches that are either denser or less dense.

“As this image shows, the density of CB 130-3 isn’t constant; the outer edges of the cloud consist of only tenuous wisps, whereas at its core CB 130-3 blots out background light entirely,” Hubble scientists said. “The gas and dust making up CB 130-3 affect not only the brightness but also the apparent color of background stars, with stars toward the cloud’s center appearing redder than their counterparts at the outskirts of this image. Astronomers used Hubble to measure this reddening effect and chart out the density of CB 130-3, providing insights into the inner structure of this stellar nursery.”

The image was taken using Hubble’s Wide Field Camera 3 instrument, which looks at the visible light spectrum. This makes Hubble a useful companion to Webb, which looks in the infrared range. By looking at objects in a variety of different wavelengths, astronomers can pick out different physical features and see interior structures which would otherwise be invisible.

Editors' Recommendations

Topics

Tech News

Georgina Torbet

Space Writer

Georgina is the Digital Trends space writer, covering human space exploration, planetary science, and cosmology. She…

Space

Researchers discover a 320-mph jet stream around Jupiter’s equator

This image of Jupiter from NASA’s James Webb Space Telescope’s NIRCam (Near-Infrared Camera) shows stunning details of the majestic planet in infrared light. In this image, brightness indicates high altitude. The numerous bright white "spots" and "streaks" are likely very high-altitude cloud tops of condensed convective storms. Auroras, appearing in red in this image, extend to higher altitudes above both the northern and southern poles of the planet. By contrast, dark ribbons north of the equatorial region have little cloud cover. In Webb’s images of Jupiter from July 2022, researchers recently discovered a narrow jet stream traveling 320 miles per hour (515 kilometers per hour) sitting over Jupiter’s equator above the main cloud decks.

The James Webb Space Telescope might be best known for its study of extremely distant galaxies, but it is also used for research on targets closer to home, like planets within our solar system. Last year, the telescope captured a stunning image of Jupiter as seen in the infrared wavelength, and now scientists who have been working on this data have published some of their findings about the planet -- including a brand-new feature that they identified in its atmosphere.

This image of Jupiter from NASA’s James Webb Space Telescope’s NIRCam (Near-Infrared Camera) shows stunning details of the majestic planet in infrared light. In Webb’s images of Jupiter from July 2022, researchers recently discovered a narrow jet stream traveling 320 miles per hour (515 kilometers per hour) sitting over Jupiter’s equator above the main cloud decks. NASA, ESA, CSA, STScI, Ricardo Hueso (UPV), Imke de Pater (UC Berkeley), Thierry Fouchet (Observatory of Paris), Leigh Fletcher (University of Leicester), Michael H. Wong (UC Berkeley), Joseph DePasquale (STScI)

Space

James Webb captures a gorgeous stellar nursery in nearby dwarf galaxy

This new infrared image of NGC 346 from NASA’s James Webb Space Telescope’s Mid-Infrared Instrument (MIRI) traces emission from cool gas and dust. In this image blue represents silicates and sooty chemical molecules known as polycyclic aromatic hydrocarbons, or PAHs. More diffuse red emission shines from warm dust heated by the brightest and most massive stars in the heart of the region. Bright patches and filaments mark areas with abundant numbers of protostars. This image includes 7.7-micron light shown in blue, 10 microns in cyan, 11.3 microns in green, 15 microns in yellow, and 21 microns in red (770W, 1000W, 1130W, 1500W, and 2100W filters, respectively).

A gorgeous new image from the James Webb Space Telescope shows a stunning sight from one of our galactic neighbors. The image shows a region of star formation called NGC 346, where new stars are being born. It's located in the Small Magellanic Cloud, a dwarf galaxy that is a satellite galaxy to the Milky Way.

The star-forming region of the Small Magellanic Cloud (SMC) was previously imaged by the Hubble Space Telescope in 2005, but this new image gives a different view as it is taken in the infrared wavelength by Webb instead of the optical light wavelength used by Hubble.

Space

Zoom into an incredibly detailed James Webb image of the Orion nebula

A short-wavelength NIRCam mosaic of the inner Orion Nebula and Trapezium Cluster.

A new image from the James Webb Space Telescope shows the majesty of the gorgeous Orion nebula in tremendous detail. The European Space Agency (ESA) has shared an extremely high-resolution version of the image that you can zoom into to see the details of this stunning cloud of dust and gas which hosts sites of star formation where new stars are being born.

The full image is available to view in the ESASky application, where you can zoom in a compare images of the same target taken in different wavelengths. There's also a very large version of the image if you want to download and pursue it at your leisure.