Skip to main content

See baby stars being born in the beautiful Butterfly Nebula

Officially known as W40, this red butterfly in space is a nebula, or a giant cloud of gas and dust. The “wings” of the butterfly are giant bubbles of gas being blown from the inside out by massive stars. NASA/JPL-Caltech

NASA’s Spitzer Space Telescope was launched in 2003 and was supposed to only be on its mission for two and a half years. But remarkably enough, 16 years later the little telescope that could is still going. Now astronomers working with the data the telescope recorded have shared this infrared image of a beautiful nebula that acts as a nursery for baby stars.

The nebula is named Westerhout 40 (W40), and has been nicknamed the Butterfly Nebula because its shape looks like the wings of a butterfly. The giant cloud of dust and gas is a space in which new stars are formed, and the “wings” of the butterfly were created when the hottest stars in the middle of the nebula blow off warm interstellar gas, forming enormous bubbles.

The picture is a composition of four images taken by Spitzer using its Infrared Array Camera (IRAC) during the prime phase of its mission. The images were taken at different wavelengths of infrared light in order to capture the different chemical features of the nebula. The wavelengths captured were 3.6, 4.5, 5.8 and 8.0 μm (shown as blue, green, orange, and red respectively).

In the image you can see lots of activity in the 8.0 μm wavelength, shown in red. This is caused by polycyclic aromatic hydrocarbons (PAHs), compounds containing only hydrogen and oxygen, which are excited by interstellar radiation and give off infrared light at this wavelength. The blue-tinted specks are stars which give off infrared radiation at a lower wavelength, and some very young stars are surrounded by clouds of dust which give off infrared radiation shown in yellow.

New stars are born in the nebula when clouds of dust and gas experience gravitational forces which pull them together into clumps. If they are dense enough, these clumps can form a star in their center. But this very process leads to stars giving off strong stellar winds which push the gas and dust away, breaking up clumps and preventing new stars from forming. This is what gave rise to the butterfly wings, as massive stars ten times the size of our Sun are formed in the center of the nebula and eject material outwards to form the bubbles.

Editors' Recommendations

Georgina Torbet
Georgina is the Digital Trends space writer, covering human space exploration, planetary science, and cosmology. She…
James Webb telescope captures the gorgeous Ring Nebula in stunning detail
JWST/NIRcam composite image of the Ring Nebula. The images clearly show the main ring, surrounded by a faint halo and with many delicate structures. The interior of the ring is filled with hot gas. The star which ejected all this material is visible at the very centre. It is extremely hot, with a temperature in excess of 100,000 degrees. The nebula was ejected only about 4000 years ago. Technical details: The image was obtained with JWST's NIRCam instrument on August 4, 2022. Images in three different filters were combined to create this composite image: F212N (blue); F300M (green); and F335M (red).

A new image from the James Webb Space Telescope shows the stunning and distinctive Ring Nebula -- a gorgeous structure of dust and gas located in the constellation of Lyra. This nebula is a favorite among sky watchers as it faces toward Earth so we can see its beautiful structure, and because it is visible throughout the summer from the Northern Hemisphere. It is different from the Southern Ring nebula, which Webb has also imaged, but both are a type of object called a planetary nebula.

Located just 2,600 light-years away, the Ring Nebula is a structure of dust and gas that was first observed in the 1770s, when it was thought to be something like a planet. With advances in technology, astronomers realized it was not a planet, but rather a cloud of dust and gas, and thanks to highly detailed observations by space telescopes like Hubble and Webb, scientists have been able to see more of its complex structure. The nebula isn't a simple sphere or blob, but is rather a central, football-shaped structure surrounded by rings of different material.

Read more
This star shredded its companion to create a stunning double-lobed nebula
A billowing pair of nearly symmetrical loops of dust and gas mark the death throes of an ancient red-giant star, as captured by Gemini South, one half of the International Gemini Observatory, operated by NSF’s NOIRLab. The resulting structure, said to resemble an old style of English jug, is a rarely seen bipolar reflection nebula. Evidence suggests that this object formed by the interactions between the dying red giant and a now-shredded companion star. The image was obtained by NOIRLab’s Communication, Education & Engagement team as part of the NOIRLab Legacy Imaging Program.

Nebulae are some of the most beautiful structures to be found in space: vast clouds of dust and gas that are illuminated by light from nearby stars. These regions are often busy sites of star formation, as new stars are born from clumps of dust that collect more material due to gravity. Within the category of nebulae, there are different types such as emission nebulae, where the gases are ionized by radiation and glow brightly, or supernova remnants, which are the structures left behind after massive stars come to the end of their lives and explode.

A recent image captured by NOIRLab's Gemini South telescope shows a rare type of nebula called a bipolar reflection nebula. Known as the Toby Jug Nebula for its similar shape to a traditional English jug, nebula IC 2220 is 1,200 light-years away in the constellation of Carina, or the Keel.

Read more
James Webb detects important molecule in the stunning Orion nebula
This image is NIRCam’s view of the Orion Bar region studied by the team of astronomers. Bathed in harsh ultraviolet light from the stars of the Trapezium Cluster, it is an area of intense activity, with star formation and active astrochemistry. This made it a perfect place to study the exact impact that ultraviolet radiation has on the molecular makeup of the discs of gas and dust that surround new stars. The radiation erodes the nebula’s gas and dust in a process known as photoevaporation; this creates the rich tapestry of cavities and filaments that fill the view. The radiation also ionises the molecules, causing them to emit light — not only does this create a beautiful vista, it also allows astronomers to study the molecules using the spectrum of their emitted light obtained with Webb’s MIRI and NIRSpec instruments.

The Orion Nebula is famous for its beauty, but it was also the site of a recent exciting scientific discovery. The James Webb Space Telescope has detected an important molecule in a planet-forming disk of debris within the nebula. The molecule, called methyl cation (CH3+), is a carbon compound that is important for the formation of life and has never been observed in space before.

This image is NIRCam’s view of the Orion Bar region studied by the team of astronomers. Bathed in harsh ultraviolet light from the stars of the Trapezium Cluster, it is an area of intense activity, with star formation and active astrochemistry. This made it a perfect place to study the exact impact that ultraviolet radiation has on the molecular makeup of the discs of gas and dust that surround new stars. ESA/Webb, NASA, CSA, M. Zamani (ESA/Webb), the PDRs4All ERS Team

Read more