Skip to content
Starts With A Bang

Inside JWST’s first view of the Local Group’s edge

By studying the dwarf galaxy Wolf-Lundmark-Melotte ~3 million light-years away, JWST reveals the Universe's star-forming history firsthand.
A wide-field view of dwarf galaxy Wolf-Lundmark-Melotte (WLM), alongside with the region that JWST imaged using its NIRCam instrument (inset). The power of JWST to reveal individual stars, even the faint, low-luminosity ones, in galaxies like this one located ~3 million light-years away is poised to set us on a better path toward understanding the star-formation history in our Universe across cosmic time.
(Credits: ESO; Acknowledgement: VST/OmegaCAM Local Group Survey; NASA, ESA, CSA, K. McQuinn (RU); Processing: Z. Levay (STScI); Edits: E. Siegel)
Key Takeaways
  • In the beginning, the Universe was made almost exclusively of hydrogen and helium, only forming heavier elements in the aftermath of star-formation.
  • While large, massive, Milky Way-like galaxies form stars continuously over many billions of years, many smaller ones formed stars practically all at once, giving us a glimpse into the cosmic past.
  • One such galaxy, Wolf-Lundmark-Melotte (WLM), resides here in our Local Group, just 3 million light-years away. Here's what the JWST saw when it looked inside.

How and when did the stars in the Universe form?

how many stars
The cluster Terzan 5 has many older, lower-mass stars present within (faint, and in red), but also hotter, younger, higher-mass stars, some of which will generate iron and even heavier elements. It contains a mix of Population I and Population II stars, indicating that this cluster underwent multiple episodes of star formation. The different properties of different generations can lead us to draw conclusions about the initial abundances of the light elements and holds clues as to the star-formation history of our cosmos.
(Credit: NASA/ESA/Hubble/F. Ferraro)

To answer, we must look back across cosmic time.

Galaxies comparable to the present-day Milky Way are numerous throughout cosmic time, having grown in mass and with more evolved structure at present. Younger galaxies are inherently smaller, bluer, more chaotic, richer in gas, and have lower densities of heavy elements than their modern-day counterparts. Because of their great distances, it’s impossible to resolve individual stars inside all but the nearest galaxies.
(Credit: NASA, ESA, P. van Dokkum (Yale U.), S. Patel (Leiden U.), and the 3-D-HST Team)

But individual stars are only resolvable in nearby galaxies.

This image, perhaps surprisingly, showcases stars in the Andromeda Galaxy’s halo. The bright star with diffraction spikes is from within our Milky Way, while the individual points of light seen are mostly stars in our neighboring galaxy: Andromeda. Beyond that, however, a wide variety of faint smudges, galaxies in their own right, lie beyond. Individual stars can be resolved in galaxies up to tens of millions of light-years away, but that represents only one-in-a-billion galaxies overall.
(Credit: NASA, ESA, and T.M. Brown (STScI))

Big, Milky Way-like galaxies form stars all throughout their history.

The grand spiral galaxy Messier 51, also known as the Whirlpool galaxy, has sweeping, extended spiral arms, most probably owing to its gravitational interactions with the nearby neighboring galaxy shown at right. Galaxies such as this often have large waves of star formation occurring along their spiral arms, but only ~10% of spirals exhibit the type of grand, spiral structure seen here.
(Credits: X-ray: NASA/CXC/SAO/R. DiStefano, et al.; Optical: NASA/ESA/STScI/Grendler)

But smaller galaxies formed stars all-at-once, long ago, within our Local Group.

Most galaxies contain only a few regions of star-formation: where gas is collapsing, new stars are forming, and ionized hydrogen is found in a bubble surrounding that region. In a starburst galaxy, pretty much the entire galaxy itself is a star-forming region, with M82, the Cigar Galaxy located just outside of the Local Group, being the closest one with those properties. The radiation from hot, young stars ionizes a variety of atomic and molecular gases, particularly in the galaxy’s central region. Flares, supernovae, and radiation will be common in these environments.
(Credits: NASA, ESA and the Hubble Heritage Team (STScI/AURA); Acknowledgment: J. Gallagher (University of Wisconsin), M. Mountain (STScI) and P. Puxley (National Science Foundation))

One such galaxy is Wolf-Lundmark-Melotte: WLM, merely 3.04 million light-years away.

This wide-field view shows the sky around the dwarf galaxy WLM in the constellation of Cetus (The Sea Monster). This picture was created from images forming part of the Digitized Sky Survey 2. The bluish clump in the center of the image is galaxy WLM; the bright, colored, spikey points, including the red and yellow ones, are simply foreground stars within our own Milky Way.
(Credit: ESO/Digitized Sky Survey 2; Acknowledgement: Davide De Martin)

WLM, in the constellation of Cetus, is gravitationally bound to us, moving toward us at 122 km/s.

This map of many of the galaxies within the Local Group highlights the three biggest members: Andromeda, the Milky Way, and Triangulum. Galaxy WLM, shown at the bottom of the image, lies about 3 million light-years from the Milky Way and is extremely isolated. It contains some of the oldest, most pristine stars within our cosmic backyard, close enough to be resolved by observatories such as JWST.
(Credit: Richard Powell; Annotation: E. Siegel)

A large fraction of its internal stars formed suddenly: 13 billion years ago.

This image, captured by ESO’s OmegaCAM on the VLT Survey Telescope, shows a lonely galaxy known as Wolf-Lundmark-Melotte (WLM). Although considered part of our Local Group of dozens of galaxies, WLM stands alone at the group’s outer edges as one of its most remote members. Its isolation from all other Local Group members is remarkable, and helps provide a unique window into our cosmic past.
(Credit: ESO; Acknowledgement: VST/OmegaCAM Local Group Survey)

Those stars are extremely pristine, with just 0.6% of the heavy elements found in the Sun.

Here on the outskirts of dwarf galaxy Wolf-Lundmark-Melotte (WLM), stars of various colors and brightnesses can be seen as revealed by ESO’s OmegaCAM on the VLT Survey Telescope. The galaxy is so isolated that it may never have interacted or merged with any other galaxy since its formation more than 13 billion years ago, and the most metal-poor stars within it, highlighted here, support that picture.
(Credit: ESO; Acknowledgement: VST/OmegaCAM Local Group Survey)

New stars still form sporadically inside, but those “old” stars represent a relic, ancient population.

WLM’s only known globular cluster is similarly old and metal-poor.

This impressive-looking globular cluster doesn’t belong to the Milky Way, but rather to the dwarf galaxy WLM located ~3.04 million light-years away. It’s extremely metal-poor, but for some reason is the only known globular cluster that belongs to WLM.
(Credit: NASA, ESA/Hubble, and J. Schmidt (Geckzilla))

But JWST’s new view provides astounding new insights.

This view represents the full field of JWST’s NIRCam view of dwarf galaxy WLM, located on the outskirts of the Local Group. The dust within this galaxy is distributed asymmetrically, and so are the stars. The left regions of this image are located closer to the galactic center, while the right side represents regions farther away, and hence more pristine.
(Credit: NASA, ESA, CSA, K. McQuinn (RU); Processing: Z. Levay (STScI))

It’s a great improvement over Spitzer’s prior infrared view.

A portion of the dwarf galaxy Wolf–Lundmark–Melotte (WLM) captured by the Spitzer Space Telescope’s Infrared Array Camera (left) and the James Webb Space Telescope’s Near-Infrared Camera (right). The images demonstrate Webb’s remarkable ability to resolve faint stars outside the Milky Way. The incredible side-by-side improvement in resolution, light-gathering power, and number of filters can all be seen immediately by even an untrained eye with these images.
(Credit: NASA, ESA, CSA, IPAC, Kristen McQuinn (RU); Image Processing: Zolt G. Levay (STScI), Alyssa Pagan (STScI))

Even its faint, dim component stars are easily resolved.

Located several million light-years away from the Milky Way, Andromeda, and Triangulum galaxies, dwarf galaxy Wolf-Lundmark-Melotte (WLM) is extremely isolated within our Local Group. The stars that are revealed inside largely formed all at once and long ago, meaning that we’re effectively looking back at a relic from the early Universe when we examine this galaxy with sufficient detail, which JWST’s NIRCam instrument provides.
(Credit: NASA, ESA, CSA, Kristen McQuinn (RU); Image processing: Zolt G. Levay (STScI))

JWST’s NIRCam reveals many thousands of individual objects.

This high-density region of stars from within dwarf galaxy Wolf-Lundmark-Melotte (WLM) contains a few bright, higher-luminosity stars, but most of the stars present here are very old and very poor in metal content, enabling astronomers who hone in on these populations to discover many facts about how such stars formed and evolved when the Universe was only a few hundred million years old.
(Credit: NASA, ESA, CSA, Kristen McQuinn (RU); Image processing: Zolt G. Levay (STScI))

Low-density regions showcase more pristine stellar populations.

The regions of low stellar and dust density within dwarf galaxy WLM are found close to the outskirts and have undergone very little star-formation since a big burst, all-at-once, 13 billion years ago. Studying these ancient stars can help us understand how stars formed in the early Universe, when less than 1 billion years had passed since the hot Big Bang.
(Credit: NASA, ESA, CSA, Kristen McQuinn (RU); Image processing: Zolt G. Levay (STScI))

The dustiest regions suggest ram-pressure stripping.

The dustiest portions of dwarf galaxy Wolf-Lundmark-Melotte (WLM) show evidence of small amounts of quiescent, ongoing star-formation, as well as some evidence that this gas is being ram-pressure stripped away. Perhaps, even though mergers and interactions have been rare for WLM, there are clumps of gaseous, intergalactic matter within the Local Group that it regularly encounters.
(Credit: NASA, ESA, CSA, Kristen McQuinn (RU); Image processing: Zolt G. Levay (STScI))

Occasionally, background galaxies peek through.

A portion of the dwarf galaxy Wolf–Lundmark–Melotte (WLM) captured by the James Webb Space Telescope’s Near-Infrared Camera. This region showcases some of the stars located within WLM, some ~3 million light-years away, along with many background galaxies of various sizes and distances. The Universe, even when we look within a nearby galaxy, can’t help but reveal itself when we look with JWST’s eyes.
(Credit: NASA, ESA, CSA, Kristen McQuinn (RU); Image processing: Zolt G. Levay (STScI))

Scientific insights will reveal how stars formed, long ago, in the early Universe’s pristine environment.

An artist’s impression of the environment in the early Universe after the first few trillion stars have formed, lived, and died. While there are sources of light in the early Universe, the light is very rapidly absorbed by the interstellar/intergalactic matter until reionization is complete. While JWST may someday reveal evidence for these early stars, the only stars that are individually resolvable are located in galaxies very close to our own.
(Credit: NASA/ESA/ESO/W. Freudling et al. (STECF))

Mostly Mute Monday tells an astronomical story in images, visuals, and no more than 200 words. Talk less; smile more.

In this article

Related

Up Next