JWST confirms: The tiniest galaxies made the cosmos visible

One remarkable patch of sky just solved a major cosmic puzzle.

This image shows the full imaging field of the JWST UNCOVER Treasury Survey, which takes up about 0.007 square degrees in the sky. In this tiny patch of space, some ~50,000 objects are revealed, with the majority of them not associated with the imaged cluster, Abell 2744, at all, but rather as background galaxies that are affected by the gravity of the cluster itself. No signs of matter-antimatter annihilation are seen here, indicating that all stars and galaxies shown are made of matter, not antimatter. However, many gravitationally lensed background galaxies are among the most distant ever discovered.

Shortly after the Big Bang — before any stars arose — the first stable, neutral atoms formed.

At early times (left), photons scatter off of electrons and are high-enough in energy to knock any atoms back into an ionized state. Once the Universe cools enough, and is devoid of such high-energy photons (right), they cannot interact with the neutral atoms, and instead simply free-stream, since they have the wrong wavelength to excite these atoms to a higher energy level.

These atoms, however, absorb visible light, rendering space opaque.

The overdense regions that the Universe was born with grow and grow over time, but are limited in their growth by the initial small magnitudes of the overdensities, the cosmic scale on which the overdensities are found (and the time it takes the gravitational force to traverse them), and also by the presence of radiation that’s still energetic, which prevents structure from growing any faster. It takes tens-to-hundreds of millions of years to form the first stars; small-scale clumps of matter exist long before that, however. Until stars form, the atoms in these clumps remain neutral, requiring ionizing, ultraviolet photons to render them transparent to visible light.

Energetic, ultraviolet photons are required to reionize atoms.

An artist’s conception of what a region within the Universe might look like as it forms stars for the first time. As they shine and merge, radiation will be emitted, both electromagnetic and gravitational. But the conversion of matter into energy does something else: it causes an increase in radiation pressure, which fights against gravitation. Surrounding the star-forming region is darkness, as neutral atoms effectively absorb that emitted starlight, while the emitted ultraviolet starlight works to ionize that matter from the inside out.

Determining how early stars and galaxies reionized the Universe is a cosmic challenge.

One of the science goals of the JWST UNCOVER survey is to track galaxy evolution across cosmic time. Here, a selection of nine galaxies pulled from the survey itself are highlighted in context with the cosmic time from which their light was emitted. JWST is shedding a whole new light on the story of galaxy evolution within our Universe, and is also helping us determine which types of galaxies, and when, helped our Universe transition from an opaque state to one transparent to light.

It’s a challenge perfectly suited for JWST, however, with help from Einstein.

The galaxies that compose Pandora’s Cluster, Abell 2744, are present within the three separate cluster components easily visually identifiable, while the remaining background sources are scattered all throughout the Universe, including many from the first ~1 billion years of cosmic history. This field of view is now known to contain many of the earliest galaxies ever found, as well as the youngest proto-cluster of galaxies ever discovered to date: just 650 million years after the Big Bang.

This image shows Pandora’s cluster, Abell 2744: a massive collection of galaxy clusters.

This gravitational lensing map shows the reconstructed magnification contours from JWST data owing to the lensing profile of the three bright components of Abell 2744, Pandora’s Cluster. All galaxy clusters have their own unique lensing magnification properties, providing maximum enhancement along specific contours.

This huge mass collection bends and distorts the surrounding spacetime.

The full set of light (left panels) received by JWST are a composite of the background sources of light with the foreground cluster sources. Attempts to map out the foreground cluster and subtract them leaves only the background signals, which can be further corrected for gravitational lensing effects. Making a lensing map is of the utmost importance if we wish to understand how the lensed objects themselves actually are, intrinsically.

Background objects, through gravitational lensing, appear magnified and stretched.

This deep-field region of the GOODS-South field contains 18 galaxies forming stars so quickly that the number of stars inside will double in just 10 million years: just 0.1% the lifetime of the Universe. The deepest views of the Universe, as revealed by space telescopes, take us back into the early history of the Universe, where star-formation rates were much greater than today, but where fewer than 1% of the Universe’s cumulative stars had already formed. Many of the most distant galaxies are found in close proximity to other foreground galaxies, whose mass distorts and magnifies the light from background objects.

This reveals galaxies too small, faint, and distant to otherwise be glimpsed.

This image shows how much of the sky (x-axis) versus how deep, in terms of magnitude (y-axis) a variety of Hubble and JWST surveys have reached. The dotted lines include enhancements due to gravitational lensing. Note that the UNCOVER survey, with lensing enhancements included, reaches the most deeply of any (cycle 1) JWST program. The deeply imaged galaxy cluster Abell 2744, also known as Pandora’s cluster, is a key part of the UNCOVER survey area.

Ultra-distant, massive galaxies create too little ultraviolet light to explain cosmic reionization.

This image reveals about 20% of the full JADES survey area: around 25 square arc-minutes in the sky. It would take nearly 6 million boxes of this size to fill the entire sky. Already, a whopping 45,000 galaxies are known within this tiny region of space, showcasing just how vast and wondrous our Universe is. The most bright, distant, massive galaxies found in surveys such as these, however, cannot account for the majority of ultraviolet, ionizing photons needed to make the Universe transparent to light.

They account for between 5% and 20% of the needed ionizing photons.

More than 13 billion years ago, during the Era of Reionization, the Universe was a very different place. The gas between galaxies was largely opaque to energetic light, making it difficult to observe young galaxies. The James Webb Space Telescope (JWST) is peering deep into space to gather more information about objects that existed during the Era of Reionization to help us understand this major transition in the history of the Universe, and finding that bright, early galaxies were common, and the intergalactic neutral matter is insufficient to stop that light from arriving at our telescopes.

Despite the hopes of some, neither can quasar emissions.

This tiny sliver of the GOODS-N deep field, imaged with many observatories including Hubble, Spitzer, Chandra, XMM-Newton, Herschel, the VLT, and more, contains a seemingly unremarkable red dot. That object, a quasar-galaxy hybrid from just 730 million years after the Big Bang, showcases how bright and powerful quasars can be. Many of the “little red dots” seen by JWST and other observatories are brightness-enhanced by the activity of the central black hole, with some jets pointing directly along our line-of-sight.

However, gravitational lensing newly revealed eight tiny, faint, distant dwarf galaxies.

These eight very faint, low-mass galaxies would be invisible to even JWST at these great distances under normal circumstances. Only from gravitational lensing’s severe brightness enhancement, an effect of Einstein’s general relativity, can these galaxies be revealed at all.

With only ~1 million stars apiece, they are ~100 times as common as their bigger, brighter counterparts.

Even at early times and great distances, the properties of the faintest, lowest-mass galaxies identified appear very similar to the same mass galaxies (with ~10^6 solar masses worth of stars inside) seen today.

They were caught producing four times as many ionizing photons as previously assumed.

Whereas young stars produce ionizing photons that freely travel throughout the Universe, early galaxies, back when the intergalactic medium was filled with neutral atoms, have their light absorbed, and only a tiny fraction escapes. However, with such great numbers of dwarf galaxies, even a small fraction of ionizing photons can be primarily responsible for reionizing the Universe.

It’s these cosmic dwarfs — not quasars or bright galaxies — that primarily reionize the Universe.

For the first 550 million years of the Universe, neutral, light-blocking atoms persist ubiquitously in the space between galaxies, continuing what’s known as the cosmic dark ages. Once the last of that neutral matter becomes reionized, starlight can propagate freely through the Universe, marking the end of the reionization epoch. In some locations, reionization happens earlier than average, but this should never happen as early as JADES-GS-z13-1-LA has been observed.

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