Pic of the Week: Colorful IC 348

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Image (Credit): IC 348 as captured by NASA’s JWST recently observed IC 348. (NASA, ESA, CSA, Kevin Luhman (PSU), Catarina Alves de Oliveira (ESA), Mahdi Zamani (ESA/Webb))

This week’s image is from the James Webb Space Telescope (JWST). With its sharp, amazing colors you would not think it is real, yet you are looking at a star-forming region about 1,000 light-years away called IC 348.

Here is NASA’s description of what you are seeing:

In regions like IC 348, cold clouds of molecular hydrogen gas collapse to form new stars, creating glowing, sculpted scenes like this one. The star-formation process can create widely varied objects, from massive stars that expire after only a few million years in core-collapse supernova explosions to the smallest and most common stars, which are long lived and produce powerful stellar storms.The smallest stars weigh in at around 8 percent of the Sun’s mass. Below this mass lies a strange class of objects called brown dwarfs. Brown dwarfs form in the same way stars do, through the collapse of molecular clouds. However, unlike stars, the cores of brown dwarfs never become hot enough to fuse ordinary hydrogen into helium (though many briefly fuse deuterium, or heavy hydrogen, early in their lives).

Study Findings: Early Metal-enriched Baryon Cycling Before the Midpoint of Cosmic Reionization

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Image (Credit): The James Webb Space Telescope’s deep field image of Galaxy cluster SMACS 0723 showing thousands of galaxies. (NASA, ESA, CSA, STScI)

Nature Astronomy abstract of study findings:

Models predict that chemical enrichment and gas redistribution should begin rapidly once star formation starts, but direct constraints at the earliest epochs have been scarce. Here we show that metal-enriched gas in multiple ionic phases was already present around galaxies before the midpoint of cosmic reionization. Using JWST/NIRSpec rest-frame ultraviolet spectroscopy from SPURS, we detect blueshifted metal absorption in three galaxies at 7.2 < z < 9.3. The detected transitions span neutral, low-ionization and high-ionization species, including O I, Si II, C II, Si IV and C IV, with velocity offsets of ∣Δv∣ ≈ 50–250 km s−1 relative to nebular systemic redshifts. The ionic coexistence, overlapping velocity structure and equivalent-width ratios are consistent with outflowing or otherwise kinematically disturbed galaxy-associated gas, implying rapid metal enrichment. These results show that key conditions for baryon cycling were established in at least a subset of luminous galaxies within the first several hundred million years of cosmic time, well before the completion of reionization.

Citation: Zhu, Y., Ji, Z., Becker, G.D. et al. Early metal-enriched baryon cycling before the midpoint of cosmic reionization. Nat Astron (2026).

DOI: https://doi.org/10.1038/s41550-026-02988-2

Study-related stories:

EurekAlert! – “JWST Finds Early Galaxies Were Already Seeding the Universe with Heavy Elements”

Cornell Chronicle – “Astronomers Discover Metal-rich Galaxies in Early Universe”

Astro Current – “JWST Finds Early Galaxies Seeded the Infant Universe with Heavy Elements”

Pic of the Week: The Black Eye Galaxy

Posted on by onespaceman2000
Image (Credit): Composite image of Messier 64 (M64) from the JWST and the Hubble Space Telescope. (NASA, CSA, ESA, F. Belfiore (ESO), J. Lee (STScI), A. Leroy (OSU), and D. Thilker (JHU); Image Processing: G. Kober (NASA/Catholic University))

This week’s image is from NASA’s Astronomy Picture of the Day. It is a composite image from the James Webb Space Telescope (JWST) and the Hubble Space Telescope showing Messier 64 (M64), which is a spiral galaxy about 17 million light-years away.

Here is a little more information from NASA explaining what you are seeing here:

Sometimes where Hubble finds darkness, Webb sees light. An example is today’s composite images of Messier 64 (M64), a nearby spiral galaxy of many names. The dark band of dust partially blocking its bright core earned it the moniker “the Black Eye Galaxy.” Webb’s Mid-InfraRed Instrument (MIRI) sees that dust, shown in red, as it absorbs and re-emits light from surrounding newborn stars. These young stars are embedded in pink star-forming regions in the secondary Hubble-only image. M64’s inner and outer gas regions counter-rotate, creating regions of increased star formation where the two gas “currents” meet and compress. A merger between M64 and a smaller galaxy was likely the cause of the opposing motion of the outer gas. Spiral galaxies were once thought to have peaceful histories. M64 was key evidence that spiral galaxies, including the Milky Way, can and do experience mergers. Webb’s view of M64 will tell astronomers about the structure, motion, and composition of the galaxy’s dust and add context to the galaxy’s merger history and evolution.

Space Stories: Dragon Delays, Odd Black Holes, and Surprising Martian Warmth

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Image (Credit): SpaceX Dragon capsule. (SpaceX)

Here are some recent space-related stories of interest.

—Space.com: “SpaceX, NASA Delay Next Astronaut Launch to ISS Due To Leak on Dragon Spacecraft”

SpaceX’s next astronaut mission to the International Space Station won’t launch on Sept. 12 after all. That flight, known as Crew-13, has been delayed due to an oxidizer leak in the propulsion system of SpaceX’s Dragon spacecraft, NASA announced on Saturday (Aug. 29). Joint NASA and SpaceX teams are performing additional tests and data review and will complete any necessary rework prior to launch,” NASA officials wrote in an update on Saturday. “A new target date will be announced once available.”

—Earth.com: “Giant Black Holes Appeared Too soon After the Big Bang, and Astronomers May Know Why“

Nearly every large galaxy keeps a giant black hole at its center. Some of those giants already weighed a billion Suns when the universe was less than 700 million years old. Astronomers have struggled for decades to explain how anything grew that heavy that fast. A new study built on James Webb Space Telescope observations suggests one possible answer. The researchers describe a young black hole wrapped in gas so dense that the whole object shines like a single enormous star. Astronomers call objects like it black hole stars. The light from this one has been traveling for 13 billion years, since a moment just 660 million years after the Big Bang, and no earlier example has been found.

—Caltech: “Thermal Anomaly Discovered Below Mars’s South Pole“

Based on gravitational measurements that give clues to the Red Planet’s interior structure, Mars’s interior southern hemisphere is around 200 to 400 degrees Celsius warmer than the northern half of the planet and partially molten. The surprising finding adds additional context to Martian history and the periods of time in which it may have hosted conditions favorable for life. The research was led by Caltech alumnus Alexander Berne (PhD ’26), who is now a postdoctoral associate at the University of Arizona. The findings are reported in a paper appearing in the journal Nature on August 27.

Note: Here is the podcast version of this post.

Pic of the Week: Galactic Gems

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Image (Credit): A collection of 16 galactic images from Chandra and other telescopes. Each galactic image contains X-ray data from Chandra combined with data from telescopes such as NASA’s Webb, Hubble, IXPE, Swift, and NuSTAR, and others both in space and on the ground. (NASA/CXC/SAO)

This week’s images of 16 galaxies are from a variety of NASA telescopes. The galaxies are generally sorted into three types – spiral, elliptical, and irregular. For example, the Milky Way galaxy is a spiral galaxy, whereas Centaurus A (Cen A above) is a giant elliptical galaxy and NGC 1569 (also above) is a compact dwarf irregular galaxy.

Please go to this NASA link to see all of these galaxies in their full glory.