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CEERS-2112

most distant barred spiral galaxy

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General referenceInterpretive dossier study · Crown Archives visual atlas
Record originEnglish Wikipedia
Text licenseCC BY-SA 4.0
Source revisionSep 3, 2026
Entity authorityQ123556206 ↗
Source-derived summary

CEERS-2112 is one of the most distant barred spiral galaxies observed as of 2023. The light observed from the galaxy was emitted when the universe was only 2.1 billion years old. It was determined to be similar in mass to the Milky Way.

Observations

The galaxy is located in the Extended Groth Strip cosmological field and it was identified as a barred spiral galaxy thanks to the observations of the NIRCam instrument onboard the James Webb Space Telescope. These observations were made in June 2022 as part of the Cosmic Evolution Early Release Science (CEERS) survey and are publicly available for the general community.

Morphology

CEERS-2112 is a barred spiral galaxy, resembling the structure of the Milky Way. It presents a concentration of stars moving on very elliptical orbits in its central region, which appears as an elongated structure (stellar bar), from which two faint spiral arms develop. In the local Universe, about 70% of galaxies show this appearance, which is quite rare in the early Universe, where the percentage diminishes to about 5% at redshift z > 2.

Stellar mass

The galaxy has a stellar mass of 3.9 billion times that of the Sun, comparable with that of the Milky Way 11.7 billion years ago.

Editorial summary

The public source identifies “CEERS-2112” as most distant barred spiral galaxy. This brief keeps that definition visible, then builds a research path around CEERS-2112, most and distant.

Editorial reviewA dependable orientation record for establishing vocabulary, names and a first evidence trail. The current lead gives the account dated anchors—2023, 2022—that can be checked directly. The selected authority fields contribute no independent date. Its value is orientation rather than verdict, with CEERS-2112, most and distant providing the first useful test.
Editorial analysis

Why this record matters

A short description can identify a subject without explaining its stakes. For “CEERS-2112”, the useful work is to connect “most distant barred spiral galaxy” to the records capable of establishing context and consequence.

Evidence profile

Named sources, stable identifiers and responsible institutions provide the strongest route from overview to verifiable evidence. The source revision retrieved here is dated Sep 3, 2026. The linked authority identifier is Q123556206. None of the 0 selected statements returned an explicit reference. The first chronological checks are 2023 and 2022.

Critical limits

Overview language is designed for orientation and should not be treated as a substitute for the evidence cited beneath it. The lead is largely declarative, so disagreement and counter-evidence require a deliberate search beyond the opening account. Authority statements aid reconciliation but still require their own references, qualifiers and ranks to be checked.

How to read it

Use the entry as an orientation point, then follow its citations and revision history. Names, dates and institutional relationships should be checked against the original record.

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  2. Expand the search: follow CEERS-2112 primary sources, CEERS-2112 archive and CEERS-2112 research across catalogues and specialist indexes.
  3. Test the account: compare the strongest cited source with the responsible institution’s current record and note any disagreement.

Questions for further research

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Source & attribution

This entry incorporates text from “CEERS-2112” on English Wikipedia. Contributors are listed in the page history. Text is available under the Creative Commons Attribution-ShareAlike 4.0 License. Selected authority identifiers and statements are retrieved from Wikidata under CC0; their references and qualifiers remain part of the verification path.