Key facts
- The ESA Gaia bulletin archive reports a cosmic three-dimensional map of about 1.3 million quasars.
- According to the ESA summary, the map represents quasar locations across space and time.
- The archive says the most distant quasars cited were shining when the universe was 1.5 billion years old.
- The source describes quasars as bright, active galaxy centres powered by supermassive black holes.
- The quasar-map item appears in the bulletin archive; the supplied material gives no exact date for that item or detailed account of the map’s methods.
- Gaia’s September 2026 announcement concerns a Milky Way map and should not be conflated with the cosmic quasar map.
Related records
A map of about 1.3 million quasars offers a different perspective from a chart of stars in the Milky Way. The European Space Agency’s (ESA) Gaia science community describes in its archive the creation of what it calls the largest cosmic three-dimensional quasar map made up to that point. The source says it shows the objects’ locations in space and time and that the most distant quasars in the sample were shining when the universe was 1.5 billion years old.
This makes the map relevant to cosmology: the account is not limited to objects in our own galaxy, but concerns a population of sources at great distances and an early period in cosmic history. The information comes from an item included in the Gaia bulletin archive. The supplied text does not give an exact date for that item or describe the map’s methods in detail. The figures should therefore be attributed to the archive and not extended into conclusions that it does not report.
What the Gaia archive reports
The ESA archive describes astronomers’ work as bringing about 1.3 million quasars together in the largest three-dimensional cosmic map of this kind at the time, in the source’s own wording. It also explains what it means by quasars: bright, active centres of galaxies powered by supermassive black holes. That description identifies the objects in the map without confusing them with individual stars.
The phrase “across space and time” is central to the result as the source summarizes it. The map is not presented simply as a collection of points with positions; it places objects whose light corresponds to different stages in the universe’s history. The 1.3 million figure describes the sample size given by the archive, while the 1.5-billion-year reference applies to the most distant quasars mentioned. It is not the universe’s present age, nor is it the age of each quasar.
Why the time dimension matters
The source links the distance of the most remote quasars to an era when the universe was 1.5 billion years old. As described in the archive, the map therefore organizes observations from different cosmic periods: it represents sources in both space and time. The account does not quantify how long the light travelled or provide a complete distance scale, so those values should not be calculated or added from the available summary.
The cosmological significance here lies in the stated reach: a large quasar sample and an explicit reference to objects seen during an early stage of the universe. The available excerpt does not report a new measurement of cosmic expansion, an estimate of cosmological parameters or an explanation of how structures originated. The result that can be stated is the existence of the map as described and its coverage across space and time—not a broader conclusion about cosmic history.
A different map from the Milky Way chart
Gaia’s wider context could lead readers to conflate two separate announcements. On its website, ESA announced on 25 September 2026 that a map of the Milky Way would be presented on 2 December that year. It is described as covering more than two billion stars and other objects, with data on position, distance, colour and motion. That announcement concerns our galaxy. The quasar map in the archive, by contrast, concerns a population of bright, active galactic centres and is described as a cosmic three-dimensional representation.
The distinction matters when interpreting the evidence, but it does not establish a scientific link that the source does not make. The September 2026 announcement does not say that the new Milky Way chart is the quasar map or that the two are the same data release. Nor does it report new cosmological results. In the archive, the quasar map is the item relevant to the large-scale universe; the later Milky Way announcement is useful only to prevent the scope of the two maps from being confused.
What is known, and what remains bounded
The information attributable to the archive is specific: according to its summary, astronomers created a three-dimensional map of about 1.3 million quasars; it represents their locations across space and time; and the most distant objects cited were shining when the universe was 1.5 billion years old. The same source describes quasars as bright, active galaxy centres powered by supermassive black holes.
The material consulted does not give a precise publication date for this item or enough detail to assess the map’s construction, distance uncertainties or full coverage. Its appearance in an institutional archive is not, by itself, evidence of peer review, and “the largest up to that point” should not be turned into a current comparison with every map. The evidence supports a narrower conclusion: Gaia’s archive reports a cosmological quasar map that places very distant sources in a framework of space and time, while further information would be needed to assess its methods and the full scope of its results.
Sources: ESA Gaia bulletin archive, which summarizes the quasar map. For the separate Milky Way announcement: ESA Gaia science community.