star · Measured Gaia DR3 astrometry
How far away is Proxima Centauri, our nearest neighbouring star?
Proxima Centauri is the closest star to the Sun, about 4.25 light-years away in the Gaia DR3 record used by COSMOS. Its light takes roughly that many years to reach us. Fly to its measured position, then pull back to see how our nearest stellar neighbour fits into the surrounding star field.
Measured facts
- Catalogue identity
- Gaia DR3 5853498713190525696
- Aliases
- Proxima · GJ 551
- Source id
- 5853498713190525696
- Distance
- 1.302 pc · 4.25 ly
- Measured catalogue
- Gaia DR3 (ESA/Gaia/DPAC and the Gaia Archive)
Try a two-minute journey to our nearest stellar neighbour
Open the 3D view above and wait for the measured star catalogue to load. Proxima is selected as a point source. Drag to orbit and scroll or pinch outward to reveal the depth of the local star field; Return to Earth brings you home.
Compare the Distance fact with Barnard’s Star in Related destinations. A light-year measures distance, not travel speed. Even light takes about 4.25 years to cross this distance in the Solar System frame. The camera flight is a navigation aid, not a spacecraft timetable.
NASA describes Proxima as a red dwarf too faint for the unaided eye. Nearby does not mean visually bright. COSMOS uses catalogue brightness and a bounded point marker, rather than presenting an invented close-up of its surface.
What COSMOS shows
A nearby Gaia source identified by SIMBAD as Proxima Centauri. Its depth and motion here are derived only from Gaia DR3 astrometry.
COSMOS renders Proxima as a measured point source with G-magnitude-driven brightness and a restrained BP−RP colour. It never draws a stellar disc, because no instrument in this catalogue measures one.
Its depth is the naive reciprocal of high signal-to-noise parallax. That is a deliberate, auditable choice: no zero-point correction and no Bayesian prior are applied, and the limitation is disclosed rather than hidden.
Measured astrometry
Every field below is copied from the shipped Gaia DR3 manifest for the Gaia DR3 high-S/N stellar catalogue inside 100 pc. The catalogue selects sources with parallax S/N of at least 10 and a non-null G magnitude, then stores measured position, colour, motion and the published radial velocity. Naive reciprocal of raw Gaia DR3 parallax for this positive, S/N >= 10 sample. No zero-point correction or Bayesian prior is applied.
- Parallax
- 768.066539 masUncertainty 0.049873 mas; signal-to-noise 15400.5.
- Derived distance
- 1.301971 pc · 4.246 lyNaive reciprocal of the raw positive parallax; no zero-point correction and no Bayesian prior.
- Right ascension / declination (ICRS)
- 217.392321° · -62.676075°Reference epoch J2016.0.
- G magnitude
- 8.9847Used only through the bounded COSMOS brightness transfer, which is not an absolute luminosity estimate.
- BP−RP colour index
- 3.8046Rendered through a restrained display transfer, not converted to a temperature.
- Proper motion (μ_α*, μ_δ)
- -3781.741 · 769.465 mas/yrμ_α* includes the cos δ factor. Positions are propagated linearly from J2016.0.
- Radial velocity
- -21.943 km/sIncluded, so all three velocity components are measured.
- RUWE
- 0.971453Gaia renormalised unit weight error, carried as provenance rather than used as a selection cut for this landmark.
- Catalogue chunk
- core-25pcPart of the 371,766-source measured volume inside 100 pc.
Provenance
- Provider
- ESA Gaia Archive
- Release
- Gaia DR3
- Licence
- Gaia public archive data; follow ESA/Gaia/DPAC acknowledgement and citation guidance for publication.
- Attribution
- ESA/Gaia/DPAC and the Gaia Archive
- Catalogue checked
- 2026-09-05
- Catalogue SHA-256
- 0069111d383d2d2014a73819b637cefee233ed468309115c267098fe6092706d
- Alias cross-identification
- https://simbad.u-strasbg.fr/simbad/sim-id?Ident=Proxima+CentauriSIMBAD supplies only the visible common name for this source; the astrometry is Gaia.
Limitations COSMOS discloses
- Astronomic distance is a derived quantity from a truncated parallax, so it is not a direct measurement and it carries the stated parallax uncertainty.
- The rendered point size and colour come from bounded display transfers and must not be read as physical size, luminosity or temperature.
- Motion is propagated linearly from J2016.0. Over decades this approximation degrades, and COSMOS does not extrapolate it indefinitely.
- COSMOS names only a small set of nearby stars. It does not claim these are the nearest stars in existence, only that they are the measured landmarks the catalogue currently renders as destinations.
Sources and further reading
Questions this page answers
- What is the nearest star to Earth?
- The Sun is the nearest star to Earth. Proxima Centauri is the nearest star outside our Solar System; COSMOS shows its Gaia-derived distance in the facts above.
- Can I see Proxima Centauri without a telescope?
- No. NASA/Hubble describes Proxima as too faint for the unaided eye. Its closeness does not make it a bright naked-eye star.
- Is the COSMOS view a photograph of Proxima’s surface?
- No. It is a measured Gaia point source in a 3D catalogue. Screen size and colour use disclosed display mappings; no measured stellar disc is shown.
Datasets behind this page
- Gaia DR3 stellar catalogue inside 100 parsecsESA Gaia Archive · measured-catalogue-data · Individual Gaia DR3 catalogue sources
Content updated 2026-10-26. Distances and astrometry are derived from the shipped Gaia DR3 record using the method stated below. General red-dwarf and visibility context is sourced to NASA/Hubble; it is not a new COSMOS observation. The 3D flight changes the viewpoint, not the speed of light.