Venus data, free to reuse

Where spacecraft reached Venus, as free CC BY 4.0 data: 11 estimated positions, one per mission page: 6 landing sites, 1 impact point, 2 points where descent signals ended, 1 balloon position fix and 1 orbiter's last measured position. Each comes with the source of its coordinate and, for 5 of them, the radius of probable error the source states. Beside them sits the whole catalogue, 46 pages: 34 missions and programmes and 12 explainers.

Catalogue verified: every row on or after 26 September 2026, the most recent re-check on 5 November 2026. Positions change only when their sources do.

Read this first

  • Every coordinate here is an estimate with its source stated. The positions come from tracking and descent data and from later re-plotting on Magellan radar maps; the best of them carry a stated radius of probable error (uncertainty_km), and the rest are figures whose method or frame their source did not publish. Read site_name and follow coordinate_source before using a row for anything that matters.
  • Each row gives its source's figures as published. azmth has not converted them between rotation models or map frames.
  • point_kind says what each point is (a landing, an impact, the end of a descent signal, a balloon fix or an orbiter's last measured position), and site_name says how good the fix is in the research's words: a landing circle centre, a published whole-degree position, a last measured position before contact was lost, a first radio fix.
  • Pages are not spacecraft. One row per mission page: a page can cover two or more craft (Venera 13 and Venera 14 share one), and its row gives the first craft's position, so counting rows or pages is not counting spacecraft. Do not derive a success rate from row counts.
  • Planetary sources state Venus longitude east-positive in 0 to 360. Both that and the -180 to 180 form are given, because mapping tools expect the latter.

For journalists, researchers, and educators

Reproduce these figures freely, including commercially, with the credit "azmth.space" linked where possible. No permission needed. Each coordinate comes from the source linked in its row; credit that source too where you lean on a specific position. Everything is provided as is, and the notes above are worth two minutes before you plot anything.

inline"...according to azmth.space's catalogue of Venus landing and impact sites."

footnote"azmth Venus site catalogue, azmth.space/venus/data, data as of 5 November 2026, methodology version 1."

Endpoints

URLFormatContents
/data/venus-sites.csvCSVOne row per catalogue page with a position on Venus: coordinates in both longitude forms, the radius where stated, what the point is, outcome, operator and the source of the coordinate
/data/venus-sites.jsonJSONThe same rows as an array of objects
/data/venus-sites.metadata.jsonJSONColumn definitions, the coordinate frame, the licence and the caveats on this page
/data/venus-missions.jsonJSONEvery page of the catalogue, including the missions that never reached Venus and the explainers, with its status and source counts
/data/venus-ephemeris.jsonJSONThe paths the globe draws for past orbiters and in History, centred on Venus, in ICRF except where a row's frame says otherwise. Each orbiter has rows of six numbers, one orbit each: periapsis time (Unix seconds, UTC), periapsis radius (km), eccentricity, then inclination, node and argument of periapsis (degrees); trackedToS marks where tracking ends and prediction begins. Each flyby is one such row at closest approach, or position vectors where an engine burn bends the path, and craft with no path are dated markers. Every orbiter, flyby and marker names its source. Source data: NASA/JPL Horizons, NAIF SPICE kernels and NASA PDS, public domain. Venera 9 and 10 are rebuilt from published elements (NSSDCA), their orientation illustrative; Venera 15 and 16 take their size from NPO Lavochkin and their plane from azmth's fit to the NASA PDS altimeter tracks. All four are marked approximate
/data/venus-balloons.jsonJSONThe two Vega balloon flights of June 1985, as measured: per balloon, the radio (VLBI) position fixes as t (seconds after the flight's epochUtc), lat and lon (degrees, planetocentric, longitude east 0 to 360), radiusKm (distance from the centre of Venus) and uMs, vMs (east and north wind, m/s). The fixes are good to about 10 km. The injection and modelEnd points, which close each track's faint "1986 model" leg, come from the Doppler model of Sagdeev et al. 1992 and are kept out of the fixes. Source: Lorenz, Crisp and Huber, Vega 1 and Vega 2 Balloon and Lander Archive, NASA PDS, 2020. The archive states no licence
/data/venus-balloon-telemetry.jsonJSONWhat the two balloons measured, for the globe's drift replay: per balloon, t (seconds after epochUtc), p (pressure, hPa), T (temperature, K) and w (the anemometer's vertical wind, m/s, up positive), with runs giving the first and last row of each unbroken stretch. Every row where one of the three carries a quality flag of 2 or more; a value with a lower flag is null, and nothing is filled, smoothed or thinned. Same source as the balloon tracks, and the archive states no licence

The catalogue files update when the catalogue does, the orbit and balloon files when their sources do, and every endpoint allows cross-origin requests. In Google Sheets: =IMPORTDATA("https://azmth.space/data/venus-sites.csv"). From a terminal: curl https://azmth.space/data/venus-sites.json.

Columns

  • slug: Stable identifier, also the page URL segment.
  • name: Page name as the catalogue presents it. One page can cover two or more craft.
  • entity: Operating organisation or organisations.
  • type: flyby, orbiter, atmospheric-probe, soft-lander, balloon, program or topic (an explainer page).
  • outcome: success, operating, ended, partial, failure, in-development, planned, cancelled or reference (an explainer page). "ended" means it succeeded and later stopped, which is distinct from failure. A probe that returned its data on the way down and was then crushed is a success on its own terms.
  • era: Catalogue era grouping.
  • latitude: Planetocentric latitude, degrees north, as the source gives it.
  • longitude_east_360: East longitude 0 to 360, as every Venus source states it. The prime meridian runs through the central peak of the crater Ariadne.
  • longitude_east_180: The same longitude as -180 to 180.
  • uncertainty_km: Radius of probable error in km where the source of this exact position states one. Blank where the source states none; a blank does not mean the position is exact.
  • point_kind: What the point is: landing (where a lander came down), impact (where a probe hit the surface), descent (where a descent capsule's signal ended on the way down), entry (where a craft entered the atmosphere), balloon (a balloon's position fix in the clouds), orbit-decay (an orbiter's last measured position before its orbit decayed). Blank where the research does not say.
  • site_name: What the point is, and how good the fix is, in the research's words. Read this.
  • coordinate_source: URL for the coordinate specifically.
  • facts_checked: ISO date the entry was last verified.
  • page: Canonical page for this entry.

Coordinate frame

  • Latitude: planetocentric, degrees north.
  • Longitude: east-positive, 0 to 360 (also given as -180 to 180).
  • Prime meridian: the central peak of the crater Ariadne.

Stability promise

Fields and CSV columns are additive only: names and meanings never change. Slugs are stable identifiers and double as URL paths. If a breaking change ever becomes unavoidable, the old shape keeps working for 12 months and this page documents the change with a date. Methodology changes bump methodology_version in the metadata file, which reads 1 today. Coordinates are corrected when better sources appear, which is why the source of each one is published beside it.

The sites

Every row of the files, as published. Latitude is planetocentric, longitude east 0 to 360; the radius is blank where the source states none.

Page and pointLatLon (E)Radius
Pioneer Venus MultiprobePioneer Venus Large Probe (Sounder) impact site, day side near the equator (project reconstruction, error not stated) 4.4304
Pioneer Venus OrbiterLast measured periapsis, orbit 5055 (7 October 1992), one orbit before contact was lost; the entry point itself is unknown -11.8789.2
Vega 1 and Vega 2Vega 1 landing site, central Rusalka Planitia (within 150 km) 8.1175.85150 km
The Vega balloonsVega 1 balloon, first VLBI position fix (02:18 UT, 11 June 1985) 8.321176.16510 km
Venera 11 and Venera 12Venera 11 landing site (whole-degree position) -14299
Venera 13 and Venera 14Venera 13 landing site, western Navka Planitia east of Phoebe Regio (within 150 km) -7.55303.69150 km
Venera 4near 19 N, 38 E (NSSDCA's 'Eisila region'); Siddiqi gives 36 E 1938
Venera 5 and Venera 6Venera 5 descent capsule, night side of Venus, published whole-degree position 3 S, 18 E (Venera 6 at 5 S, 23 E is the second pin); no method or frame stated in any source -318
Venera 75 S 351 E, within the nominal IAU extents of Unuk Dorsa and Kanykey Planitia -5351
Venera 8Eastern Vasilisa Regio (landing circle 150 km radius) -10.7335.25150 km
Venera 9 and Venera 10Venera 9 landing site near Beta Regio (within 150 km) 31.01291.64150 km
All Venus missions →Understanding Venus →Landing on Venus →What we left at Venus →Satellite numbers and data →Moon numbers and data →Mars numbers and data →azmth Venus: the planet →

Corrections are welcome, especially on the Soviet-era positions: hello@azmth.space. azmth is independent and is not affiliated with or endorsed by NASA, Roscosmos, NPO Lavochkin, ESA, JAXA, ISRO, CNSA, or any other space agency or company named on this page.