Tahmina Planitia (Venus)
Data as of 2026-10-23
What it is
- Type
- Planitia, planitiae
- IAU definition
Low plain
- Diameter
- 3,000 km, 50 % of the radius of its body
- Centre
- 23° S, 80° east (planetocentric latitude, east longitude from 0 to 360°, the IAU convention)
- Name adopted
- 1997
- Origin of the name
Iranian (Farsi) epic heroine, wife of knight Rustam.
Quoted in English, as the IAU publishes it.
In Galaxy
Opens its body in the application, the camera turned towards Tahmina Planitia.
Observed by
Instruments whose footprint touches this formation, counted by the PDS Orbital Data Explorer (data frozen on September 29, 2026). A footprint that touches it is not a study of it.
| Mission and instrument | Products | First | Last |
|---|---|---|---|
| Magellan · Radar System | 1,870 | November 14, 1990 | April 6, 1992 |
| ESA's Venus Express · Visible and Infrared Thermal Imaging Spectrometer | 4,176 | May 15, 2006 | August 11, 2014 |
| MESSENGER at Venus · MERCURY ATMOSPHERIC AND SURFACE COMPOSITION SPECTROMETER | 6 | April 15, 2007 | April 15, 2007 |
| MESSENGER at Venus · Mercury Dual Imaging System - Wide Angle Camera | 30 | June 5, 2007 | June 6, 2007 |
| MESSENGER at Venus · Mercury Dual Imaging System - Narrow Angle Camera | 9 | June 6, 2007 | June 6, 2007 |
Sources
International Astronomical Union Working Group for Planetary System Nomenclature, Gazetteer of Planetary Nomenclature, read on October 23, 2026. Feature page: https://planetarynames.wr.usgs.gov/Feature/5823
Type definitions: IAU Descriptor Terms, read on October 17, 2026. https://planetarynames.wr.usgs.gov/DescriptorTerms