Bau (crater on Ganymede)
Bau is a 77 km diameter impact crater on Jupiter's moon Ganymede, centered at 23.05° north latitude, 48.67° west longitude in the satellite's Nineveh Sulcus region, and named for the Assyro-Babylonian goddess of life and healing.
| Key fact | Detail |
|---|---|
| Feature type | Crater on Ganymede, IAU feature ID 6411 |
| Diameter | 77.00 km1 |
| Center | 23.05° latitude, 48.67° longitude (planetographic, +West, 0–360)1 |
| Name origin | Assyro-Babylonian goddess who breathed into men the breath of life; daughter of Anu and patroness of Lagash1 |
| Approval | Adopted by the IAU in 19881 |
| Recent imaging | Visible in Juno JunoCam close-up from the 7 June 2021 flyby, near the crater Tros2 |
Naming and location
The International Astronomical Union approved the name Bau in 1988, following the convention that craters on Ganymede carry names of gods and heroes of the ancient Fertile Crescent cultures. The Gazetteer of Planetary Nomenclature records the origin as the goddess "who breathed into men the breath of life; daughter of Anu and patroness of Lagash," citing the Larousse Encyclopedia of Mythology as the reference1. The crater lies at about 23° north, within the band of latitudes where most of Ganymede's named craters are found, and its listed boundaries span latitudes 22.20° to 23.90° north and longitudes 47.80° to 49.54° west1.
Size and crater class
At 77 km across, Bau falls squarely within the size range of Ganymede's central pit craters, a class of complex craters in which a central depression replaces the central peak common on rocky bodies. A survey using Voyager and Galileo imagery classified 471 central pit craters on Ganymede with diameters between 12 and 144 km3. On Ganymede these pits are dominantly floor pits, sitting on crater floors that are often upraised, and many pits in larger craters are rimmed or partially rimmed, suggesting that both uplift and collapse contribute to their formation3. Later work on Ganymede crater dimensions proposed that pit formation may occur through collapse of surface material into a void left by the release of impact-induced volatiles or by drainage of impact melt into sub-crater fractures4.
Observation history
Bau appears on the USGS global geologic map of Ganymede published in 2013, mapped within the dark cratered and light terrain units of the Nineveh Sulcus area5. NASA's Juno spacecraft imaged it directly during its close flyby of Ganymede on 7 June 2021: a processed JunoCam close-up shows the prominent craters Tros at upper left and Bau at bottom right2. A survey of candidate science targets for ESA's JUICE mission, which entered orbit at Jupiter in the 2030s, lists Bau among regions of interest on Ganymede, with coordinates 23.1° latitude, 311.3° longitude (east-positive) and the same 77 km diameter6.
References
- Bau, Gazetteer of Planetary Nomenclature, USGS Astrogeology Science Center
- PJ34, Close Up View of Ganymede's Surface, Mission Juno (NASA/SwRI/MSSS)
- Barlow, N. G. (2017). Comparison of central pit craters on Mars, Mercury, Ganymede, and the Saturnian satellites. Meteoritics & Planetary Science.
- Bray, V. J. et al. (2012). Ganymede crater dimensions – Implications for central peak and central pit formation and development. Icarus 217, 115–129.
- Collins, G. C. et al. (2013). Global Geologic Map of Ganymede, USGS Scientific Investigations Map 3237.
- Regions of interest on Ganymede's and Callisto's surfaces as potential targets for ESA's JUICE mission
Initially written Oct 21, 2026 · Edited: Oct 25, 2026
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