Abstract
The Vikram lander of the Chandrayaan-3 mission landed near the south pole of the Moon on 23rd August 2023. During the action of descent stage thrusters and the consequent landing, a significant amount of lunar surficial epiregolith material got ejected, resulting in a reflectance anomaly or ‘ejecta halo’. We compared the pre- and post-landing high-resolution panchromatic imagery from Orbiter High-Resolution Camera (OHRC) of the Chandrayaan-2 orbiter, acquired hours before and after the landing event and characterised this ‘ejecta halo’, which appears as an irregular bright patch surrounding the lander. From the mapped and classified, uncorrelated ‘ejecta halo’ pixels, an approximate areal extent of 108.4 m2 is estimated to have been covered by lunar epiregolith ejecta displaced due to the landing sequence of the Vikram lander. Further, using empirical relations, we estimate that approximately 2.06 tonnes of lunar epiregolith were ejected due to the landing event.
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Acknowledgements
We thank Space Applications Centre, ISRO, Ahmedabad, for the OHRC data. We thank all the contributors to the Chandrayaan-3 mission for their historic success.
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SS contributed to data analysis, and writing—original draft preparation; PC contributed to conceptualization, methodology, data curation, writing—reviewing and editing, and supervision. PR performed data analysis and writing—original draft preparation; TRM performed writing—reviewing and editing; ICD performed writing—reviewing and editing, and supervision.
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Singh, S., Chauhan, P., Roy, P. et al. Characterisation of Ejecta Halo on the Lunar Surface Around Chandrayaan-3 Vikram Lander Using OHRC Imagery. J Indian Soc Remote Sens 51, 1919–1922 (2023). https://doi.org/10.1007/s12524-023-01774-1
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DOI: https://doi.org/10.1007/s12524-023-01774-1