September 30, 2024
In a study published in peer-reviewed journal Icarus, scientists from PRL and ISRO have shown that Indian Lunar mission Chandrayaan-3 landed within a buried impact crater, which is around 160 km in size, ~4.4 km deep, and likely to be older than the South Pole Atkin (SPA) basin. This is revealed based on analysis of images obtained by Navigation Cameras on Chandrayaan-3 Pragyan rover and Chandrayaan-2 Orbiter’s Optical High Resolution Camera.
The Chandrayaan-3 mission with the Vikram-lander and the Pragyan rover landed in the high latitude highland region near the south pole of the Moon. The landing site is located ~350 km from the South Pole-Aitken basin rim, an ancient and the largest impact basin in the Solar System. This landing site has undergone the complex emplacement sequence of SPA basin ejecta followed by the nearby and distant impact basins and complex crater ejecta materials. We found that the SPA basin is the major contributor, which deposited nearly ~1400 m of ejecta materials, and 11 other basins deposited ~580 m of ejecta. The other complex craters contributed up to ~90 m of ejecta. Meanwhile, secondary craters of a few km's in diameter located adjacent to the Vikram lander contributed to ~0.5 m ejecta, which are crucial target materials for the Pragyan rover insitu analysis.
Figure. 1 (Left) Chandrayaan-2 OHRC image shows the Chandrayaan-3 landing site with linear, parallel grooves-like structure extending from SW to NE side and spread to several 100’ s of meters. These features indicate ejecta from distant impacts was emplaced over the landing site.(Right) The Pragyan rover Navcam images taken from the south of Vikram lander shows the linear groove-like feature present over the landing site. The other Navcam image shows the Vikram lander and the boulder distributed around the landing site. OHRC id: ch2_ohr_ncp_20200826T0303458884_d_img_d18.
The Pragyan rover Navcam and Optical High Resolution Camera images gave the first clue about the linear, distal ejecta rays or groove-like structures possibly formed due to the distant impacts deposited at the Chandrayaan-3 landing site. Figure 1. shows the CH2-OHRC and CH-3 Navcam images of landing site region mantled by linear-groove like structures. Pragyan rover images revealed the landing site is devoid of > 1 m boulders along the traverse, which reveals typical highland terrain.
Figure. 2 Black arrow shows the boundary of the semi-circular buried impact crater within which the Chandrayaan-3 mission landed. The SLDEM draped over the hill shade image to highlight the buried semi-circular structure which is the destination of the Chandrayaan-3 mission.
The regional exploration around the Chandrayaan-3 landing site revealed a near semi-circular like structure, with highly degraded in nature. This semi-circular structure encompassed the Statio Shiv Shakti (yellow star) as shown in the Figure 2. Further detailed geomorphological and topographical analysis revealed that the semi-circular structure is a heavily degraded crater structure or a buried impact crater with a diameter of ~160 km. This semi-circular structure was highly degraded due to the mantling of thick ejecta deposits from the SPA basin and followed by many other complex craters throughout the geological history of the Moon. This buried crater is one of the oldest crater on the Moon, and the Chandrayaan-3 Vikram lander and Pragyan rover landed and roved within this buried crater, which is hosting the SPA basin ejecta material and some of the most deeply excavated materials on the Moon.
The regional exploration around the Chandrayaan-3 landing site The research work is published journal Icarus https://doi.org/10.1016/j.icarus.2024.116329 with the title “Chandrayaan-3 landing site evolution by South Pole-Aitken basin and other impact craters”, authored by S Vijayan, KB Kimi, Anil Chavan, R Aditi, U Thahira, V Rama Subramanian, Rishitosh K Sinha, Santosh Vadawale, M Shanmugam, NPS Mithun, Arpit R Patel, S Amit Basu, KV Iyer, K Suresh, Ajay Prashar, G Rima, Anil Bhardwaj.