dc.contributor.author |
Karanam, Durga Prasad |
|
dc.contributor.author |
Misra, Dibyendu |
|
dc.contributor.author |
Amitabh |
|
dc.contributor.author |
Bhatt, Megha |
|
dc.contributor.author |
Ambily, G. |
|
dc.contributor.author |
Sathyan, Sachana |
|
dc.contributor.author |
Srivastava, Neeraj |
|
dc.contributor.author |
Bhardwaj, Anil |
|
dc.coverage.spatial |
United States of America |
|
dc.date.accessioned |
2023-09-01T05:25:12Z |
|
dc.date.available |
2023-09-01T05:25:12Z |
|
dc.date.issued |
2023-08 |
|
dc.identifier.citation |
Karanam, Durga Prasad; Misra, Dibyendu; Amitabh; Bhatt, Megha; Ambily, G.; Sathyan, Sachana; Srivastava, Neeraj and Bhardwaj, Anil, "Chandrayaan-3 alternate landing site: pre-landing characterisation", arXiv, Cornell University Library, DOI: arXiv:2308.10712, Aug. 2023. |
|
dc.identifier.issn |
2331-8422 |
|
dc.identifier.uri |
https://doi.org/10.48550/arXiv.2308.10712 |
|
dc.identifier.uri |
https://repository.iitgn.ac.in/handle/123456789/9146 |
|
dc.description.abstract |
India's third Moon mission Chandrayaan 3 will deploy a lander and a rover at a high latitude location of the Moon enabling us to carry out first ever in-situ science investigations of such a pristine location that will potentially improve our understanding on primary crust formation and subsequent modification processes. The primary landing site (PLS), is situated at 69.367621 degS, 32.348126 degE. As a contingency, an alternate landing site (ALS) was also selected at nearly the same latitude but nearly 450 km west to PLS. In this work, a detailed study of the geomorphology, composition, and temperature characteristics of ALS has been carried out using the best-ever high resolution Chandrayaan 2 OHRC DEMs and Ortho images, datasets obtained from Chandrayaan 1 and on-going Lunar Reconnaissance Orbiter. For understanding the thermophysical behaviour, we used a well-established thermophysical model. We found that the Chandrayaan 3 ALS is characterised by a smooth topography with an elevated central part. The ALS is a scientifically interesting site with a high possibility of sampling ejecta materials from Tycho and Moretus. Based on the spectral and elemental analysis of the site, Fe is found to be near approx. 4.8 wt.%, with Mg approx. 5 wt.%, and Ca approx. 11 wt.%. Compositionally, ALS is similar to PLS with a highland soil composition. Spatial and diurnal variability of around 40 K and 175 K has been observed in the surface temperatures at ALS. Although belonging to similar location like PLS, ALS showed reduced daytime temperatures and enhanced night-time temperatures compared to PLS, indicating a terrain of distinctive thermophysical characteristics. Like PLS, ALS is also seems to be an interesting site for science investigations and Chandrayaan 3 is expected to provide new insights into the understanding of lunar science even if it happens to land in the alternate landing site. |
|
dc.description.statementofresponsibility |
by Durga Prasad Karanam, Dibyendu Misra, Amitabh, Megha Bhatt, G. Ambily, Sachana Sathyan, Neeraj Srivastava and Anil Bhardwaj |
|
dc.language.iso |
en_US |
|
dc.publisher |
Cornell University Library |
|
dc.title |
Chandrayaan-3 alternate landing site: pre-landing characterisation |
|
dc.type |
Article |
|
dc.relation.journal |
arXiv |
|