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Deducing Lunar Regolith Porosity From Energetic Neutral Atom Emission
DOI: 10.1029/2022GL101232 Bibcode: 2022GeoRL..4901232S

Wurz, P.; Galli, A.; Jäggi, N. +6 more

The porosity of the upper layers of regolith is key to the interaction of an airless planetary body with precipitating radiation, but it remains difficult to characterize. One of the effects that is governed by regolith properties is Energetic Neutral Atom (ENA) emission in the form of reflected and neutralized solar wind protons. We simulate this…

2022 Geophysical Research Letters
Chandrayaan-1 16
Dielectric Constant Estimation of Lunar Surface Using Mini-RF and Chandrayaan-2 SAR Data
DOI: 10.1109/TGRS.2021.3103383 Bibcode: 2022ITGRS..6003383K

Kumar, Raj; Das, Anup; Putrevu, Deepak +4 more

2022 IEEE Transactions on Geoscience and Remote Sensing
Chandrayaan-1 9
Dielectric characterization and polarimetric analysis of lunar north polar crater Hermite-A using Chandrayaan-1 Mini-SAR, Lunar Reconnaissance Orbiter (LRO) Mini-RF, and Chandrayaan-2 DFSAR data
DOI: 10.1016/j.asr.2022.04.059 Bibcode: 2022AdSpR..70.4030S

Chauhan, Prakash; Singh, Awinash; Sharma, Aanchal +5 more

Studies of the lunar surface from Synthetic Aperture Radar (SAR) data have played a prominent role in the exploration of the lunar surface in recent times. This study uses data from SAR sensors from three Moon missions: Chandrayaan-1 Mini-SAR, Lunar Reconnaissance Orbiter (LRO) Mini-RF and Chandrayaan-2 Dual Frequency Synthetic Aperture Radar (DFS…

2022 Advances in Space Research
Chandrayaan-1 7
Chronological and compositional mapping of the Mare Orientale basin using Chandrayaan-1 - M3 and LRO datasets
DOI: 10.1016/j.icarus.2021.114844 Bibcode: 2022Icar..37514844K

Karthi, A.; Arivazhagan, S.

The lunar multiring mare basins have different ages, compositions and are associated with the diverse unit of mare deposits, providing evidence for the origin and evolution of the lunar crust. The multiring basins offer the opportunity to assess many unknown questions that may reveal the lunar geologic standpoint. The Mare Orientale basin is one o…

2022 Icarus
Chandrayaan-1 5
New view of the Balmer-Kapteyn region: Cryptomare distribution and formation
DOI: 10.1051/0004-6361/202142306 Bibcode: 2022A&A...659A...4Q

Li, Fei; Yan, Jianguo; Gao, Wutong +4 more

Context. The cryptomare in the Balmer-Kapteyn region is the oldest one on the Moon. Determining the extent and formation of this feature can deepen our understanding of early mare volcanism and help establish temporal and spatial constraints on lunar thermal and volcanic history.
Aims: This paper focuses on the identification of lunar cryptom…

2022 Astronomy and Astrophysics
Chandrayaan-1 4
An Investigation on the Morphological and Mineralogical Characteristics of Posidonius Floor Fractured Lunar Impact Crater Using Lunar Remote Sensing Data
DOI: 10.3390/rs14040814 Bibcode: 2022RemS...14..814S

Salem, Imen Ben; Sharma, Manish; Kumaresan, P. R. +4 more

Lunar floor-fractured craters (FFCs) are a distinguished type of crater found on the surface of the Moon with radial, concentric, and/or polygonal fractures. In the present study, we selected the Posidonius FCC to explore the mineralogy, morphology and tectonic characteristics using remote sensing datasets. The Posidonius crater is vested with a w…

2022 Remote Sensing
Chandrayaan-1 3
Geology of the Crüger-Sirsalis Basin: Evidence for prolonged volcanism in the southwestern near side of the Moon
DOI: 10.1016/j.icarus.2021.114875 Bibcode: 2022Icar..37614875S

Bhatt, Megha; Bhardwaj, Anil; Srivastava, Neeraj +1 more

The Pre-Nectarian Crüger-Sirsalis Basin (centered at 16.0°S, 293.0°E; ~ 475 km in diameter) is a primarily degraded and obscured impact basin on the Moon. This study presents the first geological description of the Crüger-Sirsalis Basin using remote sensing datasets from Lunar Reconnaissance Orbiter (LRO), Chandrayaan-1, and Kaguya missions. An in…

2022 Icarus
Chandrayaan-1 2
Mapping of Compositional Diversity and Chronological Ages of Lunar Farside Multiring Mare Moscoviense Basin: Implications to the Middle Imbrian Mare Basalts
DOI: 10.1088/1674-4527/ac8f8c Bibcode: 2022RAA....22l5002K

Sharma, Manish; Karthi, A.; Arivazhagan, S.

The Mare Moscoviense is an astonishing rare flatland multi-ring basin and one of the recognizable mare regions on the Moon's farside. The mineralogical, chronological, topographical and morphological studies of the maria surface of the Moon provide a primary understanding of the origin and evolution of the mare provinces. In this study, the Chandr…

2022 Research in Astronomy and Astrophysics
Chandrayaan-1 2
Photometric Correction of Images of Visible and Near-Infrared Bands from Chandrayaan-1 Hyper-Spectral Imager (HySI): HySI Photometric Correction
DOI: 10.1007/s11038-021-09544-0 Bibcode: 2022EM&P..126....2B

Lala, Mili Ghosh Nee; Bose, Subhadyouti; Krishna, Akhouri Pramod

Photometric correction is a necessary step in planetary image pre-processing since the images of planetary surfaces are acquired by orbiting spacecraft at various observational geometries. In this study, visible (748 nm) and near-infrared (948 nm) bands of Hyper Spectral Imager (HySI) onboard Chandrayaan-1 have been used to derive a preliminary ph…

2022 Earth Moon and Planets
Chandrayaan-1 2
Petrological and Mineralogical Characteristics of Exposed Materials on the Floors of the Lavoisier and Surrounding Craters
DOI: 10.3390/rs14174313 Bibcode: 2022RemS...14.4313Y

Moon, Seulgi; Yi, Eung Seok; Kim, Kyeong Ja +3 more

Five floor-fractured craters (FFCs), Lavoisier crater and four craters surrounding it (Lavoisier C, Lavoisier E, Lavoisier F, and Lavoisier H), are distributed along the boundary between the northwestern part of the Oceanus Procellarum and the highlands. This study examines the uplifted or exposed materials on the fractured floors of these five im…

2022 Remote Sensing
Chandrayaan-1 2