2015
DOI: 10.1016/j.pss.2015.08.018
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Indian Mars-Colour-Camera captures far-side of the Deimos: A rarity among contemporary Mars orbiters

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Cited by 8 publications
(3 citation statements)
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“…The primary scientific goal of MOM is to explore the morphology, topography and mineralogy of surface features, and analyse the atmosphere using the indigenously developed instruments (Arunan and Satish, 2015). The MOM's payload includes a Mars Colour Camera (MCC) for optical imaging (Arya et al, 2015), a Thermal Infrared Imaging Spectrometer (TIS) for surface temperature estimation and mapping composition and mineralogy (Singh et al, 2015), a Mars Exospheric Neutral Composition Analyser (MENCA) to measure in-situ composition of the low-altitude neutral exosphere and its radial distribution (Singh et al, 2015), a Lyman Alpha Photometer (LAP) to determine the deuterium-to-hydrogen abundance ratio of the upper atmosphere (Sridhar et al, 2015), and a Methane Sensor for Mars (MSM) to measure total column of methane in the atmosphere (Mathew et al, 2015).…”
Section: Mars Orbiter Missionmentioning
confidence: 99%
“…The primary scientific goal of MOM is to explore the morphology, topography and mineralogy of surface features, and analyse the atmosphere using the indigenously developed instruments (Arunan and Satish, 2015). The MOM's payload includes a Mars Colour Camera (MCC) for optical imaging (Arya et al, 2015), a Thermal Infrared Imaging Spectrometer (TIS) for surface temperature estimation and mapping composition and mineralogy (Singh et al, 2015), a Mars Exospheric Neutral Composition Analyser (MENCA) to measure in-situ composition of the low-altitude neutral exosphere and its radial distribution (Singh et al, 2015), a Lyman Alpha Photometer (LAP) to determine the deuterium-to-hydrogen abundance ratio of the upper atmosphere (Sridhar et al, 2015), and a Methane Sensor for Mars (MSM) to measure total column of methane in the atmosphere (Mathew et al, 2015).…”
Section: Mars Orbiter Missionmentioning
confidence: 99%
“…Albedo of the Martian surface using the 1.65 µm channel of Methane sensor for Mars (MSM) was also estimated (Singh and Mishra, 2016). Far side of Deimos, the smaller moon of Mars, was imaged by MCC (Arya et al, 2015b), which has not been viewed by any Mars orbiter in the recent time. Mineralogical studies using hyperspectral data enabled the identification of different minerals like sulphates and ferrous based compounds on the surface of Mars (Jain and Chauhan, 2015a), leading to the understanding of the aqueous history of Mars.…”
Section: Exploration Of Mars Through the First Indian Mars Orbiter MImentioning
confidence: 99%
“…Mars Color Camera (MCC), onboard MOM imaged the far-side of Deimos which has not been viewed for the last few decades by any Mars orbiter ( Fig. 4) (Arya et al, 2015b). Four image-frames of the Deimos was acquired on October 14, 2014 at around 13:05 UT which are used to generate a High Dynamic Range (HDR) product so as to enhance the image details.…”
Section: Imaging Of Phobos and Deimosmentioning
confidence: 99%