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Publikováno v:
In Planetary and Space Science 15 October 2018 161:68-75
Autor:
D. K. Patel, Syed A. Haider, Ashok Kumar, J. P. Pabari, B. M. Pandya, R.K. Singh, A. Bogavelly
Publikováno v:
Planetary and Space Science. 161:68-75
Dust at orbital altitude on Mars could be mainly due to interplanetary source, cometary source or natural satellites of Mars. Recent work and MAVEN observations predict that dust at orbital altitudes could be interplanetary in nature. Since, the sour