Results 151 to 160 of about 2,119 (200)

The WheelCams on the IDEFIX rover. [PDF]

Prog Earth Planet Sci
Murdoch N, Lalucaa V, Sunday C, Tardivel S, Bertrand J, Théret N, Vivet D, Amsili A, Robin C, Delton P, Duchene A, Douaglin Q, Maillard A, Virmontois C, Vernazza P, Jorda L, Groussin O, Miyamoto H, Vincent JB, Flahaut J, Biele J, Barnouin O, Hartzel C, Buse F, Barthelmes S, Ulamec S, Michel P, Baroukh J.   +27 more
europepmc   +1 more source

If Flowers grew on Deimos

, 2020
openaire   +1 more source

Correction: Effect of nanostructuration on the spin crossover transition in crystalline ultrathin films.

Chem Sci, 2019
Rubio-Giménez V, Bartual-Murgui C, Galbiati M, Núñez-López A, Castells-Gil J, Quinard B, Seneor P, Otero E, Ohresser P, Cantarero A, Coronado E, Real JA, Mattana R, Tatay S, Martí-Gastaldo C.   +14 more
europepmc   +1 more source

DePhine – The Deimos and Phobos Interior Explorer [PDF]

Advances in Space Research, 2018
Peerreview
Alexander Zakharov, Andrew Coates, Konrad Willner   +2 more
exaly   +10 more sources

Spacecraft Exploration of Phobos and Deimos [PDF]

Planetary and Space Science, 2014
AbstractWe review the previous exploration of Phobos and Deimos by spacecraft. The first close-up images of Phobos and Deimos were obtained by the Mariner 9 spacecraft in 1971, followed by much image data from the two Viking orbiters at the end of the 70s, which formed the basis for early Phobos and Deimos shape and dynamic models.
Alexander Zakharov, Edward A Guinness, Harald Hoffmann   +2 more
exaly   +4 more sources

Spatial Distribution of Impact Craters on Deimos [PDF]

Icarus, 2017
Deimos, one of the Martian moons, has numerous impact craters. However, it is unclear whether crater saturation has been reached on this satellite. To address this issue, we apply a statistical test known as nearest-neighbor analysis to analyze the ...
Hirata, Naoyuki
exaly   +2 more sources

Astrometric Observations of Phobos and Deimos With the SRC on Mars Express

Astronomy and Astrophysics, 2006
Observations of Phobos and Deimos, carried out by the SRC (Super Resolution Channel) on the Mars Express spacecraft between May 2004–April 2005, were used to determine the center-of-figure positions of the two Satellites with accuracies of 0.5–5 km ...
Thomas Roatsch, J Oberst, G Neukum
exaly   +2 more sources

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Deimos: An Obstacle to the Solar Wind

Science, 1995
Two isolated solar wind disturbances about 5 minutes in duration were detected aboard the Russian spacecraft Phobos-2 upon its crossing the wake of the martian moon Deimos about 15,000 kilometers downstream from the moon on 1 February 1989.
Sauer, K., Dubinin, E., Baumgärtel, K., Bogdanov, A.   +3 more
openaire   +3 more sources

Phobos and Deimos Cartography

Planetary and Space Science, 2014
Abstract This paper presents an overview of developments in the cartography of the Martian moons Phobos and Deimos from the early satellite images to recent maps based on data from past and on-going Mars missions, especially Viking and Mars Express. We describe in detail the definition and use of special projections for these irregular-shaped bodies.
Konrad Willner, M Wählisch, J Oberst
exaly   +2 more sources

Mars Phobos and Deimos Survey (M-PADS) – A Martian Moons Orbiter and Phobos Lander [PDF]

Advances in Space Research, 2009
We describe a Mars 'Micro Mission' for detailed study of the martian satellites Phobos and Deimos. The mission involves two ~330 kg spacecraft equipped with solar electric propulsion to reach Mars orbit.
Andrew J. Ball, John C Zarnecki
exaly   +2 more sources