Results 21 to 30 of about 5,913 (246)
Sesquinary catenae on the Martian satellite Phobos from reaccretion of escaping ejecta
The origin of the numerous linear grooves and craters that litter the Martian moon Phobos' surface remains enigmatic. Here, by modelling low-velocity escaping ejecta from impacts to Phobos, the authors show that several of these chains can be explained ...
M. Nayak, E. Asphaug
exaly +2 more sources
The Mean Moment of Inertia for Irregularly Shaped Phobos and Its Application to the Constraint for the Two-Layer Interior Structure for the Martian Moon [PDF]
The interior structure of Phobos has been the subject of debate in recent years, with the moment of inertia being a determining factor. To study this structure, we modeled Phobos with a two-layer structure and calculated its mean density and moment of ...
Zhen Zhong+3 more
doaj +2 more sources
The Mars‐moon Exploration with GAmma rays and NEutrons (MEGANE) investigation will use gamma‐ray and neutron spectroscopy to measure the elemental composition of Mars' moon Phobos.
David J. Lawrence+15 more
doaj +2 more sources
Origin of Phobos and Deimos by the impact of a Vesta-to-Ceres sized body with Mars
Phobos and Deimos are likely remnants of a low-mass disk generated by the impact of a Vesta to Ceres-sized body with Mars. It has been proposed that Mars’ moons formed from a disk produced by a large impact with the planet. However, whether such an event
Robin Canup, Julien Salmon
exaly +2 more sources
Improved version of the PHOBOS Glauber Monte Carlo
“Glauber” models are used to calculate geometric quantities in the initial state of heavy ion collisions, such as impact parameter, number of participating nucleons and initial eccentricity.
Constantin Loizides
exaly +3 more sources
The Importance of Phobos Sample Return for Understanding the Mars-Moon System [PDF]
Tomohiro Usui+2 more
exaly +2 more sources
The rheology and thermal history of Mars revealed by the orbital evolution of Phobos
Henri Samuel+2 more
exaly +2 more sources
Excitation of Tumbling in Phobos and Deimos. [PDF]
Mass-spring model simulations are used to investigate past spin states of a viscoelastic Phobos and Deimos. From an initially tidally locked state, we find crossing of a spin-orbit resonance with Mars or a mean motion resonance with each other does not excite tumbling in Phobos or Deimos. However, once tumbling our simulations show that these moons can
Quillen AC+3 more
europepmc +6 more sources
Recent Results from PHOBOS [PDF]
In this manuscript we give a short summary of recent physics results from PHOBOS. Particular emphasis is put on elliptic flow, fluctuations in the initial geometry and the recent measurements of elliptic flow fluctuations.
E. Garcı́a, Collaboration PHOBOS
+8 more sources
The importance of Phobos simulants: a review on our current knowledge
Phobos, a satellite of Mars, was successfully studied by flyby, orbiter, and landing missions to the Red Planet, but several questions remain about its origin, composition, and relationship to Mars.
Catarina Miranda+10 more
doaj +1 more source