Results 81 to 90 of about 3,391 (216)
Studying mid-range planar orbits around phobos
The goal of the present paper is to search and study mid-range planar orbits for a spacecraft traveling near Phobos. The first step is to make a numerical search and classification of natural orbits based in the concept of “Quasi Satellite Orbits” (QSO).
Cavalca, M. P.O. +4 more
core +1 more source
Context. Tianwen-1 was successfully launched in July 2020 and has been operating normally since entering its remote sensing exploration phase in February 2021. The High-Resolution Imaging Camera (HiRIC) aboard Tianwen-1 provided a valuable opportunity to
Liu Dingxin +6 more
doaj +1 more source
Multifractal model for Phobos crater size-frequency distribution [PDF]
We present analytical functions which well reproduce the essential features of empirical crater size-frequency distributions for the Martian satellite Phobos.
Uchaev, D.V. +3 more
core
An ambitious new mission seeks the origin of the moons of Mars. [PDF]
Croswell K.
europepmc +1 more source
88th Annual Meeting of the Meteoritical Society 2026: Contents
Meteoritics &Planetary Science, Volume 61, Issue S1, Page S2-S47, August 2026.
wiley +1 more source
Origin of Phobos and Deimos: Orbital Evolution Shortly after Formation from a Potential Dislocation
This paper deals with the formation and evolution of Mars’ moons, Phobos and Deimos, assuming the dislocation of a larger progenitor as the origin of these moons. The study by R. Hyodo et al.
Ryan Dahoumane +2 more
doaj +1 more source
88th Annual Meeting of the Meteoritical Society 2026: Abstracts
Meteoritics &Planetary Science, Volume 61, Issue S1, Page S48-S551, August 2026.
wiley +1 more source
JAXA’s Mars Moon eXploration (MMX) spacecraft carries a NASA-provided γ-ray and neutron spectrometer called MEGANE. MEGANE’s measurements will be used to characterize the elemental composition of Mars’ largest and innermost moon, Phobos, with the goal of
Patrick N. Peplowski +10 more
doaj +1 more source
Exogenous carbonaceous material on Phobos
Aims. We analyze Mars Express (MeX)/OMEGA Phobos’ data in the 2.5–3.9 μm range to investigate the presence of organic material. Methods. We applied a thermal correction to the OMEGA data and identified regions of interest (ROIs) to extract mean spectra ...
Beccarelli J. +9 more
doaj +1 more source
Phobos always keeps the same side facing its host planet like Earth’s Moon, making it a key comparative target for studying the coevolution of planet–satellite systems.
Yuki Uchida +4 more
doaj +1 more source

