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The Yarkovsky and YORP effects: Implications for asteroid dynamics
WF Bottke Jr, D Vokrouhlický… - Annu. Rev. Earth …, 2006 - annualreviews.org
Abstract The Yarkovsky and YORP (Yarkovsky-O'Keefe-Radzievskii-Paddack) effects are
thermal radiation forces and torques that cause small objects to undergo semimajor axis drift …
thermal radiation forces and torques that cause small objects to undergo semimajor axis drift …
Selection of the InSight landing site
The selection of the Discovery Program InSight landing site took over four years from initial
identification of possible areas that met engineering constraints, to downselection via …
identification of possible areas that met engineering constraints, to downselection via …
Mars reconnaissance orbiter's high resolution imaging science experiment (HiRISE)
AS McEwen, EM Eliason, JW Bergstrom… - Journal of …, 2007 - Wiley Online Library
The HiRISE camera features a 0.5 m diameter primary mirror, 12 m effective focal length,
and a focal plane system that can acquire images containing up to 28 Gb (gigabits) of data …
and a focal plane system that can acquire images containing up to 28 Gb (gigabits) of data …
Context camera investigation on board the Mars Reconnaissance Orbiter
MC Malin, JF Bell III, BA Cantor… - Journal of …, 2007 - Wiley Online Library
The Context Camera (CTX) on the Mars Reconnaissance Orbiter (MRO) is a Facility
Instrument (ie, government‐furnished equipment operated by a science team not …
Instrument (ie, government‐furnished equipment operated by a science team not …
Geologic history of Mars
MH Carr, JW Head III - Earth and Planetary Science Letters, 2010 - Elsevier
Mars accumulated and differentiated into crust, mantle and core within a few tens of millions
of years of Solar System formation. Formation of Hellas, which has been adopted as the …
of years of Solar System formation. Formation of Hellas, which has been adopted as the …
Surface characteristics of the Zhurong Mars rover traverse at Utopia Planitia
Abstract China's Mars rover, Zhurong, touched down on Utopia Planitia in the northern
lowlands of Mars (109.925° E, 25.066° N) in May 2021, and has been conducting in situ …
lowlands of Mars (109.925° E, 25.066° N) in May 2021, and has been conducting in situ …
Linking the collisional history of the main asteroid belt to its dynamical excitation and depletion
The main belt is believed to have originally contained an Earth mass or more of material,
enough to allow the asteroids to accrete on relatively short timescales. The present-day …
enough to allow the asteroids to accrete on relatively short timescales. The present-day …
The lunar cratering chronology
The Moon is a unique body in our Solar System that allows us to groundtruth remotesensing
data (eg, crater size–frequency distributions, or CSFDs, crater/rock degradation rates …
data (eg, crater size–frequency distributions, or CSFDs, crater/rock degradation rates …
Present-day impact cratering rate and contemporary gully activity on Mars
MC Malin, KS Edgett, LV Posiolova, SM McColley… - science, 2006 - science.org
The Mars Global Surveyor Mars Orbiter Camera has acquired data that establish the present-
day impact cratering rate and document new deposits formed by downslope movement of …
day impact cratering rate and document new deposits formed by downslope movement of …
The global martian volcanic evolutionary history
SC Werner - Icarus, 2009 - Elsevier
Viking mission image data revealed the total spatial extent of preserved volcanic surface on
Mars. One of the dominating surface expressions is Olympus Mons and the surrounding …
Mars. One of the dominating surface expressions is Olympus Mons and the surrounding …