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 …

Selection of the InSight landing site

M Golombek, D Kipp, N Warner, IJ Daubar… - Space Science …, 2017 - Springer
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 …

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 …

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 …

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 …

Surface characteristics of the Zhurong Mars rover traverse at Utopia Planitia

L Ding, R Zhou, T Yu, H Gao, H Yang, J Li, Y Yuan… - Nature …, 2022 - nature.com
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 …

Linking the collisional history of the main asteroid belt to its dynamical excitation and depletion

WF Bottke Jr, DD Durda, D Nesvorný, R Jedicke… - Icarus, 2005 - Elsevier
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 …

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 …

The Tharsis mantle source of depleted shergottites revealed by 90 million impact craters

A Lagain, GK Benedix, K Servis, D Baratoux… - Nature …, 2021 - nature.com
The only martian rock samples on Earth are meteorites ejected from the surface of Mars by
asteroid impacts. The locations and geological contexts of the launch sites are currently …

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 …