...J.W. Head; L. Wilson; J. Dickson; G. Neukum Abstract Two narrow, broadly arcuate, low ridges extend for 600–700 km in western Terra Tyrrhena, Mars, crosscut ancient Noachian terrain, and are associated with Early Hesperian plains, which cover ∼30% of Mars. Geological relationships suggest...

... evidence for liquid water in the form of abundant valley networks (e.g., Carr, 1995 ). Other works have examined hydrated minerals in Terra Tyrrhena ( Mustard et al., 2008 ), Argyre basin ( Buczkowski et al., 2008 ), Holden crater ( Grant et al., 2008 ), and Eridania basin ( Noe Dobrea et al., 2008a ). We...

... to display the images). Fraeman et al. (2009) surveyed Noachis Terra and Terra Tyrrhena. Ehlmann et al. (2009) surveyed the area west of the Isidis basin. Fe,Mg-smectites are the most commonly detected alteration minerals, though localized instances of greater mineralogic diversity are observed...

... indicate maximum P T values ( P T ,max ); red dashed outline indicates regions with low P T ,max (TT—Tyrrhena Terra). (C) White columns indicate P T ranges from coupled systems. Blue/red triangles—open/closed systems. Elevation data are from Mars Orbiter Laser Altimeter (MOLA). ...

...)98<182:SAGVIS>2.0.CO;2 . Williams R.M.E. Rogers A.D. Chojnacki M. Boyce J. Seelos K.D. Hardgrove C. Chuang F. , 2011 , Evidence for episodic alluvial fan formation in far western Terra Tyrrhena, Mars : Icarus , v. 211 , p. 222 – 237 , doi:10.1016/j.icarus...

... , 2010 ; J ackson et alii , 2011 ), Sinus Meridiani ( F lahaut et alii , 2015 ), Iani Chaos ( B aioni & T ramontana , 2015 ), Tyrrhena Terra ( B aioni & T ramontana , 2016 ) and other regions ( S chaeffer , 1990 ; S pencer & F anale ,1990 ; McKey & N edell , 1998). Moreover...

... basaltic breccia Northwest Africa 7034 : Science , v. 339 , p. 780 – 785 , doi:10.1126/science.1228858 . Arvidson R.E. 25 others , 2006 , Nature and origin of the hematite-bearing plains of Terra Meridiani based on analyses of orbital and Mars Exploration rover data sets : Journal...

... Science Team ( 2007 ) CRISM observations of hydrated craters deposits in Terra Tyrrhena, Mars . Lunar and Planetary Science Conference XXXVIII , 1994 . Pitman K.M. Wolff M.J. Cloutis E.A. ( 2013 ) Radiative transfer in clusters of regolith particles: Fundamental scattering unit...

... , Evidence for episodic alluvial fan formation in far western Terra Tyrrhena, Mars : Icarus , v. 211 , p. 222 – 237 , https://doi.org/10.1016/j.icarus.2010.10.001 . Williams , R.M. , ., 2013 , Martian fluvial conglomerates at Gale crater : Science , v. 340 , p. 1068 – 1072...

... ) Primordial clays on Mars formed beneath a steam or supercritical atmosphere . Nature , 552 , 88 – 91 . doi: 10.1038/nature24657 . Carrozzo , F.G. , Di Achille , G. , Salese , F. , Altieri , F. , and Bellucci , G. ( 2017 ) Geology and mineralogy of the Auki Crater, Tyrrhena...

.... There are no reported examples that specifically describe linkings in the planetary tectonics literature. However, many candidate examples are present in Hesperia Planum, Mars, especially folds and thrust-fault-related landforms associated with, or in the vicinity of, Hesperia and Tyrrhena Dorsa. There, landforms...