Tharsis quadrangle

[2] The quadrangle covers the area from 90° to 135° west longitude and 0° to 30° north latitude on Mars and contains most of the Tharsis Rise.[4] Pavonis Mons, the middle in a line of three volcanoes, sits at just about dead center on the equator.It has been proposed that these are the result of plate motion which on Earth makes volcanic arc islands.[5][6][7][8][9] Although Mars displays many volcanoes here and other places, there has been no evidence of recent volcanic activity, even at a very low level.Research, published in 2017, found no active release of volcanic gases during two successive Martian years.The greenhouse effect of carbon dioxide raises the temperature of a planet by trapping heat in the form of infrared radiation.[3] The Tharsis quadrangle is also home to large troughs (long narrow depressions) called fossae in the geographical language used for Mars.Sinkholes, where the ground falls into a hole (sometimes in the middle of a town) resemble pit craters on Mars.[15][16] Knowledge of the locations and formation mechanisms of pit craters and fossae is important for the future colonization of Mars because they may be reservoirs of water.[32] [33] [34] [35] Some researchers have suggested that lava flows covered the ice cap, thereby causing it to melt rather quickly.We know a lot about it because the solar panels of the Mars Rovers get covered with it, thus reducing the electrical energy.Research, published in January 2012 in Icarus, found that dark streaks were initiated by airblasts from meteorites traveling at supersonic speeds.The crater cluster lies near the equator 510 miles) south of Olympus Mons, on a type of terrain called the Medusae Fossae formation.The largest crater in the cluster is about 22 meters (72 feet) in diameter with close to the area of a basketball court.As the meteorite traveled through the Martian atmosphere it probably broke up; hence a tight group of impact craters resulted.
Image of the Tharsis Quadrangle (MC-9). The region contains the Olympus Mons , Ascraeus Mons and Pavonis Mons , three of the four largest shield volanoes on Mars. The north-central part contains Ceraunius Fossae .
Ulysses Fossae mound, as seen by HiRISE
Sulci Gordii Terraced Hills, as seen by HiRISE . Many dark slope streaks are visible.
quadrangleMars Orbiter Laser AltimeterOlympus MonsAscraeus MonsPavonis MonsCeraunius Fossaequadrangle maps of MarsUnited States Geological SurveyAstrogeology Research ProgramTartessusGuadalquivirTharsis RisePoyntingVolcanology of MarsvolcanoesplateauCrater LakeOregoncarbon dioxidegreenhouse effectinfrared radiationUlysses FossaeOlympica FossaeTractus FossaeNoctis LabyrinthusgrabenSinkholeslimestoneGlaciers on MarsglaciersSulci GordiiHiRISETharsis Tholussolar panelsMars Roversdust devilsMariner 9supersonicUniversity of ArizonascimitarsmeteoritesMedusae FossaeyardangsMars Reconnaissance OrbiterMars Global SurveyorClimate of MarsDark slope streaksFossa (geology)Geology of MarsGlacierList of mountains on MarsList of quadrangles on MarsRahe (crater)TholusTrue polar wander on MarsVolcanoWater on MarsBibcodeCiteSeerXSpace.comQuadrangles on MarsMare BoreumDiacriaArcadiaAcidaliumIsmenius LacusCasiusCebreniaAmazonisLunae PalusOxia PalusArabiaSyrtis MajorAmenthesElysiumMemnoniaPhoenicis LacusCopratesMargaritifer SinusSinus SabaeusIapygiaMare TyrrhenumAeolisPhaethontisThaumasiaArgyreNoachisHellasEridaniaMare AustraleOutline of MarsGeographyAtmosphereCirculationClimateDust devil tracksMethaneRegionsArabia TerraCerberus (Mars)CydoniaEridania LakeIani ChaosOlympia UndaePlanum AustralePlanum BoreumQuadranglesSinus MeridianiTempe TerraTerra CimmeriaTerra SabaeaTharsisVastitas BorealisPhysicalfeatures"Canals"CatenaeChaos terrainCratersFossaeGulliesMensaeMountainsby heightObserved rocksOutflow channelsPlainsValley networkValleysGravityGeologyBrain terrainCarbonatesCompositionConcentric crater fillDark slope streakDichotomyFretted terrainGeysersGroundwaterLava tubesLobate debris apronMarsquakeon Earthon MarsMud cracksNorth Polar BasinOcean theoryOre resourcesPolar capspolar wanderRecurring slope lineae (RSL)Ring mold cratersRootless conesSeasonal flowsSpherulesSurface"Swiss cheese" featureTerrain softeningVolcanismHistoryAmazonianHesperianNoachianObservation historyClassical albedo featuresAstronomyPhobosStickney craterLimtoc craterMonolithDeimosSwift craterVoltaire craterTransitsSolar eclipses on MarsMercuryAsteroidsImpactsMars-crossers2007 WD5Trojans5261 Eureka1998 VF311999 UJ72007 NS2C/2013 A1 (Siding Spring)ExplorationOrbiterLandingSample returnHuman missionPermanent settlementColonizationTerraformingList of missions to MarsThe Mars ProjectThe Case for MarsInspiration Mars FoundationMars InstituteMars SocietyMars raceArtificial objects on MarsFictionList of films set on MarsMartian scientistMythologyFlag of MarsLife on MarsSub-EarthTimekeeping on MarsSol (day on Mars)Darian calendar