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GEOS 22060/32060 – Spring 2019 – Homework 4 Due in Kite mailbox (which is in the mailroom on the 1 st floor of the Hinds building) 4pm Friday 17 th May. To get to the mailroom on the 1 st floor of the Hinds building, turn left on entering Hinds through the main (East) entrance, walk past the sofas, and just after entering a windowless corridor, the mailroom will be the first room on your left. No credit will be given for answers without working. It is OK to use e.g. Mathematica, but if you do, please print out the work. Q1. Effect of Supercontinent Formation. Mountains are important to the global weathering budget. This is because mountain uplift increases the amount of material available for weathering per year (the sediment mass flux). Because the total planet-integrated weathering must be constant (averaged over >10 7 yr timescales) in order to avoid a climate runaway, the increase in material available for weathering must be compensated by a decrease in the amount of weathering per unit sediment. The easiest way to decrease the amount of weathering per unit sediment is to lower the planet temperature. (The lowering of temperature is accommodated by a transient pulse of increased weathering. This transient increase in weathering lowers the CO2 concentration, which lowers temperature. The planet is now less efficient at weathering each sediment parcel, and so the climate re- equilibrates at a new, lower temperature). The purpose of this question is to work through the order-of-magnitude effect on planetary climate of forming new mountain belts. Earth 280 Ma. Credit: Ron Blakey (NAU). The most recent global supercontinent, Pangea, was completed ~280 Ma by collision of North America with Africa. The collision (the Alleghenian orogeny) created a mountain chain, the Central Pangean Mountains. The Appalachian Mountains approximately correspond to a remnant of this mountain belt. In this question, use the paleogeographic reconstruction above (grid spacing 30 degrees) and Earth radius = 6x10 6 m.

GEOS 32060 2019 Homework 4 - UChicago GeoScigeosci.uchicago.edu/~kite/doc/GEOS_32060_2019_Homework_4.pdf · Assume weathering efficiency (cations/yr/km^3 of sediment flux) scales

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Page 1: GEOS 32060 2019 Homework 4 - UChicago GeoScigeosci.uchicago.edu/~kite/doc/GEOS_32060_2019_Homework_4.pdf · Assume weathering efficiency (cations/yr/km^3 of sediment flux) scales

GEOS22060/32060–Spring2019–Homework4DueinKitemailbox(whichisinthemailroomonthe1stflooroftheHindsbuilding)4pmFriday17thMay.Togettothemailroomonthe1stflooroftheHindsbuilding,turn leftonenteringHinds through themain (East)entrance,walkpast thesofas,andjustafterenteringawindowlesscorridor,themailroomwillbethefirstroomonyour left.Nocreditwillbegiven foranswerswithoutworking. It isOK tousee.g.Mathematica,butifyoudo,pleaseprintoutthework. Q1. Effect of Supercontinent Formation.Mountains are important to theglobalweathering budget. This is because mountain uplift increases the amount ofmaterial available forweathering per year (the sedimentmass flux). Because thetotal planet-integrated weathering must be constant (averaged over >107 yrtimescales) inordertoavoidaclimaterunaway, the increase inmaterialavailableforweatheringmustbecompensatedbyadecreaseintheamountofweatheringperunit sediment. The easiest way to decrease the amount of weathering per unitsediment is to lower the planet temperature. (The lowering of temperature isaccommodatedbyatransientpulseofincreasedweathering.ThistransientincreaseinweatheringlowerstheCO2concentration,whichlowerstemperature.Theplanetis now less efficient at weathering each sediment parcel, and so the climate re-equilibratesatanew,lowertemperature).Thepurposeofthisquestionistoworkthroughtheorder-of-magnitudeeffectonplanetaryclimateofformingnewmountainbelts.

Earth280Ma.Credit:RonBlakey(NAU).The most recent global supercontinent, Pangea, was completed ~280 Ma bycollision of North America with Africa. The collision (the Alleghenian orogeny)created a mountain chain, the Central Pangean Mountains. The AppalachianMountains approximately correspond to a remnant of this mountain belt. In thisquestion,use thepaleogeographic reconstructionabove (grid spacing30degrees)andEarthradius=6x106m.

Page 2: GEOS 32060 2019 Homework 4 - UChicago GeoScigeosci.uchicago.edu/~kite/doc/GEOS_32060_2019_Homework_4.pdf · Assume weathering efficiency (cations/yr/km^3 of sediment flux) scales

Assume weathering efficiency (cations/yr/km^3 of sediment flux) scales as

whereE isactivationenergyandR isthegasconstant,8.314J/mol/K,andsurfacetemperature T is in K. Assume an effective activation energy for weathering(“effective”includingtheeffectoftemperatureonrainfall)ofE=74kJ/mol(Westetal.,Earth&PlanetaryScienceLetters,2005).

(a) Supposepaleomagneticdata1indicateAfricatravelledNat5cm/yrandcollidedwithastationaryNorthAmerica.Assumecontinentalcrustis35kmthick.Becausecontinentsarebuoyantrelativetothemantle,neithercontinentsubducts.Atsteadystate,continentalcrustismovinguptothesurface atmountain belts, undergoingweathering and erosion, and themass is being redistributed away from the mountain-belt, all at equalrates.What is themass flux? Suppose thepre-collision eroded fluxwasequaltoEarth’smodernsedimentfluxof8km3/yr;whatisthefractionalchangeinerodedflux(i.e.,mass/volumeavailableforweathering)?

(b) Assumeanactivationenergyforthetemperatureeffectonweatheringof74kJ/mol(Westetal.,Earth&PlanetaryScienceLetters2005).Whatisthesignandmagnitudeofplanetarytemperaturechange?

(c) SupposethattheicesheetintheSHemispheregrows.Isthisapositiveornegativefeedbackonthechangeyoucalculatedinpart(b)?Why?

(d) Itisoftensaidofwarmingclimatesthat“wetareasgetwetter,dryareasgetdrier.”2Giventhatweatheringratedependsonbothtemperatureandrainfall,explainqualitativelyhowchangesinrainfallontheCentralPangeanMountainsduetothewarmingyoucalculatedinpart(b)wouldfeedbackon(andthusmodify)youranswertopart(b).

(e) Supposethatcollisionhadoccurredinthedesertbeltat25°Ninsteadofatthehumidequator.Explainhowyouanswertopart(d)woulddiffer.

TheformationoftheHimalayasandTibetisoneleadinghypothesisforthecoolingofEarththatledtotheonsetoficesheetsonAntarctica~35Myrago.Q2. Tidally Locked Exoplanet.Many, perhapsmost, of the rockyhabitable-zoneplanets in the Universe orbit M-dwarf stars; these are also the easiest habitable-zonerockyplanetstodetectandcharacterize.However,becauseM-dwarfsarefaint,

1 Paleomagnetic data provide great constraints on latitudinal drift rates, butconstrainingpaleo-longitudinaldriftrequireslessdirectmethodssuchasmatchingupgeologicprovincesoneithersideofariftzone,orlookingforevidenceofhotspotvolcanism(hotspotsareunderlainbymantleplumes,whichmoveslowlyrelativetoplatesandsodefinea“hotspotreferenceframe”).2This is not always exactly true. For example, an expanding Hadley cell underwarming (the Hadley cells are currently expanding due to anthropogenic globalwarming)canturnthelow-latitudeedgeofthedesertbeltintoawetzone.

Page 3: GEOS 32060 2019 Homework 4 - UChicago GeoScigeosci.uchicago.edu/~kite/doc/GEOS_32060_2019_Homework_4.pdf · Assume weathering efficiency (cations/yr/km^3 of sediment flux) scales

the habitable zone is located close to the star (i.e. the ratio of planet radius r toorbital radius a ismuch smaller than on Earth). Because tidal locking timescalesscaleasa-5forconstantr,suchplanetsareveryvulnerabletotidallocking.

Surface temperature on a tidally locked planet, calculated using an idealized 1Dclimatemodel. Thenumbers 0.001à10 correspond to atmospheric pressure in bars.Localtemperature iscontrolledbythegreenhouseeffect,butalsobythetendencyofthickeratmospheres to redistributeenergy fromthe lightside to thedarkside. (FromKiteetal.ApJ2011)Considerthetidallylockedplanetfromthefigure.

(a) Asinpreviousquestion,assumeweatheringratescalesas

where E is activation energy and R is the gas constant. Assume aneffectiveactivationenergyforweathering(“effective”includingtheeffectof temperatureonrainfall)of74kJ/mol,as fortheprevioushomework.Forthe0.01bartidallylockedplanetcase,whatistheratioofweatheringrateatthesubstellarpointtoweatheringrateat60°fromthesubstellarpoint?

(b) Assumingmountainbelts/tectonicupliftzonesarerandomlydistributedwithdistancefromthesubstellarpoint,commentonwhereontheplanetmostweatheringoccurs.Considerthelikelyeffectoficecover.

(c) Now assume that the gas that is the principal constituent of theatmosphere is also the principal greenhouse gas. (This assumptionwasusedtocalculatethetemperaturesshownintheplot.Thisassumptionisnot true for theEarth,but is true forMars,Venus,Triton, andarguablyalsoTitan).Explainhowtheplanet-integratedweatheringratechangesasweincreasepressurefrom0.001à10bars.

(d) Isthishypotheticalplanetstabletoasuddentwo-foldstepincreaseinthevolcanicoutgassingrate?Why?

Page 4: GEOS 32060 2019 Homework 4 - UChicago GeoScigeosci.uchicago.edu/~kite/doc/GEOS_32060_2019_Homework_4.pdf · Assume weathering efficiency (cations/yr/km^3 of sediment flux) scales

(e) Now assume that everything is the same as in (e), but the effectiveactivationenergyisnow1000kJ/mol.Isthishypotheticalplanetstabletoa sudden two-fold step increase in the volcanic outgassing rate?Why?Hint: Recall that the threshold surface temperature for runawaygreenhouseonaplanetwithwateroceansis~330K.