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ASTR 380
Our Solar System: A worked Example
Themes in Our Solar System Temperature TrendsEnergy for Life
Rocky, Gassy. IcyAtmospheresMoonsStabilitySpecial ConditionsWinning the Lottery
Temperature Trends in our Solar System
The Sun is the primary source of energy in the Solar System.As a first approximation,
energy in = energy out equilibrium Temperature
Planets further from Sun are colder.
Temperature unit:Kelvins
373 K = boiling water273 K = 32 F Freezing77 K = air freezes
Temperature Trends in our Solar System
Mercury : 670 K on the day side70 K on the night side
Venus: 740 K on surfacelittle variation in day-night
BUT should be 350 K except foratmosphere -- greenhouse effect
Earth: average – 288 Klow – 225 K high – 325 K
But should be 255 K average ifno atmosphere
Temperature Trends in our Solar System
Jupiter: average – 150 Kdepends on depth in
atmosphere
Mars: average -- 215 low – 135 high – 290
Saturn: average – 130 Kdepends on depth in
atmosphere
Temperature Trends in our Solar System
#1 effect is heating by Sun……but
day-night and seasonal changes makes for variations!
Atmospheres tend to warm planetsand smooth out variations
Venus740K Not 350K
There remains a clear trend: 1 – 3 AU is best for life…
Temperature Trends in our Solar System
Secondary Effects:
Internal heat within planet:on Earth Geothermal
Even if the Earth were coldGeothermal activity would continue
Arises from Earth’s molten core and mantle
The heat comes from radioactive decay ofelements in the mantle and core!
Temperature Trends in our Solar System We can see that geothermal activitywas present on Venus, Mars, andeven our Moon.
But for bodies significantly smallerthan the Earth, radioactive decaydoes not generate enough heat tokeep the core molten.
We know that the Moon is solid
We suspect that Mars is solid
We expect that Venus is still active!
Olympus Mons on Mars
Moon
Temperature Trends in our Solar System Tides can heat Moons:
Io, a moon of Jupiter is theprime example in ourSolar System
Has observed lava flows withhot-spot temperaturesof 1300-1600 K
Io is a rocky moon – the other big moonsof Jupiter are icy
Temperature Trends in our Solar System Tides can heat Moons:
Titan, a moon of Saturn may be a second interesting example….
Methane volcanoes indicate that itsinterior is kept warm. Compare toits surface temperature of 94 K!
Energy for Life Basic truth: Life requires energy!
Solar, geothermal, chemical…. Energy to enable the ordered activity that is life.
From Earth’s example, life exploits all available energy.
But life is limited by the availability of energy.
Fundamental unknown:Can life originate in isolated islands of energy?Or does it require abundant, widespread availability?
Tubeworms near a vent
Bacteria 400 metersBelow the seabed
Rocky, Gassy, Icy Theme: rocky, gassy, and icy planets and dwarf planets in our Solar System.
Rocky: close to Sun; within 4 AUGassy: middle distance from Sun; 5 – 30 AUIcy: far from Sun; 30 AU an beyond
Temperature and availability of material during formation cause this trend of planet type with distance.
Rocky, Gassy, Icy Rocky: formed in the inner Solar System after most gas gone
modest amount of rocky material so no big planets
Rocky planets too small to capture gas at birth
Atmosphere created from gases in rocks and impacts of comets.
Early heat on planet kept away ices and gas.
Rocky, Gassy, Icy Gassy: grew in places where rocky cores could attract gas
rocky cores at center
primarily hydrogen and Helium gas
lots of material in this region in birth nebula
Rocky, Gassy, Icy Icy Dwarf Planets:grew in places with rock and ices
little material so never grew big
could not hold into hydrogen and helium so no big atmospheres
Big cousins of comets and perhaps millionsof Kuiper-Belt objects
Artist’s concept of SednaPlot of known Kuiper Belt Objects
Atmospheres
Solar System Atmospheres have three origins:
1. Gas captured during birth of planet Gas Giant planets did this! Hydrogen, Helium dominant
2. Outgassing from molten rock on the surfaceterrestrial planetscarbon Dioxide, sulfur dioxide, water,
methane, ammoniavolcanic activity continues this process
3. Comet impactshappened on all planets but most important
for terrestrial planets
Jupiter’s Atmosphere
Venus Atmosphere
Atmospheres Solar System Atmospheres have three origins:
1. Gas captured during birth of planet
2. Outgassing from molten rock on the surface
3. Comet impacts
Atmospheres BUT…. Why are Venus, Earth and Mars so different?
Venus probably kept all of its atmosphere
Mars lost most of its atmosphere
Earth kept just the right amount due to the collision that made the Moon.
Atmospheres Mars size impactor completely destroyed
Earth surface all moltenAtmosphere ripped off
Moon reform in orbit fromdebris
Earth crust reforms
Moons
The terrestrial planets have rocky moons, and few of them
The gas giants and icy dwarf planets have rocky and icy moonssometimes many moons.
There are different stories for many of the planets:
Mercury – no moons – too close to SunVenus – no moons -- ?Earth – 1 big moon – created by a collisionMars – 2 small moons – captured asteriodsGas Giants – many moons – some formed in
a mini-solar system during birth, others captured
Moons of Uranus
Phobos
Demos
Stability
Earth life required time to form and to evolve.
Life began on Earth 200-400 Million years afterthe crust became cool. About 1 Billion yearsafter formation.
Around 1.6 Billion years cyanobacteria
Around 3.4 Billion years multicell organisms
Earth life required sufficient stability to maintainlife but enough change and variability to driveevolution.
Special Conditions
Earth life required:rocky surfaceliquid waterright amount of atmosphereright temperature rangemulti-billion year stability
It is even argued that life required our big Moon…to get rid of the excessive atmosphere
at the collisionto raise large tides to drive evolution
Winning the Lottery One could argue that life on Earth is a
One in a millionOne in a billionOr larger
Long shot.
But we are here so may be it had to be…..
Or maybe
we are the one winners of the lifelottery in the millions of planets in our Galaxyand the millions of galaxies in the Universe!