101 Solar System – Planets Terrestrial planets – Mercury, Venus, Earth, Mars Venus: - average distance from Sun (ie. semi-major axis of orbit), a = 0.72 AU ~ ¾ Earth’s distance from Sun Porb = 0.62 yrs = 225 Earth days Kepler III: P2 = a3 - Prot = 243 Earth days Prot > Porb Venusian day longer than Venusian year very small rotation rate - Size and Mass similar to Earth Earth’s “sister planet” - Radius (R) = 0.95 REarth Volume (V) R3 V = 0.82 VEarth Mass (M) 0.82 MEarth gravitational acceleration at surface (“surface gravity”) = g/gE = (M/ME)(RE/R) 2 0.91 Venus can retain an atmosphere - Atmosphere: - visible from Earth appears cloudy, yellowish atmosphere is opaque in visible band blocks view of surface Venus rotates clockwise (CW) as seen from above Earth’s north pole Venus’s rotation is in opposite direction to its revolution has a back-spin - ALL other planets with upright axes rotate CCW (ie. have a top-spin) rotation is retrograde rotation axis is upside-down clue that Venus was struck in a glancing collision with a large body, probably during heavy bombardment era atmosphere thicker than Earth’s atmosphere atmospheric pressure at surface, P = 90 Atmospheres composition: - Carbon dioxide (CO2) – 96% - No Oxygen (O2), No Water (H2O) vapor or liquid 102 - similar to Earth’s atmosphere in earlier epoch Surface temperature of Venus, TSurf, determined by balance between solar heating and Blackbody cooling -CO2 a Greenhouse gas Venus has extreme Greenhouse effect TSurf = 700K 400oC - NOTE: albedo, A = 0.59 with d=0.72 AU TSurf4 without atmosphere = (1-A)LSun/σ16πd2 TSurf = 273 K = 0oC Why do Venus and Earth have such different atmospheres? - both planets probably began with same primordial atmosphere composition due to out-gassing: CO2, H2O, N2 - Runaway Greenhouse effect: - runaway: when a change made to a system results in the original change being amplified an unstable situation - also known as a positive feedback loop - heat baked CO2 out of surface rock (outgassing) increased CO2 in atmosphere increased Greenhouse effect increased Tsurf more CO2 baked out increased CO2 in atmosphere increased Greenhouse effect … a runaway effect - opposite effect as that of a thermostat: heating leads to changes that cause more heating - eventually all CO2 baked out of surface rock situation stabilized at 96% atmospheric CO2 and Tsurf = 700K gave rise to a thick atmoshere with large P Venus closer to Sun warmer H2O did not condense out of atmosphere no ozone (O3) UV photons from Sun eventually destroyed H2O H2O + 2H + O H escaped into space, O bound up in mineral oxides on surface modern atmosphere with no H2O, no O2 Yellow clouds: - high Ts causes sulfur to bake out of rocks and enter atmosphere clouds composed of airborne sulfur grains and droplets of sulfuric acid 103 - Interior and Surface: - atmosphere transparent in radio band surface relief studied by radar ranging - interior is chemically differentiated T and ρ are stratified with depth trapped heat of formation geologically active - Venus volcanically active, BUT no plate tectonics (ie. no faults) high Tsurf and atmospheric P surface rock plastic (like Earth’s mantle) not rigid enough to form tectonic plates Venusian volcanoes differ from Earth volcanoes lava wells up through plastic surface surface geologically young most craters destroyed by surface activity (like Earth) Mars: - average distance from Sun, a = 1.52 AU Porb = 1.88 yrs (Kepler III) Prot = 24.5 hours length of day similar to Earth inclination of rotation axis = 25o seasonal variation similar to Earth’s - Radius, R = 0.53 REarth Volume: V/VE ≈ (1/2)3 =1/8 Density, ρ < ρEarth Mass, M 1/10 MEarth surface gravity: g/gE = (M/ME)(RE/R) 2 0.4 should retain substantial atmosphere BUT, atmospheric pressure at surface, P = 0.006 Atmospheres no liquid H2O - - Interior and surface: - interior differentiated heat of formation melted planet in past extinct volcanoes on surface (eg. Olympus Mons) evidence of past volcanism BUT: Mars small most interior heat already escaped little or no molten core no global magnetic field no mantle convection no plate tectonics, no current volcanism Mars close to geologically dead 104 - has geologically old surface (like Moon) Liquid water (H2O) on Mars: - Mars today: atmospheric surface pressure, P = 0.006 atmospheres Tliquid = 0 K liquid H2O cannot exist on surface, like Moon most H2O in form of ice, small amount in vapor in atmosphere - BUT: there is evidence that there was liquid water on Mars in past - water erosion features, dried up river beds and sea beds - erosion features due to flash-flooding - may be caused by large amounts of ice melting quickly - surface geologically old water features could have been made billions of years ago - explanation: -Martian atmosphere thicker in past larger surface P Tliquid > 0 K for H2O larger Greenhouse effect surface T > Tfreeze for H2O atmosphere must have evolved over time (like Earth’s) as atmospheric P reduced liquid H2O became ice or vapor Atmosphere: - evidence of liquid H2O in past atmospheric P and surface T higher in past atmosphere must have evolved over time - primordial atmosphere: - from volcanic outgassing similar composition to Earth’s primordial atmosphere high concentration of CO2 and H2O vapor Primpordial P higher than present P CO2 and H2O are greenhouse gases greenhouse effect kept Ts higher than present Ts surface warm enough for liquid H2O - first steps in evolution same as Earth: - as Mars cooled H2O vapor in atmosphere condensed to form liquid oceans on surface - atmospheric CO2 dissolved in oceans precipitated into sedimentary rock reduced greenhouse effect cooled surface further 105 - important difference between Mars and Earth: - Mars small already lost interior heat already geologically dead no more volcanic outgassing to replenish atmospheric CO2 - on Mars: runaway icehouse effect: - due to fact that CO2 dissolves in liquid H2O (carbonation of water) - reduced atmospheric CO2 reduced greenhouse effect TSurf lower more atmospheric H2O condensed out CO2 dissolves in H2O more CO2 removed from atmosphere by dissolution in water reduced atmospheric CO2 reduced greenhouse effect TSurf lower … - - end results: - most CO2 and H2O removed from atmosphere atmosphere thinned out atmospheric P reduced to 0.006 Atmospheres - Greenhouse effect reduced Tsurf very low - problem: where did the H2O go? - may be underground, as either liquid or ice - may be under polar CO2 ice caps - - no liquid water no plant life evolved no photosynthesis no free oxygen (O2) no ozone (O3) no protection from solar UV-band photons remaining atmospheric H2O destroyed: H2O + 2H + O H escaped into space O bound up in FeO (Iron Oxide, “rust”) on surface gives Mars red color Seasonal climate variation: - rotation axis inclined to perpendicular to orbital plane by 25o similar to Earth on Mars ecliptic inclined by 25o to celestial equator Mars has seasons has tropical zones between latitudes +25o and -25o arctic zones north of +65o and south of -65o - evidence: - Mars has polar ice caps in arctic zones - polar caps made mostly of CO2 ice (“dry ice”) - there may be some H2O ice underneath CO2 ice - ice caps expand and contract in anti-phase (ie. northern cap large when southern cap small and visa versa) 106 - ice caps vary with a period equal to Martian year (Mars’ Porb) - during Spring in northern hemisphere some CO2 ice in northern cap vaporizes northern cap shrinks - during Autumn in northern hemisphere some atmospheric CO2 freezes (condenses to ice) in northern cap northern cap expands - Mars’ moons: - Phobos & Deimos both minor moons - Diameter, D <30 km asteroid sized planetesimals captured by Mars’ gravity - both moons rotate synchronously (like Earth’s moon) Prot = Porb due to tidal synchronization - Jovian Planets – Jupiter, Saturn, Uranus, Neptune Jupiter - located in outer solar system semi-major axis of orbit, a = 5.2 AU - Kepler III: P(yrs)2 = a(AU)3 P = a3/2 Porb = 11.9 yrs - Radius, R = 11.2 REarth - diameter defined by “surface” where Jupiter becomes opaque Volume: V/VE = (R/RE)3 = 1350 Mass, M = 318 MEarth - largest and most massive planet in solar system average density: /ρE = (M/V)/(ME/VE) = (M/ME)/(V/VE) = 318/1350 ≈ 0.25 Jupiter’s very large volume compensates for its large mass has low mean density surface gravity (at apparent surface), g/gE = (M/ME)(RE/R) 2 = 318/11.22 = 2.4 107 - - - larger R compensates for larger M g only a few × larger than gE Jupiter is able to retain a thicker atmosphere than Earth retains H and He in atmosphere (unlike terrestrial planets) - composition: similar to solar nebula - mostly H and He fluid (ie. gas and liquid phase) - Jupiter held together by force of gravity - Consequences of Jupiter’s fluid structure: - rotational deformation: - rapidly rotating ball of fluid shape is oblate spheroid equatorial D = 11.2 DEarth , polar D = 10.5 DEarth - differential rotation in latitude: - Prot at low latitudes (ie. near equator) < Prot at mid latitudes ie. Jupiter rotates faster near equator than at mid-latitudes Jupiter does not rotate as a solid body, Jupiter constantly sheared along lines of latitude Rotation period, Prot = 9H 50m = 0.4 Prot, Earth short rotation period - equatorial surface velocity, vrot: velocity of surface at equator due to rotation = (distance around planet’s surface)/(time to rotate once) = 2R/ Prot - where: R = equatorial radius of planet - for Earth: vrot, E = 440 m s-1 - vrot/vrot, E = (2πR/ Prot)/(2πRE/ Prot, E) = (R/RE)( Prot, E/ Prot) = 11.2/0.4 = 26 vrot = 26 × 440 km s-1 = 12000 m s-1 Jupiter is a rapid rotator! Atmosphere: - composition: 92% H, 7.8% He trace amounts of methane CH4 and ammonia NH3 gas colored same composition as solar nebula Jovian atmosphere has not evolved, unlike terrestrial atmospheres weather: - Jupiter very massive a lot of heat of formation still trapped in interior (central T = 25000 K) Jupiter emits as Blackbody radiation - Blackbody flux ~ 2 amount of E that it absorbs from sunlight - surface T < 1000 K BB spectrum peaks in IR band (λmax > few 108 - microns) heat flowing out from interior drives convection currents in interior and atmosphere hot updrafts – high pressure zones cool down-drafts – low pressure zones - Jupiter rotating rapidly fast latitudinal winds high and low pressure zones stretched out around planet along lines of latitude “Belt-zone” weather gives Jupiter banded appearance - belts are downdrafts, zones are updrafts - note: on Earth zones are cylonic, due to slower rotation rate - also has cyclonic downdrafts and updrafts at higher latitudes - eg. the great red spot - seen by Galileo in 16th C storm stable for ~400 years! Interior: - Jupiter has large mass pressure in interior very high at a depth of 20000 km P = 1.4106 atmospheres P high enough to squeeze H into liquid form Jupiter has a liquid H mantle - liquid H is a very efficient electrical conductor, like metal liquid H known as liquid metallic Hydrogen Jupiter rotating liquid metallic H circulating trapped heat of formation flowing outward liquid metallic H carries convection currents liquid metallic H zone is a dynamo generates a dipolar magnetic field Jupiter has magnetic North and South poles, like Earth - liquid metallic H an excellent electrical conductor AND mass of liquid H zone large Jupiter’s magnetic field 14 stronger than Earth’s - field traps electrically charged particles from solar wind Jupiter has polar aurorae at center: solid core of rock original proto-planet - mass of rocky core = 8 MEarth BUT R REarth mean density, 8 Earth - large due to extreme compression due to large central Pressure, P (7107 atmospheres) The Jupiter system - major moons, minor moons, and rings - Galilean Moons – major moons - four largest moons 109 - - discovered by Galileo in 16th C. - in order of increasing distance from Jupiter: Io, Europa, Ganymede, Callisto - among largest moons in solar system: - Ganymede: Mass 2 Mass of Earth’s Moon, Radius > R of Mercury - Callisto: Mass of 1.5 Mass of Earth’s Moon, Radius > R of Earth’s Moon - - orbital planes lie in plane of Jupiter’s rotational equator lie close to plane of Jupiter’s orbit - moons revolve and rotate CCW Jupiter system similar to overall solar system - - mass of moons determined from gravitational deflection of Voyager spacecraft from Earth Jupiter system is viewed almost edge-on transit: moon passes in front of Jupiter (note: this differs from definition of transit of an object on the Celestial Sphere) occultation: Jupiter passes in front of moon - ingress and egress: condition when moon is partially in transit or occultation at Jupiter’s limb as occultation or transit is beginning or ending 110 - trajectory mean density, = M/V, of moons ranges from 2000 to 3500 kg/m3 = 1/3 to 1/2 ρEarth of moons < of Earth (5500 kg/m3) outer solar system moons composed of mixture of volatile (ices) and refractory (mineral) material throughout interior - - Synchronizations due to gravitational tides - all moons rotate synchronously Prot = Porb - due to tidal synchronization (like Earth’s Moon) - orbital resonance: - Io, Europa, and Ganymede are within 6105 km of each other mutual gravitational force causes orbital periods, Porb, to become synchronized PGanymede = 2 PEuropa = 4 PIo affects size of orbits, a, via Kepler III a3 P2 - Minor Moons: - Ring system: - several rings - lie in Jupiter’s equatorial plane - composed of microscopic dust grains dust grains have low albedo (A) difficult to see discovered in late 1970’s by Voyager space craft - dust grains orbit Jupiter with prograde revolution (CCW) (like Galilean moons) - Formation of Jupiter system - similar to formation of overall solar system - local region of solar nebula collapsed into rotating disk centered on proto-Jupiter - major moons are smaller proto-planets that formed in disk - 44 known minor moons - asteroid sized - many have retrograde revolution (ie. orbit clockwise (CW)) - many have orbits inclined by large angles to plane of Jupiter’s equator gravitationally captured minor bodies 111 collapse and accretion were heierarchical - Saturn - a = 9.5 AU Porb = 29.5 years Kepler III - note: aJupiter = 5 AU planets of outer solar system widely spaced R ~ 9 REarth V ~ 730 VEarth second largest and second most massive planet in Solar System (after Jupiter) - M = 95 MEarth ~ 1/3 MJupiter = 687 kg/m3 < of water at sea level on Earth least dense planet in solar system - Prot = 10h 14m very rapid rotation (like Jupiter) vrot at surface at equator very large Saturn is most oblate planet in solar system - equatorial D = 9.5 DEarth polar D = 8.5 DEarth Interior and Atmosphere: - Saturn less massive than Jupiter interior pressure, P, smaller interior less compressed liquid metallic H mantle smaller global magnetic field weaker - tapped heat of formation flowing outward convection currents in interior and atmosphere belt-zone weather in atmosphere banded appearance The Saturn System – Rings and moons Rings: - lie in plane of Saturn’s rotational equator - main rings: three distinct rings visible from Earth - - in order of decreasing distance from Saturn: A, B and C rings - - Cassini Division: 4500 km gap between A and B rings 112 - composition: rings are belts of small solid fragments not continuous - fragment size ≈ 10 cm - - fragments composed of ices have large albedo (A) easily visible from Earth due to reflected sunlight - - individual fragments orbit around Saturn (like mini-moons) fragments obey Kepler III: P2 α a3 rings have differential rotation in radial distance are constantly sheared - appearance of rings viewed from Earth changes cyclically from prominent to invisible and back with period = ½ Porb of Saturn - - rings thin: thickness ≈ 30 km - - plane of Saturn’s rotational equator inclined to plane of ecliptic (plane of Earth’s orbit) by 27o - when Saturn’s North or South pole inclined toward Sun we see ring plane from above or below rings prominent - ring plane crossing: when Saturn’s rotation axis lies in plane of sky we see rings edge-on rings invisible - Why rings? – The Roche limit - Roche limit: distance from a body within which another body that is larger than a certain size that is held together mainly by gravity will be destroyed by tidal forces - within Roche limit: force due to tides > force of gravity holding body together - rings of Jovian planets lie within planet’s Roche limit consist of fragments that cannot accrete into a larger body due to tidal force - within a planet’s Roche limit: rings and minor moons - outside a planet’s Roche limit: major and minor moons - terrestrial planets have smaller gravitational field Roche limit close to planet’s surface terrestrial planets do not have rings - ( also, there is less building material in inner solar system to make rings) - Ring structure: - - Voyager spacecraft revealed greater detail 113 - - - additional fainter rings: - D ring inside orbit of C ring - F, G, and E rings (in order of increasing distance from Saturn) outside orbit of A ring - divisions: rings separated by gaps where density of fragments lower (eg. Cassini division) - note: divisions not completely empy - ring sub-structure: - each ring made up of 100’s of ringlets - ringlets braided - complex structure due to combination of Saturn’s gravity, moons’ gravity and mutual gravity among ring fragments - Moon-ring interaction (The cause of the Cassini Division): - - - divisions between rings due to gravity of moons - eg. Cassini division: - moons and ring fragments obey Kepler III: Porb2 a3 at Cassini division: a=1.18×108 m Porb = 11.3 hrs at moon Mimas: a=1.85×108 m Porb = 22.6 hrs Cassini division fragments in a 2:1 orbital resonance with Mimas (like orbital resonance among inner three Galilean moons of Jupiter) Cassini division particles aligned with Mimas at same place in orbit every second orbit pulled out of division by Mimas’ gravity - eg. F ring shepherd moons - F ring bracketed by two minor moons - Prometheus: a aF ring; Pandora: a aF ring from Kepler III: PPrometheus PF ring PPandora Prometheus always overtaking F ring fragments AND F ring fragments always overtaking Pandora F ring fragments pulled forward by Promethues’ gravity vorb increases a increases F ring fragments pulled backward by Pandoras’ gravity vorb decreases a decreases Prometheus & Pandora keep F ring particles confined shepherd moons Moons: - 28 moons, most minor 114 - Titan: - second largest moon in solar system - surface T very low due to large distance from Sun (recall: gas particle vave=(3kT/m)1/2 see Kinetic Theory) retains thick atmosphere; P = 1.5 Atmospheres - composition: 90% Nitrogen (N2), methane (CH4, a hydrocarbon) solar UV photons + CH4 organic chemicals Titan may be promising place to search for primitive life Pluto - neither a Jovian nor Terrestrial planet - solid surface not Jovian - interior composed of mixture of rock and ices not Terrestrial - similar in composition to a moon of a Jovian planet - BUT: orbits Sun directly considered to be a planet - Radius, R = 1/5 REarth smaller than Earth’s Moon Mean density, = 2000 kg/m3 < 1/2Earth even mixture of volatile and refractory material throughout interior - Orbit: a = 40 AU Porb = 250 years Kepler III eccentricity of elliptical orbit, e = 0.25; all other planets have e < 0.1 unusually elongated orbit perihelion distance = 30 AU; aphelion distance = 50 AU Pluto’s orbit crosses Neptune’s orbit inclination of plane of orbit to ecliptic, i = 17o - Pluto’s moon: Charon - Diameter, D = ½ DPluto Pluto-Charon system almost a binary planet - distance from Pluto = 20000 km (DEarth = 12000km) Kepler III: Porb = 6.4 days - Pluto and Charon BOTH have Prot = Porb both have rotation rate tidally synchronized to revolution rate only one period for whole system: 6.4 days both keep same face toward other neither rises or sets as viewed from other - - 115 - - - state that Earth-Moon system is evolving toward Pluto’s uncertain status: Kuiper belt: - belt of icy planetesimals beyond orbit of Neptune - named after Gerard Kuiper who first speculated that the belt existed before it was observed - origin of short period comets - Pluto and Charon may be largest, most visible members of Kuiper belt ie. Pluto not “really” a planet, really a large outer solar system planetesimal