Astronomy 301 - Wed. Oct. 6Guest lectures, Monday and today:Prof. Harriet DinersteinMonday: The outer planets & their moonsToday: asteroids, comets, & the Kuiper Belt;formation of the Solar SystemDiscovery of the Asteroid BeltCeres - Jan. 1, 1801Pallas - 1802Juno - 1804Vesta - 1807Are these new planets?Controversy over thiswas reminiscent of whathappened 200 yearslater with the discoveryof the “10th planet” Eris.Asteroids with Moons• Some large asteroidshave their own moon,e.g. Ida and Dactyl (left)• Why might this beuseful to us?• Measuring orbit of asteroid’smoon tells us asteroid’s mass• Mass and size give us density• Some asteroids are solid rock;others just piles of rubbleAsteroid Families• Most asteroids orbitin a belt betweenMars and Jupiter• The Trojan asteroidsfollow Jupiter’s orbit• Orbits of somenear-Earth asteroidscross Earth’s orbit,they include theApollos and AtensA Tale of Comet TailsClose Encounters of the Comet KindDeep Impactslams CometTempel, 2005Giotto meetsHalley,1986Where do Comets Come From?Long-Period Comets:an iceball in the OortCloud experiences ajolt or perturbation, andstarts falling in towardsthe Sun. The OortCloud is a spherical,low-density swarm ofsmall, icy bodies.Halley: An “Intermediate-Period” CometMeteor, meteorite: what’s the difference?Meteor: flash of light as a smallrocky object burns up in theEarth’s atmosphere.Bright ones: fireballs, “bolides”Meteorite: the rocky fragmentthat (sometimes) survives thetrip and reaches the ground.Meteor Showers: “Grins” of Extinct CometsPluto: To be or not to be … a Planet• Orbit: large semi-major axis (40 AU), with a relativelylarge eccentricity (e = 0.25) and tilt (17°).• Physical properties: cold (40K). Surface at least partlycoated with frozen methane (CH4).• Its moon Charon is very large relative to Pluto itself.New Kuiper Belt ObjectsVaruna, 2000Quaoar, 2002Sedna, 2003Eris: The Tenth Planet?• Size: larger than Pluto!• Orbit: semi-major axis almost twice Pluto’s (68 AU),with an even larger eccentricity (e = 0.44) and tilt (44°).• Also has a moon that is large for the planet’s size.• Its spectrum also shows the presence of methane iceon the surface, like Pluto.Trans-Neptunian Objects: A New ClassIn retrospect, Pluto was not the ninth planet, but the firstTrans-Neptunian/Kuiper Belt Object to be discoveredThe Kuiper Belt: Remnant of the SolarSystem’s protoplanetary disk← View from the side View from above ↓Any Successful Theory of Formation ofthe Solar System must explain why….1. The major planets all orbit in the same directionand roughly the same plane2. There are two classes of planets, terrestrial andJovian, with different sets of properties3. There are many small bodies in addition, mainly inthe asteroid and Kuiper Belts, and Oort Cloud4. There is evidence of violent events in the past: theEarth’s moon, odd tilts and inclinations, etc.The Nebular Theory of theFormation of the Solar System• Our solar system formed by gravitational collapse of aninterstellar cloud - called the solar nebula(Nebula is the Latin word for cloud)• Kant and Laplace proposed this idea two centuries ago• A large amount of evidence now supports this idea• It implies that the planets formed together with the Sun,which suggests that the formation of a planetary system(star plus accompanying system) must be commonNebular Theory, Part IStep 1: A cool interstellarcloud starts to contractdue to its own gravity. Atfirst it is nearly spherical.Step 2: Its initially slowrotation is amplified bycontraction, so it rotatesfaster, and flattens into aprotostellar disk.Nebular Theory,Part 2Step 3: Clumps of matterform in the disk and growby accretion, the stickingtogether of solid particles.Small bodies form, calledplanetesimals; theyeventually build up intoplanet-sized objectsAsteroids, comets, and Kuiper BeltObjects are the “leftovers,” or debrisAsteroids: rockyplanetesimals, found inthe inner Solar SystemComets & KBOs:icy planetesimalsfound in the outerSolar SystemWhy Two Types of Planets?• The inner parts of thecontracting solar nebula gethotter than the outer parts.• Since rock condenses athigher T than ice, rockybodies form in the innerdisk, icy ones further out.• Since they are composedof the heavy elements andthere isn’t much matter inthem, the inner planets haverelatively small masses.Inside the frost line: Too hot for hydrogen compounds to form ices.Outside the frost line: Cold enough for ices to form. This meansthere is a larger reservoir of matter to make the outer planets.Why Two Types of Planets?Formation of the Terrestrial Planets• Inside the “frost line,” particles of rock and metalcollided and stuck together, building planetesimals.• Gravity drew the planetesimals together until theyassembled into the terrestrial planets.• The larger bodies “mopped up” the remaining smallplanetesimals and debrisTwo Current Theories:1. Core accretion: Solidcores form first, then theirgravity draws in gases2. Gravitational Instability:clumps of gas form within aprotoplanetary disk, they havestrong enough gravity tocollapse rapidlyFormation of the Jovian PlanetsAn Epoch of Epic Collisions There seems to have beenan era when the remainingplanetesimals bombardedthe newly formed objects,leaving impact craters andtilting the rotational axes ofseveral of the planetsSome Bombardment continues todayComet Shoemaker-Levy 9 collided with Jupiter in1994, after getting caught in Jupiter’s gravity andtorn apart by tidal forces into over a dozen piecesThe falling fragments left marks that were seen forseveral days; a similar event occurred in July 2009Comet Shoemaker-Levy at JupiterCould an Asteroid Hit the Earth?It’s happened in the past; some left craters we see today.Some events were drastic enough to wipe out a number ofspecies (mass extinctions). There are some “Earth-crossing”asteroids, or NEO’s (Near Earth Objects).Astronaut Edward Lu NASA-JSC proposed that we send a smallspace probe to hover next to this asteroid, providing a gravitationaltug strong enough to pull it into a different orbit and avoid acollision. This concept is called a “gravitational tractor.”Asteroid 99942 “Apophis”will pass close to the Earthin 2029, and was at onetime projected to have a 1in 5,000 chance of hittingthe Earth in 2036, but thishas now been revised to a1:45,000 chance.Could an Asteroid Hit the Earth?Formation of Earth’s
View Full Document
Unlocking...