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Not Your Parents’ Solar System! Dr. Frank Summers Space Telescope Science Institute March 28, 2008 Your Ancient Ancestors’ Solar System Claudius Ptolemy 150 – Almagest Earth Moon Mercury Venus Sun Mars Jupiter Saturn Your Parents’ Solar System Nicholas Copernicus 1543 – On the Revolutions of Heavenly Spheres Earth Moon Mercury Venus Sun Mars Jupiter Saturn Sun Mercury Venus Earth / Moon Mars Jupiter Saturn William Herschel 1781 – Discovery of Uranus Urbain Le Verrier & John Couch Adams 1846 – Prediction and discovery of Neptune Clyde Tombaugh 1930 – Discovery of Pluto Your Parents’ Solar System Your Parents’ Solar System Mercury My Venus Very Earth Energetic Mars Mother Jupiter Just Saturn Served Uranus Us Neptune Nine Pluto Pizzas Your Parents’ Solar System Facts Are Not Knowledge • • • • • Memorization, not understanding Factoids Highlights differences Little or no relevance Little or no “big picture” The 21st Century Solar System Sun Rocky Planets Asteroid Belt Giant Planets Kuiper Belt Oort Cloud Families of the Solar System • Classes of similar objects – Size – Composition – Orbit size – Orbit shape – Orbit inclination – Moons – Rings Hollywood’s View of the Asteroid Belt Hundreds of thousands of asteroids … … about a million miles apart! 960 million miles Scientific View of the Asteroid Belt Sizes of the Giant Planets and Earth Kuiper Belt Oort Cloud • Billions of icy minor planets – comet nuclei • Roughly spherical out to 50,000 AU • Predicted by Jan Oort • Explains long-period comets Figure 1a: Comet Semimajor Axis Distribution 600 Orbital Period: 7 years 200 years 400 Long Period Short Period 300 200 100 1 / a (1/AU) 0.390 0.185 0.088 0.042 0.020 0.009 0.004 0.002 0.000 -0.002 0 -0.004 Number of Comets 500 Sedna Sedna • Orbit 76 – 840 AU • Very red color • Outer Kuiper Belt? • Inner Oort Cloud? • Planet at 70 AU? Families of the Solar System • Classification • Structure of the solar system – Similar objects lie in similar regions • Clues to solar system formation and evolution Rocky Planets Giant Planets Sun Rocky Planets Asteroid Belt Giant Planets Kuiper Belt Oort Cloud Sun Mercury Venus Earth Mars Asteroid Belt Jupiter Saturn Uranus Neptune Kuiper Belt Oort Cloud Science May View Established Models As Basic Justified Standards Until New Knowledge Bears Out Changes Sometimes My Very Energetic Mother Also Boils Jumbo Shrimp Using Nine Kettles Bubbling Over Coals The Inevitable Question … Why is Pluto No Longer a Planet? Planet Pluto January 23, 1930 January 29, 1930 The Incredible Shrinking Planet • • • • Lowell’s Planet X – 7 times Earth 1940’s – 1 times Earth 1980 – 0.1 times Earth 1985 – 0.002 times Earth Double Take: Charon • 1978 – James Christy (USNO) observations to refine Pluto’s orbit • Notices elongated images, deduces moon • 1985 – Charon occults Pluto, confirms existence • Refined sizes and masses – tiny Pluto/Charon Mimas Mercury Iapetus Miranda Proteus Tethys Dione Umbriel Europa Moon Pallas Ariel Io Hygeia Triton Titan Ganymede Vesta Oberon Callisto Ceres Rhea Titania Enceladus Pluto Charon Kuiper Belt • 1930 – Leonard mentions possibility of transPlutonian objects • 1943 – Kenneth Edgeworth postulates objects beyond Pluto • 1951 – Gerard Kuiper predicts that a massive Pluto would disperse small objects into a belt • 1980 – Fernandez predicts ‘comet belt’ that resembles what was eventually found Kuiper Belt Objects • 1992 – Jewitt & Luu find QB1 • Distance of 42 AU • First (third?) object discovered in the Kuiper Belt Kuiper Belt More and more KBOs • • • • Large searches for KBOs ensued Hundreds discovered within a decade Over 1200 discovered so far Over 70,000 predicted – diameters > 100 km – orbits 30-50 AU Pluto Defenders • Pluto is different from the KBOs • Pluto is bigger than the KBOs • Pluto has a moon, Charon Pluto/Charon orbits within Kuiper Belt KBO Size Comparison Binary KBOs • About 10% of KBOs are binaries Eris & Dysnomia (2003 UB313) Easterbunny Santa & Rudolph Eris & Dysnomia Pluto vs the Kuiper Belt • • • • Orbit similar to KBOs Size similar to KBOs KBO companions common Composition similar to KBOs Pluto vs the Kuiper Belt • • • • Orbit similar to KBOs Size similar to KBOs KBO companions common Composition similar to KBOs Pluto has found its family!! IAU Definition – August 2006 • IAU defines “planet” 1. Orbits the Sun 2. Upper mass limit • • not massive enough to produce fusion Deuterium fusion occurs at about 15x Jupiter’s mass 3. Lower mass limit • • Massive enough for gravity to make it spherical About 500 miles in diameter 4. Dominates its orbit • Dwarf planets meet 1, 2, 3, but not 4 Other Planetary Systems? • Solar system alone is category of one Beta Pictoris We Are Not Alone • • • • Lots of dust disks found Proplyds – proto-planetary disks Kuiper Belt sized and larger Some substructure seen Planets around Other Stars • Cannot see directly (yet) • Detect via gravitational pull on star – Wobble – Periodic shift of spectral lines – Monitor for many years (several orbits) – Giant planets detectable Planets around Other Stars • Current count (May 2006) – 162 planetary systems – 188 planets – 19 multiple planet systems • At least 15% of sun-like stars have planets Planets around Other Stars • • • • • Jupiter mass planets in Mercury orbits Elliptical orbits Multiple Jupiter sized planets Planets around pulsars Smallest (so far) is about 5 Earth masses Planetary System Formation • Planetary systems form in a predictable fashion from a spinning circular disk Sun Rocky Planets Asteroid Belt Giant Planets Kuiper Belt Oort Cloud So Much to Discover • Our solar system is the oddball • Need to generalize our formation and evolution scenarios • Implications for life in the universe – Lots of planets – Stability of orbits? • New era of solar system study