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Confessions of a Pluto Hater Confessions of a Pluto Hater Megan K. Pickett Megan K. Pickett Associate Professor of Physics Associate Professor of Physics Lawrence University Lawrence University QuickTime GIF decom are needed 14 November 2006 14 November 2006

Confessions of a Pluto Hater

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Confessions of a Pluto Hater. Megan K. Pickett Associate Professor of Physics Lawrence University. 14 November 2006. Friends, Students, Scientists, lend me your ears; I come to bury Pluto, not to praise it. The evil this rock does lives in our books, - PowerPoint PPT Presentation

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Page 1: Confessions of a Pluto Hater

Confessions of a Pluto HaterConfessions of a Pluto Hater

Megan K. PickettMegan K. PickettAssociate Professor of PhysicsAssociate Professor of PhysicsLawrence UniversityLawrence University

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14 November 200614 November 2006

Page 2: Confessions of a Pluto Hater

Friends, Students, Scientists, lend me your ears;I come to bury Pluto, not to praise it.The evil this rock does lives in our books, The small good was interred with Clyde's bones;So let it be with Pluto...The noble NewtonHath told you Pluto was Perturber:If it were so, it was a grievous fault,And grievously hath Pluto not answer'd it...Here, under leave of Lowell and the rest-(For Lowell was a crazy nearsighted man;who saw lines on Mars and shouted "water, ho!")-Come I to speak on Pluto, Dwarf Planet...

Page 3: Confessions of a Pluto Hater

Formerly the Ninth Planet of the Solar SystemFormerly the Ninth Planet of the Solar System

uto

Average Orbital Distance: 40 AU

Orbital Period: 248 years

Orbital Inclination: 17o

Orbital Eccentricity: 25%

Rotation Period: -6.4days

Radius: 0.6 RM

Mass: 0.3MM

Average Density: 2100 kgm-3

Surface Temperature: 33 - 55 K

Atmosphere: CH4 and N2

Surface: CH4 ice (?)

Interior (?): Silicates &

ices

Page 4: Confessions of a Pluto Hater

Formerly the Ninth Planet of the Solar SystemFormerly the Ninth Planet of the Solar System

uto

Average Orbital Distance: 40 AU

Orbital Period: 248 years

Orbital Inclination: 17o

Orbital Eccentricity: 25%

Rotation Period: -6.4days

Radius: 0.6 RM

Mass: 0.3MM

Average Density: 2100 kgm-3

Surface Temperature: 33 - 55 K

Atmosphere: CH4 and N2

Surface: CH4 ice (?)

Interior (?): Silicates &

ices

Page 5: Confessions of a Pluto Hater

Formerly the Ninth Planet of the Solar SystemFormerly the Ninth Planet of the Solar System

uto

Average Orbital Distance: 40 AU

Orbital Period: 248 years

Orbital Inclination: 17o

Orbital Eccentricity: 25%

Rotation Period: -6.4days

Radius: 0.6 RM

Mass: 0.3MM

Average Density: 2100 kgm-3

Surface Temperature: 33 - 55 K

Atmosphere: CH4 and N2

Surface: CH4 ice (?)

Interior (?): Silicates &

ices

Page 6: Confessions of a Pluto Hater

Formerly the Ninth Planet of the Solar SystemFormerly the Ninth Planet of the Solar System

uto

Average Orbital Distance: 40 AU

Orbital Period: 248 years

Orbital Inclination: 17o

Orbital Eccentricity: 25%

Rotation Period: -6.4days

Radius: 0.6 RM

Mass: 0.3MM

Average Density: 2100 kgm-3

Surface Temperature: 33 - 55 K

Atmosphere: CH4 and N2

Surface: CH4 ice (?)

Interior (?): Silicates &

ices

Page 7: Confessions of a Pluto Hater

Formerly the Ninth Planet of the Solar SystemFormerly the Ninth Planet of the Solar System

uto

Average Orbital Distance: 40 AU

Orbital Period: 248 years

Orbital Inclination: 17o

Orbital Eccentricity: 25%

Rotation Period: -6.4days

Radius: 0.6 RM

Mass: 0.3MM

Average Density: 2100 kgm-3

Surface Temperature: 33 - 55 K

Atmosphere: CH4 and N2

Surface: CH4 ice (?)

Interior (?): Silicates &

ices

Page 8: Confessions of a Pluto Hater

Formerly the Ninth Planet of the Solar SystemFormerly the Ninth Planet of the Solar System

uto

Average Orbital Distance: 40 AU

Orbital Period: 248 years

Orbital Inclination: 17o

Orbital Eccentricity: 25%

Rotation Period: -6.4days

Radius: 0.6 RM

Mass: 0.3MM

Average Density: 2100 kgm-3

Surface Temperature: 33 - 55 K

Atmosphere: CH4 and N2

Surface: CH4 ice (?)

Interior (?): Silicates &

ices

Page 9: Confessions of a Pluto Hater

The Pluto Formerly Known as PlanetThe Pluto Formerly Known as PlanetAverage Orbital Distance: 40 AU

Orbital Period: 248 years

Orbital Inclination: 17o

Orbital Eccentricity: 25%

Rotation Period: -6.4days

Radius: 0.6 RM

Mass: 0.3MM

Average Density: 2100 kgm-3

Surface Temperature: 33 - 55 K

Atmosphere: CH4 and N2

Surface: CH4 ice (?)

Interior (?): Silicates &

ices

Page 10: Confessions of a Pluto Hater

History of DiscoveryHistory of DiscoveryClassical Planets: Mercury, Venus, Mars, Jupiter & Saturn

Uranus: (1781) Herschel

Neptune: (1864) Adams & Leverrier

Ceres: (1801) Piazzi

(asteroid and now

Dwarf Planet)

Page 11: Confessions of a Pluto Hater

History of DiscoveryHistory of Discovery

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Clyde Tombaugh

Pluto: 1930

Page 12: Confessions of a Pluto Hater

I.A.U. Circulaire No. 255

BUREAU CENTRAL ASTRONOMIQUEDE L'UNION ASTRONOMIQUE INTERNATIONALEOBSERVATOIRE DE COPENHAGUE

TRANSNEPTUNIAN PLANET?

Lowell observatory telegraphs systematic search begun years ago supplementing Lowells investigations for Transneptunian planet has revealed object which for seven weeks has in rate of motion and path consistently conformed to transneptunian body at approximate distance he assigned fifteenth magnitude position march twelve three hours G.M.T. was seven seconds of time west from delta geminorum agreeing with Lowells predicted longitude.

Page 13: Confessions of a Pluto Hater

History of DiscoveryHistory of Discovery

Nix & Hydra: (2005)Pluto Companion Search Team

Charon: (1978) Christy

Page 14: Confessions of a Pluto Hater

History of DiscoveryHistory of Discovery

1990’s: Here come the Kuiper Belt Objects!

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1992: 1992 QB1

David Jewitt &Jane Luu.

Currently ~1000 KBO’sknown.

Page 15: Confessions of a Pluto Hater

History of DiscoveryHistory of Discovery

Late 1990’s to Present: A TransNeptunian Zoo.

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Page 16: Confessions of a Pluto Hater

History of DiscoveryHistory of Discovery

And then there was Eris (& Dysnomia): “Scatter Disk Object”

2005 Brown, Trujillo & Rabinowitz

Page 17: Confessions of a Pluto Hater

A Brief History of the Solar SystemA Brief History of the Solar System

1. Collapse of cold pre-stellar cloud (~5GYA)a) Initial cloud contains mass and angular momentum of

Solar systemb) Why does it collapse?

• Marginally unstable to collapse?• Triggered collapse?

100 AU0.1 pc 105 yrs

Page 18: Confessions of a Pluto Hater

A Brief History of the Solar SystemA Brief History of the Solar System

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Well, what next?

Page 19: Confessions of a Pluto Hater

A Brief History of the Solar SystemA Brief History of the Solar System

2. The Solar Nebula (Kant 1775, Laplace 1796)

a) Close to the Protosun(inside the “frostline”), volatiles are vaporized, andonly refractory elements areavailable for planet buildingby accumulation and then accretion.

~8 AU

Inner planets are rocky

Page 20: Confessions of a Pluto Hater

A Brief History of the Solar SystemA Brief History of the Solar System

2. The Solar Nebula (Kant 1775, Laplace 1796)

b) Far from the Proto-Sun, Ices are also available forBuilding planetary cores.

~80 AU

Outer Solar System is(or should be) very differentfrom inner Solar System.

Page 21: Confessions of a Pluto Hater

A Brief History of the Solar SystemA Brief History of the Solar System

3. Planet Formation

a) Terrestrial Planets: relatively straightforward.b) Gas & Ice Giant Planets: Phasers at Dawn.

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“Core Accretion”

Takes Too Long

“Spiral Instability”

Doesn’t Work

vs.

Page 22: Confessions of a Pluto Hater

A Brief History of the Solar SystemA Brief History of the Solar System

4. Planet Billiardsa) Jupiter, Saturn, Uranus & Neptune migrate after

formation (e.g., the “Nice Model” 2004)

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•Initially J,S close; Neptune inside Uranus orbit; KBO 20-30 AU•J,S migrate in and out, respectively=> fling out Neptune, KBO’s•Neptune clears primordial KB, captures Triton, perturbs PLUTO

Page 23: Confessions of a Pluto Hater

A Brief History of the Solar SystemA Brief History of the Solar System

4. Planet Billiardsb) Bombardment

•Forms Earth & Moon•May form Martian satellites•May form Pluto-Charon

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A Brief History of the Solar SystemA Brief History of the Solar System

4. Planet Billiardsc) Populate Scattered Disk, Oort Cloud.d) Delivers volatiles to inner solar system.

5. Solar Ignitiona) Hydrogen Fusion (p-p chain) begins in core of Sun

So where does this leave Poor Old Misbegotten Pluto?So where does this leave Poor Old Misbegotten Pluto?

Page 25: Confessions of a Pluto Hater

Pluto is Not a PlanetPluto is Not a Planet

1. On August 24 2006, members of the IAU finally came to their collected senses and voted Pluto out of the Ritzy Planet Club. Was this mean? Logical? Or both?

What’s the caseagainst Pluto?

Page 26: Confessions of a Pluto Hater

Real Planets don’t look like tiny plates of quicheReal Planets don’t look like tiny plates of quiche

Page 27: Confessions of a Pluto Hater

Real Planets don’t look like tiny plates of quicheReal Planets don’t look like tiny plates of quiche

a) Pluto is Bloody Tiny.a) Pluto is Bloody Tiny.

Page 28: Confessions of a Pluto Hater

Real Planets don’t look like tiny plates of quicheReal Planets don’t look like tiny plates of quiche

b) Pluto’s orbit is unlike any of the other planets.b) Pluto’s orbit is unlike any of the other planets.

Page 29: Confessions of a Pluto Hater

Real Planets don’t look like tiny plates of quicheReal Planets don’t look like tiny plates of quiche

c) There are a lot of tiny icy bodies out there, too.c) There are a lot of tiny icy bodies out there, too.

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Page 30: Confessions of a Pluto Hater

Real Planets don’t look like tiny plates of quicheReal Planets don’t look like tiny plates of quiche

d) Pluto is a binary objectd) Pluto is a binary object

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What to do about Pluto, then?What to do about Pluto, then?

Page 31: Confessions of a Pluto Hater

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Fortunately, we already have an object parked in SaturnOrbit that seems right for the job.

Page 32: Confessions of a Pluto Hater

Real Planets don’t look like tiny plates of quicheReal Planets don’t look like tiny plates of quiche

2.2. Thus Sayeth the IAU:Thus Sayeth the IAU:

A Planet is an object that 1. orbits the Sun (so far so good);A Planet is an object that 1. orbits the Sun (so far so good);2. is massive enough to pull itself into a sphere (again, 2. is massive enough to pull itself into a sphere (again, good enough); and 3. has cleared the region of objects, i.e.,good enough); and 3. has cleared the region of objects, i.e.,is in some sense locally gravitationally independent. is in some sense locally gravitationally independent.

And so, mercifully, Pluto, along with Eris andAnd so, mercifully, Pluto, along with Eris andCeres and probably many, many more areCeres and probably many, many more are‘‘Dwarf Planets’.Dwarf Planets’.

D’Oh!

Page 33: Confessions of a Pluto Hater

“Now cracks an icy sheath. Good night, odd ball,And flights of comets sing thee to Kuiper!"

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