Transcript Document

Confessions of a Pluto Hater
Megan K. Pickett
Associate Professor of Physics
Lawrence University
QuickTime™ and a
GI Fdec ompress or
are needed t o see this pict ure.
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,
The small good was interred with Clyde's bones;
So let it be with Pluto...The noble Newton
Hath 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...
Formerly the Ninth Planet of the Solar System
uto
Average Orbital Distance:
Orbital Period:
Orbital Inclination:
Orbital Eccentricity:
Rotation Period:
40 AU
248 years
17o
25%
-6.4days
Radius:
Mass:
Average Density:
Surface Temperature:
Atmosphere:
Surface:
Interior (?):
0.6 RM
0.3MM
2100 kgm-3
33 - 55 K
CH4 and N2
CH4 ice (?)
Silicates &
ices
Formerly the Ninth Planet of the Solar System
uto
Average Orbital Distance:
Orbital Period:
Orbital Inclination:
Orbital Eccentricity:
Rotation Period:
40 AU
248 years
17o
25%
-6.4days
Radius:
Mass:
Average Density:
Surface Temperature:
Atmosphere:
Surface:
Interior (?):
0.6 RM
0.3MM
2100 kgm-3
33 - 55 K
CH4 and N2
CH4 ice (?)
Silicates &
ices
Formerly the Ninth Planet of the Solar System
uto
Average Orbital Distance:
Orbital Period:
Orbital Inclination:
Orbital Eccentricity:
Rotation Period:
40 AU
248 years
17o
25%
-6.4days
Radius:
Mass:
Average Density:
Surface Temperature:
Atmosphere:
Surface:
Interior (?):
0.6 RM
0.3MM
2100 kgm-3
33 - 55 K
CH4 and N2
CH4 ice (?)
Silicates &
ices
Formerly the Ninth Planet of the Solar System
uto
Average Orbital Distance:
Orbital Period:
Orbital Inclination:
Orbital Eccentricity:
Rotation Period:
40 AU
248 years
17o
25%
-6.4days
Radius:
Mass:
Average Density:
Surface Temperature:
Atmosphere:
Surface:
Interior (?):
0.6 RM
0.3MM
2100 kgm-3
33 - 55 K
CH4 and N2
CH4 ice (?)
Silicates &
ices
Formerly the Ninth Planet of the Solar System
uto
Average Orbital Distance:
Orbital Period:
Orbital Inclination:
Orbital Eccentricity:
Rotation Period:
40 AU
248 years
17o
25%
-6.4days
Radius:
Mass:
Average Density:
Surface Temperature:
Atmosphere:
Surface:
Interior (?):
0.6 RM
0.3MM
2100 kgm-3
33 - 55 K
CH4 and N2
CH4 ice (?)
Silicates &
ices
Formerly the Ninth Planet of the Solar System
uto
Average Orbital Distance:
Orbital Period:
Orbital Inclination:
Orbital Eccentricity:
Rotation Period:
40 AU
248 years
17o
25%
-6.4days
Radius:
Mass:
Average Density:
Surface Temperature:
Atmosphere:
Surface:
Interior (?):
0.6 RM
0.3MM
2100 kgm-3
33 - 55 K
CH4 and N2
CH4 ice (?)
Silicates &
ices
The Pluto Formerly Known as Planet
Average Orbital Distance:
Orbital Period:
Orbital Inclination:
Orbital Eccentricity:
Rotation Period:
40 AU
248 years
17o
25%
-6.4days
Radius:
Mass:
Average Density:
Surface Temperature:
Atmosphere:
Surface:
Interior (?):
0.6 RM
0.3MM
2100 kgm-3
33 - 55 K
CH4 and N2
CH4 ice (?)
Silicates &
ices
History of Discovery
Classical Planets: Mercury, Venus, Mars, Jupiter & Saturn
Uranus: (1781) Herschel
Neptune: (1864) Adams & Leverrier
Ceres: (1801) Piazzi
(asteroid and now
Dwarf Planet)
History of Discovery
Pluto: 1930
Clyde Tombaugh
QuickTime™ and a
TIFF (Uncompressed) decompressor
are needed to see this picture.
Percival Lowell
I.A.U. Circulaire No. 255
BUREAU CENTRAL ASTRONOMIQUE
DE L'UNION ASTRONOMIQUE INTERNATIONALE
OBSERVATOIRE 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.
History of Discovery
Charon: (1978) Christy
Nix & Hydra: (2005)
Pluto Companion Search Team
History of Discovery
1990’s: Here come the Kuiper Belt Objects!
1992: 1992 QB1
David Jewitt &
Jane Luu.
Currently
~1000 KBO’s
known.
QuickTime™ and a
TIFF (Uncompressed) decompressor
are needed to see this picture.
History of Discovery
Late 1990’s to Present: A TransNeptunian Zoo.
QuickTime™ and a
TIFF (Uncompressed) decompressor
are needed to see this picture.
QuickTime™ and a
TIFF (Uncompressed) decompressor
are needed to see this picture.
History of Discovery
And then there was Eris (& Dysnomia): “Scatter Disk Object”
2005 Brown, Trujillo &
Rabinowitz
A Brief History of the Solar System
1. Collapse of cold pre-stellar cloud (~5GYA)
a) Initial cloud contains mass and angular momentum of
Solar system
b) Why does it collapse?
• Marginally unstable to collapse?
• Triggered collapse?
100 AU
0.1 pc
105 yrs
A Brief History of the Solar System
QuickTime™ and a
Sorenson Video decompressor
are needed to see this picture.
Well, what next?
A 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, and
only refractory elements are
available for planet building
by accumulation and then
accretion.
 Inner planets are rocky
~8 AU
A Brief History of the Solar System
2. The Solar Nebula (Kant 1775, Laplace 1796)
b) Far from the Proto-Sun,
Ices are also available for
Building planetary cores.
 Outer Solar System is
(or should be) very different
from inner Solar System.
~80 AU
A Brief History of the Solar System
3. Planet Formation
a) Terrestrial Planets: relatively straightforward.
b) Gas & Ice Giant Planets: Phasers at Dawn.
“Core Accretion”
QuickTime™ and a
Sorenson Video decompressor
are needed to see this picture.
Takes Too Long
“Spiral Instability”
vs.
QuickTime™ and a
YUV420 codec decompressor
are needed to see this picture.
Doesn’t Work
A Brief History of the Solar System
4. Planet Billiards
a) Jupiter, Saturn, Uranus & Neptune migrate after
formation (e.g., the “Nice Model” 2004)
QuickTime™ and a
TIFF (Uncompressed) decompressor
are needed to see this picture.
•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
A Brief History of the Solar System
4. Planet Billiards
b) Bombardment
•Forms Earth & Moon
•May form Martian satellites
•May form Pluto-Charon
QuickTime™ and a
Cinepak decompressor
are needed to see this picture.
A Brief History of the Solar System
4. Planet Billiards
c) Populate Scattered Disk, Oort Cloud.
d) Delivers volatiles to inner solar system.
5. Solar Ignition
a) Hydrogen Fusion (p-p chain) begins in core of Sun
So where does this leave Poor Old Misbegotten Pluto?
Pluto 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 case
against Pluto?
Real Planets don’t look like tiny plates of quiche
Real Planets don’t look like tiny plates of quiche
a) Pluto is Bloody Tiny.
Real Planets don’t look like tiny plates of quiche
b) Pluto’s orbit is unlike any of the other planets.
QuickTime™ and a
Video decompressor
are needed to see this picture.
Real Planets don’t look like tiny plates of quiche
c) There are a lot of tiny icy bodies out there, too.
QuickTime™ and a
TIFF (Uncompressed) decompressor
are needed to see this picture.
Real Planets don’t look like tiny plates of quiche
d) Pluto is a binary object
QuickTime™ and a
Cinepak decompressor
are needed to see this picture.
What to do about Pluto, then?
Fortunately, we already have an object parked in Saturn
Orbit that seems right for the job.
QuickTime™ and a
QuickTime™ and a
TIFF (Uncompressed)
decompressor
TIFF (Uncompressed) decompressor
are
needed
to
see
this
picture.
are needed to see this
picture.
Real Planets don’t look like tiny plates of quiche
2. Thus Sayeth the IAU:
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,
good enough); and 3. has cleared the region of objects, i.e.,
is in some sense locally gravitationally independent. D’Oh!
And so, mercifully, Pluto, along with Eris and
Ceres and probably many, many more are
‘Dwarf Planets’.
“Now cracks an icy sheath. Good night, odd ball,
And flights of comets sing thee to Kuiper!"
Qui ckTi me™ and a
TIFF (Uncompressed) decompr essor
are needed to see this picture.