Download Dwarf Planets - cloudfront.net

Dwarf Planets
And TNOs
The Problem of Pluto
Pluto was discovered in 1930. Named after the god of the dead.
Its position was predicted by perturbations in Neptune’s orbit
From the beginning it was unlike any other planet.
Its orbit is on a far different plane than the other planets, at a 17°
angle from them and…
is so elliptical (30 – 49 AU) that
it crosses Neptune’s
orbit.
Its size is very small, less than half Mercury’s radius
and its mass is even less at only .002 of Earth
Its Composition was at first thought to be a
terrestrial planet, though isolated beyond the Gas
Giants,
later its composition was discovered to be icy,
more like a comet than Earth.
Its moon, Charon is unusually large, at half Pluto’s
radius and orbits very close at 19,600 km.
All this made Pluto very unique until…
Eris, and a new type of planet
In 2005 another ‘planet’, called Eris after the Greek
goddess of discord, was discovered
It was very much like Pluto, a little larger
with similar composition, a tilted (44°) and elliptical (39
– 97 AU) orbit, and a large moon.
Recently more, (6+) other similar objects have been
found.
In August 2006 they and Pluto were called a new category
of celestial objects, “Dwarf Planets”
A Dwarf Planet:
• Orbits the Sun
• Has enough mass so that gravity makes them roughly
spherical
• But have not cleared their orbit of other objects
Ceres
One Dwarf planet does have a composition similar to
Earth…Ceres
It was once considered an asteroid it orbits in the asteroid
belt between Mars and Jupiter at 2.77 AU
It is between 909 & 975km in diameter.
Trans-Neptune Objects (TNO’s)
and other dwarf planets
Pluto, Eris, Sedna and Orcus are all icy dwarf planets
that cross Neptune’s orbit or come close to it
At their greatest distance they pass into the Kuiper
belt where comets orbit,
They are known as ”TNO’s”
About 10 such objects are known.
There are probably many more dwarf planets orbiting
far beyond Neptune.
Plutoids
Plutoids are icy dwarf planets similar to Pluto.
They orbit in the Kuiper Belt and in composition
resemble comets.
(Although exactly what gas the ice is varies)
They Include: Pluto
Eris
Makemake
and Haumea
Some such as Sedna, Quaoar, Orcus and Varuna
await a further observation before
determination
Pluto’s Transient
Atmosphere
Nitrogen is especially common on Pluto
It has an atmosphere of mostly nitrogen that
only exists when its closer to the Sun.
It freezes when Pluto reaches aphelion and
vaporizes again as it approaches
perihelion
Pluto and Charon are
a “binary planet”
because:
1. Charon has a
radius (635km)
more than half
that of Pluto.
2. They orbit each
other and
are tidally locked
so that both
always face the
same side to each
other
Two true moons Nix and
Hydra orbit the pair.
Eris
Eris, with a radius of 1200 km, is the largest of
the Plutoids.
It takes over 500 years to complete its 68 AU
average orbit.
It has one small Moon: Dysonomia
Makemake And Haumea
At a radius of 950 km Makemake is the third largest
plutoid.
Debate raged over the status of Haumea
Its elongated shape is the
result of it fast spin.
At a period of 4 hours,
the fastest known
So now it qualifies
It has two small moons,
Hi’iaka and Namaka