Lecture 30: Pluto and the Kuiper belt
Overview of Pluto and the Kuiper Belt
Pluto is classified as a Kuiper Belt object (KBO).
The Kuiper Belt contains many small celestial bodies beyond Neptune, mostly seen as faint specks of light.
Discovery of Pluto
Neptune's mass was originally thought too small to account for Uranus' orbit deviations.
In 1906, Percival Lowell initiated the search for a theoretical "Planet X".
Clyde Tombaugh discovered Pluto in 1930 by comparing thousands of photographic plates for movement.
The search for Pluto was based on false assumptions.
Characteristics of Pluto
Size:
Pluto's radius:
Triton's radius:
Density:
Pluto:
Triton:
Composition:
Similarities to Triton, thought to be captured from Kuiper Belt.
Measurement of Pluto's Mass
The mass of Pluto was first measured after the discovery of its moon, Charon, in 1978.
Knowing the mass of a celestial body is crucial for understanding its structure and evolution.
By 2005, Hubble discovered two additional moons: Nix and Hydra.
Research Limitations and New Insights
Prior to the New Horizons mission, limited information about Pluto's surface was available.
Observations showed that Pluto's surface varies in brightness and color, suggesting distinct terrains.
Pluto's reddish color likely results from organic molecules formed from UV exposure to methane and ammonia ice.
Internal Structure of Pluto
Notable composition: approximately 50-70% rocky and 30-50% icy materials.
Ice types present: water ice, ice, ice, and ice.
Layers of Pluto:
Layer 1: Frozen nitrogen
Layer 2: Water ice
Layer 3: Rock and iron
Heat Generation within Pluto
Radioactive decay of elements like potassium, uranium, and thorium generates internal heat.
Heat may cause melting in a potential subsurface ocean beneath Pluto's icy mantle.
Interpreting Geological Features
Predictions based on the presence or absence of a subsurface ocean:
If no ocean exists:
Should have an equatorial bulge and extensile features on the surface.
If an ocean exists:
No bulge and compressional features evident (e.g., wrinkle ridges).
New Horizons Mission
Launched in 2006 and flew past Pluto in 2015, providing significant new data.
The spacecraft's journey to Pluto involves a nearly 4.5-hour light travel time for communication.
New Horizons has redefined our understanding of Pluto and its environment.
Pluto's Atmosphere
Analysis of atmospheric thickness through sunlight refraction was conducted during the New Horizons flyby.
Pluto's atmosphere primarily consists of nitrogen and is more complex than initially expected.
Sputnik Planum
A large area of Pluto's surface showing vast nitrogen ice with interesting geological structures.
Observations suggest soft ice behavior with convective down welling.
Geology of Charon
Charon exhibits canyons resembling grabens, indicating historical crustal stresses.
Surface features suggest that if Charon had liquid water, Pluto possibly did too.
Shape Implications
Pluto's nearly spherical shape (like a basketball) suggests a potential subsurface ocean versus an onion-like layered structure.
The absence of a historical tidal bulge suggests that Pluto may be soft or liquid internally, allowing it to reform into a sphere.
Resolution of Pluto's Status
The discovery of numerous similarly sized KBOs led to Pluto's demotion from "planet" to "dwarf planet" status.
Eris, a significant KBO, has a diameter of approximately .
Gravitational Influences in the Kuiper Belt
Predictions of further celestial bodies ("Planet Nine") influencing KBO orbits have emerged as scientists explore unexplained orbital patterns.
An undiscovered planet could have a mass exceeding ten times that of Earth, influencing these distant objects.
Upcoming Topics
Future discussions will focus on extrasolar planets and related phenomena.
Additional reading: http://en.wikipedia.org/wiki/Extrasolar_planet