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: 1153extkm1153 ext{ km}

    • Triton's radius: 1353extkm1353 ext{ km}

  • Density:

    • Pluto: ext 2.0g/cm3ext{~2.0 g/cm}^3

    • Triton: 2.06extg/cm32.06 ext{ g/cm}^3

  • 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, extCO<em>2ext{CO}<em>2 ice, extCOext{CO} ice, and extN</em>2ext{N}</em>2 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 23002400extkm2300 - 2400 ext{ km}.

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