Dwarf Planets Flashcards
Dwarf Planets
- The International Astronomical Union (IAU) redefined the criteria for classifying planets in 2006.
- Criteria for a celestial object to be considered a planet:
- Must orbit the Sun.
- Must possess sufficient mass for self-gravity to pull it into a spherical shape.
- Must have cleared its orbital zone of debris (like asteroids or comets).
- Pluto was reclassified as a dwarf planet because it met the first two criteria but not the third.
Dwarf Planets Overview
- Currently, five objects are classified as dwarf planets, with many more potentially existing in the outer reaches of the solar system.
Eris
- Discovered in 2005.
- Size and mass similar to Pluto.
- Orbits the Sun at a distance of 68 AU (over twice that of Neptune).
- Highly elliptical orbit with an eccentricity of 0.44.
- Axial tilt of 78°, indicating a likely past collision with a large impactor.
- Has a moon named Dysnomia, with a diameter of 50 km (30 mi).
- Surface is highly reflective due to methane ice, with an albedo higher than Saturn's Enceladus.
Pluto
- Orbit characteristics:
- Average radius: 39.5 AU.
- Eccentric orbit takes it inside Neptune's orbital path; eccentricity slightly greater than Mercury's (0.25 vs 0.21).
- Orbital inclination of 17° and a significant axial tilt of 113° (spins retrograde).
- Physical characteristics:
- Approximately 2/3 the size of the Moon, with 18% of the Moon's mass, making it less dense than the Moon.
- Average surface temperature: 40 K (-390 °F), much colder than Antarctica.
- Surface composition includes frozen H₂O, CO₂, N₂, CH₄, and CO.
- Thin atmosphere consists of sublimated N₂, CH₄, C₂H₆ (ethane), and CO.
- Icy mountains up to 3.5 km (2 mi) high, likely formed in the last 100 million years based on a lack of craters.
- Pluto features one of the youngest surfaces in the solar system, with an unexplained internal energy source, potentially linked to radioactive decay of long half-life nuclei.
Ceres
- Discovered on January 1, 1801, by Giuseppe Piazzi.
- First asteroid discovered and largest body in the asteroid belt.
- Size and Mass:
- Diameter of about 940 km, roughly 30% the size of the Moon.
- Contains about 25% of the asteroid mass in the belt, with a specific gravity of 2.2, between Mars (3.93) and Jupiter (1.33).
- Hypothesized to have a differentiated structure with a rocky core, icy mantle, and a surface rich in hydrated minerals (clays and carbonates).
- Detection of water vapor plumes suggests the possibility of subsurface oceans.
- Evidence of organic material found in a crater (Urnutet, 52 km in diameter) by NASA’s Dawn mission, linking to the basis of life and carbon chemistry.