Reasons Why Pluto Should Be a Planet

Pluto, discovered in 1930 by Clyde Tombaugh, held the designation of the ninth planet for over seven decades. This recognition was withdrawn in 2006 when the International Astronomical Union (IAU) adopted new criteria for defining a planet, resulting in Pluto’s reclassification as a dwarf planet. The decision ignited debate among the public and the scientific community. Many experts maintain that Pluto’s complex nature and unique physical attributes make its demotion scientifically unwarranted. Arguments for restoring Pluto’s planetary status center on its inherent characteristics, the inconsistencies of the current definition, and a proposed alternative based on geophysical principles.

Intrinsic Characteristics Supporting Planethood

The argument for Pluto’s planethood begins with its sophisticated physical features, which rival those of many acknowledged planets. Data from the New Horizons mission revealed a world far more complex than a mere inert ice ball. Pluto exhibits signs of geological activity, including vast plains of flowing nitrogen ice glaciers that fill the Sputnik Planitia basin.

The surface also features towering water-ice mountains and large, dome-shaped formations like Wright Mons and Piccard Mons, interpreted as possible cryovolcanoes. These structures suggest that Pluto maintains internal heat, potentially sustaining a subsurface liquid water ocean beneath its icy crust, a characteristic associated with larger, geologically active bodies.

Furthermore, Pluto possesses a dynamic, multilayered atmosphere composed primarily of nitrogen, methane, and carbon monoxide. Its pressure fluctuates dramatically as Pluto moves closer to and farther from the Sun during its 248-year orbit.

Pluto’s system of five moons, especially Charon, also points to a complexity found in planetary systems. Charon is nearly half of Pluto’s diameter, meaning the two bodies orbit a common center of mass located between them. These intrinsic physical traits demonstrate that Pluto is an evolved, planet-like world, not simply a primitive debris object found in the Kuiper Belt.

The Flaw in the Current Planetary Definition

The core of the controversy lies in the third criterion of the 2006 IAU definition, which requires a planet to have “cleared the neighborhood” around its orbit. This rule, which Pluto failed to meet because it orbits within the crowded Kuiper Belt, is considered fundamentally flawed and inconsistent. The definition incorrectly blends a body’s intrinsic physical characteristics with its extrinsic orbital location, creating a standard that is not universally applicable.

The term “cleared the neighborhood” is vaguely defined and impossible to satisfy absolutely, as all major planets share their orbital paths with various small objects. Earth, for example, co-orbits with approximately 10,000 near-Earth asteroids, while Jupiter shares its orbit with an estimated 100,000 Trojan asteroids. Proponents argue that these bodies persist because the planet’s gravity controls their orbits, which is a state of “dynamical dominance,” not perfect clearing.

The IAU’s criterion is also location-dependent, meaning a planet’s status is determined by where it is, not what it is. The mass required for an object to effectively “clear” its orbital zone increases exponentially with its distance from the Sun. If Earth were hypothetically placed in the distant Kuiper Belt at Pluto’s location, it would not have enough mass to clear that enormous region and would be classified as a dwarf planet.

This creates a situation where two identical objects could have different classifications based solely on their orbital distance. The definition essentially penalizes objects for forming far from the Sun, where the orbital neighborhood is vast and the material is spread thin. This reliance on an external, orbital mechanic criterion is what many experts find unscientific for classifying a celestial body.

Proposed Geophysical Definition

To circumvent the issues of the current location-based standard, many planetary scientists advocate for an attribute-based “geophysical definition.” This alternative focuses on a body’s physical nature, independent of its orbital path or surroundings. The proposed definition states that a planet is any sub-stellar mass body that has never undergone nuclear fusion and has sufficient mass to assume a spheroidal shape due to its own self-gravity.

This condition is known as achieving hydrostatic equilibrium, where internal pressure balances the inward pull of gravity to create a nearly round form. This internal property is considered a clear and testable physical threshold that distinguishes a planet from an irregularly shaped asteroid or comet. This geophysical standard is consistent with how other astronomical objects, such as stars, are classified—by their intrinsic properties, not their location.

Under this definition, Pluto easily qualifies for planethood because its self-gravity has molded it into a sphere. The geophysical definition would also include all other dwarf planets, such as Ceres and Eris, as well as large, rounded moons like Titan and Ganymede, potentially expanding the number of planets in the Solar System to over 100. Proponents suggest that this expansion is an accurate reflection of the diversity of complex, evolved worlds in the Solar System. By focusing on a body’s intrinsic physical traits, the geophysical definition offers a more intuitive and scientifically consistent framework that restores Pluto’s status.