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- The International Astronomical Union’s definition of a planet created an uproar in 2006, when Pluto was demoted from full planet status.
- In recent decades, scientists have discovered more than 5,000 exoplanets, or worlds orbiting distant stars. Meanwhile, the IAU definition applies only to planets within our solar system.
- The newly proposed planet definition includes exoplanets. It specifies that “planets” may orbit one or more stars, brown dwarfs or stellar remnants. It sets mass limits that its originators say should apply to planets everywhere. But it does not return Pluto to full planet status.
UCLA released this statement originally on July 11, 2024.
Current definition is ‘sun-centric’
Planetary scientists are proposing a new definition of a planet to replace one that many researchers view as sun-centric and outdated. The current definition — established in 2006 by the International Astronomical Union, or IAU, the organization that officially names objects in space — specifies that to qualify as a planet, a celestial body must orbit the sun within our solar system.
But scientists know that celestial bodies orbiting stars outside our solar system are fairly common, and a forthcoming article in the Planetary Science Journal argues for a new definition of a planet that includes being unrestrained by the bounds of our solar system. The proposal also provides quantitative criteria to further clarify the definition of a planet.
Jean-Luc Margot, lead author of the article and UCLA professor of earth, planetary and space sciences and of physics and astronomy, will present the proposed new definition at the IAU General Assembly in August 2024.
Proposed change adds exoplanets and mass limits
Under the current definition, a planet is a celestial body that orbits the sun, is massive enough that gravity has forced it into a spherical shape, and has cleared away other objects near its orbit around the sun. Margot explained why this isn’t adequate:
The current definition specifically mentions orbiting our sun. We now know about the existence of thousands of planets, but the IAU definition applies only to the ones in our solar system. We propose a new definition that can be applied to celestial bodies that orbit any star, stellar remnant or brown dwarf.
The authors argue that while the requirement to orbit our sun is too specific, other criteria in the IAU definition are too vague. For example, it says a planet has “cleared its orbit” without stating what that means. The proposed new definition contains quantifiable criteria that can be applied for defining planets inside and outside our solar system.
In the new definition, a planet is a celestial body that:
- orbits one or more stars, brown dwarfs or stellar remnants and;
- is more massive than 2,255 pounds (1,023 kg) and;
- is less massive than 13 Jupiter masses (5.5*10^28 pounds or 2.5*10^28 kg).
High school student had hand in redefining planets
Margot and co-authors Brett Gladman of the University of British Columbia and Tony Yang, a student at Chaparral High School in Temecula, California, ran a mathematical algorithm on the properties of objects in our solar system to see which objects clustered together. The analysis revealed groups of distinct qualities shared by planets in our solar system that can be used as a starting point for creating a taxonomy for planets in general.
For example, if an object has enough gravity to clear a path by accumulating or ejecting smaller objects nearby, it is said to be dynamically dominant. Margot explained why this matters:
All the planets in our solar system are dynamically dominant, but other objects — including dwarf planets like Pluto, and asteroids — are not. So this property can be included in the definition of planet.
The requirement for dynamical dominance provides a lower limit on mass. But potential planets can also be too big to fit the new definition. Some gas giants, for example, are so large that thermonuclear fusion of deuterium occurs, and the object becomes a substar called a brown dwarf and therefore not a planet. This limit has been determined to be the mass of 13 or more Jupiters.
Do planets have to be round?
The current requirement to be spherical, on the other hand, is more problematic. Distant planets can rarely be observed in enough detail to ascertain their shape with certainty. The authors argue that the shape requirement is so difficult to implement that it is effectively useless for definitional purposes, even though planets are generally round. Gladman explained how this helps:
Having definitions anchored to the most easily measurable quantity — mass — removes arguments about whether or not a specific object meets the criterion. This is a weakness of the current definition.
The good news is that, in the solar system, celestial bodies larger than 2,250 pounds (1,021 kg) appear to be round. So all bodies that satisfy the proposed lower limit on mass of 2,255 pounds (1,023 kg) are expected to be spherical.
While any official change to the IAU definition of planet is likely a few years away, Margot and his colleagues hope their work starts a conversation that results in an improved definition.
Bottom line: Astronomers will vote on a new definition of a planet in August 2024. The update would include exoplanets and set mass limits.
Via UCLA
Read more: Scientist proposes yet another new definition of a planet
Read more: Exoplanets are worlds orbiting other stars