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| | The discovery of [[Eris]], a scatter-disk body 27% more massive than Pluto, caused a controversy concerning what does, and what does not, constitute a [[planet]]. If Pluto were to retain its historical designation of "planet," then Eris would also qualify. But Eris was held not to qualify because it was in a neighborhood with multiple other objects, a situation similar to those of similar bodies in the [[asteroid]] belt, namely [[Ceres]] and [[Eris]]. | | The discovery of [[Eris]], a scatter-disk body 27% more massive than Pluto, caused a controversy concerning what does, and what does not, constitute a [[planet]]. If Pluto were to retain its historical designation of "planet," then Eris would also qualify. But Eris was held not to qualify because it was in a neighborhood with multiple other objects, a situation similar to those of similar bodies in the [[asteroid]] belt, namely [[Ceres]] and [[Eris]]. |
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| − | In 2006, the [[International Astronomical Union]] passed the following resolution:{{cquote|'''RESOLUTION 5A''' | + | In 2006, the [[International Astronomical Union]] passed the following resolution:{{Quotebox|'''RESOLUTION 5A''' |
| | The IAU therefore resolves that planets and other bodies in our Solar System, except satellites, be defined into three distinct categories in the following way: | | The IAU therefore resolves that planets and other bodies in our Solar System, except satellites, be defined into three distinct categories in the following way: |
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| − | (1) A "planet"<sup>1</sup> is a celestial body that (a) is in orbit around the Sun, (b) has sufficient mass for its self-gravity to overcome rigid body forces so that it assumes a hydrostatic equilibrium (nearly round) shape, and (c) has cleared the neighbourhood around its orbit. | + | * (1) A "planet"<sup>1</sup> is a celestial body that |
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| − | (2) A "[[dwarf planet]]" is a celestial body that (a) is in orbit around the Sun, (b) has sufficient mass for its self-gravity to overcome rigid body forces so that it assumes a hydrostatic equilibrium (nearly round) shape<sup>2</sup>, (c) has not cleared the neighbourhood around its orbit, and (d)is not a satellite.
| + | * (a) is in orbit around the Sun, |
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| − | (3) All other objects<sup>3</sup>, except satellites, orbiting the Sun shall be referred to collectively as "Small Solar System Bodies". | + | * (b) has sufficient mass for its self-gravity to overcome rigid body forces so that it assumes a hydrostatic equilibrium (nearly round) shape, and |
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| | + | * (c) has cleared the neighborhood around its orbit. |
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| | + | * (2) A "[[dwarf planet]]" is a celestial body that **(a) is in orbit around the Sun, **(b) has sufficient mass for its self-gravity to overcome rigid body forces so that it assumes a hydrostatic equilibrium (nearly round) shape<sup>2</sup>, **(c) has not cleared the neighborhood around its orbit, and **(d)is not a satellite. |
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| | + | * (3) All other objects<sup>3</sup>, except satellites, orbiting the Sun shall be referred to collectively as "Small Solar System Bodies". |
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| | + | <sup>1</sup>''The eight planets are: Mercury, Venus, Earth, Mars, Jupiter, Saturn, Uranus, and Neptune.'' |
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| − | <sup>1</sup>The eight planets are: Mercury, Venus, Earth, Mars, Jupiter, Saturn, Uranus, and Neptune.
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| | <sup>2</sup>An IAU process will be established to assign borderline objects into either dwarf planet and other categories. | | <sup>2</sup>An IAU process will be established to assign borderline objects into either dwarf planet and other categories. |
| − | <sup>3</sup>These currently include most of the Solar System asteroids, most Trans-Neptunian Objects (TNOs), comets, and other small bodies.<ref>"[http://www.iau.org/iau0602.423.0.html IAU0602: the Final IAU Resolution on the Definition of 'Planet' Ready for Voting]," ''International Astronomical Union'', 2005. Accessed January 14, 2008.</ref> }} | + | |
| | + | <sup>3</sup>These currently include most of the Solar System asteroids, most Trans-Neptunian Objects (TNOs), comets, and other small bodies. |
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| | + | The IAU further resolves: |
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| | + | * '''''Pluto is a "dwarf planet" by the above definition and is recognized as the prototype of a new category of Trans-Neptunian Objects''''' <sup>1</sup>. |
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| | + | <sup>1</sup> An IAU process will be established to select a name for this category. |
| | + | — ''International Astronomical Union''}}<ref>"[http://www.iau.org/iau0602.423.0.html IAU0602: the Final IAU Resolution on the Definition of 'Planet' Ready for Voting]," ''International Astronomical Union'', 2005. Accessed January 14, 2008.</ref><ref>https://www.iau.org/static/resolutions/Resolution_GA26-5-6.pdf ''International Astronomical Union'', 2005. Accessed February 9, 2022</ref> |
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| | Under those rather strict criteria, Pluto does not qualify. For that reason, Pluto is no longer considered a planet. It shares the new "dwarf planet" category with Eris, Ceres, Haumea and Makemake.<ref>http://www.iau.org/public_press/news/detail/iau0807/</ref> | | Under those rather strict criteria, Pluto does not qualify. For that reason, Pluto is no longer considered a planet. It shares the new "dwarf planet" category with Eris, Ceres, Haumea and Makemake.<ref>http://www.iau.org/public_press/news/detail/iau0807/</ref> |
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| | Brown suspects the IAU wanted to demote Pluto, because Pluto violates, by its very existence, every conventional theory of planetary origin. | | Brown suspects the IAU wanted to demote Pluto, because Pluto violates, by its very existence, every conventional theory of planetary origin. |
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| − | According to Number 1 (c) and 2 (c) of the IAU definition, also [[Earth]] and [[Mars]] wouldn't be planets because they haven't "cleared" their orbits, but have several asteroids in them, also called "quasi-moons" of Earth and Mars. | + | =[[Earth]] and [[Mars]] as [[dwarf planet|dwarf planets]] under the current [[International Astronomical Union]] definition= |
| | + | According to Number 1 (c) and 2 (c) of the [[International Astronomical Union|IAU]] definition, also [[Earth]] and [[Mars]] wouldn't be planets because they haven't "cleared" their orbits as several asteroids are in their respective orbits, these asteroids are also called "quasi-moons" of Earth and Mars. The IAU precluded this possibility by arbitrarily listing the earth and mars as planets in spite of the current definition (see the quote in the above section: ''"<sup>1</sup>The eight planets are: Mercury, Venus, Earth, Mars, Jupiter, Saturn, Uranus, and Neptune."''). |
| | + | This, however, calls into question the "''scientific''" basis of downgrading Pluto to a dwarf plant as this conflicting standard(of confirming [[earth]] and [[mars]] as planets while classifying Pluto as a dwarf planet) suggests it is merely the '''''opinion''''' of the IAU that Pluto is not a planet <ref>https://www.iau.org/static/resolutions/Resolution_GA26-5-6.pdf ''International Astronomical Union'', 2005. Accessed February 9, 2022</ref> |
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| | == Orbital characteristics == | | == Orbital characteristics == |