<blockquote>
<p>... raise questions about how much we know about the <strong>true</strong> (<a href="https://en.wikipedia.org/wiki/IAU_definition_of_planet" rel="nofollow noreferrer">IAU definition</a>) <strong>number</strong> of planets in our solar system.</p>
</blockquote>
<p><strong><a href="https://en.wikipedia.org/wiki/Planet#Solar_System" rel="nofollow noreferrer">Eight</a>.</strong></p>
<blockquote>
<p>Question: Does the discovery of <a href="https://en.wikipedia.org/wiki/2012_VP113" rel="nofollow noreferrer">2012 VP<span class="math-container">$_{113}$</span></a> and <a href="https://en.wikipedia.org/wiki/90377_Sedna" rel="nofollow noreferrer">90377 .</a> increase the odds of some kind of planetary object on the edge of the known solar system (the <a href="https://en.wikipedia.org/wiki/Oort_cloud" rel="nofollow noreferrer">Oort cloud</a>)?</p>
</blockquote>
<p><a href="https://en.wikipedia.org/wiki/2012_VP113" rel="nofollow noreferrer">2012 VP<span class="math-container">$_{113}$</span></a> is a <a href="https://en.wikipedia.org/wiki/Minor_planet" rel="nofollow noreferrer">minor planet</a>, that does not imply that it is a &quot;<a href="https://en.wikipedia.org/wiki/Planet" rel="nofollow noreferrer">planet</a>&quot;.</p>
<p><a href="https://en.wikipedia.org/wiki/90377_Sedna" rel="nofollow noreferrer">90377 Sedna</a> is a large minor <a href="https://en.wikipedia.org/wiki/Minor_planet" rel="nofollow noreferrer">minor planet</a>, also not a &quot;<a href="https://en.wikipedia.org/wiki/Planet" rel="nofollow noreferrer">planet</a>&quot;.</p>
<p>The <a href="https://en.wikipedia.org/wiki/Oort_cloud" rel="nofollow noreferrer">Oort cloud</a> has so many tiny objects that they upset each other's orbit, occasionally sending comets into our solar system. Part of being a planet is having an orbit <strong>and</strong> clearing your orbit; these objects do neither.</p>
<p><a href="https://i.sstatic.net/FYbQX.jpg" rel="nofollow noreferrer"><img src="https://i.sstatic.net/FYbQX.jpg" alt="Oort Cloud - close-up slice" /></a></p>
<p><a href="https://i.sstatic.net/R7lTM.jpg" rel="nofollow noreferrer"><img src="https://i.sstatic.net/R7lTM.jpg" alt="Oort Cloud - distant view" /></a></p>
<blockquote>
<p>How could we find out if it is very cold and dark?</p>
</blockquote>
<p>Every object in space affects the movement of every other object.</p>
<p>We can detect tiny black holes at a distance, they are cold and dark; detecting a new planet in our solar system isn't beyond our ability, there simply isn't one there.</p>
<p>It's not impossible for a large object to begin orbit of the sun and establish that it will orbit a reasonably fixed path (some wobble is OK, drastic changes in direction or too close to something large enough isn't going to maintain it's orbit (and clearing ability)).</p>
<p><a href="https://en.wikipedia.org/wiki/Pluto" rel="nofollow noreferrer">Pluto</a> takes 248.00 years (90,560 days) to complete an orbit. Discovered in 1930 it lost its status as a planet in 2006. If something appears out of nowhere it will take time for it to be approved, so no surprises in the next few years.</p>
<blockquote>
<p>I mean, how many <a href="https://en.wikipedia.org/wiki/90377_Sedna" rel="nofollow noreferrer">90377 Sedna</a> or <a href="https://en.wikipedia.org/wiki/2012_VP113" rel="nofollow noreferrer">2012 VP<span class="math-container">$_{113}$</span></a> objects would we need in order to guess its position and location?</p>
</blockquote>
<p>Objects very distant to each other affect each other to a much smaller extent that objects which are closer to each other. As time passes, observations and new calculations are made, results are confirmed, <strong>and</strong> it passes IAU committee approval something might be discovered and become a new planet, instead scientists are looking outside our solar system for exoplanets.</p>
<p><a href="https://en.wikipedia.org/wiki/Beta_Pictoris" rel="nofollow noreferrer">Beta Pictoris</a> (β Pic) is the second brightest star in the constellation <a href="https://en.wikipedia.org/wiki/Pictor" rel="nofollow noreferrer">Pictor</a>. It is located 63.4 light years from the Solar System. Scientists believe there are a few planets in orbit around the star.</p>
<p>&quot;<a href="https://www.cambridge.org/core/journals/proceedings-of-the-international-astronomical-union/article/planet-companion-around-pictoris/4516DB8AC8CE30CC549B9236C78D6A39" rel="nofollow noreferrer">The planet companion around β Pictoris</a>&quot; (Oct 2010), by Anne-Marie Lagrange, Mickaël Bonnefoy, Gael Chauvin, Daniel Apai, Et al.:</p>
<blockquote>
<p><strong>Abstract</strong></p>
<p>The β Pic disk of dust and gas has been regarded as the prototype of young planetary systems since the 1980s and has revealed over the years an impressive amount of indirect signs pointing toward the presence of at least one giant planet. We present here the recently detected first giant planet around this star. We show how this planet could explain some very peculiar features of the star environment (disk, spectroscopic variability), and how it constrains the scenarios of planetary system formation (timescales, mechanisms).</p>
</blockquote>
<p>Scientists can see far and do look for planets, it's unlikely that there's a 11th planet that's been unobserved. They have nicknamed β Pic's <a href="http://www.solstation.com/stars2/beta-pic.htm#planetb" rel="nofollow noreferrer">planet &quot;b&quot;</a>. Here's its photo:</p>
<p><a href="https://i.sstatic.net/mmyVE.jpg" rel="nofollow noreferrer"><img src="https://i.sstatic.net/mmyVE.jpg" alt="Planet &quot;b&quot;" /></a></p>
<blockquote>
<p>Reading about this topic, I don't know how to quantify the odds of finding:</p>
</blockquote>
<ul>
<li>PX (Planet X): An Earth sized body perturbing the orbits of <a href="https://en.wikipedia.org/wiki/90377_Sedna" rel="nofollow noreferrer">90377 Sedna</a>, <a href="https://en.wikipedia.org/wiki/2012_VP113" rel="nofollow noreferrer">2012 VP<span class="math-container">$_{113}$</span></a> and other similar objects.</li>
</ul>
<p>There is <a href="http://iopscience.iop.org/article/10.3847/0004-6256/151/2/22" rel="nofollow noreferrer">support for the existence of the object</a>, but under the IAU definition imposed by your question it hasn't yet met the requirements to become a planet. <strong>The announcement does not mean there is a new planet in our solar system. The existence of this distant world is only theoretical at this point and no direct observation of the object nicknamed have been made</strong>. The mathematical prediction of a planet could explain the unique orbits of some smaller objects in the Kuiper Belt, a distant region of icy debris that extends far beyond the orbit of Neptune. Astronomers are now searching for the predicted planet.</p>
<ul>
<li><a href="https://en.wikipedia.org/wiki/Talk:Telisto_(hypothetical_planet)" rel="nofollow noreferrer">Thelistos</a>: A super-Earth (about 5-10 Earth masses times a O(1) factor)</li>
</ul>
<p>Misnomer. Deleted from Wikipedia, redirects to planet X.</p>
<ul>
<li><a href="https://en.wikipedia.org/wiki/Tyche_(hypothetical_planet)" rel="nofollow noreferrer">Tyche</a>: (Now disfavoured by WISE data, I think it can not be excluded if it is extremely cold and &quot;dark&quot;) Gas giant (Neptune-like, Saturn-like, etc.)</li>
</ul>
<p>Disproven. Does not exist.</p>
<ul>
<li>Nemesis: A &quot;dark star&quot;/brown dwarf object.</li>
</ul>
<p><a href="https://en.wikipedia.org/wiki/128_Nemesis" rel="nofollow noreferrer">128 Nemesis</a> is an asteroid, the <em>other</em> <a href="https://en.wikipedia.org/wiki/Nemesis_(hypothetical_star)" rel="nofollow noreferrer">Nemesis</a> is a hypothetical red dwarf or brown dwarf, originally postulated in 1984 to be orbiting the Sun at a distance of about 95,000 AU (1.5 light-years). Thought to be somewhat beyond the Oort cloud, it's <a href="https://www.google.com/search?q=postulated" rel="nofollow noreferrer">postulated</a> to explain a perceived cycle of mass extinctions in the geological record, which seem to occur more often at intervals of 26 million years.</p>
<hr />
<p>Which objects are defined as planets is precisely defined, there's only some overlap for non-planets:</p>
<p><a href="https://i.sstatic.net/Z786z.png" rel="nofollow noreferrer"><img src="https://i.sstatic.net/Z786z.png" alt="Planet or not." /></a></p>
<p>Here is the text of the <a href="https://www.iau.org/static/resolutions/Resolution_GA26-5-6.pdf" rel="nofollow noreferrer">IAU’s Resolution B5: Definition of a Planet in the Solar System</a> (.PDF):</p>
<blockquote>
<p>The IAU therefore resolves that planets and other bodies, except satellites, in our Solar System be defined into three distinct categories in the following way:</p>
<p>(<strong>1</strong>) A planet<span class="math-container">$^1$</span> is a celestial body that</p>
<p><span class="math-container">$\quad$</span> (<strong>a</strong>) is in orbit around the Sun,</p>
<p><span class="math-container">$\quad$</span> (<strong>b</strong>) has sufficient mass for its self-gravity to overcome rigid body forces so that it assumes a hydrostatic equilibrium (nearly round) shape, and</p>
<p><span class="math-container">$\quad$</span> (<strong>c</strong>) has cleared the neighbourhood around its orbit.</p>
<p>(<strong>2</strong>) A &quot;dwarf planet&quot; is a celestial body that</p>
<p><span class="math-container">$\quad$</span> (<strong>a</strong>) is in orbit around the Sun,</p>
<p><span class="math-container">$\quad$</span> (<strong>b</strong>) has sufficient mass for its self-gravity to overcome rigid body forces so that it assumes a hydrostatic equilibrium (nearly round) shape<span class="math-container">$^2$</span>,</p>
<p><span class="math-container">$\quad$</span> (<strong>c</strong>) has <em><strong>not</strong></em> cleared the neighbourhood around its orbit, and</p>
<p><span class="math-container">$\quad$</span> (<strong>d</strong>) is not a satellite.</p>
<p>(<strong>3</strong>) All other objects<span class="math-container">$^3$</span>, except satellites, orbiting the Sun shall be referred to  collectively as &quot;Small Solar System Bodies&quot;.</p>
</blockquote>
<p><strong><code>1</code></strong> <code>The eight planets are: Mercury, Venus, Earth, Mars, Jupiter, Saturn, Uranus, and Neptune.</code></p>
<p><strong><code>2</code></strong> <code>An IAU process will be established to assign borderline objects to the dwarf planet or to another category.</code></p>
<p><strong><code>3</code></strong> <code>These currently include most of the Solar System asteroids, most Trans-Neptunian Objects (TNOs), comets, and other small bodies.</code></p>

CC BY-SA 4.0
2018-06-23T18:48:04.610Z
It's worth noting that the IAU definition is either unclear or inconsistent (it's unclear if *any* planet orther than perhaps mercury has "cleared its orbit") and primarily represents the view of the dynamicists and not the planetologists. The reality is that there is a continuum of bodies from stars to meteoroids and all else is line-drawing. Lines *do* need to be drawn, but they are arbitrary (and hence not "true") and can and should change as convenient.
Mark Olson
CC BY-SA 4.0
2018-06-23T21:34:35.693Z
@MarkOlson No planet is presumed to be the *only* thing in its orbit.  It is just *the vast majority of the mass* around its orbit.  The exact threshold for what constitutes "vast majority" is currently arbitrary, yes, but there is such a massive difference between the 8 acknowledged planets and everything else (including Pluto) that it is currently pretty irrelevant what the threshold is.  It's quibbling about what "high off the floor" means when everything is either on the ground or 500 feet in the air.
zibadawa timmy
CC BY-SA 4.0
2018-06-24T00:23:09.717Z
As I said: arbitrary. A matter of definition, not of science.
Mark Olson
CC BY-SA 4.0
2018-06-24T00:42:04.130Z
The procedure to address these concerns is in the [IAU Working Rules](https://www.iau.org/administration/statutes_rules/working_rules/#WorkRulIII). It was specifically asked by riemannium that those rules, as they currently stand, be adhered to in answering the question. SE has its rules too: ["An acceptable answer is any answer that directly addresses the question asked"](https://meta.stackexchange.com/a/118597/282094).
Rob
CC BY-SA 4.0
2023-10-26T21:38:23.850Z
I noticed the spelling mistake: "...  smaller extent **that** objects which are closer ...", but I won't bump this 5 year old answer until I have a more significant update.
Rob
CC BY-SA 4.0
2018-06-23T18:04:46.070Z
2018-06-23T18:04:46.070Z
2020-06-17T09:47:40.653Z
Rob
<p>Crosslisted question from <a href="https://physics.stackexchange.com/questions/131876/sedna-vp113-and-the-likelihood-of-the-px-tyche-thelistos-hypotheses">https://physics.stackexchange.com/questions/131876/sedna-vp113-and-the-likelihood-of-the-px-tyche-thelistos-hypotheses</a></p>

<p>The recent discoveries in exoplanetary science (specially those findings of planets orbiting far far away from its parent star/stars) raise questions about how much we know about the (true, AIU definition) number of planets in our solar system.</p>

<p>Question: does the discovery of VP113 and Sedna increase the odds of some kind of planetary object in the edge of the known solar system (Oort's cloud)? How could we find it if it is very cold and dark? I mean, how many Sedna or VP113 objects we would need in order to guess its position and location?</p>

<p>Reading about this topic, I don't know how to quantify the odds of finding</p>

<ul>
<li><p>PX(Planet X): An Earth sized body perturbing the orbits of Sedna, VP113 and other similar objects.</p></li>
<li><p>Thelistos: A super-Earth (about 5-10 Earth masses times a O(1) factor)</p></li>
<li><p>Tyche: (Now disfavoured by WISE data, I think it can not be excluded if it is extremely cold and "dark") Gas giant (Neptune-like, Saturn-like, etc)</p></li>
<li><p>Nemesis: A "dark star"/brown dwarf object.</p></li>
</ul>

CC BY-SA 3.0
2018-02-21T16:42:51.040Z
@LocalFluff Please convert this into an answer.
called2voyage
CC BY-SA 3.0
2014-09-10T15:49:03.317Z
It would need to be in the direction of the Milky Way in order to have been confused with background stars up until today, if it is much larger than Mars. Attempts are planned to find microlensing of Oort cloud objects in the data from the Gaia space telescope.
LocalFluff
<exoplanet>
Sedna, VP113 and the likelihood of the PX/Tyche/Thelistos hypotheses
riemannium
# Sedna, VP113 and the likelihood of the PX/Tyche/Thelistos hypotheses

(Asked by: username_0 on 2014-09-10)

Crosslisted question from <https://physics.stackexchange.com/questions/131876/sedna-vp113-and-the-likelihood-of-the-px-tyche-thelistos-hypotheses>

The recent discoveries in exoplanetary science (specially those findings of planets orbiting far far away from its parent star/stars) raise questions about how much we know about the (true, AIU definition) number of planets in our solar system.

Question: does the discovery of VP113 and Sedna increase the odds of some kind of planetary object in the edge of the known solar system (Oort's cloud)? How could we find it if it is very cold and dark? I mean, how many Sedna or VP113 objects we would need in order to guess its position and location?

Reading about this topic, I don't know how to quantify the odds of finding

* PX(Planet X): An Earth sized body perturbing the orbits of Sedna, VP113 and other similar objects.
* Thelistos: A super-Earth (about 5-10 Earth masses times a O(1) factor)
* Tyche: (Now disfavoured by WISE data, I think it can not be excluded if it is extremely cold and "dark") Gas giant (Neptune-like, Saturn-like, etc)
* Nemesis: A "dark star"/brown dwarf object.

**Tags:** exoplanet

> **Comments:**
> **username_2**: It would need to be in the direction of the Milky Way in order to have been confused with background stars up until today, if it is much larger than Mars. Attempts are planned to find microlensing of Oort cloud objects in the data from the Gaia space telescope.  
> **username_1**: @username_2 Please convert this into an answer.  

---

## 1 answers

### Answer by username_3 on 2018-06-23. Score: 1 | Accepted answer

> ... raise questions about how much we know about the **true** ([IAU definition](https://en.wikipedia.org/wiki/IAU_definition_of_planet)) **number** of planets in our solar system.

**[Eight](https://en.wikipedia.org/wiki/Planet#Solar_System).**

> Question: Does the discovery of [2012 VP$\_{113}$](https://en.wikipedia.org/wiki/2012_VP113) and [90377 .](https://en.wikipedia.org/wiki/90377_Sedna) increase the odds of some kind of planetary object on the edge of the known solar system (the [Oort cloud](https://en.wikipedia.org/wiki/Oort_cloud))?

[2012 VP$\_{113}$](https://en.wikipedia.org/wiki/2012_VP113) is a [minor planet](https://en.wikipedia.org/wiki/Minor_planet), that does not imply that it is a "[planet](https://en.wikipedia.org/wiki/Planet)".

[90377 Sedna](https://en.wikipedia.org/wiki/90377_Sedna) is a large minor [minor planet](https://en.wikipedia.org/wiki/Minor_planet), also not a "[planet](https://en.wikipedia.org/wiki/Planet)".

The [Oort cloud](https://en.wikipedia.org/wiki/Oort_cloud) has so many tiny objects that they upset each other's orbit, occasionally sending comets into our solar system. Part of being a planet is having an orbit **and** clearing your orbit; these objects do neither.

[![Oort Cloud - close-up slice](https://i.sstatic.net/FYbQX.jpg)](https://i.sstatic.net/FYbQX.jpg)

[![Oort Cloud - distant view](https://i.sstatic.net/R7lTM.jpg)](https://i.sstatic.net/R7lTM.jpg)

> How could we find out if it is very cold and dark?

Every object in space affects the movement of every other object.

We can detect tiny black holes at a distance, they are cold and dark; detecting a new planet in our solar system isn't beyond our ability, there simply isn't one there.

It's not impossible for a large object to begin orbit of the sun and establish that it will orbit a reasonably fixed path (some wobble is OK, drastic changes in direction or too close to something large enough isn't going to maintain it's orbit (and clearing ability)).

[Pluto](https://en.wikipedia.org/wiki/Pluto) takes 248.00 years (90,560 days) to complete an orbit. Discovered in 1930 it lost its status as a planet in 2006. If something appears out of nowhere it will take time for it to be approved, so no surprises in the next few years.

> I mean, how many [90377 Sedna](https://en.wikipedia.org/wiki/90377_Sedna) or [2012 VP$\_{113}$](https://en.wikipedia.org/wiki/2012_VP113) objects would we need in order to guess its position and location?

Objects very distant to each other affect each other to a much smaller extent that objects which are closer to each other. As time passes, observations and new calculations are made, results are confirmed, **and** it passes IAU committee approval something might be discovered and become a new planet, instead scientists are looking outside our solar system for exoplanets.

[Beta Pictoris](https://en.wikipedia.org/wiki/Beta_Pictoris) (β Pic) is the second brightest star in the constellation [Pictor](https://en.wikipedia.org/wiki/Pictor). It is located 63.4 light years from the Solar System. Scientists believe there are a few planets in orbit around the star.

"[The planet companion around β Pictoris](https://www.cambridge.org/core/journals/proceedings-of-the-international-astronomical-union/article/planet-companion-around-pictoris/4516DB8AC8CE30CC549B9236C78D6A39)" (Oct 2010), by Anne-Marie Lagrange, Mickaël Bonnefoy, Gael Chauvin, Daniel Apai, Et al.:

> **Abstract**
>
> The β Pic disk of dust and gas has been regarded as the prototype of young planetary systems since the 1980s and has revealed over the years an impressive amount of indirect signs pointing toward the presence of at least one giant planet. We present here the recently detected first giant planet around this star. We show how this planet could explain some very peculiar features of the star environment (disk, spectroscopic variability), and how it constrains the scenarios of planetary system formation (timescales, mechanisms).

Scientists can see far and do look for planets, it's unlikely that there's a 11th planet that's been unobserved. They have nicknamed β Pic's [planet "b"](http://www.solstation.com/stars2/beta-pic.htm#planetb). Here's its photo:

[![Planet "b"](https://i.sstatic.net/mmyVE.jpg)](https://i.sstatic.net/mmyVE.jpg)

> Reading about this topic, I don't know how to quantify the odds of finding:

* PX (Planet X): An Earth sized body perturbing the orbits of [90377 Sedna](https://en.wikipedia.org/wiki/90377_Sedna), [2012 VP$\_{113}$](https://en.wikipedia.org/wiki/2012_VP113) and other similar objects.

There is [support for the existence of the object](http://iopscience.iop.org/article/10.3847/0004-6256/151/2/22), but under the IAU definition imposed by your question it hasn't yet met the requirements to become a planet. **The announcement does not mean there is a new planet in our solar system. The existence of this distant world is only theoretical at this point and no direct observation of the object nicknamed have been made**. The mathematical prediction of a planet could explain the unique orbits of some smaller objects in the Kuiper Belt, a distant region of icy debris that extends far beyond the orbit of Neptune. Astronomers are now searching for the predicted planet.

* [Thelistos](https://en.wikipedia.org/wiki/Talk:Telisto_(hypothetical_planet)): A super-Earth (about 5-10 Earth masses times a O(1) factor)

Misnomer. Deleted from Wikipedia, redirects to planet X.

* [Tyche](https://en.wikipedia.org/wiki/Tyche_(hypothetical_planet)): (Now disfavoured by WISE data, I think it can not be excluded if it is extremely cold and "dark") Gas giant (Neptune-like, Saturn-like, etc.)

Disproven. Does not exist.

* Nemesis: A "dark star"/brown dwarf object.

[128 Nemesis](https://en.wikipedia.org/wiki/128_Nemesis) is an asteroid, the *other* [Nemesis](https://en.wikipedia.org/wiki/Nemesis_(hypothetical_star)) is a hypothetical red dwarf or brown dwarf, originally postulated in 1984 to be orbiting the Sun at a distance of about 95,000 AU (1.5 light-years). Thought to be somewhat beyond the Oort cloud, it's [postulated](https://www.google.com/search?q=postulated) to explain a perceived cycle of mass extinctions in the geological record, which seem to occur more often at intervals of 26 million years.

---

Which objects are defined as planets is precisely defined, there's only some overlap for non-planets:

[![Planet or not.](https://i.sstatic.net/Z786z.png)](https://i.sstatic.net/Z786z.png)

Here is the text of the [IAU’s Resolution B5: Definition of a Planet in the Solar System](https://www.iau.org/static/resolutions/Resolution_GA26-5-6.pdf) (.PDF):

> The IAU therefore resolves that planets and other bodies, except satellites, in our Solar System be defined into three distinct categories in the following way:
>
> (**1**) A planet$^1$ is a celestial body that
>
> $\quad$ (**a**) is in orbit around the Sun,
>
> $\quad$ (**b**) has sufficient mass for its self-gravity to overcome rigid body forces so that it assumes a hydrostatic equilibrium (nearly round) shape, and
>
> $\quad$ (**c**) has cleared the neighbourhood around its orbit.
>
> (**2**) A "dwarf planet" is a celestial body that
>
> $\quad$ (**a**) is in orbit around the Sun,
>
> $\quad$ (**b**) has sufficient mass for its self-gravity to overcome rigid body forces so that it assumes a hydrostatic equilibrium (nearly round) shape$^2$,
>
> $\quad$ (**c**) has ***not*** cleared the neighbourhood around its orbit, and
>
> $\quad$ (**d**) is not a satellite.
>
> (**3**) All other objects$^3$, except satellites, orbiting the Sun shall be referred to collectively as "Small Solar System Bodies".

**`1`** `The eight planets are: Mercury, Venus, Earth, Mars, Jupiter, Saturn, Uranus, and Neptune.`

**`2`** `An IAU process will be established to assign borderline objects to the dwarf planet or to another category.`

**`3`** `These currently include most of the Solar System asteroids, most Trans-Neptunian Objects (TNOs), comets, and other small bodies.`

> **Comments:**
> **username_4**: It's worth noting that the IAU definition is either unclear or inconsistent (it's unclear if *any* planet orther than perhaps mercury has "cleared its orbit") and primarily represents the view of the dynamicists and not the planetologists. The reality is that there is a continuum of bodies from stars to meteoroids and all else is line-drawing. Lines *do* need to be drawn, but they are arbitrary (and hence not "true") and can and should change as convenient.  
> **username_5**: @username_4 No planet is presumed to be the *only* thing in its orbit.  It is just *the vast majority of the mass* around its orbit.  The exact threshold for what constitutes "vast majority" is currently arbitrary, yes, but there is such a massive difference between the 8 acknowledged planets and everything else (including Pluto) that it is currently pretty irrelevant what the threshold is.  It's quibbling about what "high off the floor" means when everything is either on the ground or 500 feet in the air.  
> **username_4**: As I said: arbitrary. A matter of definition, not of science.  
> **username_3**: The procedure to address these concerns is in the [IAU Working Rules](https://www.iau.org/administration/statutes_rules/working_rules/#WorkRulIII). It was specifically asked by username_0 that those rules, as they currently stand, be adhered to in answering the question. SE has its rules too: ["An acceptable answer is any answer that directly addresses the question asked"](https://meta.stackexchange.com/a/118597/282094).  
> **username_3**: I noticed the spelling mistake: "...  smaller extent **that** objects which are closer ...", but I won't bump this 5 year old answer until I have a more significant update.  

---

