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Distant minor planet

From Wikipedia, the free encyclopedia

A distant minor planet, or distant object, is any minor planet found beyond Jupiter in the outer Solar System that is not commonly thought of as an "asteroid". The umbrella term is used by IAU's Minor Planet Center (MPC),[1] which is responsible for the identification, designation and orbit computation of these objects.[2] As of May 2019, the MPC maintains 3708 distant objects in its data base.[3]

Most distant minor planets are trans-Neptunian objects and centaurs, while relatively few are damocloids, Neptune trojans or Uranus trojans. All distant objects have a semi-major axis (average distance from the Sun) greater than 6 AU.[3] This threshold, which is just beyond the orbit of Jupiter (5.2 AU), ensures that the vast majority of "true asteroids" – such as the near-Earth, Mars-crosser, main-belt and Jupiter trojan populations – are excluded from the distant minor planets.[3]

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  • ✪ A New Dwarf Planet?
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Transcription

It’s been almost 10 years since the whole kerfuffle, but a lot of people still don’t seem to be over the fact that Pluto isn’t a planet. Back in 2006, the International Astronomical Union -- the organization that makes all the rules when it comes to astronomy -- officially defined what makes a planet a planet, and Pluto didn’t qualify. Now, a researcher has come up with a new definition of a planet -- one that can be used to classify planets around other stars, too. But Pluto still doesn’t make the cut. Currently, the official definition of a planet means it has to meet three criteria. A planet has to be orbiting the Sun; have enough mass to be generally spherical; and its gravitation has to be strong enough for it to have its orbital path basically to itself, clear of any other major objects. Anything that meets the first two conditions, but not the third, is called a dwarf planet. So Pluto is a dwarf planet. But you’ll notice that the official definition includes orbiting the Sun, which means we can’t classify anything we detect in another star system as a planet. But in the past 30 years, we’ve discovered nearly 2,000 worlds orbiting other stars. And with the telescopes we have right now, it’s pretty much impossible to tell whether any of them is round, so that criterion isn’t really useful either. So last week, at the 47th meeting of the American Astronomical Society, astronomer Jean-Luc Margot proposed a new definition -- and used it to classify almost all of the exoplanets we’ve found so far. The new definition is simple: a planet has to orbit at least one star -- or the remains of one -- have a clear orbital path to itself, and have less than 13 times the mass of Jupiter. That last one is to make sure we don’t accidentally classify any of the tiny, failed brown dwarf stars as planets. If you test this new definition of our solar system, it still works -- all the planets and dwarf planets fall into the right categories, including dwarf planet Pluto. And these are all things we can measure in other star systems, by calculating things like the masses of the star and exoplanet. Turns out that if you apply this definition to all the exoplanets that have enough data … they all count as full-fledged planets. Which kinda makes sense, because our telescopes aren’t powerful enough to detect something as small as a dwarf planet orbiting another star anyway. The new definition hasn’t been adopted by the IAU, so it isn’t official. But the group will eventually have to come up with a way to classify exoplanets, and according to at least one of the higher-ups at the American Astronomical Society, Margot’s definition might be a good place to start. Closer to home, knowing how to classify new worlds is coming in handy, too. Because at that same meeting, a group of astronomers announced that they’d discovered a new possible dwarf planet in our solar system. For now it’s going by the catchy name of V774104, and it’s the farthest object ever detected in the solar system. As our technology improves, astronomers have been finding more and more worlds beyond Neptune’s orbit, including what used to be the most distant dwarf planet-sized object we knew of: 2012VP113, informally known as Biden. I say dwarf planet sized, because, along with a few other likely-looking candidates, it hasn’t been officially confirmed as a dwarf planet yet. Sometime in October, the same team that analyzed Biden’s orbit was using the Subaru telescope in Hawaii to scan the distant reaches of the solar system, when they noticed a moving dot that had never been seen before. That was the new possible dwarf planet, and it was incredibly far away. To give you some perspective, when Biden is closest to the Sun, it’s about 12 billion kilometers away -- or around 80 times the distance from Earth to the Sun. But this newly-found rock is about 15 billion kilometers from the Sun -- around 103 times as far from the Sun as we are. We just don’t know where exactly it is in its orbit, because there hasn’t been enough time to track it yet -- that will take about another year. For all we know, at some point it might end up closer to the Sun than Biden does. Still, now we know that we can spot worlds more than a hundred times farther from the Sun than we are. And, at the very least, we might have a new dwarf planet to study. So, welcome to the neighborhood! Thanks for watching this episode of SciShow Space News, and thanks especially to our patrons on Patreon. You guys are awesome.

See also

References

  1. ^ "Observable Distant Minor Planets". Minor Planet Center. Retrieved 26 October 2018.
  2. ^ "Main page". Minor Planet Center. Retrieved 26 October 2018.
  3. ^ a b c "Objects with orbit type; Distant object". Minor Planet Center. Retrieved 25 May 2019.

External links

This page was last edited on 25 May 2019, at 07:19
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