New details about planet 2007 OR10, third largest dwarf planet in solar system
gizmodo.com
gizmodo.com
Obviously it's not going to be in the inner solar system, but it seems odd not to even mention the basic comparisons to e.g. the orbits of Pluto or Eris.
Summary: It is out past Neptune, has a similar kind of orbit to Eris.
That often happens because of copyrights.
>Fair use is a legal doctrine only in the United States.[0]
In the UK, for example, their fair dealing exception is only for "non-commercial research or study, criticism or review". [1]
[0] https://en.wikipedia.org/wiki/Fair_use
[1] https://en.wikipedia.org/wiki/Fair_dealing_in_United_Kingdom...
This refers to the Kepler Mission[1] which points to a fixed spot in interstellar space and finds exoplanets. But that mission has NOTHING to do with our solar system. It isn't pointed anywhere near the solar ecliptic and couldn't see a local planet if it was.
So when it says "That lack of reflective light made it hard for Kepler to even spot the planet" it is being ignorantly misleading, and when it says "although Kepler managed to catch brief glimpse in 2014" it is just wrong. "the Konkoly researchers hadn’t thought to pair NASA Kepler data with ESA Herschel data" -- for very good reason, Kepler data would be completely irrelevant. "information about the amount of light the planet was reflecting from Kepler..." again, completely impossible and wrong.
The byline is Ria Misra, clearly a person who should not be allowed to write about astronomy anytime soon.
> We combined optical light curves provided by the Kepler Space Telescope–K2 extended mission and thermal infrared data provided by the Herschel Space Observatory.
Kepler hasn't been staring at the same patch of stars for a while now[1]
[0] http://iopscience.iop.org/article/10.3847/0004-6256/151/5/11... [1] https://en.wikipedia.org/wiki/Kepler_(spacecraft)#Second_Lig...
They can't, as one of the defining characteristics of a planet is having enough mass to be rounded under it's own gravity. Dwarf planets have no such restriction.
> They can't, as one of the defining characteristics of a planet is having enough mass to be rounded under it's own gravity.
The problem here is that "rounded" simply means "roughly spheroid". It's an imprecise term with no rules governing how far from a sphere the objects can deviate and still be considered planets or dwarf planets.
> Dwarf planets have no such restriction.
It is that restriction that separates dwarf planets from large asteroids.
The distinction between planet and dwarf planet has to do with whether or not the object has cleared its orbit of other debris.
Non-spherical objects can still be in hydrostatic equilibrium due to centrifugal forces being anisotropic.
https://en.wikipedia.org/wiki/Dwarf_planet#History_of_the_co...
What I mean is that the intricacies of spacetime is something that can be mathematically formulated, tested, and 'known' in a whole different way than how many objects reside in our solar system. It's kind of analogous to saying that not knowing how many species there are on earth means we don't understand how natural selection works.
Grammar, FTW.
The commas are not ideal, but neither are they ungrammatical.
http://crooksandliars.com/2016/05/zimmerman-gun-sale-hijacke...