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2. 2018 AG37 - Wikipedia

   en.wikipedia.org/wiki/2018_AG37

   JPL Horizons computes an aphelion around the year 2005 at about 133 AU, [11] whereas Project Pluto computes aphelion around the year 1976 slightly further out at 134 AU. [12] Its perihelion is a little less than that of Neptune .

3. Pluto - Wikipedia

   en.wikipedia.org/wiki/Pluto

   Pluto and Neptune's minimum separation is over 17 AU, which is greater than Pluto's minimum separation from Uranus (11 AU). [93] The minimum separation between Pluto and Neptune actually occurs near the time of Pluto's aphelion. [90] Ecliptic longitude of Neptune minus that of Pluto (blue), and rate of change of Pluto's distance from the sun (red).

4. List of Solar System objects most distant from the Sun

   en.wikipedia.org/wiki/List_of_Solar_System...

   One particularly distant body is 90377 Sedna, which was discovered in November 2003.It has an extremely eccentric orbit that takes it to an aphelion of 937 AU. [2] It takes over 10,000 years to orbit, and during the next 50 years it will slowly move closer to the Sun as it comes to perihelion at a distance of 76 AU from the Sun. [3] Sedna is the largest known sednoid, a class of objects that ...

5. Pluto TV Adding 200-Plus Free Movies This Summer ... - AOL

   www.aol.com/entertainment/pluto-tv-adding-200...

   The Paramount-owned ad-supported free streaming service continues to gain traction: In the first quarter, Pluto TV had 80 million monthly active users globally, up from 68 million a year earlier.

6. Comet Swift–Tuttle - Wikipedia

   en.wikipedia.org/wiki/Comet_Swift–Tuttle

   The comet's perihelion is just under that of Earth, while its aphelion is just over that of Pluto. An unusual aspect of its orbit is that it was recently captured into a 1:11 orbital resonance with Jupiter; it completes one orbit for every 11 of Jupiter. [7] It was the first comet in a retrograde orbit to be found in a resonance. [7]

7. List of Solar System objects by greatest aphelion - Wikipedia

   en.wikipedia.org/wiki/List_of_Solar_System...

   An object with an e of between 0 and 1 will have an elliptical orbit, with, for instance, an object with an e of 0.5 having a perihelion twice as close to the Sun as its aphelion. As an object's e approaches 1, its orbit will be more and more elongated before, and at e =1, the object's orbit will be parabolic and unbound to the Solar System (i ...