<\/p>\n
+ This is very similar to the 100,000 year eccentricity<\/strong> period.\n<\/p>\n <\/p>\n + In Mechanicsastrodynamics, orbital eccentricity<\/strong> shows how much the shape of an object’s orbit is different from a circle.\n<\/p>\n <\/p>\n + This orbit is at an inclination of 143\u00b0 to the ecliptic with an orbital eccentricity<\/strong> of 0.2001.\n<\/p>\n <\/p>\n + Narvi is about 7kilometres in diameter, and orbits Saturn at an average distance of 19,371,000km in 1006.541days, at an inclination of 137\u00b0 to the ecliptic, with an eccentricity<\/strong> of 0.320.\n<\/p>\n + Chaldene is about 3.8 kilometres in diameter, and orbits Jupiter at an average distance of 22,713,000km in 699.327 days, at an inclination of 167\u00b0 to the ecliptic, with an orbital eccentricity<\/strong> of 0.2916.\n<\/p>\n <\/p>\n + Euporie is about 2 kilometres in diameter, and orbits Jupiter at an average distance of 19,088,000km in 538.780 days, at an inclination of 145\u00b0 to Jupiter’s equator, with an orbital eccentricity<\/strong> of 0.0960.\n<\/p>\n <\/p>\n + Ymir is about 16 kilometres in diameter, and orbits Saturn at an average distance of 23,175,000km in 1317.137 days, at an inclination of 172\u00b0 to the ecliptic, with an eccentricity<\/strong> of 0.358.\n<\/p>\n <\/p>\n + Nessus finishes one orbit around the Sun in 122.4 years, an eccentricity<\/strong> of 0.52 and an inclination to the ecliptic of 15.6 degrees.\n<\/p>\n <\/p>\n + S\/2004 S 13 is about 6 kilometres in diameter, and orbits Saturn at an average distance of 18,056,000km in 905.848 days, at an inclination of 167\u00b0 to the ecliptic, with an eccentricity<\/strong> of 0.261.\n<\/p>\n <\/p>\n + The orbital period is about 16.50 hours, the eccentricity<\/strong> below 0.03.\n<\/p>\n <\/p>\n + The diagram illustrates the orbital parameters of the retrograde non-spherical moons of Uranus with the eccentricity<\/strong> of the orbits represented by the segments extending from the pericentre to the apocentre.\n<\/p>\n <\/p>\n + Fenrir is about 4 kilometres in diameter, and orbits Saturn at an average distance of 22,611,000km in 1269.362 days, at an inclination of 163\u00b0 to the ecliptic, with an eccentricity<\/strong> of 0.131.\n<\/p>\n <\/p>\n + The high orbital eccentricity<\/strong> of Pluto puts it mostly outside Neptune’s orbit, but partly inside.\n<\/p>\n <\/p>\n + Its orbit has an eccentricity<\/strong> of 0.13.\n<\/p>\n <\/p>\n + Bergelmir is about 6 kilometres in diameter, and orbits Saturn at an average distance of 19,372,000km in 1006.659 days, at an inclination of 157\u00b0 to the ecliptic, with an eccentricity<\/strong> of 0.152.\n<\/p>\n <\/p>\n + Around that time, the eccentricity<\/strong> of the seven-member group finally began to become a hot topic in the news and headlines.\n<\/p>\n <\/p>\n + The orbital eccentricity<\/strong> of ~0.0015 and inclination of ~ 0.03\u00b0 relative to the equator of Jupiter are very small.\n<\/p>\n <\/p>\n + The eccentricity<\/strong> of the orbits is represented by the yellow segments with the inclination represented on Y axis.\n<\/p>\n <\/p>\n + Callirrhoe is about 8.6 kilometres in diameter, and orbits Jupiter at an average distance of 24,356,000km in 776.543 days, at an inclination of 141\u00b0 to the ecliptic, with an orbital eccentricity<\/strong> of 0.264.\n<\/p>\n <\/p>\n + Taygete is about 5 kilometres in diameter, and orbits Jupiter at an average distance of 22,439,000km in 686.675 days, at an inclination of 165\u00b0 to the ecliptic, with an orbital eccentricity<\/strong> of 0.3678.\n<\/p>\n <\/p>\n + Its eccentricity<\/strong> is 0.4104.\n<\/p>\n <\/p>\n + Ananke orbits Jupiter on a high eccentricity<\/strong> and high inclination retrograde orbit.\n<\/p>\n <\/p>\n + The eccentricity<\/strong> of the orbits is represented by the yellow segments extending from the pericentre to the apocentre.\n<\/p>\n <\/p>\n + S\/2006 S 3 is about 6 kilometres in diameter, and orbits Saturn at an average distance of 21,076,300km in 1142.366 days, at an inclination of 150.8\u00b0 to the ecliptic, with an eccentricity<\/strong> of 0.4710.\n<\/p>\n <\/p>\n + It is about 6 kilometres in diameter, and orbits Saturn at an average distance of 24,505,000km in 1432 days at an inclination of 168\u00b0 to the ecliptic with an eccentricity<\/strong> of 0.186.\n<\/p>\n <\/p>\n + Hermippe is about 4 kilometres in diameter, and orbits Jupiter at an average distance of 21,182,000km in 629.809 days, at an orbital inclination of 151\u00b0 to the ecliptic, with an eccentricity<\/strong> of 0.2290.\n<\/p>\n <\/p>\n + Hyrrokkin is about 8 kilometres in diameter, and orbits Saturn at an average distance of 18,168,300km in 914.292 days, at an inclination of 153.3\u00b0 to the ecliptic, with an eccentricity<\/strong> of 0.3604.\n<\/p>\n <\/p>\n + Kalyke is about 5.2 kilometres in diameter, and orbits Jupiter at an average distance of 23,181,000km in 721.021 days, at an inclination of 166\u00b0 to the ecliptic, with an orbital eccentricity<\/strong> of 0.2140.\n<\/p>\n <\/p>\n + The potentially brightest C-type asteroid is 324 Bamberga, but that object’s very high eccentricity<\/strong> means it rarely reaches its maximum magnitude.\n<\/p>\n <\/p>\n + The eccentricity<\/strong> of this ellipse is exaggerated for visualization.\n<\/p>\n <\/p>\n + Different SDOs have different orbital eccentricity<\/strong> and orbital inclination.\n<\/p>\n <\/p>\n + Erinome is about 3.2 kilometres in diameter, and orbits Jupiter at an average distance of 22,986,000km in 711.965 days, at an inclination of 164\u00b0 to the ecliptic, with an orbital eccentricity<\/strong> of 0.2552.\n<\/p>\n <\/p>\n + The diagram illustrates the orbital parameters of Margaret, unique among the non-spherical moons of Uranus, with inclination on the vertical axis and the eccentricity<\/strong> of the orbits represented by the segments extending from the pericentre to the apocentre.\n<\/p>\n <\/p>\n + Thrymr is about 5.6 kilometres in diameter, and orbits Saturn at an average distance of 20,810,000km in 1120.809 days, at an inclination of 175\u00b0 to the ecliptic, with an eccentricity<\/strong> of 0.453.\n<\/p>\n <\/p>\n + The eccentricity<\/strong> of selected orbits is represented by the yellow segments.\n<\/p>\n <\/p>\n + Eukelade is about 4 kilometres in diameter, and orbits Jupiter at an average distance of 23,484,000km in 735.200 days, at an inclination of 164\u00b0 to the ecliptic, with an orbital eccentricity<\/strong> of 0.2829.\n<\/p>\n <\/p>\n + Pasithee is about 2 kilometres in diameter, and orbits Jupiter at an average distance of 23,307,000 km in 726.933 days, at an inclination of 166\u00b0 to the ecliptic, with an orbital eccentricity<\/strong> of 0.3289.\n<\/p>\n <\/p>\n + Sinope orbits Jupiter on a high eccentricity<\/strong> and high inclination retrograde orbit.\n<\/p>\n <\/p>\n + Isonoe is about 3.8 kilometres in diameter, and orbits Jupiter at an average distance of 23,833,000km in 751.647 days, at an inclination of 166\u00b0 to the ecliptic, with an orbital eccentricity<\/strong> of 0.166.\n<\/p>\n <\/p>\n + Aoede is about in 714.657 days, at an inclination of 160\u00b0 to the ecliptic, with an eccentricity<\/strong> of 0.6012.\n<\/p>\n <\/p>\n + Mercury has the most eccentric orbit of all the planets; its eccentricity<\/strong> is 0.21.\n<\/p>\n <\/p>\n + Kore is about 2 kilometers in diameter, and orbits Jupiter at an average distance of 23,239,000km in 723.720 days, at an inclination of 141\u00b0 to the ecliptic, with an orbital eccentricity<\/strong> of 0.2462.\n<\/p>\n <\/p>\n + Helike is about 4 kilometres in diameter, and orbits Jupiter at an average distance of 20,540,000km in 601.402 Earth days, at an inclination of 155\u00b0 to the ecliptic, with an orbital eccentricity<\/strong> of 0.1375.\n<\/p>\n <\/p>\n + S\/2004 S 12 is about 5 kilometres in diameter, and orbits Saturn at an average distance of 19,906,000km in 1048.541 days, at an inclination of 164\u00b0 to the ecliptic, with an eccentricity<\/strong> of 0.396.\n<\/p>\n <\/p>\n + Aitne is about 3kilometres in diameter, and orbits Jupiter at an average distance of 22,285,000km in 679.641 days, at an inclination of 166\u00b0 to the ecliptic, with an orbital eccentricity<\/strong> of 0.393.\n<\/p>\n <\/p>\n + S\/2004 S 7 is about 6 kilometres in diameter, and orbits Saturn at an average distance of 20,577,000km in 1101.989 days, at an inclination of 166\u00b0 to the ecliptic, with an eccentricity<\/strong> of 0.554.\n<\/p>\n <\/p>\n + The orbit of Thebe has an orbital eccentricity<\/strong> of ~0.018 and an inclination of ~1.08\u00b0 relative to the equator of Jupiter.\n<\/p>\n <\/p>\n + The orbit is at an inclination of 49.90\u00b0, with an eccentricity<\/strong> of 0.1081.\n<\/p>\n <\/p>\n + S\/2004 S 17 is about 4 kilometres in diameter, and orbits Saturn at an average distance of 19,099,000km in 985.453 days, at an inclination of 167\u00b0 to the ecliptic, with an eccentricity<\/strong> of 0.226.\n<\/p>\n <\/p>\n + Autonoe is about 4kilometres in diameter, and orbits Jupiter at an average distance of 24,264,000km in 772.168 days, at an inclination of 151\u00b0 to the ecliptic, with an orbital eccentricity<\/strong> of 0.369.\n<\/p>\n <\/p>\n + Mundilfari is about 5.6 kilometres in diameter, and orbits Saturn at an average distance of 18,360,000km in 928.806 days, at an inclination of 170\u00b0 to the ecliptic, with an eccentricity<\/strong> of 0.198.\n<\/p>\n <\/p>\n + Although its very high orbital eccentricity<\/strong> means its opposition magnitude varies a lot, at a rare opposition near perihelion Bamberga can reach a magnitude of +8.0, which is as bright as Saturn’s moon Titan.\n<\/p>\n <\/p>\n + Hegemone is about 3 kilometres in diameter, and orbits Jupiter at an average distance of 23,703,000km in 745.500 days, at an inclination of 153\u00b0 to the ecliptic, with an orbital eccentricity<\/strong> of 0.4077.\n<\/p>\n <\/p>\n + Megaclite is about 5.4 kilometres in diameter, and orbits Jupiter at an average distance of 24,687,000km in 792.437 days, at an inclination of 150\u00b0 to the ecliptic, with an orbital eccentricity<\/strong> of 0.308.\n<\/p>\n <\/p>\n + Kale is about 2 kilometres in diameter, and orbits Jupiter at an average distance of 22,409,000 km in 685.324 days, at an orbital inclination of 165\u00b0 to the ecliptic, with an eccentricity<\/strong> of 0.2011.\n<\/p>\n <\/p>\n + While such methods have been performed on the planet after its discovery, they have not yet detected what the orbital eccentricity<\/strong> of the planet actually is, and have as of March 2012 only set an upper limit on the mass of the planet.\n<\/p>\n <\/p>\n + Its orbit is much closer to the plane of the ecliptic than those of Ceres, Pallas or Interamnia, but is less circular than Ceres or Vesta with an eccentricity<\/strong> of around 12%.\n<\/p>\n <\/p>\n + Kallichore is about 2 kilometres in diameter, and orbits Jupiter at an average distance of 23,112,000km in 717.806 days, at an inclination of 165\u00b0 to the ecliptic, with an orbital eccentricity<\/strong> of 0.2042.\n<\/p>\n <\/p>\n![\"In](\"https:\/\/englishteststore.net\/blog\/wp-content\/uploads\/2021\/09\/In-sentence-examples-of-eccentricity.jpg\" "\\"In")
Example sentences of “eccentricity”:<\/h2>\n
+ Chaldene is about 3.8 kilometres in diameter, and orbits Jupiter at an average distance of 22,713,000km in 699.327 days, at an inclination of 167\u00b0 to the ecliptic, with an orbital eccentricity<\/strong> of 0.2916.\r\n
+ Euporie is about 2 kilometres in diameter, and orbits Jupiter at an average distance of 19,088,000km in 538.780 days, at an inclination of 145\u00b0 to Jupiter's equator, with an orbital eccentricity<\/strong> of 0.0960.\r\n
+ Ymir is about 16 kilometres in diameter, and orbits Saturn at an average distance of 23,175,000km in 1317.137 days, at an inclination of 172\u00b0 to the ecliptic, with an eccentricity<\/strong> of 0.358.\r\n
<\/pre>\nMore in-sentence examples of “eccentricity”:<\/h2>\n
+ The eccentricity<\/strong> of the orbits is represented by the yellow segments with the inclination represented on Y axis.\r\n
+ Callirrhoe is about 8.6 kilometres in diameter, and orbits Jupiter at an average distance of 24,356,000km in 776.543 days, at an inclination of 141\u00b0 to the ecliptic, with an orbital eccentricity<\/strong> of 0.264.\r\n
+ Taygete is about 5 kilometres in diameter, and orbits Jupiter at an average distance of 22,439,000km in 686.675 days, at an inclination of 165\u00b0 to the ecliptic, with an orbital eccentricity<\/strong> of 0.3678.\r\n
<\/pre>\n