How to use in-sentence of “eccentricity”:
+ Unlike the Hilda asteroids whose eccentricity eccentricity is fairly common of main belt asteroids, Thule has a very low eccentricity – actually much lower than that of Jupiter itself and only a bit higher than that of Earth.
+ This is very similar to the 100,000 year eccentricity period.
+ In Mechanicsastrodynamics, orbital eccentricity shows how much the shape of an object’s orbit is different from a circle.
+ This orbit is at an inclination of 143° to the ecliptic with an orbital eccentricity of 0.2001.
+ 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° to the ecliptic, with an eccentricity of 0.320.
Example sentences of “eccentricity”:
+ 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° to the ecliptic, with an orbital eccentricity of 0.2916.
+ 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° to Jupiter’s equator, with an orbital eccentricity of 0.0960.
+ 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° to the ecliptic, with an eccentricity of 0.358.
+ Nessus finishes one orbit around the Sun in 122.4 years, an eccentricity of 0.52 and an inclination to the ecliptic of 15.6 degrees.
+ 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° to the ecliptic, with an eccentricity of 0.261.
+ The orbital period is about 16.50 hours, the eccentricity below 0.03.
+ The diagram illustrates the orbital parameters of the retrograde non-spherical moons of Uranus with the eccentricity of the orbits represented by the segments extending from the pericentre to the apocentre.
+ 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° to the ecliptic, with an eccentricity of 0.131.
+ The high orbital eccentricity of Pluto puts it mostly outside Neptune’s orbit, but partly inside.
+ Its orbit has an eccentricity of 0.13.
+ 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° to the ecliptic, with an eccentricity of 0.152.
+ Around that time, the eccentricity of the seven-member group finally began to become a hot topic in the news and headlines.
+ The orbital eccentricity of ~0.0015 and inclination of ~ 0.03° relative to the equator of Jupiter are very small.
+ 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° to the ecliptic, with an orbital eccentricity of 0.2916.
+ 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° to Jupiter's equator, with an orbital eccentricity of 0.0960.
+ 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° to the ecliptic, with an eccentricity of 0.358.
More in-sentence examples of “eccentricity”:
+ The eccentricity of the orbits is represented by the yellow segments with the inclination represented on Y axis.
+ 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° to the ecliptic, with an orbital eccentricity of 0.264.
+ 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° to the ecliptic, with an orbital eccentricity of 0.3678.
+ The eccentricity of the orbits is represented by the yellow segments with the inclination represented on Y axis.
+ 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° to the ecliptic, with an orbital eccentricity of 0.264.
+ 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° to the ecliptic, with an orbital eccentricity of 0.3678.
+ Its eccentricity is 0.4104.
+ Ananke orbits Jupiter on a high eccentricity and high inclination retrograde orbit.
+ The eccentricity of the orbits is represented by the yellow segments extending from the pericentre to the apocentre.
+ 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° to the ecliptic, with an eccentricity of 0.4710.
+ 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° to the ecliptic with an eccentricity of 0.186.
+ 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° to the ecliptic, with an eccentricity of 0.2290.
+ 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° to the ecliptic, with an eccentricity of 0.3604.
+ 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° to the ecliptic, with an orbital eccentricity of 0.2140.
+ The potentially brightest C-type asteroid is 324 Bamberga, but that object’s very high eccentricity means it rarely reaches its maximum magnitude.
+ The eccentricity of this ellipse is exaggerated for visualization.
+ Different SDOs have different orbital eccentricity and orbital inclination.
+ 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° to the ecliptic, with an orbital eccentricity of 0.2552.
+ 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 of the orbits represented by the segments extending from the pericentre to the apocentre.
+ 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° to the ecliptic, with an eccentricity of 0.453.
+ The eccentricity of selected orbits is represented by the yellow segments.
+ 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° to the ecliptic, with an orbital eccentricity of 0.2829.
+ 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° to the ecliptic, with an orbital eccentricity of 0.3289.
+ Sinope orbits Jupiter on a high eccentricity and high inclination retrograde orbit.
+ 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° to the ecliptic, with an orbital eccentricity of 0.166.
+ Aoede is about in 714.657 days, at an inclination of 160° to the ecliptic, with an eccentricity of 0.6012.
+ Mercury has the most eccentric orbit of all the planets; its eccentricity is 0.21.
+ 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° to the ecliptic, with an orbital eccentricity of 0.2462.
+ 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° to the ecliptic, with an orbital eccentricity of 0.1375.
+ 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° to the ecliptic, with an eccentricity of 0.396.
+ 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° to the ecliptic, with an orbital eccentricity of 0.393.
+ 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° to the ecliptic, with an eccentricity of 0.554.
+ The orbit of Thebe has an orbital eccentricity of ~0.018 and an inclination of ~1.08° relative to the equator of Jupiter.
+ The orbit is at an inclination of 49.90°, with an eccentricity of 0.1081.
+ 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° to the ecliptic, with an eccentricity of 0.226.
+ 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° to the ecliptic, with an orbital eccentricity of 0.369.
+ 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° to the ecliptic, with an eccentricity of 0.198.
+ Although its very high orbital eccentricity 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.
+ 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° to the ecliptic, with an orbital eccentricity of 0.4077.
+ 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° to the ecliptic, with an orbital eccentricity of 0.308.
+ 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° to the ecliptic, with an eccentricity of 0.2011.
+ While such methods have been performed on the planet after its discovery, they have not yet detected what the orbital eccentricity of the planet actually is, and have as of March 2012 only set an upper limit on the mass of the planet.
+ 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 of around 12%.
+ 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° to the ecliptic, with an orbital eccentricity of 0.2042.
+ Suttungr is about 5.6 kilometres in diameter, and orbits Saturn at an average distance of 19,667,000km in 1029.703 days, at an inclination of 174° to the ecliptic, with an eccentricity of 0.131.
+ Bestla is about 7 kilometres in diameter, and orbits Saturn at an average distance of 19,959,000km in 1052.722 days, at an inclination of 147° to the ecliptic, with an eccentricity of 0.772.
+ Orbital eccentricity measures the flatness of the orbit.
+ Carpo is about 3 kilometres in diameter, and orbits Jupiter at an average distance of 17,145,000km in 458.625 days, at an inclination of 56° to the ecliptic, and with an orbital eccentricity of 0.2736.
+ Sponde is about 2 kilometres in diameter, and orbits Jupiter at an average distance of 24,253,000km in 771.604 days, at an inclination of 154° to the ecliptic, with an orbital eccentricity of 0.443.