<\/p>\n
+ Nessus finishes one orbit around the Sun in 122.4 years, an eccentricity of 0.52 and an inclination to the ecliptic<\/strong> of 15.6 degrees.\n<\/p>\n <\/p>\n + The most detailed analysis indicates that it points either towards about ecliptic<\/strong> coordinates with a 10\u00b0 uncertainty.\n<\/p>\n <\/p>\n + The plane of the Earth’s orbit around the Sun is called the ecliptic<\/strong> plane.\n<\/p>\n <\/p>\n + In particular, two planets are in opposition to each other when their ecliptic<\/strong> longitudes differ by 180\u00b0.\n<\/p>\n <\/p>\n + The ecliptic<\/strong> plane should be distinguished from the invariable plane.\n<\/p>\n <\/p>\n + The fundamental plane is the plane of the Earth’s orbit, also called the ecliptic<\/strong> plane.\n<\/p>\n <\/p>\n + Lightcurve analysis indicates that Massalia’s pole points towards either ecliptic<\/strong><\/strong> coordinate systemecliptic<\/strong><\/strong> coordinates with a 10\u00b0 uncertainty.\n<\/p>\n + The present ecliptic<\/strong><\/strong> plane is inclined to the invariable ecliptic<\/strong><\/strong> plane by about 1.5\u00b0.\n<\/p>\n <\/p>\n + Recent lightcurve analysis indicates that its pole points towards either ecliptic<\/strong><\/strong> coordinate systemecliptic<\/strong><\/strong> coordinates with a 10\u00b0 uncertainty.\n<\/p>\n <\/p>\n + This orbit is at an inclination of 143\u00b0 to the ecliptic<\/strong> with an orbital eccentricity of 0.2001.\n<\/p>\n <\/p>\n + The angle of the Earth’s axial tilt varies with respect to the ecliptic<\/strong> plane, because perturbations from other planets shift the Earth’s orbit.\n<\/p>\n <\/p>\n + It is a retrograde rotator, although its pole points almost parallel to the ecliptic<\/strong><\/strong> towards ecliptic<\/strong><\/strong> coordinates with a 10\u00b0 uncertainty.\n<\/p>\n <\/p>\n + For a planet’s orbit, the inclination is the angle to the ecliptic<\/strong> plane.\n<\/p>\n <\/p>\n + As a result of the Earth’s axial tilt, the celestial equator is inclined by 23.4\u00b0 with respect to the ecliptic<\/strong> plane.\n<\/p>\n <\/p>\n + Mneme is about 2 kilometres in diameter, and orbits Jupiter at an average distance of 21,427,000 km in 640.769 days, at an inclination of 149\u00b0 to the ecliptic<\/strong> with an orbital eccentricity of 0.2214.\n<\/p>\n <\/p>\n + It is easily the biggest of the F-type asteroids, but there are few details of what the inside is made of or shape and no lightcurve analysis has been done to find out the ecliptic<\/strong> coordinates of Interamnia’s poles.\n<\/p>\n <\/p>\n + He observed that the ecliptic<\/strong> plane is inclined with respect to the celestial equator and more accurately calculated the length of the tropical year.\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<\/strong> with an eccentricity of 0.186.\n<\/p>\n <\/p>\n + There are two versions: the geocentric ecliptic<\/strong><\/strong> coordinates centred on the Earth, and heliocentric ecliptic<\/strong><\/strong> coordinates centred on the centre of mass of the solar system.\n<\/p>\n <\/p>\n + Its orbit is much closer to the plane of the ecliptic<\/strong> than those of Ceres, Pallas or Interamnia, but is less circular than Ceres or Vesta with an eccentricity of around 12%.\n<\/p>\n <\/p>\n + Iocaste orbits Jupiter at an average distance of 20,723,000km in 609.427 days, at an inclination of 147\u00b0 to the ecliptic<\/strong> with an orbital eccentricity of 0.2874.\n<\/p>\n <\/p>\n + The heliocentric ecliptic<\/strong> system describes the planets’ orbital movement around the Sun, and centres on the barycenter of the solar system.\n<\/p>\n <\/p>\n![\"Use](\"https:\/\/englishteststore.net\/blog\/wp-content\/uploads\/2021\/09\/Use-the-word-ecliptic.jpg\" "\\"Use")
Example sentences of “ecliptic”:<\/h2>\n
+ The present ecliptic<\/strong><\/strong> plane is inclined to the invariable ecliptic<\/strong><\/strong> plane by about 1.5\u00b0.\r\n
+ Recent lightcurve analysis indicates that its pole points towards either ecliptic<\/strong><\/strong> coordinate systemecliptic<\/strong><\/strong> coordinates with a 10\u00b0 uncertainty.\r\n
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