How to use in-sentence of “ecliptic”:
+ It will also come very close to being at the same point since the 1846 discovery in late October through early-mid November 2010, when Neptune will turn from retrograde to direct motion on the exact degree of Neptune’s discovery and will then stop for a moment along the ecliptic within 2 arc minutes at that point.
+ 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.
+ The most detailed analysis indicates that it points either towards about ecliptic coordinates with a 10° uncertainty.
+ The plane of the Earth’s orbit around the Sun is called the ecliptic plane.
+ In particular, two planets are in opposition to each other when their ecliptic longitudes differ by 180°.
+ The ecliptic plane should be distinguished from the invariable plane.
+ The fundamental plane is the plane of the Earth’s orbit, also called the ecliptic plane.
+ Lightcurve analysis indicates that Massalia’s pole points towards either ecliptic coordinate systemecliptic coordinates with a 10° uncertainty.
Example sentences of “ecliptic”:
+ The present ecliptic plane is inclined to the invariable ecliptic plane by about 1.5°.
+ Recent lightcurve analysis indicates that its pole points towards either ecliptic coordinate systemecliptic coordinates with a 10° uncertainty.
+ The present ecliptic plane is inclined to the invariable ecliptic plane by about 1.5°.
+ Recent lightcurve analysis indicates that its pole points towards either ecliptic coordinate systemecliptic coordinates with a 10° uncertainty.
+ This orbit is at an inclination of 143° to the ecliptic with an orbital eccentricity of 0.2001.
+ The angle of the Earth’s axial tilt varies with respect to the ecliptic plane, because perturbations from other planets shift the Earth’s orbit.
+ It is a retrograde rotator, although its pole points almost parallel to the ecliptic towards ecliptic coordinates with a 10° uncertainty.
+ For a planet’s orbit, the inclination is the angle to the ecliptic plane.
+ As a result of the Earth’s axial tilt, the celestial equator is inclined by 23.4° with respect to the ecliptic plane.
+ 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° to the ecliptic with an orbital eccentricity of 0.2214.
+ 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 coordinates of Interamnia’s poles.
+ He observed that the ecliptic plane is inclined with respect to the celestial equator and more accurately calculated the length of the tropical year.
+ 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.
+ There are two versions: the geocentric ecliptic coordinates centred on the Earth, and heliocentric ecliptic coordinates centred on the centre of mass of the solar system.
+ 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%.
+ Iocaste orbits Jupiter at an average distance of 20,723,000km in 609.427 days, at an inclination of 147° to the ecliptic with an orbital eccentricity of 0.2874.
+ The heliocentric ecliptic system describes the planets’ orbital movement around the Sun, and centres on the barycenter of the solar system.
+ Lightcurve analysis indicates that Eugenia’s pole most likely points towards ecliptic coordinate systemecliptic coordinates with a 10° uncertainty, which gives it an axial tilt of 117°.
+ The geocentric ecliptic system was the principal coordinate system for ancient astronomy and is still useful for computing the apparent motions of the Sun, Moon, and planets.
+ Study of its light curve shows that Camilla’s geographical polepole probably points towards ecliptic coordinates with a 10° uncertainty, which gives it an axial tilt of 29°.
+ Skathi is about 6.4 kilometres in diameter, and orbits Saturn at an average distance of 15,576,000km in 725.784 days, at an inclination of 149° to the ecliptic with an eccentricity of 0.246.
+ The orbital inclinations of comets are usually high and not near the ecliptic where most solar system objects are found.