The earth's orbital time is approximately 1year or 365 days and a half.
elliptical.
Earths orbital inclination is 1.57869°
The year.
In astronomy, axial tilt, also known as obliquity, is the angle between an object's rotational axis and its orbital axis, or, equivalently, the angle between its equatorial plane and orbital plane. It differs from orbital inclination.
The Earths orbit is fairly un-eccentric when compared to the other planets, with only Neptune and Venus having more regular (less eccentric) orbits. The eccentricity of earths orbit is 0.0167, the closest to this is Neptune's, with a value of 0.00859
The primary factors affecting orbital time are the mass of the objects involved, the distance between them, and the gravitational force between them. Orbital time increases with greater mass or distance, and decreases with stronger gravitational forces. The velocity of the objects also plays a role in determining the orbital time.
The Earths orbital distance from the sun is 147,098,290km (91,402,641 miles) at its closest (Perihelion).
Orbital period is the time it takes a planet to go around its star once.
It is the time in which planets orbit the sun.
88 days
Jupiter's orbital period is only 1.53% less than1/7 the orbital period of Uranus.
The only thing the Earth orbits is the sun so the length of time it defines is 1 year. Hours, minutes and seconds were originally defined by the time it takes the Earth to spin on it's axis. One year can be expressed as hours, minutes and seconds but this time is gradually changing.