Sun and moon's orbit in ecliptic coordinates using skyfield I am new to using skyfield, is there any doc or help file that can show me on how to get the orbit of Sun and moon in ecliptic coordinate for a particular date and time. This is a follow up question of this question
I cant help you with skyfield, but i usually use JPL Horizons Web interface. No installation required, you can also print it in a text file if you want:

https://ssd.jpl.nasa.gov/horizons.cgi

Otherwise i found the documentation for skyfield:
https://rhodesmill.org/skyfield/toc.html

And if nothing of that works, i made a little astropy script for you

from astropy import units as u
from astropy.coordinates import SkyCoord, EarthLocation, AltAz, get_body
from astropy.time import Time
import numpy as np

# Create 1000 Timepoints between Time 1 and Time 2 (one year later)
t = np.linspace(2451545, 2451545+365, 1000)


pointlist = []

#Loop through this times
for tn in t:
    # For every timepoint, create an astropy_time object
    astropy_time = Time(tn, format="jd")
    # Get Planet (as string, "earth", "moon", "mercury" etc. in aequatorial coordinates
    planet_aequatorial = get_body("moon", time = astropy_time)
    #Transform to Barycentric True Ecliptic (relative to the center of mass of the solar system).
    planet_ecliptic =  planet_aequatorial.transform_to("barycentrictrueecliptic")

    # Add a point to the orbit. Every point is described as (longitude [deg], latitude (ecliptic coords), distance (km))
    pointlist.append([planet_ecliptic.lon.deg, planet_ecliptic.lat.deg, planet_ecliptic.distance.km])
    print(planet_ecliptic.distance.km)
    # So pointslist is a 2D array. The rows are all the 1000 points of the orbit

# In every point there is 3 columns for [Long, Lat, Distance]
print(pointlist)


# You can also save the result with
pointlist = np.array(pointlist)


np.save("results.npy", pointlist)