Find the position of the planet Uranus at time t D December 4, 2019, 8:00 pm EST. You will do this by following the steps shown below.
(a) Convert the time t to Universal Time (just add 5 hours to EST).
(b) Find the Julian day corresponding to time t (using the result of part (a)).
(c) Find the time elapsed from the epoch time to time t (i.e., find t T0).
(d) Find the mean daily motion n (using Kepler’s Third Law, Eq. 1). (Ans. n D 3:267686 105 rev/day)
(e) Find the mean anomaly M of Uranus at time t (Eq. 2).
(f) Solve Kepler’s equation (Eq. 3) to find the eccentric anomaly E of Uranus at time t. See Section 3 for information on solving Kepler’s Equation.
(g) Find the true anomaly f of Uranus at time t (Eq. 4).
(h) Find the distance r of Uranus from the Sun at time t (Eq. 5).
(i) Find the argument of latitude u of Uranus at time t (Eq. 6).
(j) Find the heliocentric ecliptic cartesian coordinates of Uranus at time t (x; y; z) (Eqs. 7–9).
(k) Find the geocentric ecliptic cartesian coordinates of Uranus at time t (xe; ye; ze) (Eqs. 10–12).
(l) Find the ecliptic longitude and ecliptic latitude ˇ of Uranus at time t (Eqs. 13–14).
(m) Find the right ascension ˛ and declination ı of Uranus at time t (Eqs. 15–16).
(n) Find the Greenwich sidereal time GST for time t at Washington D.C. (Eq. 17)
(o) Find the local hour angle H. (Eq. 18)
(p) Find the azimuth A and elevation h of Uranus at time t, as seen from Washington D.C. (Eqs. 19–20) Is Uranus above the horizon (h>0)? If so, you may wish to go outside and see if you can see it at the place you predict it to be. (You will need a telescope.)
Find the position of the planet Uranus at time t D December 4, 2019, 8:00 pm...