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 ? 10?5 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 (x e ; 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)
FindtheazimuthAandelevationhofUranusattimet,asseenfromWashington
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.)
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