Uranus is the next planet out from Saturn and the one in from Neptune, and at magnitude 5.7 it is two magnitudes brighter than Neptune: 6 times the light. It is in Taurus this year, six and a half degrees from the Pleiades.
Uranus only came into eclipticam's view on 21 September, near the top of the frame for the last quarter of an hour before dawn. Each night it is in view a few minutes longer: two hours by 10 October, and about five hours a night from November to early February. Opposition, when it is opposite the Sun and up all night, is about 23 November.
Of the 19 nights since it came into view, 9 were clear enough before dawn to stack. Uranus is in every one of them, between 5 and 46 sigma, and typically 1.3 arcminutes from where the ephemeris puts it. The early nights are only 5 or 6 frames; the clearest October mornings give 30 to 70.
Uranus stood still against the stars on about 10 September, and has been going backwards (westwards) since, as Earth comes round to overtake it. In the 18 nights here it moved 18 arcminutes, a little more than half a Moon.
That is barely longer than the smear of one exposure: in 60 seconds every star, and Uranus, trails about 14 arcminutes east to west at this declination. So far the walk is short, but it is speeding up. By early February it will have gone back about 3.5 degrees, and then it will stop and turn again.
Uranus's disc is 3.7 arcseconds across. An eclipticam v3w photosite covers 1.8 arcminutes at the centre of the frame, 30 times wider, so here Uranus is a point, like a star. What gives it away is that it moves.