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Uranus as seen at 9 PM mid-month from 40N, looking south. The star of similar brightness to the right of Uranus is Zeta Psc.

In November 2016 the planet Uranus is well placed for evening observation, fairly high in the sky at around 9 PM. It is in Pisces, shining at magnitude 5.7, just to the east of the 5th-magnitude faint naked-eye star Zeta Psc. 

Uranus was not known in ancient times, presumably because it is not detectable to the naked eye throughout the year. But from a dark site at the right time it is just detectable to the eye, and right now is perfect. 

Not many people can say that they have spotted Uranus with their unaided eye, and this may be your best chance. Start by going outside on a dark moonless night before 9 PM. Make sure there are no lights nearby. Enjoy the sky for about a half hour to let your eyes fully adapt to the dark. Don't use a phone, flashlight (unless it has a red light), or run inside for a snack. Bring a pair of binoculars if you have them. 

Start by identifying the bright stars in the chart above. The bright star near the center is Beta Cet. Alpha Cet is the bright star to the upper left. Once you have spotted these two stars you should be able to navigate to Uranus. If you can't spot the pair of "stars" that are Uranus and Zeta Psc, try your binoculars. The trick with binoculars is to fix your eyes on the area of the sky where you want to look, then while holding your gaze fixed, bring the binoculars up to your eyes. Look for a pair of "stars" as shown below. Uranus should stand out because of its odd blue-green color. In the chart below the bright stars are labeled with their lower-case Greek letters, starting with Mu on the left, Zeta (to the right of Uranus), Epsilon, and finally Delta on the far right.

Once you have spotted Uranus in your binoculars, try keeping your eyes fixed on the spot and lowering the binoculars. Look again with you unaided eye for the side-by-side pair of stars.

Uranus was officially discovered by William Herschel in England on the night of March 13, 1781. Herschel was a musician by trade, but he spent his nights surveying the sky. He wrote, "In examining the small stars in the neighborhood of H Geminorum I perceived one that appeared visibly larger than the rest..." Herschel's discovery was by no means an accident. He built the largest telescopes of the day--the first practical application of the reflecting telescope invented by Newton. Assisted by his sister Caroline, Herschel set out to observe every star in the sky. As he put it, "In a regular manner I examined every star in the heavens and that night it was its turn to be discovered." 

In the telescope, use as much magnification as the conditions will bear to see Uranus's featureless tiny blue-green disk. At higher magnifications any telescope will reveal more than a mere star.

Observing the Moons of Uranus


Uranus has 27 moons discovered to date, five of which can be observed from earth. Of those five, the four largest are visible in amateur instruments. The two outer moons, Titania and Oberon, are each about 1600 km in diameter, about half that of Earth's Moon. The two inner satellites are smaller, about 1200 km in diameter. The moons of Uranus are unique in that their names pay homage to the works of Shakespeare and Alexander Pope. 

Unlike the other planets, Uranus is very highly tilted with respect to its orbit; it lies nearly on its side, tilted by some 98o

The moons will appear as faint stars near the planet. Their orbits are tilted such that they trace a wide, egg-shaped path. They are best observed when farthest from the planet, which occurs when they are to the north or south of it, although they can often be observed at other times as well.

To spot the tiny satellites, use high magnification, and wait for moments of good seeing. Try averted vision--experiment with looking away from the planet and trying to spot them with your peripheral vision, which is more sensitive to faint objects.

Darker skies and an eight-inch (20 cm) telescope will be required to spot the two outer moons, Titania and Oberon. A 16-inch (41 cm) telescope is required to spot the two inner moons, Ariel and Umbriel.

Satellite Separation (arc-sec) Magnitude
Titania 17 - 31 13.9
Oberon 23 - 42 14.1
Ariel 7 - 14 14.4
Umbriel 10 - 19 15.0
Miranda 4 - 9 16.5

For best results, use software to plot the positions of the moons before you go out to observe them. Remember, they are easiest when away from the glare of the planet. More advanced software, such as my SkyTools 3, will compute the times when the satellites are farthest from the planet for you. 

Uranus will close on nearby Zeta Psc until late December, when it will be 35 arc-minutes away. After that it will begin moving back in the direction that it came from. 

SkyTools 3 was used in the preparation of this article. 

 Greg Crinklaw — Developer of SkyTools 

SkyTools 3, because the astronomy matters.

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