
Uranus may have two small moons that no one has ever seen, orbiting closer to the planet than any of its other satellites and making wavy patterns in the planetās rings.
The ice giant has 27 known moons, far fewer than the 67 and 62 of its neighbours Jupiter and Saturn, respectively. Uranus is a smaller planet, which may explain the difference.
But it might just be that we havenāt previously had a chance to look for more moons. Unlike its larger brethren, Uranus has entertained only one passing spacecraft ā Voyager 2, which tripled the number of known Uranian moons in its 1986 flyby. Uranus is also yet to receive an orbiting spacecraft like Jupiterās Galileo and Juno, or Saturnās Cassini.
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In addition to its moons, Uranus has dark, narrow rings. Scientists detected the first of these in 1977, when the planet and its rings blocked the light from a distant star. Voyager 2 later discovered two moons, Cordelia and Ophelia, on either side of the outermost ring, named Epsilon. The gravitational pulls of the two moons herd the ringās particles into a narrow formation.
Small, dark satellites
Now planetary scientists Rob Chancia and at the University of Idaho in Moscow have re-examined Voyager data and discovered wavy patterns in two other rings, Alpha and Beta. These may similarly arise from the gravitational tug of a moon that lies outside each ring.
āThese moons are pretty tiny,ā says Chancia, at only 4 to 14 kilometres across if they exist. That means theyāre probably smaller than any Uranian satellite known ā and too diminutive for Voyager to have seen clearly. Still, at least four of Saturnās moons are even smaller.
The two putative moons are probably dark, based on the colours of their neighbours. āNot only are Uranusās rings dark, so are most of the little satellites that are in that region,ā says Hedman.
The existence of the two moons is ācertainly a very plausible possibilityā, says of the SETI Institute in Mountain View, California, who has discovered moons around Saturn, Uranus, Neptune and Pluto.
In the coming months, Showalter and his colleagues will examine observations of Uranus by the Hubble Space Telescope, which spotted Plutoās four smallest moons years before the New Horizons spacecraft visited in 2015. He calls Hubble āthe best betā for finding the Uranian satellites, adding that characterising their orbits is very useful.
If a Hubble search fails, a Uranus orbiter could someday succeed ā or else rule out the moonsā existence altogether. āThat would definitely be a good way to do it,ā says Hedman.
Journal reference:Ā The Astronomical Journal, in press,
Update [17 October]: An earlier version of this article said the paper was in press in the Astrophysical Journal, when it is actually the Astronomical Journal. This has been corrected.