Moons
Moons

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Moons

3.3.3 The moons of asteroids

Find out about some moons of asteroids seen by spacecraft that have flown past, seen by optical telescopes and even imaged by radar when they pass very close to the Earth.

In March 2014 a particularly surprising discovery was announced concerning moons of asteroids. Seven southern hemisphere telescopes monitored a predicted occultation (hiding) of a star by the asteroid 10199 Chariklo, which is a 250 km diameter icy asteroid orbiting beyond Saturn (it belongs to a class of bodies known as Centaurs). The observations of this rare event were intended to refine our knowledge of Chariklo’s size and shape (which they did). However, the light from the star dimmed twice very briefly a few seconds before the main occultation, and did so again a few seconds after. This shows that Chariklo has two rings (perhaps formed of debris resulting from a collision), 7 km and 3 km wide and separated by a 9 km gap. This is the first known ring system round anything other than a giant planet. Moreover, the only known way to confine the ring system so tightly is if Chariklo also has at least one shepherd moon, analogous to Saturn’s Pan and Prometheus. Read more and see an artist’s impression of Chariklo and its rings [Tip: hold Ctrl and click a link to open it in a new tab. (Hide tip)] .

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It's not only planets and dwarf planets that can have moons - asteroids can have moons too. Images from the Galileo mission's 1993 flyby of the 54 km-long asteroid 243 Ida revealed that it has a moon, less than 2 km in size, orbiting it. This moon, later named Dactyl, was the first confirmed moon of an asteroid.
Observing the orbit of the small moon Dactyl gives astronomers information on Ida's mass and density. This information can tell us about the composition of the primary body that we couldn't get otherwise. For example, whether it's solid rock or a low-density pile of rubble.
More and more examples of moons orbiting an asteroid are being discovered. When the asteroid 1998 QE2 passed near to Earth on the 29th of May, 2013, radar images showed a small moon orbiting it. The asteroid 1998 QE2 is about 2.7 km wide, whereas its moon is only about 600 m across. The moon takes 32 hours to complete an orbit at a distance of about 6 km
When the primary body and orbiting moon are about the same size, the system is described as a binary system. One example of this is the double asteroid 90 Antiope, where each asteroid of the pair is between 80 km and 90 km across. Antiope has never been visited by a spacecraft, so we have to content ourselves with what can be seen using telescopes, such as this sequence of eight frames recorded by the Keck telescope in Hawaii.
More than 80 asteroids in the asteroid belt have been observed to have moons, and five of them have two moons. The asteroid 87 Sylvia is one of the largest asteroids in the asteroid belt, and was the first known triple asteroid system. Its two moons have been named Romulus and Remus, after the mythical founders of Rome. By analysing their orbits, the main asteroid was found to have a very low density.
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Another moon of a near-Earth asteroid, even smaller than the moon of 1998 QE2 that you saw in the video, was discovered using radar on 26 January 2015 when the 325 m asteroid 2004 BL86 passed at a distance of only 1.2 million km. Its moon is about 70 m in size making it the new record holder for the smallest known moon.

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