A Moon for Xena

by | Oct 3, 2005 | Outer Solar System

Everyone is calling 2003 UB313, the Solar System’s 10th planet, Xena. The name comes from a TV warrior princess of whom the curmudgeonly Centauri Dreams, never one for television, was utterly unaware. Now Xena has been found to have a moon, inevitably named Gabrielle after an equally incrutable character on the series (apparently the sidekick of Xena herself). One-tenth the size of Xena, Gabrielle is slated for further observations with the Hubble Space Telescope that will allow more accurate determination of its mass.

The advent of Gabrielle is good news for those wishing to learn more about Xena. From a California Institute of Technology press release quoting Michael Brown, the 10th planet’s discoverer:

“A combination of the distance of the moon from the planet and the speed it goes around the planet tells you very precisely what the mass of the planet is,” explains Brown. “If the planet is very massive, the moon will go around very fast; if it is less massive, the moon will travel more slowly. It is the only way we could ever measure the mass of Xena-because it has a moon.”

Xena and its moonGiven the distances involved (Xena is now some 97 AU from the Sun, or 9 billion miles), it’s intriguing to learn how the moon was spotted. The work was performed using adaptive optics at the Keck Observatory in Mauna Kea. The technology allowed Brown and colleagues to remove the blur of atmospheric turbulence to create images as sharp as those from space-based instruments. Keck uses a laser guide system that actually creates an artificial ‘star’ with a laser beam, bouncing its light off the atmosphere. This allows for the needed correction for atmospheric effects and an unprecedentedly clear view from a ground-based system.

Image: The discovery of the moon of the 10th planet from the W.M. Keck Observatory. The planet appears in the center, while the moon is the small dot at the 3 o’clock position. Credit: W.M. Keck Observatory.

Centauri Dreams‘ take: we keep finding moons around these odd outer system objects. In fact, 2003 EL61 was found to have a moon (also discovered by Brown using adaptive optics) in January, and we know that both Pluto and Xena have moons. All of which may force a reexamination of conventional views of gravitational capture, which is how such moons have been explained until now. It is possible that actual collisions between Kuiper Belt objects may emerge as the prime factor in their formation, although we clearly have just begun our study of this strange realm.

For more, see this page from Michael Brown’s Web site.

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In Centauri Dreams, Paul Gilster looks at peer-reviewed research on deep space exploration, with an eye toward interstellar possibilities. For many years this site coordinated its efforts with the Tau Zero Foundation. It now serves as an independent forum for deep space news and ideas. In the logo above, the leftmost star is Alpha Centauri, a triple system closer than any other star, and a primary target for early interstellar probes. To its right is Beta Centauri (not a part of the Alpha Centauri system), with Beta, Gamma, Delta and Epsilon Crucis, stars in the Southern Cross, visible at the far right (image courtesy of Marco Lorenzi).

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