[meteorite-list] Kuiper Belt Moons Are Starting to Seem Typical

From: Ron Baalke <baalke_at_meteoritecentral.com>
Date: Fri Jan 13 12:49:02 2006
Message-ID: <200601131714.k0DHEXn13051_at_zagami.jpl.nasa.gov>

Media Relations
Caltech
Pasadena, California

Contact:
Robert Tindol, (626) 395-3631

January 10, 2006

Kuiper Belt Moons Are Starting to Seem Typical

WASHINGTON, D.C. -- In the not-too-distant past, the planet Pluto was
thought to be an odd bird in the outer reaches of the solar system because
it has a moon, Charon, that was formed much like Earth's own moon was
formed. But Pluto is getting a lot of company these days. Of the four
largest objects in the Kuiper belt, three have one or more moons.

"We're now beginning to realize that Pluto is one of a small family of
similar objects, nearly all of which have moons in orbit around them,"
says Antonin Bouchez, a California Institute of Technology astronomer.

Bouchez discussed his work on the Kuiper belt Tuesday, January 10, at the
winter meeting of the American Astronomical Society (AAS).

Bouchez says that the puzzle for planetary scientists is that, as a whole,
the hundreds of objects now known to inhabit the Kuiper belt beyond the
orbit of Neptune have only about an 11 percent chance of possessing their
own satellites. But three of the four largest objects now known in the
region have satellites, which means that different processes are at work
for the large and small bodies.

Experts have been fairly confident for a decade or more that Pluto's moon
Charon was formed as the result of an impact, but that the planet seemed
unique in this. According to computer models, Pluto was hit by an object
roughly one-half its own size, vaporizing some of the planet's material. A
large piece, however, was cleaved off nearly intact, forming Pluto's moon
Charon.

Earth's moon is thought to have been formed in a similar way, though our
moon most likely formed out of a hot disk of material left in orbit after
such a violent impact.

Just in the last year, astronomers have discovered two additional moons
for Pluto, but the consensus is still that the huge Charon was formed by a
glancing blow with another body, and that all three known satellites -- as
well as anything else not yet spotted from Earth -- were built up from the
debris.

As for the other Kuiper belt objects, experts at first thought that the
bodies acquired their moons only occasionally by snagging them through
gravitational capture. For the smaller bodies, the 11 percent figure would
be about right.

But the bigger bodies are another story. The biggest of all -- and still
awaiting designation as the tenth planet -- is currently nicknamed "Xena."
Discovered by Caltech's Professor of Planetary Science Mike Brown and his
associates, Chad Trujillo of the Gemini Observatory and David Rabinowitz
of Yale University, Xena is 25 percent larger than Pluto and is known to
have at least one moon.

The second-largest Kuiper belt object is Pluto, which has three moons and
counting. The third-largest is nicknamed "Santa" because of the time of
its discovery by the Mike Brown team, and is known to have two moons.

"Santa is an odd one," says Bouchez. "You normally would expect moons to
form in the same plane because they would have accreted from a disk of
material in orbit around the main body.

"But Santa's moons are 40 degrees apart. We can't explain it yet."

The fourth-largest Kuiper belt object is nicknamed "Easterbunny" -- again,
because of the time the Brown team discovered it -- and is not yet known
to have a moon. But in April, Bouchez and Brown will again be looking at
Easterbunny with the adaptive-optics rig on one of the 10-meter Keck
telescopes, and a moon might very well turn up.

The search for new planets and other bodies in the Kuiper belt is funded
by NASA. For more information on the program, see the Samuel Oschin
Telescope's website at
     http://www.astro.caltech.edu/palomarnew/sot.html

For more information on Mike Brown's research, see
     http://www.gps.caltech.edu/~mbrown

For more information on the Keck laser-guide-star adaptive optics system,
see
     http://www2.keck.hawaii.edu/optics/lgsao/
Received on Fri 13 Jan 2006 12:14:32 PM PST