[meteorite-list] Caltech Researchers Find Evidence of a Real Ninth Planet

From: lebofsky at lpl.arizona.edu <lebofsky_at_meteoritecentral.com>
Date: Wed, 20 Jan 2016 16:48:41 -0700
Message-ID: <5463cddcf601c71efcada45715aa9e3f.squirrel_at_webmail.lpl.arizona.edu>

Everyone:

At the time that Pluto was being "reclassified," Hal Levinson from SWRI
produced a figure that shows the mass that is need to "clear one's orbit"
at any given distance from the Sun. This can be due to either accretion or
scattering of objects. At Pluto's distance of 40 AU, an Earth-mass-sized
body would not be a planet by about a factor of 10. Beyond 200 AU, neither
Uranus or Neptune (15 and 17 times the mass of the Earth) would be large
enough to clear their orbits. At 20 times Neptune's distance from the Sun,
600 AU, an object would have to be something like 80 times the mass of the
Earth, nearly the mass of Saturn, to be able to clear its orbit.

So, if there is an object that is as big as they say and at the distance
the predict (this is just a mathematical model, not an actual discovery),
this object would just be a VERY BIG dwarf planet!!

Larry Lebofsky


>
> http://www.caltech.edu/news/caltech-researchers-find-evidence-real-ninth-planet-49523
>
> Caltech Researchers Find Evidence of a Real Ninth Planet
> Caltech
> January 20, 2016
>
> Caltech researchers have found evidence of a giant planet tracing a
> bizarre,
> highly elongated orbit in the outer solar system. The object, which the
> researchers have nicknamed Planet Nine, has a mass about 10 times that
> of Earth and orbits about 20 times farther from the sun on average than
> does Neptune (which orbits the sun at an average distance of 2.8 billion
> miles). In fact, it would take this new planet between 10,000 and 20,000
> years to make just one full orbit around the sun.
>
> The researchers, Konstantin Batygin and Mike Brown, discovered the
> planet's
> existence through mathematical modeling and computer simulations but have
> not yet observed the object directly.
>
> "This would be a real ninth planet," says Brown, the Richard and Barbara
> Rosenberg Professor of Planetary Astronomy. "There have only been two
> true planets discovered since ancient times, and this would be a third.
> It's a pretty substantial chunk of our solar system that's still out there
> to be found, which is pretty exciting."
>
> Brown notes that the putative ninth planet - at 5,000 times the mass of
> Pluto - is sufficiently large that there should be no debate about whether
> it is a true planet. Unlike the class of smaller objects now known as
> dwarf planets, Planet Nine gravitationally dominates its neighborhood
> of the solar system. In fact, it dominates a region larger than any of
> the other known planets - a fact that Brown says makes it "the most
> planet-y
> of the planets in the whole solar system."
>
> Batygin and Brown describe their work in the current issue of the
> Astronomical
> Journal and show how Planet Nine helps explain a number of mysterious
> features of the field of icy objects and debris beyond Neptune known as
> the Kuiper Belt.
>
> "Although we were initially quite skeptical that this planet could exist,
> as we continued to investigate its orbit and what it would mean for the
> outer solar system, we become increasingly convinced that it is out
> there,"
> says Batygin, an assistant professor of planetary science. "For the first
> time in over 150 years, there is solid evidence that the solar system's
> planetary census is incomplete."
>
> The road to the theoretical discovery was not straightforward. In 2014,
> a former postdoc of Brown's, Chad Trujillo, and his colleague Scott
> Sheppard
> published a paper noting that 13 of the most distant objects in the Kuiper
> Belt are similar with respect to an obscure orbital feature. To explain
> that similarity, they suggested the possible presence of a small planet.
> Brown thought the planet solution was unlikely, but his interest was
> piqued.
>
> He took the problem down the hall to Batygin, and the two started what
> became a year-and-a-half-long collaboration to investigate the distant
> objects. As an observer and a theorist, respectively, the researchers
> approached the work from very different perspectives - Brown as someone
> who looks at the sky and tries to anchor everything in the context of
> what can be seen, and Batygin as someone who puts himself within the
> context
> of dynamics, considering how things might work from a physics standpoint.
> Those differences allowed the researchers to challenge each other's ideas
> and to consider new possibilities. "I would bring in some of these
> observational
> aspects; he would come back with arguments from theory, and we would push
> each other. I don't think the discovery would have happened without that
> back and forth," says Brown. " It was perhaps the most fun year of working
> on a problem in the solar system that I've ever had."
>
> Fairly quickly Batygin and Brown realized that the six most distant
> objects
> from Trujillo and Shepherd's original collection all follow elliptical
> orbits that point in the same direction in physical space. That is
> particularly
> surprising because the outermost points of their orbits move around the
> solar system, and they travel at different rates.
>
> "It's almost like having six hands on a clock all moving at different
> rates, and when you happen to look up, they're all in exactly the same
> place," says Brown. The odds of having that happen are something like
> 1 in 100, he says. But on top of that, the orbits of the six objects are
> also all tilted in the same way - pointing about 30 degrees downward in
> the same direction relative to the plane of the eight known planets. The
> probability of that happening is about 0.007 percent. "Basically it
> shouldn't
> happen randomly," Brown says. "So we thought something else must be
> shaping
> these orbits."
>
> The first possibility they investigated was that perhaps there are enough
> distant Kuiper Belt objects - some of which have not yet been discovered -
> to
> exert the gravity needed to keep that subpopulation clustered together.
> The researchers quickly ruled this out when it turned out that such a
> scenario would require the Kuiper Belt to have about 100 times the mass
> it has today.
>
> That left them with the idea of a planet. Their first instinct was to
> run simulations involving a planet in a distant orbit that encircled the
> orbits of the six Kuiper Belt objects, acting like a giant lasso to
> wrangle
> them into their alignment. Batygin says that almost works but does not
> provide the observed eccentricities precisely. "Close, but no cigar,"
> he says.
>
> Then, effectively by accident, Batygin and Brown noticed that if they
> ran their simulations with a massive planet in an anti-aligned orbit - an
> orbit in which the planet's closest approach to the sun, or perihelion,
> is 180 degrees across from the perihelion of all the other objects and
> known planets - the distant Kuiper Belt objects in the simulation assumed
> the alignment that is actually observed.
>
> "Your natural response is 'This orbital geometry can't be right. This
> can't be stable over the long term because, after all, this would cause
> the planet and these objects to meet and eventually collide,'" says
> Batygin.
> But through a mechanism known as mean-motion resonance, the anti-aligned
> orbit of the ninth planet actually prevents the Kuiper Belt objects from
> colliding with it and keeps them aligned. As orbiting objects approach
> each other they exchange energy. So, for example, for every four orbits
> Planet Nine makes, a distant Kuiper Belt object might complete nine
> orbits.
> They never collide. Instead, like a parent maintaining the arc of a child
> on a swing with periodic pushes, Planet Nine nudges the orbits of distant
> Kuiper Belt objects such that their configuration with relation to the
> planet is preserved.
>
> "Still, I was very skeptical," says Batygin. "I had never seen anything
> like this in celestial mechanics."
>
> But little by little, as the researchers investigated additional features
> and consequences of the model, they became persuaded. "A good theory
> should
> not only explain things that you set out to explain. It should hopefully
> explain things that you didn't set out to explain and make predictions
> that are testable," says Batygin.
>
> And indeed Planet Nine's existence helps explain more than just the
> alignment
> of the distant Kuiper Belt objects. It also provides an explanation for
> the mysterious orbits that two of them trace. The first of those objects,
> dubbed Sedna, was discovered by Brown in 2003. Unlike standard-variety
> Kuiper Belt objects, which get gravitationally "kicked out" by Neptune
> and then return back to it, Sedna never gets very close to Neptune. A
> second object like Sedna, known as 2012 VP113, was announced by Trujillo
> and Shepherd in 2014. Batygin and Brown found that the presence of Planet
> Nine in its proposed orbit naturally produces Sedna-like objects by taking
> a standard Kuiper Belt object and slowly pulling it away into an orbit
> less connected to Neptune.
>
> [Graphic]
> A predicted consequence of Planet Nine is that a second set of confined
> objects should also exist. These objects are forced into positions at
> right angles to Planet Nine and into orbits that are perpendicular to
> the plane of the solar system. Five known objects (blue) fit this
> prediction
> precisely.
> Credit: Caltech/R. Hurt (IPAC) [Diagram was created using WorldWide
> Telescope.]
>
> But the real kicker for the researchers was the fact that their
> simulations
> also predicted that there would be objects in the Kuiper Belt on orbits
> inclined perpendicularly to the plane of the planets. Batygin kept finding
> evidence for these in his simulations and took them to Brown. "Suddenly
> I realized there are objects like that," recalls Brown. In the last three
> years, observers have identified four objects tracing orbits roughly along
> one perpendicular line from Neptune and one object along another. "We
> plotted up the positions of those objects and their orbits, and they
> matched
> the simulations exactly," says Brown. "When we found that, my jaw sort
> of hit the floor."
>
> "When the simulation aligned the distant Kuiper Belt objects and created
> objects like Sedna, we thought this is kind of awesome - you kill two
> birds with one stone," says Batygin. "But with the existence of the planet
> also explaining these perpendicular orbits, not only do you kill two
> birds,
> you also take down a bird that you didn't realize was sitting in a nearby
> tree."
>
> Where did Planet Nine come from and how did it end up in the outer solar
> system? Scientists have long believed that the early solar system began
> with four planetary cores that went on to grab all of the gas around them,
> forming the four gas planets - Jupiter, Saturn, Uranus, and Neptune. Over
> time, collisions and ejections shaped them and moved them out to their
> present locations. "But there is no reason that there could not have been
> five cores, rather than four," says Brown. Planet Nine could represent
> that fifth core, and if it got too close to Jupiter or Saturn, it could
> have been ejected into its distant, eccentric orbit.
>
> Batygin and Brown continue to refine their simulations and learn more
> about the planet's orbit and its influence on the distant solar system.
> Meanwhile, Brown and other colleagues have begun searching the skies for
> Planet Nine. Only the planet's rough orbit is known, not the precise
> location
> of the planet on that elliptical path. If the planet happens to be close
> to its perihelion, Brown says, astronomers should be able to spot it in
> images captured by previous surveys. If it is in the most distant part
> of its orbit, the world's largest telescopes - such as the twin 10-meter
> telescopes at the W. M. Keck Observatory and the Subaru Telescope, all
> on Mauna Kea in Hawaii - will be needed to see it. If, however, Planet
> Nine is now located anywhere in between, many telescopes have a shot at
> finding it.
>
> "I would love to find it," says Brown. "But I'd also be perfectly happy
> if someone else found it. That is why we're publishing this paper. We
> hope that other people are going to get inspired and start searching."
>
> In terms of understanding more about the solar system's context in the
> rest of the universe, Batygin says that in a couple of ways, this ninth
> planet that seems like such an oddball to us would actually make our solar
> system more similar to the other planetary systems that astronomers are
> finding around other stars. First, most of the planets around other
> sunlike
> stars have no single orbital range - that is, some orbit extremely close
> to their host stars while others follow exceptionally distant orbits.
> Second, the most common planets around other stars range between 1 and
> 10 Earth-masses.
>
> "One of the most startling discoveries about other planetary systems has
> been that the most common type of planet out there has a mass between
> that of Earth and that of Neptune," says Batygin. "Until now, we've
> thought
> that the solar system was lacking in this most common type of planet.
> Maybe we're more normal after all."
>
> Brown, well known for the significant role he played in the demotion of
> Pluto from a planet to a dwarf planet adds, "All those people who are
> mad that Pluto is no longer a planet can be thrilled to know that there
> is a real planet out there still to be found," he says. "Now we can go
> and find this planet and make the solar system have nine planets once
> again."
>
> The paper is titled "Evidence for a Distant Giant Planet in the Solar
> System."
>
> Written by Kimm Fesenmaier
>
> Contact:
> Deborah Williams-Hedges
> (626) 395-3227
> debwms at caltech.edu
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Received on Wed 20 Jan 2016 06:48:41 PM PST