Astronomy - USA (2020-01)

(Antfer) #1
Mْ= 1 Earth Mass

Jupiter
Mass: 318 Mْ Saturn
Mass: 95.2 Mْ

Uranus
Mass: 14.5 Mْ

Neptune
Mass: 17.1 Mْ

Pluto
Mass: 0.003 Mْ

Planet 9
Mass: ~5–15 Mْ

Mercury
Mass: 0.055 Mْ


Venus
Mass: 0.815 Mْ

Earth
Mass: 1 Mْ

Mars
Mass: 0.107 Mْ

WWW.ASTRONOMY.COM 47

at nearly the same point in
space as a handful of other
noteworthy objects. These
include the team’s earlier dis-
covery of 2012 VP 113 (which
they nicknamed Biden as a
nod to the “VP” in its desig-
nation) and Sedna, a dwarf
planet roughly half the diam-
eter of Pluto that was discov-
ered in 2003.
It’s this recently identified
pack of perihelion-clustered
objects, which Sheppard refers
to as “extreme TNOs,” that
suggests an unseen and mas-
sive planet is hiding in the
outskirts of our solar system.

this peculiar class of extreme
TNOs indicates that dwarf
planets may not be the kings
and queens of the Kuiper
Belt. Instead, there’s a grow-
ing dossier of evidence that
suggests a colossal world
some five to 15 times the
mass of our own planet
is lurking far beyond,
playing puppeteer to the
oddly clustered collection
of distant bodies.
In 2016, Caltech
astronomers Kostantin
Batygin and Mike Brown
published a paper titled
“Evidence for a Distant Giant
Planet in the Solar System.”
In it, they discuss a unique
population of TNOs that
make their closest approaches
to the Sun at roughly the
same point in space, despite
having different orbital trajec-
tories. According to that
study, the odds that such clus-
tering is the result of chance

is about 0.007 percent (or 1 in
14,000). Furthermore, at the
beginning of 2019, Batygin
and Brown also showed
there’s only about a 0.2 per-
cent chance (or 1 in 500) that

the clustering is the result
of observational biases.
“Based on the clustering of
the objects we are finding that
are way out there like The
Goblin,” Sheppard says, “a
super-Earth planet that is a
few hundred AU away” could
be shepherding them into
position. Thanks to cutting-
edge simulations, the
researchers expect Planet
Nine (sometimes referred to
as Planet X), to be in a some-
what eccentric orbit that takes
it about 400 AU from the Sun.
But, Sheppard says, “the
planet could be up to some
1,500 AU away in the more
massive planet models.”
But if Planet Nine really
exists, why does it orbit so far
from the Sun?
That’s still a heavily
debated question. “There’s
two main theories for how
the planet got out there,”
Sheppard says. “The most

likely scenario I like to call
the ‘runt of the giant planet
family.’ ” In this scenario,
Planet Nine formed alongside
Jupiter, Saturn, Uranus, and
Neptune, which Sheppard

The hunt for
Planet Nine
With the advancement of
powerful survey telescopes, as
well as sophisticated software
that can sift through massive

amounts of data like never
before, we are just now begin-
ning to scour the distant
reaches of the solar system
for icy dwarf planets and
the like. But the discovery of

Planet Nine is expected to be about five to 15 times as
massive as Earth, which would make it pretty similar to the
large super-Earths and small sub-Neptunes astronomers are
increasingly finding around other stars. ASTRONOMY: ROEN KELLY AFTER KARL TATE

THE DISCOVERY OF THIS PECULIAR CLASS OF
EXTREME TNOS INDICATES THAT DWARF PLANETS MAY NOT
BE THE KINGS AND QUEENS OF THE KUIPER BELT.

SIZING UP
PLANET NINE

In recent years, astronomers have
identified a mysterious group of
extreme TNOs with distant, clustered
perihelia, as well as relatively aligned
orbits that seem decoupled from the
gravitational influence of the solar
system’s giant planets. Based on the
orbits of these objects — which
include Sedna (orange), “The Goblin”
(green), “Biden” (blue), and a handful
of other bodies with less-colorful
names (shown in gray) — some
researchers think a massive world
called Planet Nine is shepherding the
extreme TNOs into position. ASTRONOMY:
ROEN KELLY AFTER CALTECH/R. HURT (IPAC)
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