Astronomy - USA (2020-01)

(Antfer) #1
500 AU

Beginning of
Oort Cloud
2,000 AU

Top down view

2012 VP 113
“Biden”

Planet 9

Sedna

48 ASTRONOMY • JANUARY 2020


Saturn and got tossed out-
ward.” This ended up pushing
the still-forming Planet Nine
out of the feeding zone, which
stunted its growth before it
could reach the size of a true
giant planet.
Alternatively, Sheppard
says, “it could be a captured
object from another star sys-
tem.” Because stars form out
of massive clouds of condens-
ing gas and dust, they are
born in litters, not in isolation.
So, early in the solar system’s
history, the Sun was sur-
rounded by many other
nearby stars that all gravita-
tionally interacted with one
another. According to
Sheppard, this means other
stars “were tossing objects out
of their solar system, so there
was probably a lot of free-
f loating planets being ejected
from all these different stars.”
And if one of the rogue plan-
ets strayed too close to the
Sun, there’s a chance it was
seized by our own solar sys-
tem, where it’s since remained.
However, for the Sun to
capture such a planet, “you’d
have to slow it down some-
how,” Sheppard says. “So
that’s the questionable factor.”
Although capturing an ejected
planet isn’t the easiest thing to
do, Sheppard points out it
could happen. For example, he
says, there was probably a lot
more gas and dust around in

the early solar system, mean-
ing an approaching planet
“could have been frictionally
slowed down and captured.”
There’s also a third possi-
bility: the solar system was
shaken up in its past by a
wandering star. In research
published last year, astrono-
mers announced the discovery
of an exoplanet named
HD 106906 b, which they
think was exiled into a large,
perturbed orbit thanks to a
pair of passing stars that
strayed too close to its system.
According to Batygin, it’s fea-
sible that a similar process
could have happened when
the Sun was still near other
stars from its birth cluster.

Proving Planet
Nine’s existence
The problem with Planet Nine
is that in order for us to be
100 percent sure it exists, we
need to see it with our own
eyes. Fortunately, Sheppard
says, “our survey is designed
to not simply find the planet,
but to triple the known [num-
ber of] very distant objects.
These very distant objects are
the ones that are sensitive to

says all likely began their lives
within about 5 to 15 AU of
one another. “There’s prob-
ably several Earth-mass-sized
objects and bigger which


formed in that area,” he says.
As Planet Nine was forming,
“it got to several Earth masses
in size, but then it probably
got too close to Jupiter and

ABOVE AND RIGHT: To carry out their
survey of the most distant objects in
the solar system, Sheppard and his
colleagues rely on the Subaru
Telescope (above), perched atop the
summit of Mauna Kea in Hawaii, as
well as the Victor Blanco Telescope
(right), located at Cerro Tololo Inter-
American Observatory in Chile. SUBARU:
ROBERT LINSDELL/FLICKR; BLANCO: NOAO/AURA/NSF

MORE EVIDENCE


FOR PLANET NINE


If Planet Nine exists, there should be a set of objects with orbits that are
perpendicular to the ecliptic plane of the solar system. Five such objects
(shown in magenta) are known, and according to Batygin, they perfectly
fit the models. ASTRONOMY: ROEN KELLY AFTER CALTECH/R. HURT (IPAC)

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