In fact, Jupiter sidled all the way up to
where Mars is now, about 1. 5 astronomical units from the sun, according to this
idea, reported last year in Nature. A big
planet like Jupiter would sweep material from the disk at that location, with
the leftovers eventually forming Mars.
Such housecleaning could explain why
Mars is smaller than researchers would
expect.
“It explains why, among the terrestrial
planets, there is a big difference between
the Earth and Mars in terms of mass,”
Morbidelli says of the theory, which he
calls the Grand Tack.
And the Grand Tack explains more
than just a tiny Mars. Jupiter’s inward
wandering would have scattered the
busted-up chunks sitting in a then-embryonic asteroid belt. When it moved
back out, Jupiter would reassemble the
rocky swath and drag in a second population of objects from farther away. The
product? An asteroid belt between Mars
and Jupiter with two distinct types of
space rocks, a feature observed today but
not explained by the Nice model.
Morbidelli’s next step is to rewind
the tape even further and really tackle
the process of cooking a giant planet.
“The Grand Tack makes some assumptions about where the planets are, which
sequence they formed in, and we are not
sure these assumptions are correct,”
he says. Morbidelli will also help test
Levison’s tumbleplanets idea, which
may explain the small size of Mars via
a different recipe than the Grand Tack
(SN Online: 10/4/10 ).
Simulations suggest that this ejected
fifth planet preserves the solar system
observed today when it resides for a
short time between Saturn and the ice
giants, Nesvorny reported in December
in Astrophysical Journal Letters. “I’m
able to match the current solar system,
starting with five planets, up to 10 times
more frequently than starting with just
four planets,” Nesvorny says. According
to him, a young solar system populated
by five giant planets is much more likely
than one populated with just four.
“Five-planet systems seem to work
better,” Bottke says. “But is there a way
we can find a smoking gun telling us that
this must be true?”
Batygin, who has also tried saving
Earth with what he calls a “sacrificial
goat,” thinks such a find is unlikely, since
an ejected planet probably wouldn’t goat,” thinkssuchafindisunlikely, since
an ejected planet probably wouldn’t
purporting to explain the current state
of planetary affairs.
Scientists including David Nesvorny
of the Southwest Research Institute proposed that the best way to save Earth
was to offer an ice giant — Neptune or
Uranus—to the Jovian bully. A larger
planet interacting with Jupiter alters
Jupiter’s orbit almost instantaneously,
causing it to skip over the deadly encounter with Earth.
But when Nesvorny simulated the
interaction, he found that Jupiter and
Saturn usually expelled the ice giant,
leaving behind three giant planets
instead of the four currently found in
the outer solar system. So he added a fifth
giant planet to the young solar system — a
sibling who enters a deadly dance with
Jupiter, spurring its own ejection and
perturbing Jupiter’s and Saturn’s orbits. Jupiter, spurring its own ejection and
perturbing Jupiter’s and Saturn’s orbits.
Jupiter’s journey
A few million years after
the solar system was born,
a young Jupiter may have
journeyed inward, with an early
Saturn following (chart shows
masses and distances of outer
planets from the sun over
time). This trip could explain
Mars’ small size (far right, in
comparison with Earth); as
Jupiter moved, it swept away
much of the material that
would have otherwise come
together to form Mars.
journeyed inward, with an early Saturn following (chart shows
masses and distances of outer
time). This trip could explain
Mars’ small size (far right, in
Jupiter moved, it swept away
Mass and distance from sun over time
Jupiter
Planetboot
Some parts of the main act have turned
out to be a challenge for the Nice model,
too. Over time, its architects discovered
a complication. “We ran into a roadblock
having to do with the survivability of the
Earth,” Levison says. “It ends up hitting
Venus, mostly.”
An evil encounter with Jupiter’s grav-
ity during the solar system’s period of
rebellion, when planets and asteroids
are flying all over the place, sends Earth
careening into its sister planet—an
undesirable outcome for a model
Earth masses
100
10
Saturn
Neptune
Uranus
0
Average distance to the sun (AU)
10
5
Neptune
Uranus
Jupiter
Saturn
0
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May 5, 2012 | SCIENCE NEWS | 27