Astronomy

(Sean Pound) #1

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Abell 1687 (galaxy cluster)
2.40 billion light-years

WWW.ASTRONOMY.COM 29

“ice giants.” Both planets are about four
times the size of Earth.

Icing over
The Kuiper Belt is a doughnut-shaped
region located 30 to 50 AU from the Sun,
and Neptune plays a key role in shaping it.
In fact, astronomers think that Neptune’s
largest moon, Triton, may be a captured
Kuiper Belt object (KBO). Like its rocky
counterpart between Mars and Jupiter,
the Kuiper Belt is a faint echo of the Sun’s
vast debris disk, the construction zone
of our planetary system. In this region,
orbits in favorable resonances can protect
KBOs from disruptive encounters with
Neptune. Pluto, at 39 AU, is the brightest
of a KBO family locked in a
2:3 resonance, complet-
ing two orbits for every
three trips Neptune
takes around the Sun;
stable groups also
occupy other resonances.
KBOs in resonances

that are unfavorable are swept out of the
belt, scattered by Neptune inward and
outward onto more tilted and elongated
orbits. Comets like 2P/Encke and 67P/
Churyumov-Gerasimenko, subject of
ESA’s Rosetta orbiter, may have originated
as fragments of scattered KBOs whose
orbits were tightened up by encounters
with Jupiter.
Now that its f lyby of Pluto is complete,
scientists hope NASA’s New Horizons
spacecraft will be able to provide close-
up information on additional KBOs as
it heads through the belt and out of the
solar system. NASA’s Voyager 1 spacecraft,
now 132 AU out, has already done so in
one sense. It has left the heliosphere, the
magnetic bubble shaped by the outflow of
charged particles from the Sun, and most of
the particles now detected by the spacecraft
have traveled to it from interstellar space.
From Voyager 1’s location, the Sun is a bril-
liant point about 24 times brighter than
a Full Moon as seen from
Earth. Still, the probe will

take millennia to coast through the solar
system’s biggest structural component.
This is the Oort Cloud, where per-
haps a trillion comets randomly orbit in
a spherical shell centered on the Sun. It
extends from 5,000 to 100,000 AU — that’s
1.6 light-years, about 40 percent of the
way to Proxima Centauri, the nearest star.
Astronomers think the Oort Cloud formed
early in the solar system’s history, when icy
objects much closer to the Sun were hurled
outward by gravitational interactions with
the planets. They now may take as long as
30 million years to complete an orbit. These
comets are so feebly gripped by the Sun
that other forces, such as the overall gravi-
tational field of the galaxy’s irregular mass
distribution (known as the galactic tide)
along with passing stars and massive molec-
ular clouds, strongly affect them. Eventually
these gravitational tugs can alter a comet’s
path so that it starts the long fall toward the
Sun for the first time since it was cast out.
These “dynamically new” comets travel on
extremely elongated and randomly oriented
paths. Gravitational interactions with the
planets can divert them into shorter orbits,
and astronomers think the famous Halley’s
Comet is one example.
At the fringes of the cloud, comets eas-
ily escape into interstellar space via the
same tugs that nudge them sunward.
Comets from our solar system already may
have raced around another star. Might we
one day see a comet from an alien Oort
Cloud, another star’s realm of ice? As far as
astronomers know, it hasn’t happened yet,
but it’s definitely possible.

With New Horizons’ Pluto flyby in July, humans have now explored every object in the solar system
that has, at least at some point, been classified as a planet. Pluto’s moon Charon is shown as well,
each of them to scale in both size and separation. NASA/JHUAPL/SWRI

NASA’s Solar Dynamics Observatory captured the June 5, 2012, transit of Venus more than 250 years
after astronomers’ first attempt to use such a transit to measure the absolute distance scale of the
solar system. NASA/GSFC/SDO

Comets like 67P/Churyumov-Gerasimenko, now
under careful investigation by the European
Space Agency’s Rosetta spacecraft, might be
swept into their extreme orbits after gravitation-
al nudges from Jupiter or another large planet.

ESA/ROSETTA/NAVCAM

NASA/ESA/HUBBLE ( 3C 273); NASA/ESA/N. BENITEZ (JHU), ET AL./ACS SCIENCE TEAM (ABELL 1689); DSS (ABELL 1687)

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