ASTRONEWS
FAST
FAC T
Polaris, currently 0.77° from
the North Celestial Pole, will
be closest to that point in 2102,
when it will lie 0.46° away.
Thuban
22300 to 24100
Vega
13100 to
15000
North
Celestial Pole
2017
to 8000
Polaris
500 to 3000
Alrai
Iota 3000 to 5200
5200 to 6800
Alderamin
6800 to 8000
Deneb
9600 to
10300
Delta
11000 to
12000
Ta u
18500 to 21700 Edasich
21700 to 22300 Kochab24100 to 26500
0
5000
10000
15000
20000
CYGNUS CEPHEUS
LY R A
HERCULES
BIG
DIPPER
URSA
MINOR
DRACO
12 ASTRONOMY • JANUARY 2018
CHIMING IN. The new Canadian Hydrogen Intensity Mapping Experiment (CHIME) will probe nearly
the entire observable universe in 3-D while studying dark energy and gravitational waves.
BRIEFCASE
NEIGHBORHOOD WATCH
Coryn Bailer-Jones of the Max
Planck Institute for Astronomy
has published the first system-
atic estimate of how often
other stars wander into our
solar neighborhood. Using
data from the European Space
Agency satellite Gaia, Bailer-
Jones found that every million
years, between 490 and 600
stars typically pass within
5 parsecs (16.3 light-years) of
the Sun. Astronomers are inter-
ested in these close stellar
encounters because they can
nudge comets out of the Oort
Cloud and into the inner solar
system, potentially wreaking
havoc on unsuspecting planets
like Earth.
- TURBULENCE AHEAD
Researchers once thought
Jupiter’s aurorae were created
the same way as Earth’s, where
energetic particles are acceler-
ated by differences in strength
between atmospheric mag-
netic fields, called electric
potentials. But the strongest
aurorae on Jupiter are not
always associated with the big-
gest electric potentials, as on
Earth. Instead, it appears a dif-
ferent cause is responsible for
the most powerful displays. “At
Jupiter, the brightest aurorae
are caused by some kind of tur-
bulent acceleration process
that we do not understand
very well,” Johns Hopkins
University Applied Physics
Laboratory researcher Barry
Mauk said in a press release. At
high energies, he said, “a new
acceleration process takes
over,” which Juno scientists are
now working to understand.
MIDDLE GROUND
In a paper published
September 4 in Nature
Astronomy, a team of astrono-
mers led by Tomoharu Oka of
Keio University in Yokohama,
Japan, shows evidence that a
gas cloud called CO-0.40-0.
near our galaxy’s center may
harbor an intermediate-mass
black hole. Gas particles inside
CO-0.40-0.22 have motions
consistent with an object
100,000 times the Sun’s mass.
Radio emission measured from
the cloud also bears striking
similarities to the radio source
associated with our galaxy’s
4 million-solar-mass supermas-
sive black hole, Sagittarius A*,
though 500 times fainter, sug-
gesting a black hole a few hun-
dred times smaller. — J.P.,
John Wenz, Alison Klesman
F
rom prompting star forma-
tion to driving accretion
around supermassive black
holes, magnetic fields
inf luence nearly every astro-
physical process. However, one
of the biggest hurdles in study-
ing the magnetic fields that
pervade galaxies is their lack of
strength. Millions of times
weaker than Earth’s magnetic
field, galactic magnetic fields
are difficult to measure at great
distances.
But in an August 28 paper in
Nature Astronomy, a team of researchers reported
the best measurements yet of a magnetic field in a
galaxy located a record-breaking 4.6 billion light-
years away. The team, led by Sui Ann Mao of the
Max Planck Institute for Radio Astronomy,
detected a magnetic field similar to the Milky
Way’s in a host nearly 5 billion years younger, pro-
viding new insight into how these fields have
evolved in the universe over cosmic timescales.
The scientists investigated the galaxy using a phe-
nomenon called gravitational lensing, which occurs
when a massive object — the galaxy in this study
— lines up between Earth and a distant object — in
this case, a quasar (CLASS B1152+199). As divergent
light rays from the quasar pass by the intervening
galaxy, the galaxy’s gravity bends their path.
YOUNG GALAXIES MAY HAVE OLD MAGNETIC FIELDS
The light passing through
the galaxy’s edges is further
affected by any local mag-
netic fields, which can
change the light’s polariza-
tion, or the direction of its
vibration. This effect is called Faraday rotation, and
the stronger the magnetic field, the more the light’s
polarization is rotated.
By measuring this rotation in the light received
from the background quasar, the researchers deter-
mined the young galaxy’s magnetic field is similar
in size and strength to those found in the Milky
Way and other nearby, older galaxies.
One of the leading theories on the evolution of
galactic magnetic fields is that they begin scrawny
and tangled, then strengthen and organize over
time. But that doesn’t seem to be the case here.
“By catching magnetic fields when they’re so young,
we can rule out some of the theories of where they
come from,” Ellen Zweibel, a co-author on the
study, said in a press release. — Jake Parks
MAGNETIC FINGERPRINTS.
The Hubble Space Telescope
captured two gravitationally
lensed images of a distant quasar
behind a young foreground galaxy.
The two images are light that
has traveled through opposite
ends of the galaxy, picking up
information about its magnetic field
along the way. MAO ET AL., NASA
ASTRONOMY
: ROEN KELLY
FUTURE
NORTH STARS
POLAR EXPRESS. Because of
gravitational influences from
the Sun and Moon, our planet
wobbles like a top with a period
of 25,772 years. That means the
point above the North Pole
(the North Celestial Pole, or
NCP) traces a circle in that
span. Currently, the closest
bright star to the NCP is
Polaris, the brightest star in
the constellation Ursa Minor
the Bear Cub. But 10 other
relatively bright stars will
lie closer to the NCP before
Polaris once again assumes
the mantle of North Star.
— Michael E. Bakich
Foreground
galaxy
Lensed images of
CLASS B1152+