Astronomy

(Tina Meador) #1

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+
Free download pdf