Astronomy - September 2015

(Nandana) #1

ASTRONEWS


ASTRONEWS


ASTROCONFIDENTIAL BY KARRI FERRON


Nanoflares are spontaneous solar heating
bursts that each reach some 18 million
degrees F (10 million degrees C).

FAST
FACT

20 ASTRONOMY • SEPTEMBER 2015

EATING HABITS. Astronomers read galaxy NGC 1512’s past eating habits in the processed clumps of gas scattered
across its face, material that it must have absorbed from other smaller galaxies.

WHAT HEATS THE SUN’S OUTER ATMOSPHERE?


At several million kelvins, the Sun’s outer
atmosphere, called the corona, is a thousand
times hotter than the underlying solar sur-
face. Understanding what heats the corona
to its extreme temperatures is one of the
cornerstone questions in space science. New
evidence has revealed that coronal heating
takes the form of impulsive energy bursts
called nanof lares. Although puny by solar
standards, each one is the equivalent of a
50-megaton hydrogen bomb, the largest ever
detonated on Earth. Millions of nanoflares
occur every second across the Sun, and
together they pack a real wallop.
Nanoflares have been difficult to study
because we are unable to observe individual
occurrences. Even with the resolution of our
most powerful telescopes, we are stuck see-
ing multiple overlapping events along the
line of sight. As a consequence, progress has
had to rely on a combination of observa-
tions and theoretical modeling. By compar-
ing what we see with what we expect to see

based on computer simulations,
we can infer the properties of the
energy release. Recently, we have
detected faint emission from super-
hot plasma (highly ionized gas).
This only can be produced by nanoflares,
and we consider it to be the “smoking gun.”
So, what is a nanof lare? That’s still an
open question, but the most likely expla-
nation is that it represents the sudden
breaking of stressed magnetic fields that
extend upward from the solar surface and
permeate the corona. Turbulent motions
at the surface cause the coronal fields to
become tangled and twisted much like rub-
ber bands. Eventually, the fields break and
release bursts of energy — nanof lares — in
a process called magnetic reconnection. It
is at the heart of many different phenomena
occurring throughout the solar system and
the universe. By studying nanof lares, we
hope to learn more about these other phe-
nomena as well.

NASA’s next Mars lander readies for launch


The hunt for major cosmic game is on. And
while scientists have spent a century seeking
the gravitational waves that Albert Einstein first
predicted as a consequence of his general theory
of relativity, this time could be different. In May,
the Laser Interferometer Gravitational-wave
Observatories (LIGO) finished a seven-year
upgrade that increases its sensitivity tenfold.
Astronomers expect these ripples in the fabric of
space-time are created during violent events like
supernova explosions and colliding black holes.
Their hope is to one day use gravitational waves
to unravel new details of the cosmos’ most vio-
lent events. First they have to find them. — E. B.

LIGO ramps up search


for gravitational waves


James A. Klimchuk
Astrophysicist in the Heliophysics Division
at NASA Goddard Space Flight Center,
Greenbelt, Maryland

COURTESY JAMES A. KLIMCHUK

NASA/JPL-CALTECH/LOCKHEED MARTIN
BEST PRACTICE. This is how NASA’s next Mars lander, InSight, will look when it deploys on the Red Planet’s
surface one year from now and begins to study its crust, mantle, and core for the first time. Lockheed Martin
Space Systems in Denver has finished building the spacecraft and moved on to the final testing phase ahead
of the March 2016 launch. InSight deployed its solar panels during tests April 30, and engineers entered a
seven-month environmental testing phase that will expose the car-sized craft to space-like hazards. NASA also
announced plans to deploy CubeSats as InSight enters orbit at Mars and use the tiny instruments to observe
the landing. If it succeeds, the lander could help tell astronomers how rocky planets form. — E. B.

GRAVITY LAB. Physicists have put Einstein to the
test for more than a century, and yet general relativ-
ity’s gravity waves remain unconfirmed. LIGO hopes
to change that beginning this fall. LIGO LABORATORY
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