Astronomy

(Ann) #1
JunoCam image
North
Visible light
Depth below
cloud tops
0 km
20 km
50 km
90 km
150 km
350 km

Cooler Warmer

Microwave

ASTRONEWS


WWW.ASTRONOMY.COM 21

In July 2017, NASA’s Juno spacecraft made its
first-ever pass over Jupiter’s Great Red Spot,
sending back data that show just how deep
the massive storm extends.
Juno found that the storm stretches
roughly 200 miles (300 kilometers) into
Jupiter’s atmosphere and is nearly as wide as
1.5 Earths, or 10,000 miles (16,000 km) across.
The storm’s depth was measured using Juno’s
Microwave Radiometer instrument, which can
see far below Jupiter’s cloud tops.
The Great Red Spot, which contains clouds
spinning rapidly in a counterclockwise motion
around its oval perimeter, has actually dimin-
ished in size over the past few decades. Its
width has decreased by one-third and its
height by one-eighth since NASA’s Voyager 1
and 2 passed by Jupiter in 1979.
Juno’s pass also brought evidence of a new

radiation zone hovering over Jupiter’s atmo-
sphere, close to its equator. The Jupiter
Energetic Particle Detector Instrument spot-
ted energetic hydrogen, sulfur, and oxygen
ions within the zone, traveling close to light
speed. Scientists believe these particles origi-
nate from fast-moving neutral atoms created
around Io and Europa, two of Jupiter’s moons.
The atoms turn into ions when contact with
Jupiter’s atmosphere strips their electrons.
Juno’s Stellar Reference Unit star camera
also detected energetic heavy ions along the
inner edge of Jupiter’s relativistic electron
radiation belt, an area that hadn’t been stud-
ied by previous spacecraft. However, the ori-
gin of these particles remains a mystery. Juno
continues to orbit Jupiter, with December 16,
2017, marking its ninth close pass to our plane-
tary neighbor. — Amber Jorgenson

Juno charts the Great Red Spot’s depths


A next-generation planet hunt begins


FIRST LIGHT. On December 6, the European Southern Observatory announced that the Echelle
SPectrograph for Rocky Exoplanet and Stable Spectroscopic Observations (ESPRESSO), mounted on the
Very Large Telescope at the Paranal Observatory in Chile, had achieved first light. Echelle spectrographs
separate incoming light into its constituent parts and are used in many astronomical instruments. ESPRESSO
is designed to detect tiny shifts in a star’s motion as planets orbit it; because of its extreme sensitivity,
ESPRESSO should enable astronomers to identify some of the lightest rocky planets ever found. In addition
to its planet-hunting capabilities, ESPRESSO also can be used to test the laws of physics and improve
astronomers’ understanding of the universe and its evolution over time. — A.K.

ESO/ESPRESSO TEAM

MOON MAN. President Donald Trump signed a policy directive
that aims to send humans to the Moon for the first time since 1972.

SLICE IT UP. Juno’s Microwave Radiometer
instrument took vertical “slices” of the Great Red
Spot (above) as it peered below Jupiter’s clouds.
(The topmost slice is a visible-light image from
JunoCam.) The storm’s large-scale structure
remains coherent even at the greatest depth the
instrument observed, meaning it extends deep
into the atmosphere. The Great Red Spot (right) is
a counterclockwise-rotating storm that stands out
in stark contrast to the clouds around it.
ILLUSTRATION: ROEN KELLY AFTER NASA/JPL-CALTECH/S

WRI. GREAT RED SPOT: NASA/JPL-CALTECH/S

WRI/MSSS/GERALD EICHSTADT/JUSTIN COWART
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