Hubble Sees Neptune 's
Mysterious Shrinking Storm
NASA – February 15, 2018 -- Three billion miles away on the farthest known major planet in our solar system, an ominous, dark storm – once big enough to stretch across the Atlantic Ocean fromBoston to Portugal – is shrinking out of existence as seen
in pictures of Neptune taken by NASA’s Hubble
Space Telescope.
Neptune ’s deep winds, which can’t be directly measured.
The dark spot material may be hydrogen sulfide, with the pungent smell of rotten eggs. Joshua Tollefson from theUniversity of California at Berkeley
explained, “The particles themselves are still highly reflective; they are just
slightly darker than the particles in the surrounding atmosphere.”
Spain . “It is
most likely that they arise from an instability in the sheared eastward and
westward winds.”
Neptune
spot is not as tightly constrained by numerous alternating wind jets (seen as
bands in Jupiter’s atmosphere). Neptune seems
to only have three broad jets: a westward one at the equator, and eastward ones
around the north and south poles. The vortex should be free to change traffic
lanes and cruise anywhere in between the jets.
Neptune and its
storms: https://www.nasa.gov/feature/goddard/2018/hubble-sees-neptunes-mysterious-shrinking-storm
NASA – February 15, 2018 -- Three billion miles away on the farthest known major planet in our solar system, an ominous, dark storm – once big enough to stretch across the Atlantic Ocean from
Immense dark
storms on Neptune were first discovered in the
late 1980s by NASA’s Voyager 2 spacecraft. Since then, only Hubble has had the
sharpness in blue light to track these elusive features that have played a game
of peek-a-boo over the years. Hubble found two dark storms that appeared in the
mid-1990s and then vanished. This latest storm was first seen in 2015, but is
now shrinking.
Like Jupiter’s
Great Red Spot (GRS), the storm swirls in an anti-cyclonic direction and is
dredging up material from deep inside the ice giant planet’s atmosphere. The
elusive feature gives astronomers a unique opportunity to study The dark spot material may be hydrogen sulfide, with the pungent smell of rotten eggs. Joshua Tollefson from the
Unlike Jupiter’s
GRS, which has been visible for at least 200 years, Neptune ’s
dark vortices only last a few years. This is the first one that actually has
been photographed as it is dying.
"We have no
evidence of how these vortices are formed or how fast they rotate,” said
Agustín Sánchez-Lavega from the University of the Basque Country in
The dark vortex
is behaving differently from what planet-watchers predicted. “It looks like
we’re capturing the demise of this dark vortex, and it’s different from what
well-known studies led us to expect,” said Michael H. Wong of the University of
California at Berkeley, referring to work by Ray LeBeau (now at St. Louis
University) and Tim Dowling’s team at the University of Louisville. “Their
dynamical simulations said that anticyclones under Neptune ’s
wind shear would probably drift toward the equator. We thought that once the
vortex got too close to the equator, it would break up and perhaps create a
spectacular outburst of cloud activity.”
But the dark
spot, which was first seen at mid-southern latitudes, has apparently faded away
rather than going out with a bang. That may be related to the surprising
direction of its measured drift: toward the south pole, instead of northward
toward the equator. Unlike Jupiter’s GRS, the
“No facilities
other than Hubble and Voyager have observed these vortices. For now, only
Hubble can provide the data we need to understand how common or rare these
fascinating neptunian weather systems may be,” said Wong.
The first images
of the dark vortex are from the Outer Planet Atmospheres Legacy (OPAL) program,
a long-term Hubble project that annually captures global maps of our solar
system’s four outer planets. Only Hubble has the unique capability to probe
these worlds in ultraviolet light, which yields important information not
available to other present-day telescopes. Additional data, from a Hubble
program targeting the dark vortex, are from an international team including
Wong, Tollefson, Sánchez-Lavega, Andrew Hsu, Imke de Pater, Amy Simon, Ricardo
Hueso, Lawrence Sromovsky, Patrick Fry, Statia Luszcz-Cook, Heidi Hammel, Marc
Delcroix, Katherine de Kleer, Glenn Orton, and Christoph Baranec.
Wong’s paper
appears online in the Astronomical Journal on Feb. 15, 2018.
Link with
text as above and images of
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