The shrinking of Jupiter’s Great Red Spot — Hubble snaps stormy region at its smallest size ever
Jupiter's trademark Great Red Spot — a
swirling storm feature larger than Earth — is shrinking. This
downsizing, which is changing the shape of the spot from an oval into a
circle, has been known about since the 1930s, but now these striking new
NASA/ESA Hubble Space Telescope images capture the spot at a smaller
size than ever before.
Jupiter's Great Red Spot is a churning anticyclonic storm [1].
It shows up in images of the giant planet as a conspicuous deep red eye
embedded in swirling layers of pale yellow, orange and white. Winds
inside this Jovian storm rage at immense speeds, reaching several
hundreds of kilometres per hour.Historic observations as far back as the late 1800s [2] gauged this turbulent spot to span about 41 000 kilometres at its widest point — wide enough to fit three Earths comfortably side by side. In 1979 and 1980 the NASA Voyager fly-bys measured the spot at a shrunken 23 335 kilometres across. Now, Hubble has spied this feature to be smaller than ever before.
"Recent Hubble Space Telescope observations confirm that the spot is now just under 16 500 kilometres across, the smallest diameter we've ever measured," said Amy Simon of NASA's Goddard Space Flight Center in Maryland, USA.
Amateur observations starting in 2012 revealed a noticeable increase in the spot's shrinkage rate. The spot's "waistline" is getting smaller by just under 1000 kilometres per year. The cause of this shrinkage is not yet known.
"In our new observations it is apparent that very small eddies are feeding into the storm," said Simon. "We hypothesised that these may be responsible for the accelerated change by altering the internal dynamics of the Great Red Spot."
Simon's team plan to study the motions of these eddies, and also the internal dynamics of the spot, to determine how the stormy vortex is fed with or sapped of momentum.
This full-disc image of Jupiter was taken on 21 April 2014 with Hubble's Wide Field Camera 3 (WFC3).
Notes
[1] The Great Red Spot is a high-pressure anticyclone. It rotates in an anti-clockwise direction in Jupiter's southern hemisphere.[2] The Great Red Spot itself may have been mentioned in writings before the late 1800s. There are references to Jupiter's "permanent spot" dating back as far as the late 1600s, although some astronomers disagree that the permanent spot mentioned is the Great Red Spot.
Jupiter and its shrunken Great Red Spot
This full-disc image of Jupiter was taken on 21 April 2014 with Hubble's Wide Field Camera 3 (WFC3).
Credit:
Image Credit: NASA, ESA, and A. Simon (Goddard Space Flight Center)
Acknowledgement: C. Go
Science Credit: A. Simon (Goddard Space Flight Center), G. Orton (Jet Propulsion Laboratory), J. Rogers (University of Cambridge, UK), and M. Wong and I. de Pater (University of California, Berkeley)
Credit:
Image Credit: NASA, ESA, and A. Simon (Goddard Space Flight Center)
Acknowledgement: C. Go
Science Credit: A. Simon (Goddard Space Flight Center), G. Orton (Jet Propulsion Laboratory), J. Rogers (University of Cambridge, UK), and M. Wong and I. de Pater (University of California, Berkeley)
Jupiter with comparison images of the Great Red Spot from 1995, 2009 and 2014
In this comparison image the photo at the top was taken by Hubble's
Wide Field Planetary Camera 2 in 1995 and shows the spot at a diameter
of just under 21 000km; the second down shows a 2009 WFC3 photo of the
spot at a diameter of just under 18 000km; and the lowest shows the
newest image from WFC3 taken in 2014 with the spot at its smallest yet,
with diameter of just 16 000km.
Credit:
Image Credit: NASA, ESA, and A. Simon (Goddard Space Flight Center)
Science Credit: A. Simon (Goddard Space Flight Center), G. Orton (Jet Propulsion Laboratory), J. Rogers (University of Cambridge, UK), and M. Wong and I. de Pater (University of California, Berkeley)
Acknowledgment: C. Go, H. Hammel (SSI and AURA) and R. Beebe (NMSU)
Credit:
Image Credit: NASA, ESA, and A. Simon (Goddard Space Flight Center)
Science Credit: A. Simon (Goddard Space Flight Center), G. Orton (Jet Propulsion Laboratory), J. Rogers (University of Cambridge, UK), and M. Wong and I. de Pater (University of California, Berkeley)
Acknowledgment: C. Go, H. Hammel (SSI and AURA) and R. Beebe (NMSU)
Jupiter's Great Red Spot in 2014
An image of Jupiter's Great Red Spot taken in 2014 with Hubble's WFC3 camera. The spot has a diameter here of 16 000km.
Credit:
NASA, ESA and A. Simon (Goddard Space Flight Center)
Credit:
NASA, ESA and A. Simon (Goddard Space Flight Center)
Jupiter's Great Red Spot in 2009
An image of Jupiter's Great Red Spot taken in 2009 with Hubble's WFC3 camera. The spot’s diameter here is just under 18 000km.
Credit:
NASA, ESA and H. Hammel (SSI and AURA)
Credit:
NASA, ESA and H. Hammel (SSI and AURA)
Jupiter's Great Red Spot in 1995
An image of Jupiter's Great Red Spot taken by Hubble's Wide Field
Planetary Camera 2 in 1995. The spot's diameter here is just under 21
000km.
Credit:
NASA, ESA and R. Beebe (NMSU)
VIDEOS -VIDEOS
Credit:
NASA, ESA and A. Simon (Goddard Space Flight Center) Music: movetwo
Credit:
NASA, ESA and R. Beebe (NMSU)
VIDEOS -VIDEOS
Pan across Jupiter
This video shows a pan across the surface of Jupiter, revealing the
Great Red Spot — a storm which rages on its surface — and which Hubble
images have shown to be shrinking.
Credit:
NASA, ESA and A. Simon (Goddard Space Flight Center) Music: movetwo
Jupiter’s shrinking spot
This video shows where Jupiter’s trademark spot can be found on its
surface and showcases the comparison images that demonstrate how the
spot has shrunk over the last nineteen years.
Credit:
NASA, ESA, and G. Bacon (STScI)
Science Credit: A. Simon (Goddard Space Flight Center), G. Orton (Jet Propulsion Laboratory), J. Rogers (University of Cambridge, UK), and M. Wong and I. dePater (University of California, Berkeley) Acknowledgment: H. Hammel (SSI and AURA) and R. Beebe (NMSU)
Credit:
NASA, ESA, and G. Bacon (STScI)
Science Credit: A. Simon (Goddard Space Flight Center), G. Orton (Jet Propulsion Laboratory), J. Rogers (University of Cambridge, UK), and M. Wong and I. dePater (University of California, Berkeley) Acknowledgment: H. Hammel (SSI and AURA) and R. Beebe (NMSU)
FUENTE: ESA/Hubble Information Centre
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