Wind vectors in Jupiter's Little Red Spot measured from the New Horizons Long Range Reconnaissance Imager (LORRI) frames, plotted on the first time step. The wind vectors have been slightly exaggerated for clarity and diamond symbols indicate the starting point of the vector. The LRS is the counterclockwise circulating oval to the right of center. A south tropical disturbance is seen at the top, north of 29 degrees south. Winds to the west are observed near 40 degrees south outside the small oval at lower right. See the motion of the Little Red Spot in this MPEG video. Credit: NASA/Johns Hopkins University Applied Physics Laboratory/Southwest Research Institute
In this quasi-true-color view of Jupiter's Little Red Spot, generated using a New Horizons-LORRI mosaic in the red and green channels and a Hubble Space Telescope 410 nm map in the blue channel, the "LRS" appears with distinctly redder color than the south tropical disturbance to the north or the small oval to the southeast.Credit: NASA/Johns Hopkins University Applied Physics Laboratory/Southwest Research Institute/HST
This Hubble Space Telescope mosaic from Feb. 26, 2007, shows the Great Red Spot and Little Red Spot regions, with an average zonal wind field plotted over. Color is generated using a 410 nm map (blue) and 673 nm map (red), with a composite of the two in the green channel. The "GRS" is at the left near 20 degrees south, and the "LRS" with the south tropical disturbance to the north is seen at right. The south tropical disturbance is darker than other whitish clouds in its latitude band which overlaps that of the GRS.Credit: NASA/Johns Hopkins University Applied Physics Laboratory/Southwest Research Institute/HST
A multi-wavelength comparison of Jupiter's Little Red Spot (top) and Great Red Spot (bottom). Images are not to scale, and all wavelengths are listed in microns. The 0.26, 0.41 and 0.89 µm images are from Hubble Space Telescope, acquired on Feb. 26, 2007. The 8.59 and 10.77 µm images were acquired on Feb. 28, 2007 (LRS) and March 1 (GRS) at the VLT. The 0.26 µm filter is sensitive to stratosphere haze, 0.41 µm to troposphere clouds and haze color, 0.89 µm to upper troposphere cloud and haze opacity, 8.59 µm to troposphere cloud opacity and temperature, and 10.77 µm to troposphere temperature and ammonia gas. The black arrow marks a small oval southeast of the LRS. The southern portion of the GRS is brighter at 8.59 and 10.77 µm. Credit: NASA/ESO/HST/Johns Hopkins University Applied Physics Laboratory/Southwest Research Institute
(a) Visible image of Jupiter's Little Red Spot, taken by the New Horizons spacecraft. Temperature maps on constant pressure surfaces at 400 mbar (b), 300 mbar (c), and 200 mbar (d) from inversion of images of Jupiter's thermal radiances taken through approximately 1 µm-wide filters centered at 13.04, 17.65, 18.72, and 19.50 µm, which are primarily sensitive to temperatures in the 200-400 mbar pressure range. The spatial resolution is equivalent to 1.5 degrees in longitude and 1.8 degrees in latitude. The LRS and small oval are cold anticyclones, as is the south tropical disturbance nearby. A warm, cyclonic region is seen south of the LRS. Credit: NASA/Johns Hopkins University Applied Physics Laboratory/Southwest Research InstituteUsing data from NASA’s New Horizons spacecraft and two telescopes at Earth, an international team of scientists has found that one of the solar system’s largest and newest storms – Jupiter’s Little Red Spot – has some of the highest wind speeds ever detected on any planet.
The New Horizons researchers combined observations from their Pluto-bound spacecraft, which flew past Jupiter in February 2007; data from the Hubble Space Telescope orbiting Earth, and the European Southern Observatory’s Very Large Telescope, perched on an Atacama Desert mountain in Chile. This is the first time that high resolution, close–up imaging of the Little Red Spot has been combined with powerful Earth–orbital and ground-based imagery made at ultraviolet through mid–infrared wavelengths.
Jupiter’s "LRS" is an anticyclone, a storm whose winds circulate in the opposite direction to that of a cyclone – counterclockwise, in this case. It is nearly the size of Earth and as red as the similar, but larger and more well known, Great Red Spot (or GRS). The dramatic evolution of the LRS began with the merger of three smaller white storms that had been observed since the 1930s. Two of these storms coalesced in 1998, and the combined pair merged with a third major Jovian storm in 2000. In late 2005 – for reasons still unknown — the combined storm turned red.
The new observations confirm that wind speeds in the LRS have increased substantially over the wind speeds in the precursor storms, which had been observed by NASA’s Voyager and Galileo missions in past decades. Researchers measured the latest wind speeds and directions using two image mosaics from New Horizons' telescopic Long Range Reconnaissance Imager (LORRI), taken 30 minutes apart in order to track the motion of cloud features. New Horizons obtained the images from a distance of approximately 2.4 million kilometers (1.5 million miles) from Jupiter at a resolution of 14.4 kilometers (8.9 miles) per pixel. The LRS' maximum winds speeds of about 384 miles per hour (between 155 – 190 meters per second) far exceed the156 mile-per-hour threshold that would make it a Category 5 storm on Earth.
"This storm is still developing, and some of the changes remain mysterious,” says Dr. Andrew Cheng of the Johns Hopkins University Applied Physics Laboratory (APL), Laurel, Md., who led the study team. “This unique set of observations is giving us hints about the storm's structure and makeup; from this, we expect to learn much more about how these large atmospheric disturbances form on worlds across the solar system."
Jupiter's venerable Great Red Spot has decreased steadily in size over the past several decades. In addition, a rare "global upheaval" in Jupiter's atmosphere began before New Horizons visited last year. This upheaval involved the disappearance of activity in the South Equatorial Belt (which left the GRS as an isolated storm), the appearance of a south tropical disturbance north of the Little Red Spot, and other spectacular cloud changes.
"This was a rare opportunity to combine observations from a powerful suite of instruments, as Jupiter will not be visited again by a spacecraft until 2016 at the earliest," says Cheng, whose team publishes its work in the June 2008 Astronomical Journal.
Scientists combined LORRI image maps of cloud motions with visible-color images from Hubble, and mid-infrared images from the Very Large Telescope. The latter technique allows scientists to "see" thermal structure and dynamics beneath the visible cloud layers, because thermal infrared wavelengths (indicating heat) can pass through the higher clouds. "The new observations confirm that the thermal structures, wind speeds, and cloud features of the LRS are very similar to those of the GRS," says Dr. Hal Weaver, a member of the study team from APL and the New Horizons project scientist. "Both the LRS and the GRS extend into the stratosphere, to far higher altitudes than for the smaller storms on Jupiter."
The observations offer clues to the mystery of why the GRS, and now also the LRS, may be so red. The wind speeds and overall strength of the LRS increased substantially in the seven years between the Galileo and the New Horizons observations, during which the storm became red. "This supports the idea that a common dynamical mechanism explains the reddening of the two largest anticyclonic systems on Jupiter, one possibility of which is that storm winds dredge up material from below," says Dr. Amy Simon-Miller of NASA’s Goddard Space Flight Center, Greenbelt, Md.
In their report, the scientists also wonder about the future evolution of Jupiter’s two giant storms. The LRS already rivals the steadily shrinking GRS in size and wind speed. The new thermal and wind field observations hint at an interaction between the south tropical disturbance, the Little Red Spot, and a warm cyclonic region south of the LRS, forming a complex that could dwarf the Great Red Spot.
"The Great Red Spot may not always be the largest and strongest storm on Jupiter,” says Dr. Glenn Orton of NASA’s Jet Propulsion Laboratory, Pasadena, Calif. “Continued monitoring of Jupiter's constantly evolving atmosphere will surely yield more surprises."
New Horizons is the first mission in NASA's New Frontiers Program of medium-class spacecraft exploration projects. Dr. Alan Stern leads the mission and science team as principal investigator; APL manages the mission for NASA’s Science Mission Directorate. The mission team also includes Southwest Research Institute, Ball Aerospace Corporation, the Boeing Company, NASA Goddard Space Flight Center, NASA Jet Propulsion Laboratory, Stanford University, KinetX Inc. (navigation team), Lockheed Martin Corporation, University of Colorado, the U.S. Department of Energy, and a number of other firms, NASA centers, and university partners.
The New Horizons researchers combined observations from their Pluto-bound spacecraft, which flew past Jupiter in February 2007; data from the Hubble Space Telescope orbiting Earth, and the European Southern Observatory’s Very Large Telescope, perched on an Atacama Desert mountain in Chile. This is the first time that high resolution, close–up imaging of the Little Red Spot has been combined with powerful Earth–orbital and ground-based imagery made at ultraviolet through mid–infrared wavelengths.
Jupiter’s "LRS" is an anticyclone, a storm whose winds circulate in the opposite direction to that of a cyclone – counterclockwise, in this case. It is nearly the size of Earth and as red as the similar, but larger and more well known, Great Red Spot (or GRS). The dramatic evolution of the LRS began with the merger of three smaller white storms that had been observed since the 1930s. Two of these storms coalesced in 1998, and the combined pair merged with a third major Jovian storm in 2000. In late 2005 – for reasons still unknown — the combined storm turned red.
The new observations confirm that wind speeds in the LRS have increased substantially over the wind speeds in the precursor storms, which had been observed by NASA’s Voyager and Galileo missions in past decades. Researchers measured the latest wind speeds and directions using two image mosaics from New Horizons' telescopic Long Range Reconnaissance Imager (LORRI), taken 30 minutes apart in order to track the motion of cloud features. New Horizons obtained the images from a distance of approximately 2.4 million kilometers (1.5 million miles) from Jupiter at a resolution of 14.4 kilometers (8.9 miles) per pixel. The LRS' maximum winds speeds of about 384 miles per hour (between 155 – 190 meters per second) far exceed the156 mile-per-hour threshold that would make it a Category 5 storm on Earth.
"This storm is still developing, and some of the changes remain mysterious,” says Dr. Andrew Cheng of the Johns Hopkins University Applied Physics Laboratory (APL), Laurel, Md., who led the study team. “This unique set of observations is giving us hints about the storm's structure and makeup; from this, we expect to learn much more about how these large atmospheric disturbances form on worlds across the solar system."
Jupiter's venerable Great Red Spot has decreased steadily in size over the past several decades. In addition, a rare "global upheaval" in Jupiter's atmosphere began before New Horizons visited last year. This upheaval involved the disappearance of activity in the South Equatorial Belt (which left the GRS as an isolated storm), the appearance of a south tropical disturbance north of the Little Red Spot, and other spectacular cloud changes.
"This was a rare opportunity to combine observations from a powerful suite of instruments, as Jupiter will not be visited again by a spacecraft until 2016 at the earliest," says Cheng, whose team publishes its work in the June 2008 Astronomical Journal.
Scientists combined LORRI image maps of cloud motions with visible-color images from Hubble, and mid-infrared images from the Very Large Telescope. The latter technique allows scientists to "see" thermal structure and dynamics beneath the visible cloud layers, because thermal infrared wavelengths (indicating heat) can pass through the higher clouds. "The new observations confirm that the thermal structures, wind speeds, and cloud features of the LRS are very similar to those of the GRS," says Dr. Hal Weaver, a member of the study team from APL and the New Horizons project scientist. "Both the LRS and the GRS extend into the stratosphere, to far higher altitudes than for the smaller storms on Jupiter."
The observations offer clues to the mystery of why the GRS, and now also the LRS, may be so red. The wind speeds and overall strength of the LRS increased substantially in the seven years between the Galileo and the New Horizons observations, during which the storm became red. "This supports the idea that a common dynamical mechanism explains the reddening of the two largest anticyclonic systems on Jupiter, one possibility of which is that storm winds dredge up material from below," says Dr. Amy Simon-Miller of NASA’s Goddard Space Flight Center, Greenbelt, Md.
In their report, the scientists also wonder about the future evolution of Jupiter’s two giant storms. The LRS already rivals the steadily shrinking GRS in size and wind speed. The new thermal and wind field observations hint at an interaction between the south tropical disturbance, the Little Red Spot, and a warm cyclonic region south of the LRS, forming a complex that could dwarf the Great Red Spot.
"The Great Red Spot may not always be the largest and strongest storm on Jupiter,” says Dr. Glenn Orton of NASA’s Jet Propulsion Laboratory, Pasadena, Calif. “Continued monitoring of Jupiter's constantly evolving atmosphere will surely yield more surprises."
New Horizons is the first mission in NASA's New Frontiers Program of medium-class spacecraft exploration projects. Dr. Alan Stern leads the mission and science team as principal investigator; APL manages the mission for NASA’s Science Mission Directorate. The mission team also includes Southwest Research Institute, Ball Aerospace Corporation, the Boeing Company, NASA Goddard Space Flight Center, NASA Jet Propulsion Laboratory, Stanford University, KinetX Inc. (navigation team), Lockheed Martin Corporation, University of Colorado, the U.S. Department of Energy, and a number of other firms, NASA centers, and university partners.
Media Contacts:
M. Buckley, Johns Hopkins University Applied Physics Laboratory
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