Great White Spot

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Major Storm On Saturn.jpg
Hubble observation of the 1990 GWS
Storm on Saturn.jpg
The 1994 Storm seen by Hubble
Saturn Storm December 2010.jpg
The 2010/2011 GWS in December 2010 seen by Cassini
Saturn Storm.jpg
The GWS in 2011 seen by Cassini

The Great White Spot, also known as Great White Oval (named by analogy to Jupiter's Great Red Spot) is a series of periodic storms on the planet Saturn that are large enough to be visible from Earth by telescope by their characteristic white appearance. The spots can be several thousands of kilometers wide.

Contents

The Cassini orbiter was able to track the 2010–11 instance of the storm, [1] also known as the Northern Electrostatic Disturbance, because of an increase in radio and plasma interference, or the Great Springtime Storm. [2]

Cassini data has revealed a loss of acetylene in the white clouds, an increase of phosphine, and an unusual temperature drop in the center of the storm. [3] After the visible aspects of the storm subsided, in 2012, a "belch" of heat and ethylene was emitted from two hotspots that merged. [2] [4]

Occurrence

The phenomenon is somewhat periodic at 28.5-year intervals, when Saturn's northern hemisphere tilts most toward the sun. Usually this is during the solar longitude of around 90-180°, only the 2010 GWS was ahead of its time shortly after equinox. The following is a list of recorded sightings. Six events are recognized as Great White Spots. [5]

Equatorial (1.8°N to 9.8°N) [5]

Mid-latitudes

Polar

Mid-sized synoptic-scale storms are sometimes related to the GWS. Such as the 1994 storm studied by ground-based observers and the Hubble Space Telescope. [7] This storm was located at 9.4°N and is probably related to the 1990 GWS. Pre 2010 GWS storms in the "storm alley" occurred in mid-latitudes in the southern hemisphere (2002–2010 at 36.2°S; 1.5° wide). These storms appeared in episodes. The first three in early 2004, late 2004 (dragon storm) and early 2006 (observed by Erick Bondoux and Jean-Luc Dauvergne [8] ) lasted for a couple of months. The episode beginning in late 2007 and lasting the first half of 2008 was a long episode. With the beginning of 2009 storms were erupting continuously in the southern hemisphere "storm allay" until the eruption of the 2010 GWS in the northern hemisphere. During the Voyager 2 flyby in 1981 a similar "storm alley" was observed in the northern hemisphere (33.5°N–38°N) at the position of the 1903 and 2010 GWSs. [5]

No southern GWS was discovered so far. This could be due to an observational bias in the visibility of the southern hemisphere. In the near future between 2025 and 2038 Saturns southern hemisphere will be visible, giving observers the possibility to observe a southern GWS. If such southern GWS exists and behaves similar to most northern GWS, the next GWS could occur after May 12, 2032 when the south pole of Saturn is most inclined towards to the sun. [5]

That none were recorded before 1876 is a mystery, in some ways akin to the long observational gap of the Great Red Spot in the 18th and early 19th centuries; the 1876 Great White Spot (GWS) was extremely prominent, being visible in apertures as small as 60 mm. It is not known if the earlier record was simply poor, or if the 1876 GWS was truly a first for the telescopic era. Some believe that neither scenario is likely.[ clarification needed ] [9]

In 1992, Mark Kidger described three significant GWS patterns:

  1. The GWSs alternate in latitude, with one apparition being limited to the North Temperate Zone (NTZ) or higher, and the following being limited to the Equatorial Zone (EZ). For instance, the 1960 GWS was high-latitude, and the 1990 GWS was equatorial.
  2. The high-latitude GWSs recur at a slightly shorter interval than the equatorial GWSs (~27 versus ~30 years).
  3. The high-latitude GWSs tend to be much less prominent than their equatorial counterparts.

Based on these apparent regularities, in 1992 Kidger forecasted (incorrectly, given the 2010–2011 storm) that the next GWS would occur in the North Temperate Zone in 2016, and would probably be less spectacular than the 1990 GWS. [10]

Characteristics and causes

The Great White Spot typically begins as discrete "spots", but then rapidly expands in longitude, as the 1933 and 1990 GWSs did; in fact, the latter eventually lengthened enough to encircle the planet. [11] The storms usually form a complex "head" that grows in size over a few days reaching sizes larger than 10,000 km. This head creates a wake that encircles the planet, creating a planetary-scale storm. The 1990 and 2010 GWSs did rise 40-50 km above the surrounding clouds and were more reflective. This high reflectance suggests that the particles in the storm are coated in fresh water ice. [5]

Though computer modelling had by the early 1990s suggested these massive atmospheric upwellings were caused by thermal instability, [12] in 2015 two Caltech planetary scientists proposed a more detailed mechanism. [13] The theory is that as Saturn's upper atmosphere undergoes seasonal cooling, it first gets less dense as the heavier water rains out, passes a density minimum, and then gets more dense as the remaining hydrogen and helium continue to cool. Low-density upper-layer gases tend to suppress convection, but high-density upper layers are unstable and cause a thunderstorm when they break into lower layers. The theory is that storms are significantly delayed from the winter solstice due to the time it takes for the very large atmosphere to cool. The team proposes that similar storms are not seen on Jupiter because that planet has less water vapor in its upper atmosphere.

The storm head of the 2010 GWS was probably made up by 55% ammonia, 22% water ice and 23% ammonium hydrosulfide. The water ice is delivered by powerful convections originating from about 200 km deep in Saturn's atmosphere. [14] The 2010 GWS also had an increased level of lightning. It had 10 Saturn Electrostatic Discharges (SED) per second, while synoptic-scale storms on Saturn had a few SEDs per seconds. [5]

Saturn's rings block the view of the northern hemisphere from Earth during the winter solstice, so historical data on the GWS is unavailable during this season, [15] but the Cassini space probe has been able to observe the whole planet since it arrived shortly after the winter solstice in 2004. [16]

Saturn Storm Panoramas.jpg
Panorama views of the GWS taken on Feb. 26, 2011 with the Cassini probe. The images show the GWS in near-infrared.

See also

Related Research Articles

<span class="mw-page-title-main">Saturn</span> Sixth planet from the Sun

Saturn is the sixth planet from the Sun and the second largest in the Solar System, after Jupiter. It is a gas giant, with an average radius of about nine times that of Earth. It has an eighth the average density of Earth, but is over 95 times more massive. Even though Saturn is almost as big as Jupiter, Saturn has less than a third the mass of Jupiter. Saturn orbits the Sun at a distance of 9.59 AU (1,434 million km), with an orbital period of 29.45 years.

<span class="mw-page-title-main">Uranus</span> Seventh planet from the Sun

Uranus is the seventh planet from the Sun. It is a gaseous cyan-coloured ice giant. Most of the planet is made of water, ammonia, and methane in a supercritical phase of matter, which astronomy calls "ice" or volatiles. The planet's atmosphere has a complex layered cloud structure and has the lowest minimum temperature of all the Solar System's planets. It has a marked axial tilt of 82.23° with a retrograde rotation period of 17 hours and 14 minutes. This means that in an 84-Earth-year orbital period around the Sun, its poles get around 42 years of continuous sunlight, followed by 42 years of continuous darkness.

<span class="mw-page-title-main">Titan (moon)</span> Largest moon of Saturn and second-largest moon in Solar System

Titan is the largest moon of Saturn and the second-largest in the Solar System. It is the only moon known to have an atmosphere denser than the Earth's and is the only known object in space—other than Earth—on which there is clear evidence that stable bodies of liquid exist. Titan is one of seven gravitationally rounded moons of Saturn and the second-most distant among them. Frequently described as a planet-like moon, Titan is 50% larger in diameter than Earth's Moon and 80% more massive. It is the second-largest moon in the Solar System after Jupiter's Ganymede and is larger than Mercury; yet Titan is only 40% as massive as Mercury, because Mercury is mainly iron and rock while much of Titan is ice, which is less dense.

<span class="mw-page-title-main">Great Red Spot</span> Persistent storm in Jupiters atmosphere

The Great Red Spot is a persistent high-pressure region in the atmosphere of Jupiter, producing an anticyclonic storm that is the largest in the Solar System. It is the most recognizable feature on Jupiter, owing to its red-orange color whose origin is still unknown. Located 22 degrees south of Jupiter's equator, it produces wind-speeds up to 432 km/h (268 mph). It was first observed in September 1831, with 60 recorded observations between then and 1878, when continuous observations began. A similar spot was observed from 1665 to 1713; if this is the same storm, it has existed for at least 359 years, but a study from 2024 suggests this is not the case.

<i>Cassini–Huygens</i> NASA/ESA mission sent to study Saturn and its moons (1997–2017)

Cassini–Huygens, commonly called Cassini, was a space-research mission by NASA, the European Space Agency (ESA), and the Italian Space Agency (ASI) to send a space probe to study the planet Saturn and its system, including its rings and natural satellites. The Flagship-class robotic spacecraft comprised both NASA's Cassini space probe and ESA's Huygens lander, which landed on Saturn's largest moon, Titan. Cassini was the fourth space probe to visit Saturn and the first to enter its orbit, where it stayed from 2004 to 2017. The two craft took their names from the astronomers Giovanni Cassini and Christiaan Huygens.

<span class="mw-page-title-main">Iapetus (moon)</span> Moon of Saturn

Iapetus is the outermost of Saturn's large moons. With an estimated diameter of 1,469 km (913 mi), it is the third-largest moon of Saturn and the eleventh-largest in the Solar System. Named after the Titan Iapetus, the moon was discovered in 1671 by Giovanni Domenico Cassini.

<span class="mw-page-title-main">Great Dark Spot</span> Large storm in Neptunes atmosphere

The Great Dark Spot was one of a series of dark spots on Neptune similar in appearance to Jupiter's Great Red Spot. In 1989, GDS-89 was the first Great Dark Spot on Neptune to be observed by NASA's Voyager 2 space probe. Like Jupiter's spot, the Great Dark Spots are anticyclonic storms. However, their interiors are relatively cloud-free, and unlike Jupiter's spot, which has lasted for hundreds of years, their lifetimes appear to be shorter, forming and dissipating once every few years or so. Based on observations taken with Voyager 2 and since then with the Hubble Space Telescope, Neptune appears to spend somewhat more than half its time with a Great Dark Spot. Little is known about the origins, movement, and disappearance of the dark spots observed on the planet since 1989.

<span class="mw-page-title-main">Rings of Saturn</span>

The rings of Saturn are the most extensive and complex ring system of any planet in the Solar System. They consist of countless small particles, ranging in size from micrometers to meters, that orbit around Saturn. The ring particles are made almost entirely of water ice, with a trace component of rocky material. There is still no consensus as to their mechanism of formation. Although theoretical models indicated that the rings were likely to have formed early in the Solar System's history, newer data from Cassini suggested they formed relatively late.

<span class="mw-page-title-main">Magnetosphere of Saturn</span> Cavity in the solar wind the sixth planet creates

The magnetosphere of Saturn is the cavity created in the flow of the solar wind by the planet's internally generated magnetic field. Discovered in 1979 by the Pioneer 11 spacecraft, Saturn's magnetosphere is the second largest of any planet in the Solar System after Jupiter. The magnetopause, the boundary between Saturn's magnetosphere and the solar wind, is located at a distance of about 20 Saturn radii from the planet's center, while its magnetotail stretches hundreds of Saturn radii behind it.

<span class="mw-page-title-main">Dragon Storm (astronomy)</span> Thunderstorm on Saturn

The Dragon Storm is a giant thunderstorm located in Saturn's Southern hemisphere, which is labeled as the "storm alley" region. The storm could have a range of 2,000 miles (3,200 km) or more, and can be compared to the electric thunderstorms of Earth. It acquires its energy in the deep layers of Saturn's atmosphere and produces radio waves that reflect during its burst of short static which helped Cassini detect it.

<span class="mw-page-title-main">Small Dark Spot</span> Southern cyclonic storm on the planet Neptune

The Small Dark Spot, sometimes also called Dark Spot 2 or The Wizard's Eye, was an extraterrestrial vortex on the planet Neptune. It was the second largest southern cyclonic storm on the planet in 1989, when Voyager 2 flew by the planet. When the Hubble Space Telescope observed Neptune in 1994, the storm had disappeared.

An extraterrestrial vortex is a vortex that occurs on planets and natural satellites other than Earth that have sufficient atmospheres. Most observed extraterrestrial vortices have been seen in large cyclones, or anticyclones. However, occasional dust storms have been known to produce vortices on Mars and Titan. Various spacecraft missions have recorded evidence of past and present extraterrestrial vortices. The largest extraterrestrial vortices are found on the gas giants, Jupiter and Saturn; and the ice giants, Uranus and Neptune.

<span class="mw-page-title-main">Atmosphere of Uranus</span> Layer of gases surrounding the planet Uranus

The atmosphere of Uranus is composed primarily of hydrogen and helium. At depth, it is significantly enriched in volatiles such as water, ammonia, and methane. The opposite is true for the upper atmosphere, which contains very few gases heavier than hydrogen and helium due to its low temperature. Uranus's atmosphere is the coldest of all the planets, with its temperature reaching as low as 49 K.

<span class="mw-page-title-main">Climate of Titan</span>

The climate of Titan, the largest moon of Saturn, is similar in many respects to that of Earth, despite having a far lower surface temperature. Its thick atmosphere, methane rain, and possible cryovolcanism create an analogue, though with different materials, to the climatic changes undergone by Earth during the far shorter year of Earth.

<span class="mw-page-title-main">Climate of Uranus</span> Weather of Uranus

The climate of Uranus is heavily influenced by both its lack of internal heat, which limits atmospheric activity, and by its extreme axial tilt, which induces intense seasonal variation. Uranus's atmosphere is remarkably bland in comparison to the other giant planets which it otherwise closely resembles. When Voyager 2 flew by Uranus in 1986, it observed a total of ten cloud features across the entire planet. Later observations from the ground or by the Hubble Space Telescope made in the 1990s and the 2000s revealed bright clouds in the northern (winter) hemisphere. In 2006 a dark spot similar to the Great Dark Spot on Neptune was detected.

<span class="mw-page-title-main">Equator</span> Imaginary line halfway between Earths North and South poles

The equator is a circle of latitude that divides a spheroid, such as Earth, into the Northern and Southern hemispheres. On Earth, the Equator is an imaginary line located at 0 degrees latitude, about 40,075 km (24,901 mi) in circumference, halfway between the North and South poles. The term can also be used for any other celestial body that is roughly spherical.

<span class="mw-page-title-main">Atmosphere of Jupiter</span> Layer of gases surrounding the planet Jupiter

The atmosphere of Jupiter is the largest planetary atmosphere in the Solar System. It is mostly made of molecular hydrogen and helium in roughly solar proportions; other chemical compounds are present only in small amounts and include methane, ammonia, hydrogen sulfide, and water. Although water is thought to reside deep in the atmosphere, its directly-measured concentration is very low. The nitrogen, sulfur, and noble gas abundances in Jupiter's atmosphere exceed solar values by a factor of about three.

<span class="mw-page-title-main">Saturn's hexagon</span> Hexagonal cloud pattern around north pole of Saturn

Saturn's hexagon is a persistent approximately hexagonal cloud pattern around the north pole of the planet Saturn, located at about 78°N. The sides of the hexagon are about 14,500 km (9,000 mi) long, which is about 2,000 km (1,200 mi) longer than the diameter of Earth. The hexagon may be a bit more than 29,000 km (18,000 mi) wide, may be 300 km (190 mi) high, and may be a jet stream made of atmospheric gases moving at 320 km/h (200 mph). It rotates with a period of 10h 39m 24s, the same period as Saturn's radio emissions from its interior. The hexagon does not shift in longitude like other clouds in the visible atmosphere.

<span class="mw-page-title-main">Amy Simon</span> American planetary scientist

Amy Simon is an American planetary scientist at NASA's Goddard Space Flight Center, involved in several missions of the Solar System Exploration Program.

Saturn Electrostatic Discharges are atmospheric lightning events in convective weather storms on Saturn that produce high frequency (HF) radio emissions (1-40 MHz). Terrestrial lighting events on Earth, in comparison, occur in the very low frequency (VLF) radio band, between 3 Hz and 30 kHz. This makes SED signals at least 10,000 times stronger. While first discovered by NASA's Voyager 1 mission, the scientific community has gained further understanding through the following Voyager 2 and Cassini missions in conjunction with ground-based observation and data gathering methods.

References

  1. 1 2 Cassini Helps Solve Saturn’s Mysterious Great White Spots | Space Exploration | Sci-News.com
  2. 1 2 Mann, Adam. "Saturn Storm Creates Largest and Hottest Vortex Ever Seen in Solar System". Wired.
  3. Krishnan, Shweta (May 20, 2011). "Dissecting Saturn's Big Storm". Sky & Telescope . Archived from the original on September 10, 2012. Retrieved May 22, 2011.
  4. NASA: Rare, enormous gas storm detected on Saturn - CNN.com
  5. 1 2 3 4 5 6 7 8 9 Sánchez-Lavega, Agustín; Fischer, Georg; Li, Cheng; García-Melendo, Enrique; del Río-Gaztelurrutia, Teresa (2024-01-01). "Moist Convective Storms on Saturn". arXiv: 2401.13294 [astro-ph.EP].
  6. "Vast Storm Rampages Across Saturn: Discovery News". Archived from the original on 2011-09-03. Retrieved 2011-01-08.
  7. HubbleSite - NewsCenter - Hubble Observes A New Saturn Storm (12/21/1994) – Release Text
  8. "APOD: 2006 January 27 - A New Storm on Saturn". apod.nasa.gov. Retrieved 2024-07-30.
  9. Kidger (1992) p. 179
  10. Kidger (1992) p. 180
  11. Kidger (1992) p. 187-189
  12. Kidger (1992) p. 211-212
  13. Explaining Saturn’s Great White Spots | Caltech
  14. Sromovsky, L. A.; Baines, K. H.; Fry, P. M. (2013-09-01). "Saturn's Great Storm of 2010-2011: Evidence for ammonia and water ices from analysis of VIMS spectra". Icarus. 226 (1): 402–418. arXiv: 1502.05893 . Bibcode:2013Icar..226..402S. doi:10.1016/j.icarus.2013.05.043. ISSN   0019-1035.
  15. Kidger (1992) p. 213-214
  16. Cassini Solstice Mission: Introduction archive

Notes