Open main menu

Wikipedia β

Saturn - North polar hexagon and vortex as well as rings (April 2, 2014).

Saturn's hexagon is a persisting hexagonal cloud pattern around the north pole of Saturn, located at about 78°N.[1][2][3] The sides of the hexagon are about 13,800 km (8,600 mi) long, which is more than the diameter of Earth[4] (about 12,700 km (7,900 mi)). It rotates with a period of 10h 39m 24s, the same period as Saturn's radio emissions from its interior.[5] The hexagon does not shift in longitude like other clouds in the visible atmosphere.[6]

Saturn's hexagon was discovered during the Voyager mission in 1981 and was later revisited by Cassini-Huygens in 2006. During the Cassini mission, the hexagon changed from a mostly blue color to more of a golden color. Saturn's south pole does not have a hexagon, according to Hubble observations; however, it does have a vortex, and there is also a vortex inside the northern hexagon.[7] Multiple hypotheses for the hexagonal cloud pattern have been developed.



Saturn's polar hexagon discovery was made by the Voyager mission in 1981,[8] and it was revisited in 2006 by NASA's Cassini mission.[9] Cassini was only able to take thermal infrared images of the hexagon, until it passed into sunlight in January 2009.[10] Cassini was also able to take a video of the hexagonal weather pattern while traveling at the same speed as the planet, therefore recording only the movement of the hexagon.[11] After its discovery, and after it came back into the sunlight, amateur astronomers managed to get images showing the hexagon from Earth.[12]


2013 and 2017: hexagon color changes

Between 2012 and 2016, the hexagon changed from a mostly blue color to more of a golden color.[13] One theory for this is that sunlight is creating haze as the pole is exposed to sunlight due to the change in season. These changes were observed by the Cassini spacecraft.[13]

Explanations for hexagon shapeEdit

False-color image from the Cassini probe

One hypothesis, developed at Oxford University, is that the hexagon forms where there is a steep latitudinal gradient in the speed of the atmospheric winds in Saturn's atmosphere.[14] Similar regular shapes were created in the laboratory when a circular tank of liquid was rotated at different speeds at its centre and periphery. The most common shape was six sided, but shapes with three to eight sides were also produced. The shapes form in an area of turbulent flow between the two different rotating fluid bodies with dissimilar speeds.[14][15] A number of stable vortices of similar size form on the slower (south) side of the fluid boundary and these interact with each other to space themselves out evenly around the perimeter. The presence of the vortices influences the boundary to move northward where each is present and this gives rise to the polygon effect.[15] Polygons do not form at wind boundaries unless the speed differential and viscosity parameters are within certain margins and so are not present at other likely places, such as Saturn's south pole or the poles of Jupiter.

Other researchers claim that lab studies exhibit vortex streets, a series of spiraling vortices not observed in Saturn's hexagon. Simulations show that a shallow, slow, localized meandering jetstream in the same direction as Saturn's prevailing clouds is able to match the observed behaviors of Saturn's Hexagon with the same boundary stability.[16]

Rostami et al. [17] in their article demonstrate that developing barotropic instability of the Saturn's North Polar hexagonal circumpolar jet (Jet) plus North Polar vortex (NPV) system produces a long-living structure akin to the observed hexagon, which is not the case of the Jet-only system, which was studied in this context in a number of papers in literature. The north polar vortex (NPV), thus, plays a decisive dynamical role to stabilize hexagon jets. The influence of moist convection, which was recently suggested to be at the origin of Saturn's north polar vortex system in the literature, is investigated in the framework of the barotropic rotating shallow water model model and does not alter the conclusions.

See alsoEdit

Rostami et al. (2017)[18] published an article in ICARUS in which they explain detailed dynamics of Saturn's North Polar Hexagon and a few new discoveries related to stability of hexagon, linear stability analysis, appropriate range of Rossby deformation radius, nonlinear evolution of instability, dependence of hexagon on north polar vortex, etc. Furthermore, it is shown that why there is not the same hexagon on the south pole.


  1. ^ Godfrey, D. A. (1988). "A hexagonal feature around Saturn's North Pole". Icarus. 76 (2): 335. Bibcode:1988Icar...76..335G. doi:10.1016/0019-1035(88)90075-9. 
  2. ^ Sánchez-Lavega, A.; Lecacheux, J.; Colas, F.; Laques, P. (April 16, 1993). "Ground-based observations of Saturn's north polar SPOT and hexagon". Science. American Association for the Advancement of Science. 260 (5106): 329–32. Bibcode:1993Sci...260..329S. PMID 17838249. doi:10.1126/science.260.5106.329. 
  3. ^ Overbye, Dennis (August 6, 2014). "Storm Chasing on Saturn". New York Times. Retrieved August 6, 2014. 
  4. ^ "New images show Saturn's weird hexagon cloud". MSNBC. December 12, 2009. Archived from the original on 2011-10-05. Retrieved December 5, 2013. 
  5. ^ Godfrey, D. A. (March 9, 1990). "The Rotation Period of Saturn's Polar Hexagon". Science. 247 (4947): 1206–1208. Bibcode:1990Sci...247.1206G. PMID 17809277. doi:10.1126/science.247.4947.1206. 
  6. ^ Baines, Kevin H.; et al. (December 2009). "Saturn's north polar cyclone and hexagon at depth revealed by Cassini/VIMS". Planetary and Space Science. 57 (14–15): 1671–1681. Bibcode:2009P&SS...57.1671B. doi:10.1016/j.pss.2009.06.026. 
  7. ^ Sánchez-Lavega, A.; Pérez-Hoyos, S.; French, R. G. (October 8, 2002). "Hubble Space Telescope Observations of the Atmospheric Dynamics in Saturn's South Pole from 1997 to 2002". American Astronomical Society. American Astronomical Society. 34: 13.07. Bibcode:2002DPS....34.1307S. Archived from the original on September 5, 2008. Retrieved December 5, 2013. 
  8. ^ Caldwell, John; Benoit, Turgeon; Hua, Xin-Min; Barnet, Christopher D.; Westphal, James A. (April 16, 1993). "The Drift of Saturn's North Polar Spot Observed by the Hubble Space Telescope". Science. AAAS. 260 (5106): 326–329. Bibcode:1993Sci...260..326C. ISSN 0036-8075. PMID 17838248. doi:10.1126/science.260.5106.326. Retrieved December 5, 2013. 
  9. ^ "Saturn's Strange Hexagon". NASA. March 27, 2007. Retrieved May 1, 2013. 
  10. ^ "Saturn's Mysterious Hexagon Emerges From Winter Darkness". NASA. December 9, 2009. Retrieved May 1, 2013. 
  11. ^ Staff (December 4, 2013). "NASA's Cassini Spacecraft Obtains Best Views of Saturn Hexagon". Jet Propulsion Laboratory (NASA). Retrieved December 5, 2013. 
  12. ^ Fletcher, Leigh (February 1, 2013). "Saturn's Hexagon Viewed from the Ground". The Planetary Society. 
  13. ^ a b Staff (October 21, 2016). "Changing Colors in Saturn's North". NASA. Retrieved December 26, 2016. 
  14. ^ a b Barbosa Aguiar, Ana C.; Read, Peter L.; Wordsworth, Robin D.; Salter, Tara; Yamazaki, Y. Hiro (April 2010). "A laboratory model of Saturn's North Polar Hexagon". Icarus. 206 (2): 755–763. Bibcode:2010Icar..206..755B. doi:10.1016/j.icarus.2009.10.022. 
  15. ^ a b Lakdawalla, Emily (May 4, 2010). "Saturn's hexagon recreated in the laboratory". Retrieved 2014-02-07. 
  16. ^ Morales-Juberías, R.; Sayanagi, K.M.; Simon, A.A.; Fletcher, L.N.; Cosentino, R.G. (10 June 2015). "Meandering Shallow Atmospheric Jet as a Model of Saturn's North-Polar Hexagon". The Astrophysical Journal Letters. doi:10.1088/2041-8205/806/1/L18. 
  17. ^ Masoud Rostami and Vladimir Zeitlin, and Aymeric Spiga "On the dynamical nature of Saturn's North Polar hexagon", Icarus, 2017, doi:org/10.1016/j.icarus.2017.06.006. ,
  18. ^ Masoud Rostami and Vladimir Zeitlin, and Aymeric Spiga "On the dynamical nature of Saturn's North Polar hexagon", Icarus, 2017, doi:org/10.1016/j.icarus.2017.06.006. ,

External linksEdit