Nowadays, Hagal dune field is a topic that has captured the attention of people all over the world. From its impact on society to its relevance in popular culture, Hagal dune field has proven to be a topic worthy of exploration and discussion. With a vast reach and significant influence, it is no surprise that Hagal dune field is the center of attention in numerous debates and conversations. In this article, we will explore the importance of Hagal dune field and how it has shaped our world in ways we may not even realize. From its rich history to its future implications, there is no doubt that Hagal dune field will continue to be a topic of interest for many in the near future.
Hagal is the informal name of a dune field on Mars located below the north pole of Mars.[3][4] Its name derives from the sand dunes in Frank Herbert's novel Dune and the fictional planet Hagal.[4] It is located at coordinates 78.0° N latitude, 84.0° E longitude, and consists of linear and round dunes with a southeast slipface orientation.[4] It was one of the dune formations targeted for imaging by the HiRISE camera, on board the Mars Reconnaissance Orbiter, at the rate of one image every six weeks. in the third year (MY31–Mars Year 31)[5] of its seasonal expedition.[4] It is also known as the "Martian Morse Code" due to the linear and rounded formations of its dunes, which have the appearance of dots and dashes.[3][1][6][7]
Although normally it is possible to obtain information about the wind direction from the orientation and form of sand dunes, the complexity of shapes of the Hagal dunes makes it difficult to determine the direction of the forming winds. In the case of the Hagal dunes, it is theorised that a local circular crater, probably formed due to meteorite impact and filled with sand, has decreased the quantity of dune-forming sand; this, in turn, impacted the local topography, causing a change in wind patterns.[3][1]
The linear dunes (dashes) were formed through the action of bidirectional winds, acting perpendicular to the line of the sand dune, causing a funneling effect directing the sand to accumulate along the linear axis of the dune. The round-shaped dunes (dots) were formed when the winds that caused the linearly-shaped accumulations were interrupted. The round dunes are classified as "barchanoid dunes". However, the exact mechanism of either formation is still unknown and this is the reason the area was chosen for imaging by the HiRISE mission.[1]
Veronica Bray, HiRISE camera targeting specialist, commented that there are similarly shaped dunes in other locations on Mars, but the Hagal field provides better images of these shapes due to the uncommon characteristics of its topography. Bray also decoded the "Morse Code" of a formation as "NEE NED ZB 6TNN DEIBEDH SIEFI EBEEE SSIEI ESEE SEEE !!".[8][9]
Please see note at Table 1 page 883: Table 1 Sites imaged systematically by HiRISE in study year 3 (MY31) of seasonal campaign. The names are informal, some based on the sand dunes in the science fiction book Dune.
Six sites were discovered in the northern summer of Mars Year 29 (MY29), seven in MY30, and seven in MY31. (MY refers to the Mars calendar of Clancy et al. , and this notation will be used throughout this paper; years begin at LS = 0°, the beginning of northern spring. MY32 began on 31 July 2013.)
NASA calls the formation the "Martian Morse Code,"