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Cthulhu macula

The meaning of «cthulhu macula»

Cthulhu Macula (formerly Cthulhu Regio[1][2]) is a prominent surface feature of the dwarf planet Pluto, that is reminiscent of a whale in shape. It is an elongated dark region along Pluto's equator, 2,990 km (1,860 mi) long and one of the darkest features on Pluto.[3] It is west of the Sputnik Planitia region of Tombaugh Regio, also known as Pluto's "heart", and to the east of Meng-P'o, the easternmost of Pluto's "Brass Knuckles".[4]

The dark color of the region is speculated to be the result of a "tar" made of complex hydrocarbons called tholins covering the surface, which form from methane and nitrogen in the atmosphere interacting with ultraviolet light and cosmic rays.[5][6][7] Tholins have been observed on other planetary bodies, such as Iapetus, Umbriel, and in the atmosphere of Titan, although the irregular and disconnected nature of the dark spots on Pluto has not yet been explained.[5] The presence of craters within Cthulhu indicates that it is perhaps billions of years old, in contrast to the adjacent bright, craterless Sputnik Planitia, which may be as little as 100 million years old;[8] however, some areas of Cthulhu Macula are smoother and much more modestly cratered, and may be intermediate in age. The eastern 'head' region consists mostly of heavily cratered 'alpine' terrain. The middle part of Cthulhu Macula is meanwhile a smooth plain, probably formed through large cryovolcanic eruptions, like Vulcan Planum on Charon. This part appears to be younger than the alpine terrain to the east, but there are nevertheless several large craters located in this region. The western 'tail' region of Cthulhu Macula was imaged in much lower resolution than the eastern part, but it can be inferred that this is a hilly landscape bordered by mountains to the west.[9][10][11] Higher-resolution images of the border between the two regions indicate that lighter material from Sputnik Planitia, composed of nitrogen, carbon monoxide, and methane ices, may be invading and overlaying the easternmost part of the dark Cthulhu Macula.[12] As of 30 July 2015, the eastern "head" region had been imaged in much higher resolution than the western "tail" region.[13]

The "head" region of the Cthulhu feature, with Sputnik Planitia at right

The "tail" region of Cthulhu, at the bottom of this image. The "head" extends beyond the right side of the visible portion of Pluto. Meng-P'o is visible at the extreme bottom left.

This image shows a region at the border between Cthulhu's "head" (left) and the light, flat Sputnik Planitia (right), with Hillary Montes at center.

The white snow caps on a mountain range within Cthulhu Macula (enhanced color, center) coincide with the spectral signature of methane ice (purple in false-color MVIC image, right).

The feature was first identified in the initial image, first published on 8 July 2015, of Pluto returned after the New Horizons probe recovered from an anomaly that temporarily sent it into safe mode. NASA initially referred to it as the Whale in reference to its overall shape.[14] By 14 July 2015, the provisional name "Cthulhu" was being used by the New Horizons team. It was named after the fictional deity from the works of H. P. Lovecraft and others.[4] The character Cthulhu initially appeared in Lovecraft's 1928 short story "The Call of Cthulhu", as a malevolent entity hibernating within an underwater city in the South Pacific. In the book, it is the subject of worship by a number of human cults asserting that while it is currently trapped, Cthulhu will eventually return.[15] In many of Lovecraft's stories, particularly The Whisperer in Darkness, the transneptunian planet Yuggoth is implied to be the same as Pluto, which was discovered around the time Lovecraft was writing the stories.[16]

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