Cthulhu Macula

Belton Regio (formerly Cthulhu Macula or Cthulhu Regio) is a prominent surface feature of the dwarf planet Pluto. It is an elongated dark region along Pluto's equator, long and one of the darkest features on its surface.

After its discovery in 2015, the feature was provisionally named after the fictional deity Cthulhu from the works of H. P. Lovecraft and others, as it was most popular name in its category in an online poll conducted earlier that year. In 2023, an official name was adopted by the International Astronomical Union honoring astronomer Michael J. Belton.

Naming

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.

Surface features of Pluto were initially given provisional, informal names that are selected from a list generated from an online poll conducted earlier in 2015, along the theme of "creatures related to underworld mythologies." "Cthulhu" was the most popular name in this category of the poll, and by 14 July 2015, it was used by the ''New Horizons'' team to refer to the feature. It was named after the fictional deity from the works of H. P. Lovecraft and others, which 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 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.

The name received positive reaction from the press and social media, with a ''Chicago Tribune'' editorial supporting the name and its democratic origin. It was reported that the name Cthulhu may be submitted to the IAU as an official name. Cthulhu Macula was initially called a regio, but was renamed as the largest of the maculae that span Pluto's equator.

On 22 September 2023, the name "Belton Regio" was approved by the International Astronomical Union (IAU) for the feature, after astronomer Michael J. Belton.

Description

The macula lies 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".

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. 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.

The presence of craters within Belton 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; however, some areas of Belton Regio 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 Belton Regio 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 Belton Regio 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. 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 Belton Regio. As of 30 July 2015, the eastern "head" region had been imaged in much higher resolution than the western "tail" region.

Belton Regio contains many craters and linear features that have also been given informal names. Oort Crater, K. Edgeworth Crater, and Elliot Crater are large craters along Belton's northern edge; Brinton Crater, Harrington Crater, and H. Smith Crater are near Belton's eastern edge, and Virgil Fossa and Beatrice Fossa are linear depressions in Belton's interior.

File:Head of Cthulhu 2.jpg, The "head" region of the Belton feature, with Sputnik Planitia at right
File:Pluto by LORRI, 9 July 2015.jpg, The "tail" region of Belton, 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.
File:NH-Pluto-TombaughRegio-MountainRange-20150714-IFV.jpg, This image shows a region at the border between Belton's "head" (left) and the light, flat Sputnik Planitia (right), with Hillary Montes at center.
File:Pluto - methane snow on Cthulhu Regio peaks.jpg, The white snow caps on a mountain range within Belton Regio (enhanced color, center) coincide with the spectral signature of methane ice (purple in false-color MVIC image, right).

See also

* Geography of Pluto
* Lovecraft (crater) – a crater on Mercury

References

External links

*

{{Pluto

Regions of Pluto
Cthulhu Mythos