Han Kan (crater)

Last updated
Han Kan
Han Kan crater 7374372.png
MESSENGER NAC image
Planet Mercury
Coordinates 72°08′S146°24′W / 72.13°S 146.40°W / -72.13; -146.40
Quadrangle Bach
Diameter 50.0 km (31.1 mi)
Eponym Han Gan

Han Kan is a crater on Mercury. It has a diameter of 50 kilometers. [1] Its name was adopted by the International Astronomical Union (IAU) in 1985. Han Kan is named for the Chinese painter Han Gan, who lived from 720 to 780. [2]

On the eastern floor of Han Kan is a dark spot of low reflectance material (LRM), closely associated with hollows. [3]

Han Kan has an extensive ray system extending for hundreds of kilometers.

Related Research Articles

<span class="mw-page-title-main">Matisse (crater)</span> Crater on Mercury

Matisse is an impact crater on the southern hemisphere of Mercury. Matisse takes its name from the French artist Henri Matisse, and it was named by the IAU in 1976.

<span class="mw-page-title-main">Mozart (crater)</span> Crater on Mercury

Mozart is a crater on Mercury, named by the IAU in 1976 after Austrian composer Wolfgang Amadeus Mozart.

<span class="mw-page-title-main">Eminescu (crater)</span> Crater on Mercury

Eminescu is a peak ring crater on Mercury 125 kilometers (78 mi) in diameter. Since there are very few later craters superposed on it, Eminescu appears to be a young crater formed around one billion years ago. It has a transitional morphology between larger more complex impact basins like Raditladi and smaller simpler central peak craters.

<span class="mw-page-title-main">Xiao Zhao (crater)</span> Crater on Mercury

Xiao Zhao crater is small in comparison with many other craters on Mercury. However, Xiao Zhao's long bright rays make it a readily visible feature. The fresh, bright rays, which were created by material ejected outward during the impact event that formed the crater, indicate that Xiao Zhao is a relatively young crater on Mercury's surface.

<span class="mw-page-title-main">Sander (crater)</span> Crater on Mercury

Sander is a crater on Mercury within Caloris Basin. It has dark walls and bright patches on its floor. Unlike the rays of Bashō crater, the bright areas are not believed to be immature, but they are inherently bright. It is named after the German photographer August Sander (1876–1964).

<span class="mw-page-title-main">Amaral (crater)</span> Crater on Mercury

Amaral is a crater on the planet Mercury. With its smooth floor, surrounding ejecta, and small secondary craters, it appears noticeably younger than the heavily cratered surface around it. Along with a smooth crater floor, Amaral also has a central peak. Bright material on this peak is of particular interest as it appears to have an unusual color. In color-enhanced images, the central peak of Amaral appears as a bright blue color in striking contrast to the otherwise orange tones of surface material nearby. The different color of the central peak likely indicates rocks with different chemical composition from those on the neighboring surface.

<span class="mw-page-title-main">Berkel (crater)</span> Crater on Mercury

Berkel is a crater on the planet Mercury. Its name was approved by the IAU on July 9, 2009. It was named after the modernist painter Sabri Berkel.

<span class="mw-page-title-main">Alencar (crater)</span> Crater on Mercury

Alencar is a crater on Mercury. It has a diameter of 120 kilometers. Its name was adopted by the International Astronomical Union (IAU) in 1979. Alencar is named for the Brazilian novel writer José de Alencar, who lived from 1829 to 1877.

<span class="mw-page-title-main">Bartók (crater)</span> Crater on Mercury

Bartók is a crater on Mercury. Its name was adopted by the International Astronomical Union (IAU) in 1979. Bartók is named for the Hungarian composer Béla Bartók, who lived from 1881 to 1945.

<span class="mw-page-title-main">Bello (crater)</span> Crater on Mercury

Bello is a crater on Mercury. It has a diameter of 129 kilometers. Its name was adopted by the International Astronomical Union (IAU) in 1976. Bello is named for the Venezuelan poet Andrés Bello, who lived from 1781 to 1865.

<span class="mw-page-title-main">Kipling (crater)</span> Crater on Mercury

Kipling is a crater on Mercury. It has a diameter of 164 kilometers. Its name was adopted by the International Astronomical Union (IAU) in 2010. Kipling is named for the British author Rudyard Kipling, who lived from 1865 to 1936.

<span class="mw-page-title-main">Balanchine (crater)</span> Crater on Mercury

Balanchine is a crater on the planet Mercury. It possesses a ray system of slightly bluish rays. These rays inspired the name of the crater due to their similarity to the tutu in George Balanchine's Serenade.

<span class="mw-page-title-main">Kulthum (crater)</span> Crater on Mercury

Kulthum is a crater on Mercury. It has a diameter of 31 kilometers. Its name was suggested by Molouk Ba-Isa from Saudi Arabia, Swiss individual Riana Rakotoarimanana, and American residents Yehya Hassouna, David Suttles, Thorayya Said Giovannelli and Matt Giovannelli in a naming contest which was eventually adopted by the International Astronomical Union (IAU) on 2015. Kulthum is named for the Egyptian singer Umm Kulthum.

<span class="mw-page-title-main">Tyagaraja (crater)</span> Crater on Mercury

Tyagaraja is a crater on Mercury. Its name was adopted by the International Astronomical Union in 1976. Tyagaraja is named for the Indian composer Tyagaraja.

<span class="mw-page-title-main">Alver (crater)</span> Crater on Mercury

Alver is a crater on Mercury. It has a diameter of 151.49 kilometers. Its name was adopted by the International Astronomical Union (IAU) on March 15, 2013. Alver is named for the Estonian poet Betti Alver.

<span class="mw-page-title-main">David (crater)</span> Crater on Mercury

David is a small crater on Mercury, which has a bright ray system. Its name was adopted by the International Astronomical Union (IAU) in 2013. David is named for the French painter Jacques-Louis David.

<span class="mw-page-title-main">Rustaveli (crater)</span> Crater on Mercury

Rustaveli is a crater on Mercury. Its name was adopted by the International Astronomical Union in 2012, after the Georgian poet Shota Rustaveli.

<span class="mw-page-title-main">Hafiz (crater)</span> Crater on Mercury

Hafiz is a crater on Mercury. It has a diameter of 280 kilometres. Its name was adopted by the International Astronomical Union (IAU) on June 23, 2014. Hafiz is named for the Persian poet Hafez.

<span class="mw-page-title-main">Heaney (crater)</span> Crater on Mercury

Heaney is a crater on Mercury. It has a diameter of 125 kilometres. Its name was adopted by the International Astronomical Union (IAU) on March 20, 2017. Heaney is named for the Irish poet and playwright Seamus Heaney.

<span class="mw-page-title-main">Sibelius (crater)</span> Crater on Mercury

Sibelius is a crater on Mercury. It has a diameter of 94 kilometres. Its name was adopted by the International Astronomical Union (IAU) in 1985. Sibelius is named for the Finnish composer Jean Sibelius.

References

  1. Moore, Patrick (2000). The Data Book of Astronomy. Institute of Physics Publishing. ISBN   0-7503-0620-3.
  2. "Han Kan". Gazetteer of Planetary Nomenclature. NASA . Retrieved 7 June 2022.
  3. Zhiyong Xiao, Robert G. Strom, David T. Blewett, Paul K. Byrne, Sean C. Solomon, Scott L. Murchie, Ann L. Sprague, Deborah L. Domingue, Jörn Helbert, 2013. Dark spots on Mercury: A distinctive low-reflectance material and its relation to hollows. Journal of Geophysical Research Planets. doi.org/10.1002/jgre.20115