Sholem Aleichem (crater)

Last updated
Sholem Aleichem
EN0108821596M Sholem Aleichem crater on Mercury.png
MESSENGER photo of Sholem Aleichem in lower right foreground
Planet Mercury
Coordinates 51°00′N56°30′W / 51°N 56.5°W / 51; -56.5
Quadrangle Victoria
Diameter 190 km (120 mi)
Eponym Sholom Aleichem

Sholem Aleichem is a crater on Mercury, named after the Yiddish writer Sholem Aleichem. The inter-crater plain deposits have been deformed by linear ridges. [1]

Adjacent to the Sholem Aleichem crater to the southeast is the older and larger Vyāsa crater. Further to the east is Stravinsky crater. To the south and southeast are the similarly sized Al-Hamadhani crater and Scarlatti crater. To the west are To Ngoc Van crater and Bruegel crater. To the northwest is Al-Akhtal crater.

Hollows

Related Research Articles

<span class="mw-page-title-main">Sholem Aleichem</span> Russian Jewish author and playwright

Solomon Naumovich Rabinovich, better known under his pen name Sholem Aleichem, was a Yiddish author and playwright who lived in the Russian Empire and in the United States. The 1964 musical Fiddler on the Roof, based on Aleichem's stories about Tevye the Dairyman, was the first commercially successful English-language stage production about Jewish life in Eastern Europe.

<i>MESSENGER</i> Seventh mission of the Discovery program; orbital reconnaissance of the planet Mercury (2004–2015)

MESSENGER was a NASA robotic space probe that orbited the planet Mercury between 2011 and 2015, studying Mercury's chemical composition, geology, and magnetic field. The name is a backronym for "Mercury Surface, Space Environment, Geochemistry, and Ranging", and a reference to the messenger god Mercury from Roman mythology.

<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">Vyāsa (crater)</span> Crater on Mercury

Vyāsa is a crater on Mercury. It was named by the IAU in 1979, after the Indian poet Vyasa.

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

Apollodorus is an impact crater on Mercury. Its unusual appearance, with radiating dark troughs, led to a nickname of "the Spider" by scientists before its official name was decided. Apollodorus is located near the center of Pantheon Fossae, which is a system of radial grabens situated in the inner part of the Caloris basin. The floor, rim and walls of Apollodorus expose a low reflectance material (LRM) excavated during the impact from beneath the light volcanic plains, which cover the central part of the Caloris.

<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">Praxiteles (crater)</span> Crater on Mercury

Praxiteles is a crater on Mercury. It is one of 110 peak ring basins on Mercury.

<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">Raditladi (crater)</span> Crater on Mercury

Raditladi is a large impact crater on Mercury with a diameter of 263 km. Inside its peak ring there is a system of concentric extensional troughs (graben), which are rare surface features on Mercury. The floor of Raditladi is partially covered by relatively light smooth plains, which are thought to be a product of the effusive volcanism. The troughs may also have resulted from volcanic processes under the floor of Raditladi. The basin is relatively young, probably younger than one billion years, with only a few small impact craters on its floor and with well-preserved basin walls and peak-ring structure. It is one of 110 peak ring basins on Mercury.

<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">Calvino (crater)</span> Crater on Mercury

Calvino is a crater on Mercury. Its name was adopted by the IAU in 2016, after the Italian writer Italo Calvino.

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

Rachmaninoff is an impact crater on Mercury. This basin, first imaged in its entirety during MESSENGER's third Mercury flyby, was quickly identified as a feature of high scientific interest, because of its fresh appearance, its distinctively colored interior plains, and the extensional troughs on its floor. The morphology of Rachmaninoff is similar to that of Raditladi, which is one of the youngest impact basins on Mercury. The age of Raditladi is estimated at one billion years. Rachmaninoff appears to be only slightly older.

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

Derain is a crater on Mercury named after André Derain, a French artist, painter, sculptor and co-founder of Fauvism with Henri Matisse. It has uncommonly dark material within and surrounding the crater. The material is darker than the neighboring terrain such that this crater is easily identified even in a distant global image of Mercury. The dark halo may be material with a mineralogical composition different from the majority of Mercury's visible surface. Craters with similar dark material on or near their rims were seen on the floor of the Caloris basin during MESSENGER’s first flyby.

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

Dominici is a crater on Mercury. Dominici's bright rays indicate that it is relatively young, and the young rays appear light blue in enhanced-color images. Dominici also has bright material on its floor and is surrounded by crater ejecta and material that appears orange in enhanced color. These color differences, as in nearby Titian crater, suggest that the impact crater excavated material from beneath Mercury's surface that differs in composition from the surrounding surface. Dominici lies within a much larger impact structure, the Homer basin.

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

Ahmad Baba is a crater on Mercury. It has a diameter of 127 kilometers. Its name was adopted by the International Astronomical Union (IAU) in 1979.

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

Al-Hamadhani is a crater on Mercury. It has a diameter of 186 kilometers. Its name was adopted by the International Astronomical Union in 1979. Al-Hamadhani is named for the Iranian writer Badi' al-Zaman al-Hamadani, who died in 1007 C.E.

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

Balzac is a crater on Mercury. Its name was adopted by the International Astronomical Union in 1976. Balzac is named for the French writer Honoré de Balzac, who lived from 1799 to 1850.

<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">Dürer (crater)</span> Crater on Mercury

Dürer is a crater on Mercury. It has a diameter of 195 kilometers. Its name was adopted by the International Astronomical Union (IAU) in 1976. Durer is named for the German artist Albrecht Dürer, who lived from 1471 to 1528.

Hollows are a landform on the planet Mercury, discovered during the MESSENGER mission that orbited the planet from 2011 to 2015.

References

  1. "MESSENGER VIEWS MERCURY'S HORIZON" . Retrieved May 11, 2022.
  2. "MESSENGER - Featured Image March 12, 2014". Archived from the original on March 14, 2014. Retrieved May 11, 2022.