Vonnegut (crater)

Last updated
Vonnegut
Vonnegut crater EW0219776652G.jpg
MESSENGER image
Planet Mercury
Coordinates 82°43′N249°55′W / 82.72°N 249.91°W / 82.72; -249.91
Quadrangle Borealis
Diameter 26.61 km
Eponym Kurt Vonnegut

Vonnegut is a crater on Mercury, near the north pole. It was named by the IAU in 2017 after the American author Kurt Vonnegut. [1] Part of Vonnegut's 1959 novel The Sirens of Titan takes place on Mercury. The crater was referred to as e5 in scientific literature prior to naming. [2]

S band radar data from the Arecibo Observatory collected between 1999 and 2005 indicates a radar-bright area along the southern interior of Vonnegut, which is probably indicative of a water ice deposit, and lies within the permanently shadowed part of the crater. [3] [4] [5] MESSENGER 's Mercury Laser Altimeter (MLA) was used to measure surface reflectance of the surface of the planet, and the radar-bright material is covered by low-reflectance material. [2]

Radar-bright deposits near the north pole. Vonnegut is above center. Radar-bright Deposits near Mercury's North Pole messenger orbit image20120322.jpg
Radar-bright deposits near the north pole. Vonnegut is above center.

Vonnegut is north of the slightly larger Yoshikawa crater.

Related Research Articles

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

Chao Meng-Fu is a 167 km (104 mi) diameter crater on Mercury named after the Chinese painter and calligrapher Zhao Mengfu (1254–1322). Due to its location near Mercury's south pole and the planet's small axial tilt, an estimated 40% of the crater lies in permanent shadow. This combined with bright radar echoes from the location of the crater leads scientists to suspect that it may shelter large quantities of ice protected against sublimation into the near-vacuum by the constant −171 °C (−276 °F) temperatures.

<span class="mw-page-title-main">Geology of Mercury</span> Geologic structure and composition of planet Mercury

The geology of Mercury is the scientific study of the surface, crust, and interior of the planet Mercury. It emphasizes the composition, structure, history, and physical processes that shape the planet. It is analogous to the field of terrestrial geology. In planetary science, the term geology is used in its broadest sense to mean the study of the solid parts of planets and moons. The term incorporates aspects of geophysics, geochemistry, mineralogy, geodesy, and cartography.

A cold trap is a concept in planetary sciences that describes an area cold enough to freeze (trap) volatiles. Cold-traps can exist on the surfaces of airless bodies or in the upper layers of an adiabatic atmosphere. On airless bodies, the ices trapped inside cold-traps can potentially remain there for geologic time periods, allowing us a glimpse into the primordial solar system. In adiabatic atmospheres, cold-traps prevent volatiles from escaping the atmosphere into space.

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

Despréz is a crater on Mercury with a diameter of 47.05 kilometers. Its name was adopted by the International Astronomical Union (IAU) in 1979. Despréz is named for the French composer Josquin des Prez, who lived from 1440 to 1521.

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

Prokofiev is a crater near the north pole of the planet Mercury, named after the Russian composer Sergei Prokofiev. Data from the MESSENGER spacecraft indicates that it contains water ice and organic compounds. Although other craters in Mercury's north polar region are also believed to contain ice, Prokofiev is the largest of them, with probable surface ice along the southern crater floor that is in perpetual darkness.

<span class="mw-page-title-main">Permanently shadowed crater</span> Permanently shadowed region of a body in the Solar System

A permanently shadowed crater is a depression on a body in the Solar System within which lies a point that is always in darkness.

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

Kandinsky is a deep crater on Mercury, located near the planet's north pole. It was named by the IAU in 2012 for Russian painter Wassily Kandinsky.

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

Tolkien is one of the northernmost craters on Mercury, located in the Borealis quadrangle at 88.82 N, 211.08 W. It is 50 km in diameter. It was named after the South African born British writer J. R. R. Tolkien. The name was approved by IAU's Working Group for Planetary System Nomenclature on August 6, 2012. Since Tolkien is very close to the north pole, and Mercury has almost no axial tilt, Tolkien receives very little sunlight. S band radar data from the Arecibo Observatory collected between 1999 and 2005 indicates a radar-bright area covers the entire floor of Tolkien, which is probably indicative of a water ice deposit.

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

Carolan is a crater on Mercury. Its name was suggested by an Irishman, Fergal Donnelly, and two Americans, Joseph Brusseau and Deane Morrison, in a naming contest which was eventually adopted by the International Astronomical Union (IAU) on 2015. Carolan is named for the Irish composer and performer Turlough O'Carolan, who lived from 1670 to 1738 C.E. The craters Kulthum, Enheduanna, Karsh, and Rivera were also named as part of the contest.

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

Yoshikawa is a crater on Mercury, near the north pole. It was named by the IAU in 2012 after the Japanese novelist Eiji Yoshikawa.

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

Sapkota is a crater on Mercury, located near the north pole. It was named by the IAU in 2015, after Nepalese poet Mahananda Sapkota.

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

Laxness is a crater on Mercury, located near the north pole. It was named by the IAU in 2013, after Icelandic writer Halldór Laxness.

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

Fuller is a crater on Mercury, located near the north pole. It was named by the IAU in 2013, after American engineer and architect Richard Buckminster Fuller.

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

Tryggvadóttir is a crater on Mercury. The north pole of Mercury is located next to its northern rim. It was named by the IAU in 2012 after the Icelandic artist Nína Tryggvadóttir.

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

Chesterton is a crater on Mercury, near the north pole. Its name was adopted by the International Astronomical Union in 2012, after the English author G. K. Chesterton.

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

Gordimer is a crater on Mercury, near the north pole. Its name was adopted by the International Astronomical Union (IAU) in 2019, after the South African writer Nadine Gordimer.

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

Josetsu is a crater on Mercury, located near the north pole. Its name was adopted by the International Astronomical Union (IAU) in 2019. It is named for the Japanese painter Taikō Josetsu. The crater was referred to as o7 in scientific literature prior to naming.

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

Remarque is a crater on Mercury. Its name was adopted by the International Astronomical Union (IAU) on December 16, 2013. Remarque is named for the German author Erich Maria Remarque.

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

Petronius is a crater on Mercury. It has a diameter of 36 kilometres. Its name was adopted by the International Astronomical Union (IAU) on the August 6, 2012. Petronius is named for the Roman author Petronius.

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

Morrison is a crater on Mercury. Its name was adopted by the International Astronomical Union in September 2022. Morrison is named for the American author Toni Morrison, who lived from 1931 to 2019.

References

  1. "Vonnegut (crater)". Gazetteer of Planetary Nomenclature. USGS Astrogeology Research Program.
  2. 1 2 New evidence for surface water ice in small‐scale cold traps and in three large craters at the north polar region of Mercury from the Mercury Laser Altimeter, Ariel N. Deutsch, Gregory A. Neumann, James W. Head. 14 September 2017. Geophysical Research Letters, Volume 44, Issue 18. doi.org/10.1002/2017GL074723
  3. Chabot, N. L., D. J. Lawrence, G. A. Neumann, W. C. Feldman, and D. A. Paige, 2018. Mercury's Polar Deposits. In Mercury: The View After MESSENGER edited by Sean C. Solomon, Larry R. Nittler, and Brian J. Anderson. Cambridge Planetary Science. Chapter 13, Figure 13.2.
  4. PIA19411: Water Ice on Mercury, NASA/Johns Hopkins University Applied Physics Laboratory/Carnegie Institution of Washington
  5. John K. Harmon, Martin A. Slade, Melissa S. Rice, 2011. Radar imagery of Mercury’s putative polar ice: 1999–2005 Arecibo results. Icarus, 211, p37-50. doi.org/10.1016/j.icarus.2010.08.007