Tir Planitia Explained

Tir Planitia
Location:Tolstoj quadrangle, Mercury
Coordinates:0.8°N -176.1°W
Eponym:Persian word for Mercury

Tir Planitia is a large plain on the planet Mercury. The name Tir (تیر) is the Persian word for "Mercury",[1] and the name was approved in 1976.[2] It was first observed in detail by Mariner 10.[3] It lies between the large crater Mozart and the ancient Tolstoj basin.

Tir Planitia is one of four named plains that surround the Caloris basin (with Mearcair Planitia, Stilbon Planitia, and Odin Planitia). All of these plains are classified as smooth, as opposed to intracrater plains which have rougher topography. They also contain areas where kilometer-scale knobs protrude above the plains, and these areas are called the Odin Formation. The Odin Formation is interpreted as a mixture of impact melt and blocky basin ejecta, formed by the Caloris impact event.[4]

The crater Fet is near the center of Tir Planitia. Hovnatanian crater is southwest of Fet. The craters Amru Al-Qays and Nureyev are in northern Tir Planitia.

Notes and References

  1. Book: Grego . Peter . Venus and Mercury, and how to Observe Them . 2008 . Springer . 48 . 27 August 2020.
  2. Web site: Tir Planitia . . Gazetteer of Planetary Nomenclature . 20 August 2023.
  3. https://history.nasa.gov/SP-423/p82.htm SHADED RELIEF MAP OF THE TOLSTOJ QUADRANGLE OF MERCURY
  4. Denevi, B. W., Earnst, C. M., Prockter, L. M., and Robinson, M. S., 2018. The Geologic History of Mercury. In Mercury: The View After MESSENGER edited by Sean C. Solomon, Larry R. Nittler, and Brian J. Anderson. Cambridge Planetary Science. Section 6.3.3.