Sinus Iridum

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Sinus Iridum
Wac sinus iridum300m.png
Annotated Sinus Iridum by LRO
Coordinates 44°06′N 31°30′W / 44.1°N 31.5°W / 44.1; -31.5Coordinates: 44°06′N 31°30′W / 44.1°N 31.5°W / 44.1; -31.5
Diameter 236 km
Eponym Bay of Rainbows
Detail map of Imbrium's features. Sinus Iridum is the feature marked "A".

Sinus Iridum (Latin for "Bay of Rainbows") is a plain of basaltic lava that forms a northwestern extension to the Mare Imbrium on Earth's moon. It is surrounded from the northeast to the southwest by the Montes Jura range. Close to the bay in the range in the northwest is the crater Bianchini; west of the bay is the crater Sharp. The protruding part of the range at the southwest end is named Promontorium Heraclides, while that at the northeast end is called Promontorium Laplace. This bay and the surrounding mountains is considered one of the most beautiful features on the Moon, and is a favorite among lunar observers.

Sinus Iridum is formed from the remains of a large impact crater, which was subsequently flooded with basaltic lava, inundating the "sea" wall. The bay itself does not contain any notable impact craters, but does include the satellite crater Heraclides E in the south, Laplace A along the eastern edge, and Bianchini G in the north. The surface is level, but is marked by a number of wrinkle ridges (dorsa).

The selenographic coordinates of this bay are 44.1° N, 31.5° W, and the diameter is 236 km.[1]


View of Sinus Iridium and its surrounding features at about 100 km above the lunar surface as taken by the Kaguya spacecraft on October 31, 2007, this was the first high definition image of the Moon

One of the first image including video by JAXA's probe Kaguya were taken and recorded alongside Montes Jura and Mare Imbrium and the promontories of Heraclides and Laplace on October 31, 2007. The spacecraft took the world's first high definition image data of the Moon from an altitude about 100 kilometers away from the Moon on October 31, 2007.[2]

It was the planned landing site of Chang'e 3, China's 2013 lunar exploration mission, which instead landed nearby in Mare Imbrium.


The feature was given the Latin name for the Bay of Rainbows by Giovanni Riccioli, whose 1651 nomenclature system has become standardized.[3] Earlier lunar cartographers had given the feature different names: Michael van Langren's 1645 map calls it "Sinus Geometricus", the "Bay of Geometry" referring to its geometric shape.[4], and Johannes Hevelius called it "Sinus Apollonis" after Apollo, a bay in the north of Africa.[5]

Satellite craters[edit]

By convention these features are identified on lunar maps by placing the letter on the side of the crater midpoint that is closest to Promontorium Heraclides.

Heraclides Latitude Longitude Diameter
A 40.9° N 34.2° W 6 km
E 42.9° N 32.7° W 4 km
F 38.5° N 33.7° W 3 km

The following satellite craters are associated with the Promontorium Laplace.

Laplace Latitude Longitude Diameter
A 43.7° N 26.8° W 9 km
B 51.3° N 19.8° W 5 km
D 47.3° N 25.5° W 11 km
E 50.3° N 19.8° W 6 km
F 45.6° N 19.8° W 6 km
L 51.7° N 21.0° W 7 km
M 52.2° N 19.9° W 6 km

External links[edit]


  1. ^ "Gazetteer of Planetary Nomenclature - Sinus Iridum". United States Geological Survey. International Astronomical Union (IAU). 18 October 2010. Retrieved 2013-12-04. 
  2. ^ "Mare Imbrium on HDTV". Kaguya. October 31, 2007. 
  3. ^ Ewen A. Whitaker, Mapping and Naming the Moon (Cambridge University Press, 1999), p.211.
  4. ^ Ewen A. Whitaker, Mapping and Naming the Moon (Cambridge University Press, 1999), p. 197.
  5. ^ Ewen A. Whitaker, Mapping and Naming the Moon (Cambridge University Press, 1999), p. 202.