.png) Shaded relief map, based on the LRO laser altimetry data. Peary is the large crater at center; north pole is situated on its northern (upper) rim | |
| Coordinates | 88°38′N24°24′E / 88.63°N 24.4°E /88.63; 24.4 |
|---|---|
| Diameter | 79 km |
| Depth | 1.5 km |
| Colongitude | 25° at sunrise |
| Eponym | Robert Peary |
Peary is the closest largelunarimpact crater to thelunar north pole. At this latitude the crater interior receives little sunlight, and portions of the southernmost region of the crater floor remain permanently cloaked in shadow. From theEarth the crater appears on the northern lunar limb, and is seen from the side.
Since Peary is located nearly on the limb of the Moon as viewed from Earth, high-quality images of the crater were not available until space probes started photographing the Moon; the first high-quality images came from the USLunar Orbiter 4 spacecraft.[1] Since it is located nearly at the lunar north pole, it was named after the polar explorerRobert Peary.[2]
Peary is nearly circular, with an outward bulge along the northeast rim. There is a gap in the southwestern rim, where it joins the slightly smaller craterFlorey. The outer rim of Peary is worn and eroded, creating a rugged mountainous ring that produces long shadows across the crater floor. The crater floor itself is relatively flat, but is marked by several small craterlets, particularly in the southeastern half. The southern third of the interior remains cloaked in shadows, and so its features can be readily discerned only by means of ranging methods (for example,laser altimetry).
Because of the low sun angle, the average temperature on the crater floor of Peary is between 30 and 40 K, one of the coldest locations in the Solar System.[3]
In 2004, a team led by DrBen Bussey ofJohns Hopkins University, using images taken by theClementine mission, determined that four mountainous regions on the rim of Peary appeared to remain illuminated for the entire lunar day.[4] These unnamed "peaks of eternal light" are due to the Moon's extremely small axial tilt, which also gives rise to permanent shadow at the bottoms of many polar craters.Clementine's images were taken during the northern lunar hemisphere's summer season, and more detailed lunar topography collected by theLunar Reconnaissance Orbiter (LRO) showed that no points on the Moon receive perpetual light during both winter and summer.[5]
The northern rim of Peary is considered a likely site for a futureMoon base,[6] due to this near-constant illumination, which would provide both a relatively stable temperature and a nearly uninterrupted solar power supply. It is also near permanently shadowed areas that may contain some quantity of frozen water.[7]
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