The Moon's North Pole

Lat: 90.0°N, Long: --, Rükl 4
external image normal_North_Pole-Galileo_LTVT.JPG
external image normal_North_Pole-Clementine_LTVT.JPG
Left: Galileo Spacecraft Image taken at a distance of 111623 km, from a position roughly over Mare Humboldtianum. The light is coming from the Moon’s Earthward side, and an astronaut standing at the Moon’s pole (marked by the intersection of the grid lines) would see the Sun’s upper limb in a horizontal direction (the Sun, at the Moon's pole, can be as much as 1.7° higher at favorable seasons). The labeled dots on the four craters around Byrd and Peary are part of the 1994 ULCN and the grid lines are based on them. Control points G1001 and G1002 (of the 1994 ULCN) have recently been named Whipple and Erlanger by the IAU. The deeply-shadowed circle at 4 o'clock from G1002/Erlanger is now known as Fibiger, the low circular basin to the left of G1003 has become Florey, and the shadowed crater touching the rim of Peary at about the 10 o'clock position is now known as Hinshelwood.
Right: Clementine Taken looking vertically down from 768 km. As seen from the pole, the Sun would have been shining from the Moon's farside with its center 0.9 degrees above the horizontal. The image has been matched to points of ULCN 2005 that were measured on this frame, resulting in a slight misregistration of the G1001/Whipple control point. The exact location of the Moon's north pole is probably uncertain by at least this much.

Images

LPOD Photo Gallery Smart-1 mosaic
  • An intermediate image, showing the location of the North Pole on a Lunar Orbiter image registered to the 1994 ULCN is also available.
  • Mosaic of LROC Narrow Angle Camera images of the north pole area.
  • Animation of illumination changes over a 1-year period assembled from LROC Wide Angle Camera images.

Maps

(LAC zone 1A1) USGS Digital Atlas PDF Lunar Orbiter version
  • note: the first of these two IAU nomenclature maps, using a color-coded shaded relief background, gives the impression that there is a crater of about the size of Hinshelwood tangent to the pole, and smaller craters between that and Whipple. These appear to be artistic artifacts. The Kaguya topo map (see below) shows no substantial craters at these locations.

Description

The Moon's north pole is the point at which its spin axis pierces the surface features at the end most northward as viewed from Earth. This axis is fixed relative to those features, although relative to the stars the direction of the spin axis precesses over a cycle of about 18.6 years.

Wikipedia


Additional Information

  • The location of the spin axis defines the 90° point in the most common system of lunar ("selenographic") coordinates (the "Mean Earth/Polar" system). The actual position of the pole must be determined by experiment, and gradual improvements in locating it necessitate small refinements in the coordinates of all surface features (as do improvements in the location of the Mean Earth point).
  • The Moon's north pole was designated a Constellation Program Region of Interest.
  • Mini-RF radar views
    mini-rf.jpg
    • Click image for larger view (~ 1.7 Mb)
    • Image above shows the first month's systematic polar mapping results obtained by the Mini-RF radar instrument onboard NASA's Lunar Reconnaissance Orbiter (LRO). The Mini-RF (Miniature Radio Frequency) instrument is specifically designed to map the lunar poles, and search for any potential water deposits that may lie hidden in permanently-shadowed craters. A similar instrument (Mini-SAR) was also launched in 2008 onboard the Indian spacecraft, Chandrayaan-1, that covered more than 90 precent of both polar regions. However, as that mission ended in August 2009, the data collected is used in tandem with this new data obtained by LRO. The images are mosaics of numerous images stitched together as taken by the Mini-RF, and cover regions from 70 degrees upwards to the poles (left-hand images = radar brightness, right-hand = circular polarisation ratio). - JohnMoore2 JohnMoore2

Topography

  • The following image is a preliminary map of the topography within 5° (in latitude) of the Moon's north pole created from data collected by the Kaguya laser altimeter as reported in the February 13, 2009 issue of Science magazine, with all current IAU feature names superimposed:

    • external image Kaguya_NorthPole_TopoMap.JPG?size=64 <- click to see full-sized image

    • Observers on Earth see this scene roughly as viewed looking up from the bottom, but with extreme foreshortening due to the highly oblique angle of view.

    • The Kaguya map is probably the best, and most accurate, information currently available regarding the locations and heights of the polar features. It is believed to be independent data based on celestial navigation of the spacecraft, but it agrees very well with the previous estimates of the pole's location. The misregistration of some of the circles representing IAU names is due to the imprecise coordinates listed in the IAU database (which are intended only to be close enough for unambiguous identification).

  • Informative, but still very preliminary, maps of both poles can also be found on the Diviner webpages -- a LRO instrument which, by imaging in the infrared, can show topographic details in shadowed regions.

Features Visible From Earth


The following thumbnails link to images showing three-dimensional simulations of the appearance of the Moon's north pole as seen from Earth with a maximum libration of +7° in latitude and with the Sun at its maximum northerly latitude of +1.6°. They were prepared using LTVT and the Kaguya north-polar digital elevation model. The nominal locations of the IAU feature names (not always accurate) are indicated by the white dots next to the names. The letters for the satellite features on the side towards the primary feature after which they are named (one of the two "U's" in the upper right is Rozhdestvenskiy U, the other is Plaskett U; the "A" at the left is Hermite A).

Waxing
Full
Waning
external image KaguyaDEM_NorthPole_fromEarth_IAU_names_1.jpg?size=64
external image KaguyaDEM_NorthPole_fromEarth_IAU_names_2.jpg?size=64
external image KaguyaDEM_NorthPole_fromEarth_IAU_names_3.jpg?size=64

The image on the left shows the pole with the subsolar point 60° east of the prime meridian (colongitude 30°). The center image is a Full Moon condition with the sub-solar point at 0° longitude (colongitude 90°). The one on the right is with the sub-solar point at 60° west (colongitude 150°).

It is possible for observer's in the Earth's northern hemisphere to see the Moon's north pole with slightly more tilt; but the north polar features are never illuminated at a higher angle than that shown here.

Example of an Earth-based View

As an example of an actual observation British amateur Stefan Lammel photographed the Moon's north pole from London on April 23, 2010 at 20:10 UT when the libration in latitude, from that site, was +5.39°. The first image is a portion of Stefan's photo, resized and rotated. The second is a simulation created with the LTVT software and the LOLA 240 m resolution polar DEM. The third is the same as the second, but with the full IAU nomenclature of the region automatically superimposed. The last image is an animation combining the previous three. Click on the thumbnails to see the full-sized images.
Observed
Simulation
Nomenclature
Animation
external image StefanLammel_NorthPole_2010Apr23.JPG?size=64
external image StefanLammel_NorthPole_2010Apr23_LOLA_simulation.JPG?size=64
external image StefanLammel_NorthPole_2010Apr23_LOLA_simulation_with_nomenclature.JPG?size=64
external image StefanLammel_NorthPole_2010Apr23_animation.gif?size=64
As previously noted, the diameters of the automatic nomenclature ellipses give a good indication of the sizes of the named features, but the features themselves tend to be located above the positions at which the ellipses are plotted -- an effect most noticeable for the smaller craters such as Aepinus, Hermite A, and Erlanger. A small blue plus symbol marks the exact three dimensional location of the pole in the simulations. Since the topographic element responsible for each pixel in the simulations is precisely known, this position should be as accurate as the registration of the LOLA data itself. The simulation has been "juiced up," slightly, with a gamma correction of 1.5, bringing out small, dimly lit features that are difficult to capture photographically.

To better understand what is being seen, it is helpful to "rectify" Stefan's Earth-based image and compared it to the simulated view expected looking directly down on the north pole under these lighting conditions. Here is what the immediate polar region looks like unrolled at the same scale:
Rectified
Simulation
external image StefanLammel_NorthPole_2010Apr23_rectified.JPG?size=64
external image StefanLammel_NorthPole_2010Apr23_LOLA_simulation_aerial.JPG?size=64
Peary is responsible for the large sunlit plain in the simulation. The circular shadowed crater to its lower left is Hermite A. Whipple is to the upper right of the blue polar plus mark, with Hinshelwood roughly half-way between them (but almost entirely in shadow).

In the simulation, the areas of the lunar surface that were in sunlight, but not visible from Earth (due to being blocked by intervening topography) are highlighted in red. The north pole surface point is not one of these, so it should visible in Stefan's photo, although nearly in shadow. The rectification is not perfect, but the general correspondence of features is evident. Setting the LTVT mouse options to display locations in the raw Earth-based image, one concludes that the north pole point in the simulation correspondends to approximately pixel (1766,134) in the x1.1 version of Stefan's photo.

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This page has been edited 24 times. The last modification was made by - JohnMoore2 JohnMoore2 on Jan 29, 2013 3:35 am - afx3u3