Hadley–Apennine

Orbital photo of the Hadley-Apennine site; Apollo 15 landing site is marked with a circle.

Hadley–Apennineis a region on thenear sideofEarth's Moonthat served as the landing site for theAmericanApollo 15mission, the fourth crewed landing on the Moon and the first of the "J-missions",in July 1971.The site is located on the eastern edge ofMare Imbriumon a lava plain known asPalus Putredinis.Hadley–Apennine is bordered by theMontes Apenninus(often referred to as "Apennine Front" ), a mountain range, and Hadley Rille, a meandering channel, on the east and west, respectively.

Data obtained from the composition of soil samples collected on Apollo 15 show that most (about 90%) of the samples from the Apennine Front are brown-glassbreccias,and approximately 60–70% obtained from themaresurface arebasalt.Although the basalts seem to vary in their texture, their ages appear to be approximately the same. Most of the samples obtained on the Apennine Front areKREEP(potassium,rare-earth elements,phosphorus) materials,anorthosites,recrystallizednorite,or recrystallized breccia.

Geography and geology

Location

Orbital photo of Hadley-Apennine with Apollo 15 traverses labeled

AstronautDavid ScottlandsApollo 15'sLunar ModuleFalconat Hadley, with navigational assistance fromJames Irwin,on July 30, 1971. Starts at about 5,000 feet (1,500 m).

TheLunar ModuleFalconbackdropped by the Swann Range of theMontes Apenninus

Hadley–Apennine is located west of theMontes Apenninusand east of Hadley Rille. The Apennine mountains form a 15,000 foot (4,600 m)escarpmentthat rises higher above the Hadley plain than theHimalayanfront above the plains ofIndiaandNepal.Hadley Rille (also referred to as Rima Hadley)is located to the west of the Apollo 15 landing site and was the subject of substantial investigation during that mission. The feature, named from nearbyMons Hadley,is a channel that was likely formed byvolcanicprocesses earlier in thehistory of the Moon.

Apollo 15 landing site

See also:Apollo 15andApollo 15 operations on the Lunar surface

The AmericanApollo 15mission, the first of the J-series missions that featured both increased scientific capability and the use of theLunar Roving Vehicle,landed in an area of the Hadley–Apennine region to the west of the Apennine Front situated between the mountains Mons Hadley andMons Hadley Deltato the northeast and south, respectively. This landing site was selected with the objectives of exploring the Apennine Front, Hadley Rille, and other geologic features in the area.

Apollo 15 was the first mission in which landing sites were not restricted to equatorial areas. The Hadley–Apennine site was chosen with the specific objectives of sampling material from deeper within the Moon than had been obtained from theFra Mauro formationonApollo 14and investigating Hadley Rille, a sinuous rille possibly formed by volcanic activity.The site had been of interest to mission planners since early in the program. During the early stages of Apollo landing site planning,Apollo 19(which was originally planned to be the fourth and penultimate J-mission of the initial exploration portion of the Apollo program) was tentatively set to land in the Hadley–Apennine region, albeit at a point south of the eventual Apollo 15 site and west of Hadley Rille—near the Carlos pit at the southwestern terminus of the rille.

TheMarius Hillsarea inOceanus Procellarumwas also considered for Apollo 15, but mission planners determined that a landing on the edge of Mare Imbrium at the Hadley–Apennine site would be more scientifically fruitful than the Marius Hills alternative, and placing aseismometerat Hadley–Apennine, given the locations of seismic packages from previous Apollo expeditions, would create a more optimal configuration for seismic study.

Apennine Front

See also:Montes Apenninus

The Apennine mountains are hypothesized to befault-block mountainsdisplaced upward and segmented by the impact that formed Mare Imbrium. The frontal escarpment of Mons Hadley Delta is believed to be an exposed segment of the pre-Imbrium impact lunar crust. This made the mountain one of the mission's primary locations to visit, as doing so would allow the astronauts to obtain samples of the lunar crust as it was before the creation of Mare Imbrium.

The area of the Apennine mountains between Mons Hadley and Silver Spur (a mountain just southeast of Mons Hadley Delta), although lacking an official designation on maps and other official mission literature, was informally referred to as the "Swann Range" by Apollo 15 astronautsDavid ScottandJames Irwin,after mission geology team leader Gordon Swann. One of the mountains in the Swann Range was informally referred to by the astronauts as "Big Rock Mountain", after the Apollo Program Director at the time of the mission,Rocco Petrone. The composition of the samples collected by the Apollo 15 astronauts from the Apennine Front, other thanKREEP(potassium,rare-earth elements,phosphorus) materials, includedanorthosite,and recrystallized norite and breccia.

Unknown before the Apollo 15 mission, there are parallel linear patterns on the faces of the mountains in the area. Although they appeared to be occurrences offracturingorlayeringappearing through the regolith, determining this is made difficult by the lighting circumstances during the mission. A dark band on Mount Hadley, believed to be a marking left by lava after receding, was observed by the Apollo 15 crew. Additionally, a thickregolithlayer on the lower slopes of the mountains and a thin cover of debris on the upper slopes are suggested by the relative absence of large boulders on the lower mountain flanks.

Rima Hadley

Hadley Rille, taken byApollo 15astronautJames Irwin.

Rima Hadley, asinuousrillelocated west of the Apollo 15 landing site, begins in an area of lowdomesat an elongated crater,Béla,and runs on to the North along the Apennine Mountain Range. Some research has suggested that both the rille and Béla arevolcanic vents,andlavaflows created the features. Another hypothesis suggests that the rille was originally alava tube,the roof of which collapsed, creating the current appearance of the rille. Several large boulders, some of which are as large as houses, are strewn about the feature's floor.The elongated crater Béla, which forms the beginning of Rima Hadley, could have been formed by the collapse of a shallowmagma chamber.Visual observation suggests that the same is the case with other lunar rilles with similar features at their beginnings.

Rima Hadley typically ranges in depth between 600 and 900 feet (180 and 270 m), but is approximately 1,200 feet (370 m) deep at the Apollo 15 landing site. The feature has a cumulative length of about 80 kilometres (50 mi) and an average width of about 0.75 miles (1.21 km). The sides of the rille, at the Apollo 15 site, slope downwards at an angle of about 25 degrees. Before samples were returned from the Moon during theApollo program,several scientists believed that the feature and other similar features were formed by flowing water. This hypothesis has since been changed, however, to attribute the process of the feature's creation to volcanism.

Rima Hadley is interpreted as one of the most defined sinuous rilles on the lunar surface. Outcrops of rock were observed by the Apollo 15 crew on both the near and far sides of the rille and were photographed and, in the case of outcrops on the near rim, were sampled. Layering in these outcrops is evident from the photos taken of them by the crew. Some of the strata observed have thicknesses of up to about 60 metres (200 ft) and appear to vary inalbedo(reflectivity) and texture. Large boulders near the bottom of the rille are believed to be blocks that have broken off of the outcrops above.

South Cluster and North Complex

The South Cluster, a crater cluster located to the south of the Apollo 15 site near Mons Hadley Delta, is believed to have formed as a result of asecondary impact,or the impact ofejecta/debris from a larger impact elsewhere on the Moon, probably the craterAutolycusabout 100 mi (160 km) northwest of the cluster's location. This meant that the Apollo 15 astronauts were able to sample material from other parts of the lunar surface without traversing a great distance. The feature also allowed the astronauts to sample material that was originally located deep within the Moon.The south rim ofDunecrater within the cluster was visited by the astronauts.

TheNorth Complexis a collection of several landforms, including craters, that were thought to have been formed by volcanic activity.Although the Apollo 15 astronauts were to visit this feature, they were unable to do so due to time constraints and time-consuming issues in obtainingcore samples.

See also

• Apollo 15
• Apollo 15, Lunar surface
• Montes Apenninus
• Mons Hadley
• Mons Hadley Delta
• Palus Putredinis
• Mare Imbrium
• Bridge (crater)
• Dandelion (crater)
• Dune (crater)
• Earthlight (crater)
• Elbow (lunar crater)
• Index (crater)
• Last (crater)
• Rhysling (crater)
• Spur (lunar crater)
• St. George (crater)
• North Complex
• Bennett Hill
• Hill 305

External links

• Hadley Rille and the Mountains of the Moon— Labeled oblique LROC image
• LTO-41B4 Hadley— Lunar Topographic Orthophotomap
• Apollo Image Atlas— Images of Hadley–Apennine
• LAC-41 Montes Apenninus— Area map
• I-463 Montes Apenninus— USGS Geologic Atlas area map
• 41B4S4(25) Apollo 15 Traverses— Apollo 15 traverse map
• Apollo 15 Sample CatalogArchived2019-07-21 at theWayback Machine— Catalog of samples from Hadley–Apennine