60 AUSTRALIAN SKY & TELESCOPE July 2017
LUNAR SHOWCASE
9.Pico and PitonThe titanic impact that created the
Imbriumbasin3.9billionyearsagoleftbehindanenormous
multi-ringed depression some 1,380 kilometres across. It also
fracturedthecrusttogreatdepth,andintimemoltenrock
escaped along these pathways and flooded the basin’s floor,
creatingMareImbrium.Todaylittleremainsofthebasin’s
innerring,butafewbitsofitjutupthroughthelavaplain
southofPlato,andtwooftheseareMonsPicoandMons
Piton (monsisLatinformountain).Theycastlong,dramatic
shadowsacrossthelavaplainwhenevertheSunisjustabove
the local horizon. But actually their heights are modest —
only about 2.5 km each.
10.ArchimedesLocated near the eastern shore of Mare
Imbrium, this ‘ghost crater’ has lost all of its rays, central
peaks and many other details. That’s because lava erupted from
below and inundated the floor with a layer at least 1.5 km
deep. Still, the 80-km-wide rim displays interesting terracing
that becomes more obvious when sunlight strikes it obliquely.
- Montes Apenninus Distinct mountainous arcs to the
east and south of Mare Imbrium mark what remains of
the Imbrium basin’s outer rim. Of these, the Apennine
Mountains (as they’re commonly known) are most
prominent and rise up to 4.5 km above the surrounding lava
plain. To the southwest of the Apennines, the peaks taper to
an arc of summits north of Copernicus known as Montes
Carpatus. Their extension to the northeast, abutting Mare
Serenitatis, is called Montes Caucasus.
12.PtolemaeusThisbig,obviouscrater(150kmacross)
sitsalmostdead-centreinthelunardiskandshowsupbest
aroundthetimesoffirstandlastquarter.Lookcloselyatits
floor,andyou’llseeassortedshallowdepressionsthatare
probably buried craters.
13.ArzachelAlthough not particularly large (95 kilometres
across),thiscraterhasalottooffertelescopicobservers.It’s
relativelyfresh,witharugged,terracedrim.A1.5-km-high
centralpeakrisesfromalava-coveredfloorthat’scrisscrossed
by faulting.
14.Rupes RectaMore commonly called theStraight Wall,
this ancient fault slices across the eastern edge of Mare
Nubiumfornearly110km.It’smostconspicuousnearthe
timesoflocalsunrise(9daysafternewMoon)orsunset(22
days).It’snotcompletelystraight—there’sashortbendat
eachend.Thisfaultscarp,about300metreshigh,probably
formed when the great mass of mare lava to the west caused
theunderlyingrocktocrackandsink.
15.Tycho Eventhoughit'snotespeciallylarge,85-km-wide
Tychosportsthemostimpressivesetofspoke-likeraysof
anycraterontheMoon.Thisbrightsplashradiatesforupto
1,600kilometresinalldirections,andit’sespeciallyobvious
aroundthetimeoffullMoon.Theraysaresoobvious
S MYSTERIOUS WHORL The unusual marking Reiner Gamma itself is only about 35 km wide, but narrow surface swirls extend far to the upper
left and lower right of this frame. At right is the 30-km-wide crater Reiner. Lunar Orbiter 4 took this photo in 1967.
S URIOUS AND COMPLEX C This high-magnification view shows
the complex terracing in the walls of Aristarchus crater. Above it lies the
meandering rille known as Vallis Schröteri (Schröter’s Valley).
WES HIGGINS
NASA / LPI