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Sample 78597

Figure 1: Photo of 78597. Scale in cm. S73-21421

Figure 2: Location where 78597 was found.

78597 is a vuggy, medium-grained high-Ti basalt (figure 1 and 3). It was collected as part of a rake sample and large comprehensive sample at station 8, Apollo 17 (figure 2).

78597 is an olivine-microporphritic ilmenite basalt with large olivine grains set in a predominantly variolitic groundmass (figure 5). Plagioclase laths in the groundmass have hollow cores (interfaciculate) and are bundled in sheaths with intergrown pyroxene. Ilmenite occurs in chains. Trace tranquillityite has been reported (Warner et al. 1978).

Warner et al. (1975) and Rhodes et al. (1976) reported the chemical composition of 78597 (table 1, figures 6,

Figure 3: Phot of 78597. Scale in cm. S73-21422

7 and 8). Note that the Rb content is low, compared with other Apollo 17 basalts.

Gibson et al. (1976) reported 1990 ppm S.

Nyquist et al. (1976) studied the Rb-Sr isotope system, but did not determine an age. However, the age of Apollo 17 basalt is 3.72 b.y.

O’Kelley et al. (1974) determined the cosmic-rayinduced activity of 22Na = 33 dpm/kg., 26Al = 48 dpm/ kg., 46Sc = 25 dpm/kg., 54Mn = 80 dpm/kg and 56Co = 80 dpm/kg.

Figure 4: Composition of olivine and pyroxene in 78597 (Warner et al. 1978).

ProcessingOlivine5.9
There is only one (small) thin section of 78597.Pyroxene42.2
Plagioclase29.5
Opaques16.5
Silica5.4
Meostasis0.5

Figure 5: Photomicrgraph of thin section 78597,11. 2.8 mm across

weightreference Eldridge74Rhodes76
Nyquist76
Warner75A17
78597
12
SiO2 %
TiO2
Al2O3
FeO
MnO
MgO
CaO
Na2O
K2O
P2O5
S %
sum
0.04638.54
12.39
8.85
19.67
0.29
7.83
10.94
0.39
(a) 0.04
0.11
0.19
(d)
(d) 11.8
(d) 9
(d) 18
(d) 0.24
(d) 7.1
(d) 10.7
(d) 0.42
(d) 0.06
(d)
(d)
(b)
(b)
(b)
(b)
(b)
(b)
(b)
(b)
A11
10
8
TiO2
6
4
A12
A15
2
0
0
5
10
15
MgO
Sc ppm
V
85(b) 75
100
(b)
(b)
Figure 6: Composition of lunar basalts.
Cr
Co
Ni
Cu
2190
20.7
(d)
(b) 18.5
(b)300
Apollo 17 basalts
250
Zn
Ga
Ge ppb
As
Se
Rb
Sr
Y
Zr
Nb
Mo
Ru
Rh
Pd ppb
Ag ppb
Cd ppb
0.37
130
(c )
(c )
200
Ba/
78597
/Rb
group A
150
group B
100
50
group C
0
5
7
9
11
13
Sm ppm
Figure 7: Trace element characteristics of Apollo
In ppb
Sn ppb
Sb ppb
Te ppb
Cs ppm
Ba
La
Ce
Pr
Nd
Sm
Eu
Gd
Tb
Dy
Ho
Er
Tm
Yb
Lu
Hf
Ta
W ppb
Re ppb
Os ppb
Ir ppb
Pt ppb
Au ppb
Th ppm
0.38
(a)
60.6
5.67
17.9
18.8
7.17
1.48
11.2
13
7.94
7.37
1.07
6.8
(c )
(c ) 5.3
(c ) 18
(c )
(c ) 7.3
(c ) 1.4
(c )
1.9
(c ) 12
(c )
(c ) 6.7
(b) 1
(b) 6.2
1.5
(b)
(b)
(b)
(b)
(b)
(b)
(b)
(b)
(b)
(b)
17 basalts.
Figure 8: Normalized rare-earth-element diagram
for 78597 compared with A and B types of Apollo 17
basalt.
U ppm0.11
(a)
technique: (a) radiation count., (b) INAA, (c ) IDMS, (d) XRF

Figure 7: Trace element characteristics of Apollo

Figure 8: Normalized rare-earth-element diagram for 78597 compared with A and B types of Apollo 17 basalt.

Brown G.M., Peckett A., Emeleus C.H., Phillips R. and Pinsent R.H. (1975a) Petrology and mineralogy of Apollo 17 mare basalts. Proc. 6th Lunar Sci. Conf. 1-13.

Butler P. (1973) Lunar Sample Information Catalog Apollo 17. Lunar Receiving Laboratory. MSC 03211 Curator’s Catalog. pp. 447.

Gibson E.K., Usselman T.M. and Morris R.V. (1976a) Sulfur in the Apollo 17 basalts and their source regions. Proc. 7th Lunar Sci. Conf. 1491-1505.

LSPET (1973) Apollo 17 lunar samples: Chemical and petrographic description. Science 182, 659-672.

LSPET (1973) Preliminary Examination of lunar samples. Apollo 17 Preliminary Science Rpt. NASA SP-330. 7-1 – 7-46.

Ma M-S., Schmitt R.A., Warner R.D., Taylor G.J. and Keil K. (1979b) Composition, petrography, and genesis of Apollo 17 high-Ti mare basalts (abs). Lunar Planet. Sci. X, 765-767. Lunar Planetary Institute, Houston.

Meyer C. (1994) Catalog of Apollo 17 rocks. Vol. 4 North Massif

Muehlberger et al. (1973) Documentation and environment of the Apollo 17 samples: A preliminary report. Astrogeology 71 322 pp superceeded by Astrogeology 73 (1975) and by Wolfe et al. (1981)

Muehlberger W.R. and many others (1973) Preliminary Geological Investigation of the Apollo 17 Landing Site. In Apollo 17 Preliminary Science Report. NASA SP-330.

Neal C.R. (2001) Interior of the moon: The presence of garnet in the primitive deep lunar mantle. J. Geophys. Res. 106, 27865-27885.

Nyquist L.E., Bansal B.M. and Wiesmann H. (1976a) Sr isotopic constraints on the petrogenesis of Apollo 17 mare basalts. Proc. 7th Lunar Sci. Conf. 1507-1528.

O’Kelley G.D., Eldridge J.S. and Northcutt K.J. (1974a) Cosmogenic radionuclides in samples from Taurus-Littrow: Effects of the solar flare of August 1972. Proc. 5th Lunar Sci. Conf. 2139-2147.

Rhodes J.M., Hubbard N.J., Wiesmann H., Rodgers K.V., Brannon J.C. and Bansal B.M. (1976a) Chemistry, classification, and petrogenesis of Apollo 17 mare basalts. Proc. 7th Lunar Sci. Conf. 1467-1489.

Ryder G. (1993) Catalog of Apollo 17 rocks. Vol. 1 South Massif

Warner R.D., Keil K., Prinz M., Laul J.C., Murali A.V. and Schmitt R.A. (1975b) Mineralogy, petrology, and chemistry of mare basalts from Apollo 17 rake samples. Proc. 6th Lunar Sci. Conf. 193-220.

Warner R.D., Taylor G.J., Conrad G.H., Northrop H.R., Barker S., Keil K., Ma M.-S. and Schmitt R. (1979a) Apollo 17 high-Ti mare basalts: New bulk compositional data, magma types, and petrogenesis. Proc. 10th Lunar Planet. Sci. Conf. 225-247.

Wolfe E.W., Bailey N.G., Lucchitta B.K., Muehlberger W.R., Scott D.H., Sutton R.L and Wilshire H.G. (1981) The geologic investigation of the Taurus-Littrow Valley: Apollo 17 Landing Site. US Geol. Survey Prof. Paper, 1080, pp. 280