Table 2. Meteorites from the Nullarbor Region, Australia. Hughes meteorites are from South Australia, and Mundrabilla and Reid meteorites are from Western Australia.

Name Latitude Longitude Wt. Pcs Found Class Fa1 Fs Shock2 WG3 Analysis4 Specimens5
      (g)       mol% mol%        

Hughes 026 30�0'S (�5') 129�10'E (�5') 360 1 1995 Brachinite 34.5       (a) 26 g AMNH
Hughes 027 30�33.40'S 129�38.32'E 68 1 1993 H5 19.1 17.7 S2 W5 (b) UH 265
Hughes 028 30�36.53'S 129�37.54'E 62 1 1993 H6 18.9 17.5 S4 W5 (b) UH 266
Hughes 029 30�24.49'S 129�20.30'E 74 1 1993 H5 18.9 17.7 S2 W2 (b) UH 268
Hughes 030 30�40.08'S 129�27.72'E <100 1 1991 R3-6 See separate entry          
Hughes 031 30�10'23"S 129�32'10"E 120 2 1991 L4 22.9 18.8 S4-5 W1 (c) SML
Hughes 032 30�10'6"S 129�30'E 42.7 1 1991 L5 24.6 20.8 S2 W3 (c) SML
Hughes 033 30�8'2"S 129�3'45"E 20 1 1991 CO3 0.6�61 (26) 1.0�47.8 (17) S1 W3 (c) SML
Mundrabilla 020 30�50'S(�15') 127�30'E (�15') 31 1 1989 Howardite See separate entry            
Reid 016 30�10'S (�5') 129�0'E (�5') 110 1 1995 Ureilite 3�24 (18.4)       (a) 27 g AMNH
Reid 017 30�10'S (�5') 128�55'E (�5') unk 1 1995 L3.7 1�46 (20.5)       (a) 43 g AMNH
Reid 018 30�05.00'S 128�55.00'E 121 1 1993 L5 24.2 21.1 S4 W3 (b) UH 262
Reid 019 30�31.04'S 128�28.57'E 56 1 1993 L6 24.4 21.8 S4 W1 (b) UH 263
Reid 020 30�31.0'S 128�27.5'E 32 1 1993 L6 25.6 22.8 S2 W2 (b) UH 264
Reid 021 30�04.07'S 128�59.09'E 20 1 1993 L6 25.0 22.4 S4 W5 (b) UH 267
Reid 022 30�18.17'S 128�31.57'E 188 1 1993 H4 18.7 17.3 S1 W1 (b) UH 269
Reid 023 30�18.05'S 128�31.53'E 59 1 1993 H5 18.7 17.8 S2 W2 (b) UH 270
Reid 024 30�19.10'S 128�23.00'E 96 1 1993 H5 18.4 17.1 S2 W3 (b) UH 271
Reid 025 30�17'12"S 128�34'24"E 21.4 1 1991 L6 24.0 19.3 S4 W4 (c) SML
Reid 026 30�14'54"S 128�38'7"E 100.6 1 1991 LL6 31.5 25.4 S2 W4 (c) SML
Reid 027 30�19'5"S 128�22'24"E 19.7 1 1991 Brachinite See separate entry          

1Average fayalite contents shown in parentheses.
2Shock classification after St�ffler et al. (1991).
3Weathering grade after Wlotzka (1993).
4Description and analysis by: (a) M. Prinz, AMNH; (b) G. Benedix, UHaw; (c) J. Otto, Frei.
5Numbers starting with UH represent type specimens at UHaw; the main masses for these are owned by J. Y. Murakami. The locations of the main masses of the three meteorites at AMNH are unknown