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. 2016 May 31;113(24):E3322–E3331. doi: 10.1073/pnas.1603030113

Fig. S1.

Fig. S1.

Additional meteoritic 3C and 4C sugar acid analyses. (A) Glyceric acid and 4C acids from the Murray meteorite. Murray has a much longer residence time on Earth than Murchison, possibly resulting in more contamination of l-threonic acid. HMG was not identified in Murray; this may be due to a general lower abundance of compounds in this sample. (B) HMG and 4C acids from a sample of Murchison 52. (separate from that in Fig. 4C)