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Items: 4

1.

Fe-oxide concretions formed by interacting carbonate and acidic waters on Earth and Mars.

Yoshida H, Hasegawa H, Katsuta N, Maruyama I, Sirono S, Minami M, Asahara Y, Nishimoto S, Yamaguchi Y, Ichinnorov N, Metcalfe R.

Sci Adv. 2018 Dec 5;4(12):eaau0872. doi: 10.1126/sciadv.aau0872. eCollection 2018 Dec.

2.

High-temperature water-rock interactions and hydrothermal environments in the chondrite-like core of Enceladus.

Sekine Y, Shibuya T, Postberg F, Hsu HW, Suzuki K, Masaki Y, Kuwatani T, Mori M, Hong PK, Yoshizaki M, Tachibana S, Sirono SI.

Nat Commun. 2015 Oct 27;6:8604. doi: 10.1038/ncomms9604.

3.

Early post-mortem formation of carbonate concretions around tusk-shells over week-month timescales.

Yoshida H, Ujihara A, Minami M, Asahara Y, Katsuta N, Yamamoto K, Sirono SI, Maruyama I, Nishimoto S, Metcalfe R.

Sci Rep. 2015 Sep 15;5:14123. doi: 10.1038/srep14123.

4.

Ongoing hydrothermal activities within Enceladus.

Hsu HW, Postberg F, Sekine Y, Shibuya T, Kempf S, Horányi M, Juhász A, Altobelli N, Suzuki K, Masaki Y, Kuwatani T, Tachibana S, Sirono SI, Moragas-Klostermeyer G, Srama R.

Nature. 2015 Mar 12;519(7542):207-10. doi: 10.1038/nature14262.

PMID:
25762281

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