Activation of gas bubble emissions indicated by the upward decreasing Lead-210 activity at a submarine mud volcano (TY1) offshore southwestern Taiwan. (November 2017)

• Record Type: Journal Article
• Authors: Hiruta, Akihiro; Yang, Tsanyao Frank; Lin, Saulwood; Su, Chih-Chieh; Chen, Nai-Chen; Chen, Yi-Jyun; Chen, Hsuan-Wen; Yang, Tsung-Han; Huang, Yu-Chun; Wei, Kuo-Yen; Huang, Jyh-Jaan; Chen, Song-Chuen; Song, Sheng-Rong
• Is Part Of: Journal of Asian earth sciences. Volume 149(2017)
• Page Start: 160
• Page End: 171
• Publication Date: 2017-11
• Subjects: Submarine mud volcano -- Mud breccia -- Radiograph -- Gas bubble emission -- 210Pb; Earth sciences -- Asia -- Periodicals; Sciences de la terre -- Asie -- Périodiques; Earth sciences; Asia; Periodicals; 555.05
• DOI: 10.1016/j.jseaes.2017.08.007
• Languages: English
• ISSNs: 1367-9120

Abstract

Graphical abstract: Highlights: TY1 submarine mud volcano offshore southwestern Taiwan was studied. Mud volcanism change was revealed by radiograph and grain size analysis. The size and abundance of mud clasts suggest weakened mud eruption activity. Gas bubble emission activity generated a sediment unit with particle size sorting. Activation of gas bubble emission is suggested by upward decrease in 210 Pb activity. Abstract: A submarine mud volcano (MV) known as TY1 is one of the largest conical structures found offshore southwestern Taiwan. Active gas bubble emissions at the flat crest of the mud volcano disperse sediment particles into the water column. Changes in the mud volcanism of TY1 were revealed by radiograph and grain size analysis of the sediment cores. 210 Pb geochronology was applied to the near-seafloor sediments to reveal the detailed mud volcanism from the deposition rate. In a 58-cm long sediment core taken from the northern margin of the crest, known as TY1-N.170, the size and frequency of the mud clasts decrease upward. The clasts are smaller than 8 mm above a sediment depth of 34 cm below the sea floor (cmbsf). Sediments between 0 and 19 cmbsf are massive, and particles larger than 2 mm are absent. An enrichment of coarse, silt-sized particles in the massive sediment unit and the restricted distribution of the unit suggest that the massive unit was generated by re-deposition of sediment particles that were dispersed into the water column by gas bubble emission. These characteristics suggest that during the last mud volcanism of TY1, there was a decrease in mud eruption energy, and gas bubble emission became the main activity. In core TY1-S.440, taken from the southern slope, a massive sediment unit enriched with coarse, silt-sized particles, is intercalated between mud breccia structures. This suggests repeated mud breccia flows caused by TY1. The excess 210 Pb activity present in the massive sediment unit of TY1-N.170 suggests activation of gas bubble emission. In the massive unit, a decrease in excess 210 Pb activity appears upward toward the seafloor. The highest value is 3.1 dpm/g at 19.8 cmbsf (26.4 g/cm 2 in cumulative mass); values lower than 1.0 dpm/g are distributed 2.8–6.8 cmbsf (3.6–8.8 g/cm 2 ). The upwardly decreasing trend is opposite that of the reference core from which a reasonable areal sedimentation rate was obtained using a constant-flux constant-sedimentation model. The anomalous depth profile at the massive unit indicates an increasing rate of sediment deposition, which originated from the activation of gas bubble emission.