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Multi-band search for volcanic outgassing in the Tharsis and Syrtis Major regions on Mars.

机译:在火星上的塔里西斯(Tharsis)和锡尔蒂斯(Syrtis)主要地区进行多波段火山脱气搜索。

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摘要

We carried out the first and most comprehensive to date (2015), ground-based, semisimultaneous, multi-band and multi-species search for sulphuretted gases (SO2, H2S, OCS and SO) above the Tharsis and Syrtis volcanic regions on Mars. The submillimeter search extended between 23 November 2011 and 25 May 2014 which corresponded to Mars' mid Northern Spring and mid Northern Summer seasons (Ls = 34 - 135°). SO2, SO and H2S were targeted at their rotational transitions at 346.652 GHz, 304.078 GHz and 300.505 GHz, respectively, using the high-resolution heterodyne receiver Barney on the 10.4 m single-dish antenna of the Caltech Submillimeter Observatory (CSO), and SO2 at HARP on the 15 m James Clerk Maxwell Telescope (JCMT) at Maunakea, Hawai'i. No sulphuretted gases were detected. We infer 2sigma upper limits across the disk of the planet using the CSO of 1.1 ppb, 0.7 ppb and 1.3 ppb for SO2, SO and H2S, respectively, and 3.1 ppb on SO2 using the JCMT. The infrared search covered OCS in its combination band (nu1+nu3) at 3.42 mum (2924 cm -1), during Mars' late Northern Spring and mid Northern Summer seasons, spanning Ls= 43° and Ls= 145°, between 15 Dec. 2011 and 13 June 2014, using the high resolution infrared spectrometer CSHELL on the 3 m NASA Infrared Telescope Facility (IRTF). No absorption of atmospheric OCS has been detected, and we infer a 2sigma upper limit of 0.8 ppb on OCS. Our current limit 1.1 ppb for SO2 yields an outgassing rate of less than 55 tons/day. Compared to two terrestrial analogs, we would have been able to detect any volcanic release that is more than 4% the size of Kilauea (Hawai'i) or one twentieth the size of the Masaya volcano (Nicaragua). The mass rate of magma that is able to degas 55 tons of SO2 per day is estimated as 37 kilotons of magma per day, or 12,000 m3 per day (0.14 m3/s). The non-detection of any of the sulfur compounds in the atmosphere of Mars provides limits to the level of current volcanic activity in the crust of Mars.
机译:我们进行了迄今为止最全面的首次(2015年)地面,半同时,多波段和多物种搜索,在火星上的塔里西斯和Syrtis火山区上方搜寻含硫的气体(SO2,H2S,OCS和SO)。亚毫米搜索持续了2011年11月23日至2014年5月25日,对应于火星的北部春季中期和北部夏季中期(Ls = 34-135°)。使用Caltech亚毫米天文台(CSO)的10.4 m单碟天线上的高分辨率外差接收器Barney,SO2,SO和H2S分别针对其在346.652 GHz,304.078 GHz和300.505 GHz的旋转跃迁。在位于夏威夷Maunakea的15 m James Clerk Maxwell望远镜(JCMT)上的HARP上。没有检测到硫磺化气体。我们使用CJ分别推断出SO2,SO和H2S的CSO分别为1.1 ppb,0.7 ppb和1.3 ppb,而使用JCMT推断出SO2的3.1 ppb,则推断出整个行星盘的2sigma上限。在12月15日至12月15日之间,火星的北春末和北夏中中期,红外搜索覆盖了3.42毫米(2924 cm -1)的组合带(nu1 + nu3)中的OCS,跨度为Ls = 43°和Ls = 145°。 2011年和2014年6月13日,在3 m NASA红外望远镜设施(IRTF)上使用高分辨率红外光谱仪CSHELL。尚未检测到大气中OCS的吸收,我们推断OCS的2sigma上限为0.8 ppb。我们目前对二氧化硫的限制为1.1 ppb,产生的脱气率小于55吨/天。与两个陆地类似物相比,我们将能够检测到超过基拉韦厄(夏威夷)大小的4%或马萨亚火山(尼加拉瓜)大小的二十倍的任何火山释放。每天能够对55吨SO2脱气的岩浆质量速率估计为每天37吨岩浆,或每天12,000 m3(0.14 m3 / s)。在火星大气层中未检测到任何硫化合物,这限制了火星地壳中当前火山活动的水平。

著录项

  • 作者

    Khayat, Alain S. J.;

  • 作者单位

    University of Hawai'i at Manoa.;

  • 授予单位 University of Hawai'i at Manoa.;
  • 学科 Astronomy.;Planetology.
  • 学位 Ph.D.
  • 年度 2015
  • 页码 197 p.
  • 总页数 197
  • 原文格式 PDF
  • 正文语种 eng
  • 中图分类
  • 关键词

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