Luminescence characteristics of terrestrial Jarosite from Kachchh, India: A Martian analogue

IF 2.4 4区 地球科学 Q2 GEOCHEMISTRY & GEOPHYSICS
Malika Singhal, Himela Moitra, Souvik Mitra, Aurovinda Panda, Jayant Kumar Yadav, D. Srinivasa Sarma, Devender Kumar, Naveen Chauhan, Saibal Gupta, Ashok Kumar Singhvi
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Abstract

In this study, naturally occurring jarosite samples from Kachchh, India (considered to be Martian analogue) were characterized using Fourier Transform Infrared Spectroscopy (FTIR), Cathodoluminescence–Energy Dispersive X-ray Spectroscopy (CL-EDXS), and Luminescence (thermoluminescence [TL], blue and infrared stimulated luminescence [BSL and IRSL]) methods. FTIR and CL-EDXS studies suggested that jarosite preserves its luminescence characteristics even after annealing the samples to 450°C. This facilitated luminescence studies (TL/BSL/IRSL) to assess the potential use of luminescence-dating methods to establish the chronology of jarosite formation or its transport. Jarosite exhibited TL, BSL, and IRSL signals with varied sensitivities. The TL glow curve of jarosite comprised glow peaks at 100, 150, 300, and 350°C, reproducible over multiple readout cycles. The least bleachable TL glow peak at 350°C is reduced to (1/e)th of its glow peak intensity (i.e., 36%) with ~100 min of light exposure under a sunlamp. BSL and IRSL optical decay signals comprised three components. These signals exhibited athermal fading of g ~ 6%/decade, but pIRIR signal at 225°C showed a near zero fading. The saturation doses (2D0) ranged from 700 Gy to 2600 Gy for different signals, which suggests a dating range of ~25 ka using a reported Martian total dose rate of 65 Gy/ka, primarily due to cosmic rays. Multiple TL glow peaks and their widely differing stability also offer promise to discern changes in cosmic ray fluxes over a century to millennia time scale through inverse modeling and laboratory experiments.

印度Kachchh陆生黄钾铁矾的发光特性:火星上的类似物
在本研究中,利用傅里叶变换红外光谱(FTIR)、阴极发光-能量色散x射线光谱(CL-EDXS)和发光(热释光[TL]、蓝色和红外激发发光[BSL和IRSL])方法对印度Kachchh天然黄钾铁铁矿样品(被认为是火星类似物)进行了表征。FTIR和CL-EDXS研究表明,即使将样品退火至450°C,黄钾铁矾仍保持其发光特性。这有助于发光研究(TL/BSL/IRSL)评估发光测年方法在确定黄钾铁矾形成或运输年代学方面的潜在应用。黄钾矾表现出不同灵敏度的TL、BSL和IRSL信号。黄钾铁矾的TL发光曲线包括在100、150、300和350°C时的发光峰,可以在多个读出周期内重现。在350°C下,太阳光照射~100 min,最不可漂白的TL发光峰值降低到其发光峰值强度的(1/e)(即36%)。BSL和IRSL光衰减信号由三部分组成。这些信号表现出g ~ 6%/ 10年的非热衰减,而在225℃时,pIRIR信号表现出接近于零的衰减。不同信号的饱和剂量(2D0)从700 Gy到2600 Gy不等,根据报道的火星总剂量率为65 Gy/ka,这表明测年范围为~25 ka,主要是由于宇宙射线。通过逆向建模和实验室实验,多个TL辉光峰及其广泛不同的稳定性也为辨别宇宙射线通量在一个世纪到千年时间尺度上的变化提供了希望。
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来源期刊
Meteoritics & Planetary Science
Meteoritics & Planetary Science 地学天文-地球化学与地球物理
CiteScore
3.90
自引率
31.80%
发文量
121
审稿时长
3 months
期刊介绍: First issued in 1953, the journal publishes research articles describing the latest results of new studies, invited reviews of major topics in planetary science, editorials on issues of current interest in the field, and book reviews. The publications are original, not considered for publication elsewhere, and undergo peer-review. The topics include the origin and history of the solar system, planets and natural satellites, interplanetary dust and interstellar medium, lunar samples, meteors, and meteorites, asteroids, comets, craters, and tektites. Our authors and editors are professional scientists representing numerous disciplines, including astronomy, astrophysics, physics, geophysics, chemistry, isotope geochemistry, mineralogy, earth science, geology, and biology. MAPS has subscribers in over 40 countries. Fifty percent of MAPS'' readers are based outside the USA. The journal is available in hard copy and online.
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