Spectroscopic Study of Aqueous Alteration of Asteroids Based on Carbonaceous Chondrites

YU Jinfei1,2,3, ZHAO Haibin1,2,4, WU Yunzhao1,4

PDF(1613 KB)
PDF(1613 KB)
Journal of Deep Space Exploration ›› 2023, Vol. 10 ›› Issue (6) : 667-676. DOI: 10.15982/j.issn.2096-9287.2023.20220077

Spectroscopic Study of Aqueous Alteration of Asteroids Based on Carbonaceous Chondrites

  • YU Jinfei1,2,3, ZHAO Haibin1,2,4, WU Yunzhao1,4
Author information +
History +

Abstract

The aqueous alteration spectral features of carbonaceous chondrites for were studied for future volatile-rich asteroids exploration and remote sensing. The 1-20 μm infrared spectral features and petrographic characteristics of 15 carbonaceous chondrites with different alteration degrees were analyzed, and the spectral variation laws of the aqueous alteration were summarized. The findings demonstrate that as the degree of alteration of carbonaceous chondrites increases, the 3 μm absorption band, which indicates phyllosilicates and water molecules, and the 6 μm absorption band, which indicates only water molecules, both features increasing in strength and absorption centers shift to the short-wave. With more alteration, the 3 μm absorption band sharpens and resembles serpentine’s 3 μm absorption feature. However, as the degree of alteration increases, the 6 μm absorption band shape does not significantly change. The degree of alteration also affects the spectral shape of the 10-13 μm region. This region indicates silicate features. The 12.4 μm /11.4 μm reflectance ratio reduces as a result of the conversion of anhydrous silicates to phyllosilicates. Also discuss possible effects that the spectra and parameters discovered during this study may have on the outcomes from asteroids.

Keywords

asteroid / spectrum / spectroscopy / mineralogy

Cite this article

Download citation ▾
YU Jinfei, ZHAO Haibin, WU Yunzhao. Spectroscopic Study of Aqueous Alteration of Asteroids Based on Carbonaceous Chondrites. Journal of Deep Space Exploration, 2023, 10(6): 667‒676 https://doi.org/10.15982/j.issn.2096-9287.2023.20220077

References

[1] BATES H C,KING A J,HANNA K L D,et al. Linking mineralogy and spectroscopy of highly aqueously altered CM and CI carbonaceous chondrites in preparation for primitive asteroid sample return[J]. Meteoritics & Planetary Science,2020,1(71-101):13411.
[2] DEMEO F E,BINZEL R P,SLIVAN S M,et al. An extension of the Bus asteroid taxonomy into the near-infrared[J]. Icarus,2009,202(1):160-180
[3] GEHRELS T. Asteroids III[M]. Tucson,AZ:University of Arizona Press,2002.
[4] AMELIN Y,KROT A N,HUTCHEON I D,et al. Lead isotopic ages of chondrules and calcium-aluminum-rich inclusions[J]. Science,2002,297(5587):1678-1683
[5] BINZEL R P,GEHRELS T,MATTHEWS M S. Asteroids II[M]. Tucson,AZ:The University of Arizona Press,1989.
[6] ALEXANDER C M O,BOWDEN R,FOGEL M L,et al. The provenances of asteroids,and their contributions to the volatile inventories of the terrestrial planets[J]. Science,2012,337(6095):721-723
[7] MARUYAMA S, EBISUZAKI T, KUROKAWA K. Origin and evolution of Earth and life: towards the establishment of astrobiology from universe to genome[C]//Proceedings of Frontier Research in Astrophysics – III — PoS(FRAPWS2018). Mondello (Palermo), Italy: Sissa Medialab, 2019.
[8] BECK P. Hydrous mineralogy of CM and CI chondrites from infrared spectroscopy and their relationship with low albedo asteroids[J]. Geochimica et Cosmochimica Acta,2010,74(16):4881-4892
[9] TAKIR D,EMERY J P,MCSWEEN H Y,et al. Nature and degree of aqueous alteration in CM and CI carbonaceous chondrites[J]. Meteoritics & Planetary Science,2013:48(9),1618-1637.
[10] BECK P,GARENNE A,QUIRICO E,et al. Transmission infrared spectra (2–25 lm) of carbonaceous chondrites (CI,CM,CV-CK,CR,C2 ungrouped): mineralogy,water,and asteroidal processes[J]. Icarus,2014,229:263-277
[11] GARENNE A. Bidirectional reflectance spectroscopy of carbonaceous chondrites:Implications for water quantification and primary composition[J]. Icarus,2016,264:172-183
[12] KING A J. Characterising the CI and CI-like carbonaceous chondrites using thermogravimetric analysis and infrared spectroscopy[J]. Earth,Planets and Space,2015,67:198
[13] RUSSELL C T,RAYMOND C A. The Dawn mission to Vesta and Ceres[J]. Space Science Reviews,2011,163(1):3-23
[14] LAURETTA D S,BALRAM-KNUTSON S S,BESHORE E,et al. OSIRIS-REx:sample return from Asteroid (101955) Bennu[J]. Space Science Reviews,2017,212(1):925-984
[15] TSUDA Y,YOSHIKAWA M,ABE M,et al. System design of the Hayabusa 2—asteroid sample return mission to 1999 JU3[J]. Acta Astronautica,2013,91:356-362
[16] LEVISON H F,OLKIN C,NOLL K S,et al. Lucy:surveying the diversity of the trojan asteroids:the fossils of planet formation[C]//Proceedings of 48th Annual Lunar and Planetary Science Conference. The Woodlands,Texas:[s. n. ]:2017.
[17] CANTILLO D C, REDDY V, SHARKEY B N L, et al. Constraining the regolith composition of Asteroid (16) Psyche via laboratory visible near-infrared spectroscopy[EB/OL]. (2021)[2022-08-19]. https://doi.org/10.3847/PSJ/abf63b.
[18] HIROI T, ZOLENSKY M E, PIETERS C M. The Tagish Lake meteorite: a possible sample from a d-type asteroid[J]. Science, 2001, 293(5538): 2234-2236.
[19] GILMOUR C M,HERD C D K,BECK P. Water abundance in the Tagish Lake meteorite from TGA and IR spectroscopy:evaluation of aqueous alteration[J]. Meteoritics & Planetary Science, 2019, 54(9): 1951-1972.
[20] CLARK R N. Detection of adsorbed water and hydroxyl on the Moon[J]. Science,2009,326(5952):562-564
[21] LI S,LUCEY P G,MILLIKEN R E,et al. Direct evidence of surface exposed water ice in the lunar polar regions[J]. Proceedings of the National Academy of Sciences of the United States of America,2018,115(36):8907-8912
[22] MILLIKEN R E,MUSTARD J F. Estimating the water content of hydrated minerals using reflectance spectroscopy II. effects of particle size[J]. Icarus,2007,189(2):574-588
[23] MILLIKEN R E,MUSTARD J F. Estimating the water content of hydrated minerals using reflectance spectroscopy I. effects of darkening agents and low-albedo materials[J]. Icarus,2007,189(2):550-573
[24] DUAN A,WU Y,CLOUTIS E A,et al. Heating of carbonaceous materials:insights into the effects of thermal metamorphism on spectral properties of carbonaceous chondrites and asteroids[J]. Meteoritics & Planetary Science,2021,56(11):2035-2046
[25] SIMON A A,KAPLAN H H,HAMILTON V E,et al. Widespread carbon-bearing materials on near-Earth asteroid (101955) Bennu[J]. Science :2020,370(6517):eabc3522.
[26] HONNIBALL C I. Molecular water detected on the sunlit Moon by SOFIA[J]. Nature Astronomy,2021,5(2):121-127
[27] BATES H C,HANNA K L D,KING A J,et al. A spectral investigation of aqueously and thermally altered CM,CM‐An,and CY chondrites under simulated asteroid conditions for comparison with OSIRIS‐REx and Hayabusa2 observations[J]. Journal of Geophysical Research,2021,126(7):e2021JE006827
[28] BECK P, MATURILLI A, GARENNE A, et al. What is controlling the reflectance spectra (0.35-150 μm) of hydrated (and dehydrated) carbonaceous chondrites?[J]. Icarus, 20183, 13: 124-138.
[29] RUBIN A E,TRIGO-RODRÍGUEZ J M,HUBER H,et al. Progressive aqueous alteration of CM carbonaceous chondrites[J]. Geochimica et Cosmochimica Acta,2007,71(9):2361-2382
[30] HOWARD K T,BENEDIX G K,BLAND P A,et al. Modal mineralogy of CM2 chondrites by X-ray diffraction (PSD-XRD). part 1:total phyllosilicate abundance and the degree of aqueous alteration[J]. Geochimica et Cosmochimica Acta,2009,73(15):4576-4589
[31] MILLIKEN R E,HIROI T,PATTERSON W. The NASA Reflectance Experiment Laboratory (RELAB) facility:past,present,and future[C]//Proceedings of 47th Annual Lunar and Planetary Science Conference. The Woodlands,Texas:NASA,2016.
[32] CLOUTIS E A,HUDON P,HIROI T,et al. Spectral reflectance properties of carbonaceous chondrites:2. CM chondrites[J]. Icarus,2011,216(1):309-346
[33] MCADAM M M. Aqueous alteration on asteroids:linking the mineralogy and spectroscopy of CM and CI chondrites[J]. Icarus,2015,245:320-332
[34] BROWNING L B,MCSWEEN H Y,ZOLENSKY M E. Correlated alteration effects in CM carbonaceous chondrites[J]. Geochimica et Cosmochimica Acta,1996,60(14):2621-2633
[35] BROWNING L,MCSWEEN JR. H Y,ZOLENSKY M E. On the origin of rim textures surrounding anhydrous silicate grains in CM carbonaceous chondrites[J]. Meteoritics & Planetary Science,2000,35(5):1015-1023
[36] LEBOFSKY L A. Infrared reflectance spectra of asteroids :a search for water of hydration.[J]. The Astronomical Journal,1980,85:573-585
[37] RIVKIN A S,DAVIES J K,JOHNSON J R,et al. Hydrogen concentrations on C-class asteroids derived from remote sensing[J]. Meteoritics & Planetary Science,2003,38(9):1383-1398
[38] TAKIR D,EMERY J P. Outer Main Belt asteroids:Identification and distribution of four 3-μm spectral groups[J]. Icarus,2012,219(2):641-654
[39] HOWELL E,RIVKIN A,SODERBERG A,et al. Aqueous alteration of asteroids:correlation of the 3 μm and 0.7 μm hydration bands[J]. Bulletin of the American Astronomical Society,1999,31:1074.
[40] VILAS F. A cheaper,faster,better way to detect water of hydration on solar system bodies[J]. Icarus,1994,111(2):456-467
[41] USUI F, HASEGAWA S, OOTSUBO T, et al. AKARI/IRC near-infrared asteroid spectroscopic survey: AcuA-spec[EB/OL]. [2023-02-27]. https://academic.oup.com/pasj/article/doi/10.1093/pasj/psy125/5238131.
[42] CAMPINS H,HARGROVE K,PINILLA-ALONSO N,et al. Water ice and organics on the surface of the asteroid 24 Themis[J]. Nature,2010,464(7293):1320-1321
[43] BECK P,QUIRICO E,SEVESTRE D,et al. Goethite as an alternative origin of the 3.1 μm band on dark asteroids[J]. Astronomy & Astrophysics,2011,526:A85
[44] KUROKAWA H, SHIBUYA T, SEKINE Y, et al. Distant formation and differentiation of outer main belt asteroids and carbonaceous chondrite parent bodies[J]. AGU Advances, 2022, 3(1): e2021AV000568. DOI:10.1029/2021AV000568.
[45] KITAZATO K,MILLIKEN R E,IWATA T,et al. The surface composition of asteroid 162173 Ryugu from Hayabusa2 near-infrared spectroscopy[J]. Science,2019,364(6437):272-275
[46] GALIANO A,PALOMBA E,D’AMORE M,et al. Characterization of the Ryugu surface by means of the variability of the near-infrared spectral slope in NIRS3 data[J]. Icarus,2020,351:113959
[47] KITAZATO K,MILLIKEN R E,IWATA T,et al. Thermally altered subsurface material of asteroid (162173) Ryugu[J]. Nature Astronomy,2021,5(3):246-250
[48] HAMILTON V E,SIMON A A,CHRISTENSEN P R,et al. Evidence for widespread hydrated minerals on asteroid (101955) Bennu[J]. Nature Astronomy,2019,3(4):332-340
[49] PILORGET C,OKADA T,HAMM V,et al. First compositional analysis of Ryugu samples by the MicrOmega hyperspectral microscope[J]. Nature Astronomy,2022,6(2):221-225.
[50] AMANO K,MATSUOKA M,NAKAMURA T,et al. Reassigning CI chondrite parent bodies based on reflectance spectroscopy of samples from carbonaceous asteroid Ryugu and meteorites[J]. Science Advances,2023,9(49):eadi3789.
[51] NAKAMURA T, MATSUMOTO M, AMANO K, et al. Formation and evolution of carbonaceous asteroid Ryugu: direct evidence from returned samples[J]. Science,2022,379(6634):eabn8671
PDF(1613 KB)

Accesses

Citations

Detail

Sections
Recommended

/