ePrints@IIScePrints@IISc Home | About | Browse | Latest Additions | Advanced Search | Contact | Help

Isotopes in cosmochemistry: recipe for a Solar System

Goderis, Steven and Chakrabarti, Ramananda and Debaille, Vinciane and Kodolanyi, Janos (2016) Isotopes in cosmochemistry: recipe for a Solar System. In: JOURNAL OF ANALYTICAL ATOMIC SPECTROMETRY, 31 (4). pp. 841-862.

[img] PDF
Jou_Ana_Ato_Spe_31-4_841_2016.pdf - Published Version
Restricted to Registered users only

Download (991kB) | Request a copy
Official URL: http://dx.doi.org/10.1039/c5ja00411j


Extreme isotopic variations among extraterrestrial materials provide great insights into the origin and evolution of the Solar System. In this tutorial review, we summarize how the measurement of isotope ratios can expand our knowledge of the processes that took place before and during the formation of our Solar System and its subsequent early evolution. The continuous improvement of mass spectrometers with high precision and increased spatial resolution, including secondary ion mass spectrometry (SIMS), thermal ionization mass spectrometry (TIMS) and multi collector-inductively coupled plasma-mass spectrometry (MC-ICP-MS), along with the ever growing amounts of available extraterrestrial samples have significantly increased the temporal and spatial constraints on the sequence of events that took place since and before the formation of the first Solar System condensates (i.e., Ca-Al-rich inclusions). Grains sampling distinct stellar environments with a wide range of isotopic compositions were admixed to, but possibly not fully homogenized in, the Sun's parent molecular cloud or the nascent Solar System. Before, during and after accretion of the nebula, as well as the formation and subsequent evolution of planetesimals and planets, chemical and physical fractionation processes irrevocably changed the chemical and isotopic compositions of all Solar System bodies. Since the formation of the first Solar System minerals and rocks 4.568 Gyr ago, short-and long-lived radioactive decay and cosmic ray interaction also contributed to the modification of the isotopic framework of the Solar System, and permit to trace the formation and evolution of directly accessible and inferred planetary and stellar isotopic reservoirs.

Item Type: Journal Article
Additional Information: Copy right for this article belongs to the ROYAL SOC CHEMISTRY, THOMAS GRAHAM HOUSE, SCIENCE PARK, MILTON RD, CAMBRIDGE CB4 0WF, CAMBS, ENGLAND
Department/Centre: Division of Mechanical Sciences > Centre for Earth Sciences
Date Deposited: 11 May 2016 07:47
Last Modified: 11 May 2016 07:47
URI: http://eprints.iisc.ac.in/id/eprint/53796

Actions (login required)

View Item View Item