Constraints on the formation environment of two chondrule‐like igneous particles from comet 81P/Wild 2. (24th April 2015)

• Record Type: Journal Article
• Authors: Gainsforth, Zack; Butterworth, Anna L.; Stodolna, Julien; Westphal, Andrew J.; Huss, Gary R.; Nagashima, Kazu; Ogliore, Ryan; Brownlee, Donald E.; Joswiak, David; Tyliszczak, Tolek; Simionovici, Alexandre S.
• Is Part Of: Meteoritics & planetary science. Volume 50:Number 5(2015:May)
• Page Start: 976
• Page End: 1004
• Publication Date: 2015-04-24
• Subjects: Meteorites -- Periodicals; Planetology -- Periodicals; 523.4
• DOI: 10.1111/maps.12445
• Languages: English
• ISSNs: 1086-9379

Abstract

<abstract abstract-type="main" id="maps12445-abs-0001"> <title>Abstract</title> <p>Using chemical and petrologic evidence and modeling, we deduce that two chondrule‐like particles named Iris and Callie, from Stardust cometary track C2052, 12, 74, formed in an environment very similar to that seen for type II chondrules in meteorites. Iris was heated near liquidus, equilibrated, and cooled at ≤100 °C h^‐1 and within ≈2 log units of the IW buffer with a high partial pressure of Na such as would be present with dust enrichments of ≈10³. There was no detectable metamorphic, nebular, or aqueous alteration. In previous work, Ogliore et al. (2012) reported that Iris formed late, &gt;3 Myr after CAIs, assuming ²⁶Al was homogenously distributed, and was rich in heavy oxygen. Iris may be similar to assemblages found only in interplanetary dust particles and Stardust cometary samples called Kool particles. Callie is chemically and isotopically very similar, but not identical to Iris.</p> </abstract>