Asset Details
Do you wish to reserve the book?
An evolutionary system of mineralogy; Part II, Interstellar and solar nebula primary condensation mineralogy (>4.565 Ga)
Hey, we have placed the reservation for you!
By the way, why not check out events that you can attend while you pick your title.
Oops! Something went wrong.
Looks like we were not able to place the reservation. Kindly try again later.
Are you sure you want to remove the book from the shelf?
An evolutionary system of mineralogy; Part II, Interstellar and solar nebula primary condensation mineralogy (>4.565 Ga)
Do you wish to request the book?
An evolutionary system of mineralogy; Part II, Interstellar and solar nebula primary condensation mineralogy (>4.565 Ga)
Please be aware that the book you have requested cannot be checked out. If you would like to checkout this book, you can reserve another copy
We have requested the book for you!
Your request is successful and it will be processed during the Library working hours. Please check the status of your request in My Requests.
Oops! Something went wrong.
Looks like we were not able to place your request. Kindly try again later.
Journal Article
An evolutionary system of mineralogy; Part II, Interstellar and solar nebula primary condensation mineralogy (>4.565 Ga)
2020
Overview
The evolutionary system of mineralogy relies on varied physical and chemical attributes, including trace elements, isotopes, solid and fluid inclusions, and other information-rich characteristics, to understand processes of mineral formation and to place natural condensed phases in the deep-time context of planetary evolution. Part I of this system reviewed the earliest refractory phases that condense at T>1000 K within the turbulent expanding and cooling atmospheres of highly evolved stars. Part II considers the subsequent formation of primary crystalline and amorphous phases by condensation in three distinct mineral-forming environments, each of which increased mineralogical diversity and distribution prior to the accretion of planetesimals >4.5 billion years ago. Interstellar molecular solids: Varied crystalline and amorphous molecular solids containing primarily H, C, O, and N are observed to condense in cold, dense molecular clouds in the interstellar medium (10
We currently cannot retrieve any items related to this title. Kindly check back at a later time.