Skip to main content

Main menu

  • Home
  • Content
    • Current
    • Archive
    • Special Volumes and Special Issue
  • Subscriptions
    • Subscribers
    • FAQ
    • Terms & Conditions for use of AJS Online
  • Instructions to Authors
    • Focus and paper options
    • Submit your manuscript
  • Site Features
    • Alerts
    • Feedback
    • Usage Statistics
    • RSS
  • About Us
    • Editorial Board
    • The Journal

User menu

  • Register
  • Subscribe
  • My alerts
  • Log in
  • My Cart

Search

  • Advanced search
American Journal of Science
  • Register
  • Subscribe
  • My alerts
  • Log in
  • My Cart
American Journal of Science

Advanced Search

  • Home
  • Content
    • Current
    • Archive
    • Special Volumes and Special Issue
  • Subscriptions
    • Subscribers
    • FAQ
    • Terms & Conditions for use of AJS Online
  • Instructions to Authors
    • Focus and paper options
    • Submit your manuscript
  • Site Features
    • Alerts
    • Feedback
    • Usage Statistics
    • RSS
  • About Us
    • Editorial Board
    • The Journal
  • Follow ajs on Twitter
  • Visit ajs on Facebook
  • Follow ajs on Instagram
Research ArticleArticles

Ti3+ – and Ti4+ – rich fassaites at the birth of the solar system: Thermodynamics and applications

Richard O. Sack and Mark S. Ghiorso
American Journal of Science September 2017, 317 (7) 807-845; DOI: https://doi.org/10.2475/07.2017.02
Richard O. Sack
* OFM Research Corporation, Redmond, Washington 98053
  • Find this author on Google Scholar
  • Find this author on PubMed
  • Search for this author on this site
  • For correspondence: fahlore@centurytel.net
Mark S. Ghiorso
** OFM Research Corporation, Seattle, Washington 98115;
  • Find this author on Google Scholar
  • Find this author on PubMed
  • Search for this author on this site
  • For correspondence: ghiorso@ofm-research.org
  • Article
  • Figures & Data
  • References
  • Info & Metrics
  • PDF
Loading

This article requires a subscription to view the full text. If you have a subscription you may use the login form below to view the article. Access to this article can also be purchased.

Log in using your username and password

Forgot your user name or password?

Purchase access

You may purchase access to this article. This will require you to create an account if you don't already have one.
PreviousNext
Back to top

In this issue

American Journal of Science: 317 (7)
American Journal of Science
Vol. 317, Issue 7
1 Sep 2017
  • Table of Contents
  • Table of Contents (PDF)
  • Cover (PDF)
  • About the Cover
  • Index by author
  • Ed Board (PDF)
Print
Download PDF
Article Alerts
Sign In to Email Alerts with your Email Address
Email Article

Thank you for your interest in spreading the word on American Journal of Science.

NOTE: We only request your email address so that the person you are recommending the page to knows that you wanted them to see it, and that it is not junk mail. We do not capture any email address.

Enter multiple addresses on separate lines or separate them with commas.
Ti3+ – and Ti4+ – rich fassaites at the birth of the solar system: Thermodynamics and applications
(Your Name) has sent you a message from American Journal of Science
(Your Name) thought you would like to see the American Journal of Science web site.
CAPTCHA
This question is for testing whether or not you are a human visitor and to prevent automated spam submissions.
14 + 5 =
Solve this simple math problem and enter the result. E.g. for 1+3, enter 4.
Citation Tools
Ti3+ – and Ti4+ – rich fassaites at the birth of the solar system: Thermodynamics and applications
Richard O. Sack, Mark S. Ghiorso
American Journal of Science Sep 2017, 317 (7) 807-845; DOI: 10.2475/07.2017.02

Citation Manager Formats

  • BibTeX
  • Bookends
  • EasyBib
  • EndNote (tagged)
  • EndNote 8 (xml)
  • Medlars
  • Mendeley
  • Papers
  • RefWorks Tagged
  • Ref Manager
  • RIS
  • Zotero
Share
Ti3+ – and Ti4+ – rich fassaites at the birth of the solar system: Thermodynamics and applications
Richard O. Sack, Mark S. Ghiorso
American Journal of Science Sep 2017, 317 (7) 807-845; DOI: 10.2475/07.2017.02
Reddit logo Twitter logo Facebook logo Mendeley logo
  • Tweet Widget
  • Facebook Like
  • Google Plus One

Jump to section

  • Article
    • Abstract
    • INTRODUCTION
    • THERMODYNAMIC FORMULATION
    • DISCUSSION
    • SUMMARY
    • ACKNOWLEDGMENTS
    • Footnotes
    • REFERENCES
  • Figures & Data
  • Info & Metrics
  • References
  • PDF

Related Articles

  • No related articles found.
  • Google Scholar

Cited By...

  • Thermochemistry of melilites I. Towards resolving an inconsistency in nebular condensation calculations
  • Historical natural kinds and mineralogy: Systematizing contingency in the context of necessity
  • Google Scholar

More in this TOC Section

  • Timing and Nd-Hf isotopic mapping of early Mesozoic granitoids in the Qinling Orogen, central China: Implication for architecture, nature and processes of the orogen
  • India in the Nuna to Gondwana supercontinent cycles: Clues from the north Indian and Marwar Blocks
  • Unravelling the P-T-t history of three high-grade metamorphic events in the Epupa Complex, NW Namibia: Implications for the Paleoproterozoic to Mesoproterozoic evolution of the Congo Craton
Show more Articles

Similar Articles

Keywords

  • fassaites
  • thermodynamics
  • oxygen cosmobarometry

Navigate

  • Current Issue
  • Archive

More Information

  • RSS

Other Services

  • About Us

© 2023 American Journal of Science

Powered by HighWire