English (United Kingdom)

https://curated-unify.zendy.io/wp-json/zendy-region/v1/featured_content/oa?rat=en

https://curated-unify.zendy.io/wp-json/zendy-region/v1/highlighted_journal/

Global: Zendy Plus annual

Presents the access of premium content as premium feature

Premium Content

Presents the keyphrase highlighting as premium feature

Keyphrase Highlighting

Presents the summarisation as premium feature

Summarisation

Insights

Presents the pdf analysis as premium feature

PDF Analysis

Presents the zaia usage as premium feature

ZAIA

Global: Zendy Tools annual

Global: Zendy Free Plan

Global: Zendy Tools monthly

Global: Zendy Plus monthly

Erosive collisions among planetary embryos in the inner solar system can leadto multiple remnant bodies, varied in mass, composition and residual velocity.Some of the smaller, unbound debris may become available to seed the mainasteroid belt. The makeup of these collisionally produced bodies is differentfrom the canonical chondritic composition, in terms of rock/iron ratio and maycontain further shock-processed material. Having some of the material in theasteroid belt owe its origin from collisions of larger planetary bodies mayhelp in explaining some of the diversity and oddities in composition ofdifferent asteroid groups.

Erosive Hit-and-Run Impact Events: Debris Unbound