It’s a bit arbitrary with Meteoritics & Planetary Science. Meteors and planets are both relevant to asteroids, but we have to cut things off somewhere. The June issue (vol. 60, #6) includes:
Alevy, E. G. Dunn, T. L. Krot, A. N. et al. Multiple CV chondrite lithologies in Camel Donga 003 (CK3): Implications for the CV and CK parent bodies Page 1336 .14358
Carbonaceous chondrite meteorites and asteroids are true wonders, if you’ve been following this blog. Both contain water, organics, and other crucial volatiles like nitrogen and sulfur. Dive a little deeper, and the blanket term “carbonaceous chondrite” turns out to include a rich spectrum of subtypes. These include the CV-chondrite meteorites, warmer and drier, and the recently announced CK-chondrites. Here, “V” stands for the Vigarano meteorite, the type specimen (held up as the prototype for all other CVs), while “K” is for Karoonda, the meteorite that set the CK group.
Alevy et al., in this paper, note that a CK meteorite contains clasts- bits of displaced material- that apparently came from a CV body. This indicates mixing in the Solar System. Not a revelation, since the CV and CK groups are related and broadly similar, and we see other examples of mixing among other asteroids. But since the CK meteorites are still a bit rare, relatively, and not much is known about a greater CK parent or parents, this is a worthy contribution.