Arecibo radar observations of 41P/Tuttle-Giacobini-Kresák constrain the nucleus size and rotation
E. S. Howell(Planetary Science Institute), Walter M. Harris(University of Arizona), Carolina Rodriguez Sánchez-Vahamonde, E. G. Rivera‐Valentín, Cassandra Lejoly, Betzaida Aponte-Hernández(Universities Space Research Association), B. E. A. Mueller(Optica), Nalin H. Samarasinha, M. C. Nolan(Planetary Science Institute), Patrick Taylor(York University), S. S. Bhiravarasu, L. F. Zambrano-Marin, Jon D. Giorgini(Jet Propulsion Laboratory)
AAS/Division for Planetary Sciences Meeting Abstracts #49
October 1, 2017
Cited by 1
Related Papers
The operational environment and rotational acceleration of asteroid (101955) Bennu from OSIRIS-REx observations
|Nature Communications|2019|903
OSIRIS-REx: Sample Return from Asteroid (101955) Bennu
|Space Science Reviews|2017|651
H <sub>2</sub> O at the Phoenix Landing Site
|Science|2009|568
The unexpected surface of asteroid (101955) Bennu
|Nature|2019|527
Evidence for widespread hydrated minerals on asteroid (101955) Bennu
|Nature Astronomy|2019|333