Nomenclature in the Outer Solar System
By B. Gladman, B. Marsden, C. Vanlaerhoven. 2008
200 citations recorded by the source corpus.
View Paper: https://www.semanticscholar.org/paper/9e4b711101674d05ed939aa6c87bbb3687966c2b
How researchers see this paper
The researchers whose trusted networks rank it highest, strongest advocate first. Every researcher gets a different order.
- D. Nesvorný
- A. Morbidelli
- Harold Levison
- K. Batygin
- R. Gomes
- Fred C. Adams
- M. Brown
- Kleomenis Tsiganis
Citations in the corpus
- The planet nine hypothesis (2019, methodology): “For more comprehensive discussion of specific attributes of the trans-Neptunian solar system, we direct the reader to reviews of the observational characteristics of the Kuiper belt (Luu and Jewitt 2002; Gladman et al. 2008), planet formation (Armitage, 2010), early dynamical evolution (Nesvorný, 20”
- Origin of the structure of the Kuiper belt during a dynamical instability in the orbits of Uranus and Neptune (2007, background): “Conversely, the cold population objects are mostly red.”
- Oort cloud and Scattered Disc formation during a late dynamical instability in the Solar System (2012, background): “Thus we follow Gladman et al. (2008) and additionally impose that a JFC must have q < 7.35 AU so that the object is most likely dynamically controlled by Jupiter.”