Pluto's structure and composition suggest origin in the solar, not a planetary, nebula
- 1 September 1988
- journal article
- Published by Springer Nature in Nature
- Vol. 335 (6187) , 240-243
- https://doi.org/10.1038/335240a0
Abstract
No abstract availableKeywords
This publication has 25 references indexed in Scilit:
- Numerical Evidence That the Motion of Pluto Is ChaoticScience, 1988
- The Pluto-Charon system: The escape of charon's primordial atmosphereIcarus, 1988
- IRAS Serendipitous Survey Observations of Pluto and CharonScience, 1987
- Improved Orbital and Physical Parameters for the Pluto-Charon SystemScience, 1987
- Thermal evolution of a differentiated Ganymede and implications for surface featuresIcarus, 1987
- On the origin of Triton and PlutoNature, 1984
- Graphite-CH4-H2O-CO2 equilibria at low-grade metamorphic conditionsGeology, 1984
- The asteroids as outcomes of catastrophic collisionsIcarus, 1982
- Kinetic inhibition of CO and N2 reduction in circumplanetary nebulae - Implications for satellite compositionThe Astrophysical Journal, 1981
- How fast can an asteroid spin?Icarus, 1981