๐”– Bobbio Scriptorium
โœฆ   LIBER   โœฆ

The Impactor Flux in the Pluto-Charon System

โœ Scribed by Paul R. Weissman; S.Alan Stern


Publisher
Elsevier Science
Year
1994
Tongue
English
Weight
484 KB
Volume
111
Category
Article
ISSN
0019-1035

No coin nor oath required. For personal study only.


๐Ÿ“œ SIMILAR VOLUMES


Tidal evolution and the Pluto-Charon sys
โœ Paolo Farinella; Andrea Milani; Anna M. Nobili; Giovanni B. Valsecchi ๐Ÿ“‚ Article ๐Ÿ“… 1979 ๐Ÿ› Springer Netherlands ๐ŸŒ English โš– 389 KB
Dynamical and Observational Constraints
โœ S.Alan Stern; Joel William Parker; Martin J. Duncan; J.Clark Snowdall Jr.; Harol ๐Ÿ“‚ Article ๐Ÿ“… 1994 ๐Ÿ› Elsevier Science ๐ŸŒ English โš– 632 KB

It is not known if Pluto has other satellites besides its massive partner Charon. In the past, searches for additional satellites in the Pluto-Charon system have extended from the solar-tidal stability boundary ( \(\approx 90\) arcsec from Pluto) inward to about 1 arcsec from Pluto: Here we further

The Charon-Pluto Mass Ratio from MKO Ast
โœ L.A. Young; C.B. Olkin; J.L. Elliot; D.J. Tholen; M.W. Buie ๐Ÿ“‚ Article ๐Ÿ“… 1994 ๐Ÿ› Elsevier Science ๐ŸŒ English โš– 691 KB
Chemical and physical properties of the
โœ F. Merlin; M.A. Barucci; C. de Bergh; F.E. DeMeo; A. Alvarez-Candal; C. Dumas; D ๐Ÿ“‚ Article ๐Ÿ“… 2010 ๐Ÿ› Elsevier Science ๐ŸŒ English โš– 992 KB

We present new photometric and spectroscopic observations of the Pluto-Charon system carried out at the VLT-ESO (Chile) with two 8-m telescopes equipped with the FORS2, ISAAC and SINFONI instruments. The spectra were obtained in the 0.6-2.45 lm range with a spectral resolution from 300 to 1500. The