𝔖 Bobbio Scriptorium
✦   LIBER   ✦

Late stage of accumulation and chemical composition of the terrestrial planets

✍ Scribed by S. V. Kozlovskaya; G. V. Pechernikova

Publisher
Springer Netherlands
Year
1992
Tongue
English
Weight
407 KB
Volume
57
Category
Article
ISSN
1573-0794

No coin nor oath required. For personal study only.

πŸ“œ SIMILAR VOLUMES

On the Character and Consequences of Lar
On the Character and Consequences of Large Impacts in the Late Stage of Terrestrial Planet Formation
✍ Craig B. Agnor; Robin M. Canup; Harold F. Levison πŸ“‚ Article πŸ“… 1999 πŸ› Elsevier Science 🌐 English βš– 201 KB

We perform three-dimensional N-body integrations of the final stages of terrestrial planet formation. We report the results of 10 simulations beginning with 22-50 initial planetary embryos spanning the range 0.5-1.5 AU, each with an initial mass of 0.04-0.13M βŠ• . Collisions are treated as inelastic

Theory of the late-stage crystallization
Theory of the late-stage crystallization of eutectic composition melts
✍ S.A. Kukushkin; D.A. Grigoriev πŸ“‚ Article πŸ“… 2000 πŸ› Elsevier Science 🌐 English βš– 117 KB

A theory of late-stage crystallization in eutectic point of binary eutectic melts whose pure components have close melting points is developed. A complete system of equations describing the evolution of an ensemble of nuclei has been obtained. An asymptotic solution to this system of equations shows

Love numbers of the moon and of the terr
Love numbers of the moon and of the terrestrial planets
✍ C. Z. Zhang πŸ“‚ Article πŸ“… 1992 πŸ› Springer Netherlands 🌐 English βš– 658 KB

In the IERS Standards (1989), for the Moon the adopted value of the tide Love number, k2, is equal to 0.0222. In this paper using the latest geodetic parameters of the Moon a group of internal structure models are constructed for this celestial body (see Table ), then the dependence of the Moon's co