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Molecular genetics as evidence of environmental harm in ecocriminological analysis. [PDF]
Open Res EurMorelle-Hungría E.
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Nature, 1977
A hypothesis based on the accretion model of planet formation is proposed which can explain why minor planets could not grow into full-sized planets. Temperature and impact-velocity conditions for bouncing, accumulation, and fragmentation of planetesimals are evaluated for silicate and iron planetesimals at the heliocentric distances of Mercury, Venus,
TAKAFUMI MATSUI, HITOSHI MIZUTANI
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A hypothesis based on the accretion model of planet formation is proposed which can explain why minor planets could not grow into full-sized planets. Temperature and impact-velocity conditions for bouncing, accumulation, and fragmentation of planetesimals are evaluated for silicate and iron planetesimals at the heliocentric distances of Mercury, Venus,
TAKAFUMI MATSUI, HITOSHI MIZUTANI
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Minor Planets: The Discovery of Minor Satellites
Science, 1979The recent confirmation of the discovery of a satellite of the minor planet 532 Herculina indicates that other similar anomalous sightings are probably also due to satellites, which must therefore be numerous and commonplace. There are now 23 candidate satellites for eight minor planets, and no one of these minor planets occulting a star has failed to ...
R P, Binzel, T C, VAN Flandern
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Annual Review of Earth and Planetary Sciences, 2006
A review of observations and theories regarding binary asteroids and binary trans-Neptunian objects [collectively, binary minor planets (BMPs)] is presented. To date, these objects have been discovered using a combination of direct imaging, lightcurve analysis, and radar.
Derek C. Richardson, Kevin J. Walsh
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A review of observations and theories regarding binary asteroids and binary trans-Neptunian objects [collectively, binary minor planets (BMPs)] is presented. To date, these objects have been discovered using a combination of direct imaging, lightcurve analysis, and radar.
Derek C. Richardson, Kevin J. Walsh
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The Resonant Remains of Broken Chains from Major and Minor Mergers
Astronomical JournalTESS and Kepler have revealed that practically all close-in sub-Neptunes form in mean-motion resonant chains, most of which unravel on timescales of 100 Myr.
Rixin 日新 Li 李 +3 more
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Minor Planet Center: data processing challenges
Proceedings of the International Astronomical Union, 2015M. Rudenko
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