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Kidney health for all: caring for people, protecting the planet. [PDF]
Vanholder R +10 more
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Comparison of three conventional impression techniques for flabby tissues with intraoral digital scans. [PDF]
Bhagat M +6 more
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Carbon monoxide dehydrogenase-encoding microorganisms in volcanic astrobiological analogues: an enzyme system to investigate the evolution of life. [PDF]
Latorre V +3 more
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Oceanic fronts shape hemispheric contrasts in polar stratospheric extremes. [PDF]
Omrani NE +5 more
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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
openaire +3 more sources
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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