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Climate Change Challenge Faced by Italian Children: A Nationwide Study. [PDF]
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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,
Hitoshi Mizutani, Takafumi Matsui
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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,
Hitoshi Mizutani, Takafumi Matsui
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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 ...
T. C. Van Flandern, R. P. Binzel
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Photographic positions of Minor Planets
Astronomische Nachrichten, 1992AbstractPhotographic precise positions of 13 minor planets obtained with the G.P.O. astrograph at E.S.O. (La Silla, Chile) in September 1987 are given.
H. Debehogne +2 more
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2014
A brief overview is presented of the current and historical processing of observations and orbits by the Minor Planet Center (MPC). The MPC is delegated by the International Astronomical Union with organizing the cataloging of minor bodies in the solar system. G.V. Williams (*) • T.B.
Timothy B. Spahr, G. V. Williams
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A brief overview is presented of the current and historical processing of observations and orbits by the Minor Planet Center (MPC). The MPC is delegated by the International Astronomical Union with organizing the cataloging of minor bodies in the solar system. G.V. Williams (*) • T.B.
Timothy B. Spahr, G. V. Williams
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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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Astronomische Nachrichten, 1982
AbstractWe represent 266 positions of 77 minor planets determined from plates taken in 1972 and in 1979–1980 with the Schmidt telescope 1340/2000/4000 of KARL SCHWARZSCHILD Observatory Tautenburg.
F. Börngen +2 more
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AbstractWe represent 266 positions of 77 minor planets determined from plates taken in 1972 and in 1979–1980 with the Schmidt telescope 1340/2000/4000 of KARL SCHWARZSCHILD Observatory Tautenburg.
F. Börngen +2 more
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2010
I n our chapters on the Sun and Moon, on the Earth and Venus, and on Mercury and Mars, we have been usually discussing the features and the movements of globes of vast dimensions. The least of all these bodies is the moon, but even our moon is a ball 2,000 miles from one side to the other.
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I n our chapters on the Sun and Moon, on the Earth and Venus, and on Mercury and Mars, we have been usually discussing the features and the movements of globes of vast dimensions. The least of all these bodies is the moon, but even our moon is a ball 2,000 miles from one side to the other.
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2016
The Distant Minor Planets include the cis-Neptunian objects, and the trans-Neptunian objects (TNOs). The TNOs include Kuiper Belt Objects (KBOs), Scattered Disc Objects (SDOs), Detached Objects, and Oort Cloud Objects (OCOs).
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The Distant Minor Planets include the cis-Neptunian objects, and the trans-Neptunian objects (TNOs). The TNOs include Kuiper Belt Objects (KBOs), Scattered Disc Objects (SDOs), Detached Objects, and Oort Cloud Objects (OCOs).
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Photographic observations of Minor Planets
Astronomische Nachrichten, 1928H. van Gent, C. Jackson, H. E. Wood
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