Results 251 to 260 of about 5,829 (302)
Four-million-year Marinoan snowball shows multiple routes to deglaciation. [PDF]
Proc Natl Acad Sci U S ATasistro-Hart AR +3 more
europepmc +1 more source
Automated Mineralogy Analysis of the Apollo 17 73002 Continuous Core Thin Sections Using QEMSCAN Mapping Techniques. [PDF]
J Geophys Res PlanetsBell SK +7 more
europepmc +1 more source
Photoelectric lightcurves of the minor planets 29 Amphitrite, 121 Hermione and 185 Eunike
, 1978 H. Debehogne, Anna Surdej, Jean Surdej
openalex +1 more source
Some of the next articles are maybe not open access.
Related searches:
Related searches:
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
openaire +2 more sources
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
openaire +1 more source
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
openaire +1 more source
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.
Gareth V. Williams, Timothy B. Spahr
openaire +1 more source
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.
Gareth V. Williams, Timothy B. Spahr
openaire +1 more source
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).
openaire +1 more source
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).
openaire +1 more source
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
openaire +1 more source
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 +1 more source
1996
Vesta, the third-largest known asteroid in our solar system, is the only asteroid that can be seen with the naked eye. Vesta is smaller than Ceres and Pallas, the first- and second-largest asteroids, respectively, but its reflective surface allows it to be seen occasionally, without the aid of a telescope, in the nighttime sky.
openaire +1 more source
Vesta, the third-largest known asteroid in our solar system, is the only asteroid that can be seen with the naked eye. Vesta is smaller than Ceres and Pallas, the first- and second-largest asteroids, respectively, but its reflective surface allows it to be seen occasionally, without the aid of a telescope, in the nighttime sky.
openaire +1 more source