Results 31 to 40 of about 18,734 (209)
Terrestrial Planet Formation Constrained by Mars and the Structure of the Asteroid Belt
, 2015 Reproducing the large Earth/Mars mass ratio requires a strong mass depletion in solids within the protoplanetary disk between 1 and 3 AU. The Grand Tack model invokes a specific migration history of the giant planets to remove most of the mass initially ...
Izidoro, André +3 more
core +4 more sources
The collisional evolution of undifferentiated asteroids and the formation of chondritic meteoroids [PDF]
, 2016 Most meteorites are fragments from recent collisions experienced in the asteroid belt. In such a hyper-velocity collision, the smaller collision partner is destroyed, whereas a crater on the asteroid is formed or it is entirely disrupted, too.
Beitz, Eike +3 more
core +2 more sources
ACCURACY OF MYKOLAIV ASTEROID OBSERVATIONS WITH DIFFERENT REFERENCE CATALOGUES
Odessa Astronomical Publications, 2017 The results of astrometric reductions of main belt asteroid observations with usage of 3 different reference catalogues are presented. The high precision catalogs CMC15, UCAC4 and GAIA DR1 were used as reference catalogues for calculation
N. V. Maigurova +3 more
doaj +1 more source
Jovian Early Bombardment: planetesimal erosion in the inner asteroid belt
, 2012 The asteroid belt is an open window on the history of the Solar System, as it preserves records of both its formation process and its secular evolution.
Coradini, Angioletta +2 more
core +1 more source
The distribution of basaltic asteroids in the Main Belt [PDF]
Icarus, 2008 We present the observational results of a survey designed to target and detect asteroids whose colors are similar to those of Vesta family members and thus may be considered as candidates for having a basaltic composition. Fifty basaltic candidates were selected with orbital elements that lie outside of the Vesta dynamical family.
Moskovitz, Nicholas A. +6 more
openaire +2 more sources
Size and Albedo Constraints for (152830) Dinkinesh Using WISE Data
The Astrophysical Journal Letters, 2023 Probing small main-belt asteroids provides insight into their formation and evolution through multiple dynamical and collisional processes. These asteroids also overlap in size with the potentially hazardous near-Earth object population and supply the ...
Kiana D. McFadden +9 more
doaj +1 more source
Study the genesis of the Moons of Jupiter and their Physical Properties
مجلة بغداد للعلوم, 2015 A developed model has been put for the hypothesis of capturing moons in explaining the origin of Jupiter moons, and study the change of the orbital properties of these satellites as well as the distance from the planet.
Baghdad Science Journal
doaj +1 more source
The Astronomical Journal, 2023 With a Jupiter-like exoplanet and a debris disk with both asteroid and Kuiper Belt analogs, ϵ Eridani has a fascinating resemblance to our expectations for a young solar system.
Schuyler Grace Wolff +4 more
doaj +1 more source
Mean Motion Resonances in the Asteroid Belt [PDF]
International Astronomical Union Colloquium, 1999 The Kirkwood gaps in the main asteroidal belt (2 – 3.5 AU) coincide with the mean motion resonances with Jupiter (4/1, 3/1, 5/2, 7/3, 2/1). Similarly, several narrower gaps are observed in the outer asteroid belt (3.5 – 4 AU) at places of 11/6, 9/5, 7/4 and 5/3 Jovian resonances (Holman and Murray 1996).
D. Nesvorný, A. Morbidelli
openaire +1 more source
X-Ray Emission Spectroscopy Analysis for Near-Asteroid Belt of Atmospheric of the Comets
Iraqi Journal of Physics, 2022 According to Chandra Survey Observatory Near-Asteroid Belt Comets, the solar wind's contact with the comet produces a variety of spectral characteristics. The study of X-ray spectra produced by charge exchange is presented here. The spectrum of
Rasha S. Najm +2 more
doaj +1 more source