Results 21 to 30 of about 9,728 (156)
IRAS Minor Planet Survey [PDF]
This chapter describes the contents and organization of the IRAS Minor Planet Survey Data Base and tells how to obtain hard-copy and machine-readable versions of the data.
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Has Kronos Devoured Planet Nine and Its Epigones?
The Planet Nine hypothesis encompasses a body of about 5–8 Earth’s masses whose orbital plane would be inclined to the ecliptic by one or two tens of degrees and whose perihelion distance would be as large as about 240–385 astronomical units. Recently, a
Lorenzo Iorio
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Semi-analytical Ansatz for Approximating Dynamics of Asteroid Rotation Approaching Planet [PDF]
The main motivation of this research is the analytical exploration of the dynamics of asteroid rotation approaching planet, in view of future approach Apophis 2029 to Earth.
Sergey Ershkov
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Asteroid phase curves from Lowell observatory photometric database
We present results obtained from processing large photometric data base. We make use of low-precision (generally rounded to 0.1 mag) and low-accuracy (rms magnitude uncertainties of ±0.2 to 0.3 mag) data obtained from the Minor Planet Center and modified
D. A. Oszkiewicz +6 more
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heliostack: A Novel Approach to Minor Planet Discovery
The study of faint solar system objects is a promising avenue for understanding the origin and evolution of planetary systems. However, such objects are difficult to detect in conventional surveys.
Kevin J. Napier +4 more
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Strong Nongravitational Accelerations and the Potential for Misidentification of Near-Earth Objects
Nongravitational accelerations in the absence of observed activity have recently been identified on near-Earth objects (NEOs), opening the question of the prevalence of anisotropic mass loss in the near-Earth environment.
Aster G. Taylor +7 more
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: The choice of Adams methods with divided differences has been validated for solving of the equations of motion of small bodies of the Solar system. The numerical integration with a variable step size of differential equations of motion of the asteroid ...
V. V. Abramov
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Formation of Multiple Dynamical Classes in the Kuiper Belt via Disk Dissipation
Planetesimal formation likely lasted for millions of years in the solar nebula, and the cold classicals in the Kuiper Belt are suggested to be the direct products of streaming instability.
Tommy Chi Ho Lau +3 more
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Emergence, Evolution and Economics of Coronaviruses
Viruses are the most abundant biological entities on our planet. On the basis of parameters like capsid structure, morphology, genetic material, etc., they are classified into different families.
Sidhant Jain, Meenakshi Rana, Pooja Jain
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DIGITAL ARCHIVE OF UKRVO: THE POSITIONAL ACCURACY OF MINOR PLANETS DETERMINATIONS
Scanning and astrometric processing of two 30x30 cm photographic plates with images of minor planets were conducted. The plates were obtained at the double wide-angle astrograph (DWAA, 400/2000) on the program of photographic sky survey and the program ...
V. Golovnya, V. Andruk
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