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Open AccessJournal ArticleDOI

Asteroid pairs: A complex picture

Petr Pravec, +54 more
- 15 Nov 2019 - 
- Vol. 333, pp 429-463
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TLDR
In this paper, the authors studied a sample of 93 asteroid pairs, i.e., pairs of genetically related asteroids that are on highly similar heliocentric orbits, and derived the absolute magnitude differences of the studied asteroid pairs that provided their mass ratios q.
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This article is published in Icarus.The article was published on 2019-11-15 and is currently open access. It has received 49 citations till now. The article focuses on the topics: Asteroid.

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Citations
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Absolute Magnitudes of Asteroids and a Revision of Asteroid Albedo Estimates from WISE Thermal Observations

TL;DR: In this paper, the authors obtained estimates of the Johnson V absolute magnitude (H ) and slope parameters (G ) for 583 main-belt and near-Earth asteroids observed at Ondřejov and Table Mountain Observatory from 1978 to 2011.

Rotation Rates In The Koronis Family, Complete To H≈11.2

TL;DR: Slivan et al. as discussed by the authors reported the results of an observational survey of rotation lightcurves for members of the Koronis asteroid family that they conducted using CCD imaging cameras at seven different observatories during the period 1998-2005.
References
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Journal ArticleDOI

Phase II of the Small Main-Belt Asteroid Spectroscopic Survey: A Feature-Based Taxonomy

TL;DR: The second phase of the Small Main Belt Asteroid Spectroscopic Survey (SMASSII) produced an internally consistent set of visible-wavelength charge-coupled device (CCD) spectra for 1447 asteroids.
Journal ArticleDOI

The Long-Term Dynamical Behavior of Short-Period Comets

TL;DR: In this paper, the authors developed and tested a new computer code to follow the long-term dynamical evolution of a swarm of test particles in the solar system and found that the Tisserand parameter, T, does not vary substantially for most comets.
Journal ArticleDOI

REBOUND: an open-source multi-purpose N-body code for collisional dynamics

TL;DR: The authorsOUND The authors is a multi-purpose N-body code for collisional dynamics such as planetary rings but can also solve the classical N -body problem, which is highly modular and can be customized easily to work on a wide variety of different problems in astrophysics and beyond.
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