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Journal ArticleDOI

In search of the source of asteroid (101955) Bennu: Applications of the stochastic YORP model

TLDR
In this paper, the authors used a suite of numerical simulations to determine the ages of the families above, how Bennu reached its current orbit, and the most probable source family for Bennu.
About
This article is published in Icarus.The article was published on 2015-02-01. It has received 144 citations till now. The article focuses on the topics: Asteroid family & Asteroid.

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OSIRIS-REx: Sample Return from Asteroid (101955) Bennu

TL;DR: The OSIRIS-REx spacecraft departed for near-Earth asteroid (101955) Bennu via an United Launch Alliance Atlas V 411 evolved expendable launch vehicle at 7:05 p.m. EDT on September 8, 2016, on a seven-year journey to return samples from Bennu as discussed by the authors.
Journal ArticleDOI

The geomorphology, color, and thermal properties of Ryugu: Implications for parent-body processes

Seiji Sugita, +132 more
- 19 Apr 2019 - 
TL;DR: Spectral observations and a principal components analysis suggest that Ryugu originates from the Eulalia or Polana asteroid family in the inner main belt, possibly via more than one generation of parent bodies.
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Hayabusa2 Mission Overview

TL;DR: The Hayabusa2 mission as mentioned in this paper was the first mission to explore a C-type near-Earth asteroid (162173) Ryugu (1999 JU3) to observe and explore the 900 m-sized object, and return samples collected from the surface layer.
Journal ArticleDOI

Debiased orbit and absolute-magnitude distributions for near-Earth objects

TL;DR: In this article, the authors presented a new four-dimensional model of the near-Earth objects population that describes debiased steady-state distributions of semimajor axis, eccentricity, inclination, and absolute magnitude H in the range 17.962 − 56 + 52 + 52 ( 802 − 42 + 48 × 10 3 ) NEOs with H.
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Asteroid family ages

TL;DR: In this paper, a catalog of proper elements with ∼384,000 numbered asteroids and on new methods is available, including a least squares fit of the two sides of a V-shape plot in the proper semimajor axis, inverse diameter plane to determine the corresponding slopes, an advanced error model for the uncertainties of asteroid diameters, an iterative outlier rejection scheme and quality control.
References
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Journal ArticleDOI

Rotational dynamics of a solar system body under solar radiation torques

TL;DR: In this paper, the rotational dynamics of a small solar system body subject to solar radiation torques is investigated, and a set of averaged evolutionary equations are derived as an analytic function of the set of spherical harmonic coefficients.
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Temperature History and Dynamical Evolution of (101955) 1999 RQ 36: A Potential Target for Sample Return from a Primitive Asteroid

TL;DR: In this paper, a model of the orbital evolution of near-Earth objects and thermal models were used to investigate the temperature history of (101955) 1999 RQ{sub 36} (the primary target of the mission OSIRIS-REx, proposed in the program New Frontiers of NASA).
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Thermophysical properties of near-Earth asteroid (341843) 2008 EV5 from WISE data

TL;DR: In this paper, the authors derived the thermal inertia of 2008 EV5, the baseline target for the Marco Polo-R mission proposal, and infer information about the size of the particles on its surface.
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Thermophysical properties of near-Earth asteroid (341843) 2008 EV5 from WISE data

TL;DR: In this article, the authors derived the thermal inertia of the Marco Polo-R mission and inferred the size of the regolith particles on its surface by fitting an asteroid thermophysical model to NASA's WISE infrared data.
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The YORP effect on 25 143 Itokawa

TL;DR: In this paper, the Yarkovsky-O'Keefe-Radzievskii-Paddack (YORP) effect in the rotation period of the asteroid 25143 Itokawa was investigated.
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